Typedefs
using	code = ===========================================================================V4.1.3 12/18/2002============================================================================Changes which do not affect scientific output:1. The R LUT was eliminated and the equivalent formulation for R , i.e. 1/(m1 e_sun_over_pi), was substituted for it in the only instance of its use, which is in the calculation of the RSB uncertainty index. This reduces the size of the Reflective LUT HDF file by approximately 1/4 to 1/3. The equivalent formulation of R differed from the new by at most 0.056% in test granules and uncertainty differences of at most 1 count(out of a range of 0-15) were found in no more than 1 in 100, 000 pixels. 2. In Preprocess.c, a small error where the trailing dropped scan counter was incremented when the leading dropped scan counter should have been was fixed. This counter is internal only and is not yet used for any purpose. 3. NEW MYD02OBC Metadata Configuration Files. MCST wishes to have the OBC files archived even when the Orbit Number is recorded as "-1". Accordingly, ECS has delivered new MCF files for OBC output having all elements in the OrbitCalculatedSpatialDomain container set to "MANDATORY=FALSE". 4. pgs_in.version is now reset to "1" in Metadata.c before the call to look up the geolocation gringpoint information.============================================================================V4.1.1 CODE SPECIFIC TO MODIS/AQUA(FM1) 10/03/2002============================================================================Two changes were made to the code which do not affect scientific output:1. A bug which caused PGE02 to fail when scans were dropped between granules was fixed.(The length of the error message generated was shortened.) 2. Messages regarding an invalid MCST LUT Version or an invalid Write High Resolution Night Mode Output value in the PCF file were added.==============================================================================V4.1.0 CODE SPECIFIC TO MODIS/AQUA(FM1)(NEVER USED IN PRODUCTION) 07/30/2002==============================================================================Changes which impact scientific output of code:1. The LUT type of the RVS corrections was changed to piecewise linear. In addition the RVS LUTs were changed from listing the RVS corrections to listing the quadratic coefficients necessary to make the RVS corrections. The coefficients are now calculated by interpolating on the granule collection time and the RVS corrections are then generated using the interpolated coefficients. Previously used Emissive and Reflective RVS LUT tables were eliminated and new ones introduced. Several changes were made to the code which should not affect scientific output. They are:1. The ADC correction algorithm and related LUTs were stripped from the code.(The ADC correction has always been set to "0" so this has no scientific impact.) 2. Some small changes to the code, chiefly to casting of variables, were added to make it LINUX-compatible. Output of code run on LINUX machines displays differences of at most 1 scaled integer(SI) from output of code run on IRIX machines. The data type of the LUT "dn_sat_ev" was changed to float64 to avoid discrepancies seen between MOD_PR02 run on LINUX systems and IRIX systems where values were flagged under one operating system but not the other. 3. Checking for non-functioning detectors, sector rotation, incalculable values of the Emissive calibration factor "b1", and incalculable values of SV or BB averages was moved outside the loop over frames in Emissive_Cal.c since none of these quantities are frame-dependent. 4. The code was altered so that if up to five scans are dropped between the leading/middle or middle/trailing granules, the leading or trailing granule will still be used in emissive calibration to form a cross-granule average. QA bits 25 and 26 are set for a gap between the leading/middle and middle/trailing granules respectively. This may in rare instances lead to a change in emissive calibration coefficients for scans at the beginning or end of a granule. 5.(MODIS/AQUA ONLY) The name of the seed(error message) file was changed from "MODIS_36100.h" to "MODIS_36110.h". 6. Metadata.c was changed so that the source of the geolocation metadata is the input geolocation file rather than the L1A granule. 7. To reduce to overall size of the reflective LUT HDF files, fill values were eliminated from all LUTs previously dimensioned "BDSM"([NUM_REFLECTIVE_BANDS] [MAX_DETECTORS_PER_BAND] [MAX_SAMPLES_PER_BAND] [NUM_MIRROR_SIDES]) in the LUT HDF files. Each table piece is stored in the HDF file with dimensions NUM_REFLECTIVE_INDICES, where NUM_REFLECTIVE_INDICES=[NUM_250M_BANDS DETECTORS_PER_250M_BAND SAMPLES_PER_250M_BAND NUM_MIRROR_SIDES]+[NUM_500M_BANDS DETECTORS_PER_500M_BAND SAMPLES_PER_500M_BAND NUM_MIRROR_SIDES]+[NUM_1000M_BANDS DETECTORS_PER_1KM_BAND SAMPLES_PER_1KM_BAND NUM_MIRROR_SIDES] with SAMPLES_PER_250M_BAND=4, SAMPLES_PER_500M_BAND=2, and SAMPLES_PER_1KM_BAND=1. Values within each table piece appear in the order listed above. The overall dimensions of time dependent BDSM LUTs are now[NUM_TIMES] *[NUM_REFLECTIVE_INDICES], where NUM_TIMES is the number of time dependent table pieces. 8. Checking for non-functioning detectors, sector rotation, incalculable values of the Emissive calibration factor "b1", and incalculable values of SV or BB averages was moved outside the loop over frames in Emissive_Cal.c since none of these quantities are frame-dependent. 9. The code was altered so that if up to five scans are dropped between the leading/middle or middle/trailing granules, the leading or trailing granule will still be used in emissive calibration to form a cross-granule average. QA bits 25 and 26 are set for a gap between the leading/middle and middle/trailing granules respectively. This may in rare instances lead to a change in emissive calibration coefficients for scans at the beginning or end of a granule. 10. The array of b1s in Preprocess.c was being initialized to -1 outside the loop over bands, which meant that if b1 could not be computed, the value of b1 from the previous band for that scan/detector combination was used. The initialization was moved inside the band loop.============================================================================V3.1.0(Original Aqua-specific code version) 02/06/2002============================================================================AQUA-Specific changes made:1. A correction to a problem with blackbody warmup on bands 33, 35, and 36 was inserted. PC Bands 33, 35, and 36 on MODIS Aqua saturate on BB warmup before 310K, which means current code will not provide correct b1 calibration coefficients when the BB temperatures are above the saturation threshold. A LUT with default b1s and band-dependent temperature thresholds will be inserted in code. If the BB temperature is over the saturation threshold for the band, the default b1 from the table is used. 2. The number of possible wavelengths in the Emissive LUT RSR file was changed to 67 in order to accommodate the Aqua RSR tables. 3. Several changes to the upper and lower bound limits on LUT values were inserted. Changes to both Aqua and Terra Code:1. A check was put into Emissive_Cal.c to see whether the value of b1 being used to calibrate a pixel is negative. If so, the pixel is flagged with the newly created flag TEB_B1_NOT_CALCULATED, value 65526, and the number of pixels for which this occurs is counted in the QA_common table. 2. The array of b1s in Preprocess.c was being initialized to -1 outside the loop over bands, which meant that if b1 could not be computed, the value of b1 from the previous band for that scan/detector combination was used. The initialization was moved inside the band loop. 3. Minor code changes were made to eliminate compiler warnings when the code is compiled in 64-bit mode. 4. Temperature equations were upgraded to be MODIS/Aqua or MODIS/Terra specific and temperature conversion coefficients for Aqua were inserted.========================================================================================================================================================ALL CHANGES BELOW ARE TO COMMON TERRA/AQUA CODE USED BEFORE 02/06/2002========================================================================================================================================================v3.0.1 11/26/2001============================================================================Several small changes to the code were made, none of which changes the scientific output:1. The code was changed so that production of 250m and 500m resolution data when all scans of a granule are in night mode may be turned off/on through the PCF file. 2. A check on the times of the leading and trailing granules was inserted. If a leading or trailing granule does not immediately precede or follow(respectively) the middle granule, it is treated as a missing granule and a warning message is printed. 3. The code now reads the "MCST Version Number"(e.g. "3.0.1.0_Terra") from the PCF file and checks it against the MCST Version number contained in the LUT HDF files. This was done to allow the user to make sure the code is being run using the correct LUT files.(The designators "0_Terra", "1_Terra", etc.) refer to the LUT versions.) 4. A small bug in Preprocess.c was corrected

Functions
*******************************************HISTORY FILE for MOD_PR02AQUA Version ****Point of no algorithm change is made in this so the	scans (one mirror side) after the sector rotation are contaminated with anomalously high radiance values. A similar timing issue appeared before the sector rotation was fixed in V6.1.3. Our analysis indicates the ‘SET_FR_ENC_DELTA’ telemetry correlates well with the sector rotation encoder position. The use of this telemetry point to determine scans that are sector rotated should fix the anomaly occured before and after the sector rotation(usually due to the lunar roll maneuver). The fix related to the sector rotation in V6.1.3 is removed in this version.

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are	even (e.g. 4.2.0, 5.6.8) and all MODIS/Aqua PGE02 code versions are odd(e.g. 4.2.1

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration	File (PCF) so that direct broadcast users may change it if they wish. 6. The metadata environment variable "ProcessingEnvironment" was added. Its value is obtained by calling the appropriate POSIX function. 7. New metadata configuration files were introduced which change the PGE Collection number to "4" and add the "ProcessingEnvironment" variable.

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out	Box (SV KOB). If the Moon is in the KOB

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be	calibrated (i.e., the BB DNs are not used as a backup for the SWIR bands). 3. Piecewise linear LUT capability was added to the code. If a LUT table is marked as piecewise linear

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT	table (e.g. m1) to be used for interpolation. The table values will be linearly interpolated using the tables corresponding to the node times bracketing the granule time. If the granule time falls before the time of the first node or after the time of the last node

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration	files (MCFs) were changed to remove "ASSOCIATEDPLATFORMSHORTNAME.2"

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact	details (Other changes) 1. Following a suggestion by Xinmin Hua of EOS

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off there was no difference to the product The CPU time decreased by about for a day case and for a night case A minor bug in calculating the uncertainty index for emissive bands was corrected The frame	index (0-based) was previously being used the frame number(1-based) should have been used. There were only a few minor changes to the uncertainty index(maximum of 1 digit). 3. Some inefficient arrays(Sigma_RVS_norm_sq) were eliminated and some code lines in Preprocess_L1A_Data were moved into Process_OBCEng_Emiss. There were no changes to the product. Required RAM was reduced by 20 MB. Now

Variables
*******************************************HISTORY FILE for MOD_PR02AQUA Version **	August

*******************************************HISTORY FILE for MOD_PR02AQUA Version ****Point of	Contact

*******************************************HISTORY FILE for MOD_PR02AQUA Version ****Point of no algorithm change is made in this	delivery

*******************************************HISTORY FILE for MOD_PR02AQUA Version ****Point of no algorithm change is made in this so the and when the blackbody temperature is above a threshold Since the LWIR FPA temperature oscillates on	orbit

*******************************************HISTORY FILE for MOD_PR02AQUA Version ****Point of no algorithm change is made in this so the and when the blackbody temperature is above a threshold Since the LWIR FPA temperature oscillates on its impact to the default b1 increases gradually A new algorithm to calculate the default b1 on orbit considering the impact of the real time LWIR FPA temperature is applied in this code	change

u2	__pad0__

u3	__pad1__

u4	__pad2__

u5	__pad3__

u5	Uncertainty

u5 which has been done in	V6

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific	output

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a	result

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are	inaccurate

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT	production

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT	detector_quality_flag2_values_table

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe	lists

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV	Data

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead	detectors

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments	correction

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly	interpreted

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track	direction

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS	keywords

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector	dependency

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non	functioning

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for	Band

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive	bands

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in	L1A

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	SV_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	SRCA_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	BB_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	SD_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	SV_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific	SRCA_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the	to

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this	case

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV	data

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips	creating

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips	opening

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV	file

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning	of

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf	files

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA	flags

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA has been changed Until	now

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA has been changed Until Level has set the maneuver bit flag on a scan by scan basis by keying on the SS_FR_SCIABNORM flag passed to Level by the Level telemetry data This flag is manually set by Flight Operations	personnel

PGE01	__pad4__

PGE01 indicating that PGE02 Version and PGE01 Version were used to produce the granule	PGE02

PGE01	__pad5__

PGE01	__pad6__

PGE01 indicating that PGE02	Version

PGE01 indicating that PGE02 PGE01 V6 for	MOD01

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in	late

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration	March

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration A sign used in error in the second order term was changed to	a

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration A sign used in error in the second order term was changed to already in place for MODIS TERRA was implemented for MODIS AQUA A time dependent LUT was added which gives coefficients for a detector specific crosstalk correction based on the aggregated Band radiances The Band scaled integers are adjusted by the Band correction	term

actual height is km The height is used only	once

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out the SV data	average

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out the SV data which is subtracted from Earth View data before	calibration

an array had not been initialized Several spelling and grammar corrections were	made

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF	Previously

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old	algorithm

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body	DNs

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of	tables

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration	ASSOCIATEDSENSORSHORTNAME

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification	documents

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands	preprocessing

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off	differences

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off there was no difference to the product The CPU time decreased by about for a day case and for a night case A minor bug in calculating the uncertainty index for emissive bands was corrected The frame the required RAM for each execution is MB on the DEC ALPHA and MB on the SGI Octane	v2

Typedef Documentation

◆ code

instead the metadata field ProcessingEnvinronment is filled in from the output of a call to the POSIX compliant function uname from within the L1B code A small bug in L1B_Tables an incorrect comparison of RVS coefficients for TEBs to RVS coefficients for RSBs was being made This was replaced with a comparison between TEB coefficients This error never resulted in an incorrect RVS correction but did lead to recalculating the coefficients for each detector in a thermal band even if the coefficients were the same for all detectors To reduce to overall size of the reflective LUT HDF fill values were eliminated from all LUTs previously dimensioned where and where NUM_TIMES is the number of time dependent table pieces In Preprocess a small error where the trailing dropped scan counter was incremented when the leading dropped scan counter should have been was fixed This counter is internal only and is not yet used for any chiefly to casting of were added to make it LINUX compatible Output of code run on LINUX machines displays differences of at most scaled sector incalculable values of the Emissive calibration factor and incalculable values of SV or BB averages was moved outside the loop over frames in Emissive_Cal c since none of these quantities are frame dependent Initialization of b1 and XMS values in Preprocess c routine Process_OBCENG_Emiss was moved inside the detector loops The code was altered so that if up to five scans are dropped between the leading middle or middle trailing the leading or trailing granule will still be used in emissive calibration to form a cross granule average QA bits and are set for a gap between the leading middle and middle trailing granules respectively This may in rare instances lead to a change in emissive calibration coefficients for scans at the beginning or end of a granule A small bug in the Band correction algorithm was corrected an uncertainty value was being checked against an upper bound whereas the proper quantity to be checked was the corresponding which is the product of the Band radiance times the ratio of the Band to Band scaling factors times the LUT correction value for that detector In addition a new LUT which allows for a frame offset with regard to the Band radiance was added A LUT which switches the correction off or on was also added Changes which do not affect scientific output of the code

Definition at line 661 of file HISTORY.txt.

Function Documentation

◆ Box()

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out Box ( SV KOB )

◆ calibrated()

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be calibrated	(	i.	e.,
		the BB DNs are not used as a backup for the SWIR	bands
	)

◆ details()

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact details ( Other changes )

◆ even()

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are even	(	e.g. 4.2.	0,
		5.6.	8
	)

◆ File()

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration File ( PCF )

◆ files()

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration files ( MCFs )

◆ index()

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off there was no difference to the product The CPU time decreased by about for a day case and for a night case A minor bug in calculating the uncertainty index for emissive bands was corrected The frame index ( 0- based )

◆ scans()

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about scans ( one mirror side )

Initial value:

============================================================================
  V5.0.37 (Aqua)                                                   06/29/2009
  ============================================================================
  Changes from v5.0.35 which do not affect scientific output:
  1. If the ReprocessingActual from pcf is "Near Real Time"

◆ table()

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT table ( e.g. m1 )

Variable Documentation

◆ pad0

u2 __pad0__

Definition at line 127 of file HISTORY.txt.

◆ pad1

u3 __pad1__

Definition at line 128 of file HISTORY.txt.

◆ pad2

u4 __pad2__

Definition at line 129 of file HISTORY.txt.

◆ pad3

u5 __pad3__

Definition at line 131 of file HISTORY.txt.

◆ pad4

PGE01 __pad4__

Definition at line 392 of file HISTORY.txt.

◆ pad5

PGE01 __pad5__

Definition at line 395 of file HISTORY.txt.

◆ pad6

PGE01 __pad6__

Definition at line 395 of file HISTORY.txt.

◆ a

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration A sign used in error in the second order term was changed to a

Initial value:

============================================================================
  V4.1.5                                                            04/25/2003
  ============================================================================
  Changes which affect scientific output:
  
  1.  Changed SWIR out-of-band correction "sending" band from being
      hard-coded as Band 28 to being determined by a LUT value.  This was
      done because MODIS/AQUA data shows significantly better SWIR
      out-of-band correction if Band 25 is the "sending" band.  
 
  2.  The destriping algorithm devised by C. Moeller for Band 26

Definition at line 424 of file HISTORY.txt.

◆ algorithm

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old algorithm

Definition at line 682 of file HISTORY.txt.

◆ ASSOCIATEDSENSORSHORTNAME

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration ASSOCIATEDSENSORSHORTNAME

Definition at line 703 of file HISTORY.txt.

◆ August

******************************************** * HISTORY FILE for MOD_PR02AQUA* * Version* * August

Definition at line 4 of file HISTORY.txt.

◆ average

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out the SV data average

Definition at line 450 of file HISTORY.txt.

◆ Band

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for Band

Definition at line 299 of file HISTORY.txt.

◆ bands

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR bands

Definition at line 299 of file HISTORY.txt.

◆ BB_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific BB_250m

Definition at line 334 of file HISTORY.txt.

◆ calibration

actual height is km The height is used only to determine whether the Moon is in the Space View Keep Out the SV data which is subtracted from Earth View data before calibration

Definition at line 450 of file HISTORY.txt.

◆ case

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this case

Definition at line 343 of file HISTORY.txt.

◆ change

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the change

Initial value:

============================================================================
  V6.1.13 (Aqua)                                                    04/15/2011
       Changes shown below are differences from MOD_PR02 V6.1.11 (Aqua)
  ============================================================================
  A minor code typo error correction.
 
  ============================================================================
  V6.1.11 (Aqua)                                                    03/31/2011
       Changes shown below are differences from MOD_PR02 V6.1.9 (Aqua)
  ============================================================================
  1. The algorithm to calculate uncertainties for reflective solar bands (RSB)
     is updated. The current uncertainty in L1B code includes 9 terms from
     prelaunch analysis. The new algorithm regroups them with the new added
     contributions into 5 terms:
     u1: the common term (AOI and time independent)

Definition at line 111 of file HISTORY.txt.

◆ Contact

******************************************** * HISTORY FILE for MOD_PR02AQUA* * Version * * * * Point of Contact

Definition at line 37 of file HISTORY.txt.

◆ correction

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments correction

Initial value:

============================================================================
  V5.0.7 (Aqua)                                                     03/01/2005
  ============================================================================
  Changes from v5.0.5 which do not affect scientific output:
 
  1.  Corrected setting of the geo to data dimension mapping offset value
      (track direction for 250m band data only) in the current PGE02 code
      (Collect 4 and 5).
 
  ============================================================================
  V5.0.5 (Aqua)                                                     2005-01-13
  ============================================================================
  Changes from 5.0.1 which do not affect scientific output:
 
  1.  Added new file attributes prefixed with HDFEOS_FractionalOffset to each
      dimension of the swath in every MODIS product file

Definition at line 256 of file HISTORY.txt.

◆ creating

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips creating

Definition at line 344 of file HISTORY.txt.

◆ Data

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV Data

Definition at line 222 of file HISTORY.txt.

◆ data

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV data

Definition at line 344 of file HISTORY.txt.

◆ delivery

******************************************** * HISTORY FILE for MOD_PR02AQUA* * Version * * * * Point of no algorithm change is made in this delivery

Initial value:

============================================================================
  V6.1.37 (Aqua)                                                    04/19/2017
       Changes shown below are differences from MOD_PR02 V6.1.35 (Aqua)
  ============================================================================
  Only PGE02 version is updated for MODIS processing on CentOS 7 system with
  SDP toolkit 5.2.19
 
  ============================================================================
  V5.0.43 (Aqua)                                                    03/23/2015
       Changes shown below are differences from MOD_PR02 V5.0.41 (Aqua)
  ============================================================================
  Changes noted for V6.1.35 (Aqua) below were also instituted for this
  version.
 
  ============================================================================
  V6.1.35 (Aqua)                                                    03/12/2015
       Changes shown below are differences from MOD_PR02 V6.1.33 (Aqua)
  ============================================================================
  Changes from v6.1.33 which may affect scientific output:
  A situation can occur in which a scan which contains sector rotated data has
  a telemetry value indicating the completeness of the sector rotation. This 
  issue is caused by the timing of the instrument command to perform the 
  sector rotation and the recording of the telemetry point that reports the 
  status of sector rotation. In this case a scan is considered valid by L1B 
  and pass through the calibration - reporting extremely high radiances. 
  Operationally the TEB calibration uses a 40 scan average coefficient

Definition at line 39 of file HISTORY.txt.

◆ dependency

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector dependency

Definition at line 293 of file HISTORY.txt.

◆ detector_quality_flag2_values_table

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT detector_quality_flag2_values_table

Definition at line 219 of file HISTORY.txt.

◆ detectors

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead detectors

Initial value:

============================================================================
  V5.0.35 (Aqua)                                                    01/15/2008
  ============================================================================
  Changes from v5.0.33 which do not affect scientific output:
 
  1.  Relax the RVS correction limit range from [0.8, 1.2] to [0.4, 2.4].
 
  ============================================================================
  V5.1.1 (Aqua)    NEVER USED IN DATA PRODUCTION                    02/28/2007
  ============================================================================
  This is a prototype code version to be used it to create test data not only
  for PGE02

Definition at line 226 of file HISTORY.txt.

◆ differences

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off differences

Definition at line 714 of file HISTORY.txt.

◆ direction

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track direction

Definition at line 273 of file HISTORY.txt.

◆ DNs

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body DNs

Definition at line 683 of file HISTORY.txt.

◆ documents

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification documents

Definition at line 707 of file HISTORY.txt.

◆ file

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV file

Definition at line 347 of file HISTORY.txt.

◆ files

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf files

Initial value:

============================================================================
  V4.3.1 (Aqua)                                                     11/07/2003
  ============================================================================
 
  Changes which do not affect scientific output:
 
  1.  The derivation of the maneuver flag

Definition at line 354 of file HISTORY.txt.

◆ flags

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA flags

Definition at line 361 of file HISTORY.txt.

◆ functioning

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non functioning

Definition at line 294 of file HISTORY.txt.

◆ inaccurate

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are inaccurate

Definition at line 188 of file HISTORY.txt.

◆ interpreted

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly interpreted

Definition at line 272 of file HISTORY.txt.

◆ keywords

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS keywords

Initial value:

============================================================================
  V4.3.15 (Aqua)                                                     2004-12-30
  ============================================================================
  Changes from 4.3.1 which do not affect scientific output:
 
  1. Changed makefile to allow building with SDP Toolkit 5.2.9.
 
  ============================================================================
  V5.0.1 (Aqua)                                                     12/10/2004
  ============================================================================
 
  Changes which affect scientific output:
 
  1.  Code change for adding a new look-up-table

Definition at line 278 of file HISTORY.txt.

◆ L1A

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in L1A

Definition at line 318 of file HISTORY.txt.

◆ late

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in late

Definition at line 399 of file HISTORY.txt.

◆ lists

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe lists

Definition at line 221 of file HISTORY.txt.

◆ made

an array had not been initialized Several spelling and grammar corrections were made

Initial value:

============================================================================
  v3.0.0                                                          4/01/2001
  ============================================================================
  (Principal changes)
  1. The mechanics of setting some ECS core metadata was changed.
     ReprocessingPlanned and ReprocessingActual are now set using run-time
     parameters from the PCF (LUNs 800600 and 800605, respectively).
     The "vvv" field of the LocalGranuleID is now set from the VersionID

Definition at line 665 of file HISTORY.txt.

◆ March

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration March

Definition at line 421 of file HISTORY.txt.

◆ MOD01

PGE01 indicating that PGE02 PGE01 V6 for MOD01

Definition at line 396 of file HISTORY.txt.

◆ now

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA has been changed Until now

Definition at line 361 of file HISTORY.txt.

◆ of

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning of

Definition at line 352 of file HISTORY.txt.

◆ once

actual height is km The height is used only once

Definition at line 448 of file HISTORY.txt.

◆ opening

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips opening

Definition at line 344 of file HISTORY.txt.

◆ orbit

******************************************** * HISTORY FILE for MOD_PR02AQUA* * Version * * * * Point of no algorithm change is made in this so the and when the blackbody temperature is above a threshold Since the LWIR FPA temperature oscillates on orbit

Definition at line 106 of file HISTORY.txt.

◆ output

instead the metadata field ProcessingEnvinronment is filled in from the output of a call to the POSIX compliant function uname from within the L1B code A small bug in L1B_Tables an incorrect comparison of RVS coefficients for TEBs to RVS coefficients for RSBs was being made This was replaced with a comparison between TEB coefficients This error never resulted in an incorrect RVS correction but did lead to recalculating the coefficients for each detector in a thermal band even if the coefficients were the same for all detectors To reduce to overall size of the reflective LUT HDF fill values were eliminated from all LUTs previously dimensioned where and where NUM_TIMES is the number of time dependent table pieces In Preprocess a small error where the trailing dropped scan counter was incremented when the leading dropped scan counter should have been was fixed This counter is internal only and is not yet used for any chiefly to casting of were added to make it LINUX compatible Output of code run on LINUX machines displays differences of at most scaled sector incalculable values of the Emissive calibration factor and incalculable values of SV or BB averages was moved outside the loop over frames in Emissive_Cal c since none of these quantities are frame dependent Initialization of b1 and XMS values in Preprocess c routine Process_OBCENG_Emiss was moved inside the detector loops The code was altered so that if up to five scans are dropped between the leading middle or middle trailing the leading or trailing granule will still be used in emissive calibration to form a cross granule average QA bits and are set for a gap between the leading middle and middle trailing granules respectively This may in rare instances lead to a change in emissive calibration coefficients for scans at the beginning or end of a granule A small bug in the Band correction algorithm was corrected an uncertainty value was being checked against an upper bound whereas the proper quantity to be checked was the corresponding which is the product of the Band radiance times the ratio of the Band to Band scaling factors times the LUT correction value for that detector In addition a new LUT which allows for a frame offset with regard to the Band radiance was added A LUT which switches the correction off or on was also added Changes which do not affect scientific output of the the pixel is flagged with the newly created flag and the number of pixels for which this occurs is counted in the QA_common table The array of b1s in Preprocess c was being initialized to outside the loop over which meant that if b1 could not be the value of b1 from the previous band for that scan detector combination was used The initialization was moved inside the band loop Minor code changes were made to eliminate compiler warnings when the code is compiled in bit mode Temperature equations were upgraded to be MODIS AQUA or MODIS TERRA specific and temperature conversion coefficients for AQUA were MOD_PR02 will not cease execution if the value of this parameter is not but will print a none of which changes the scientific output

Definition at line 186 of file HISTORY.txt.

◆ personnel

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata and the closing of the L1B OBC hdf which is Bit in the scan by scan bit QA has been changed Until Level has set the maneuver bit flag on a scan by scan basis by keying on the SS_FR_SCIABNORM flag passed to Level by the Level telemetry data This flag is manually set by Flight Operations personnel

Definition at line 364 of file HISTORY.txt.

◆ PGE02

PGE01 indicating that PGE02 Version and PGE01 Version were used to produce the granule PGE02

Definition at line 395 of file HISTORY.txt.

◆ preprocessing

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands preprocessing

Definition at line 712 of file HISTORY.txt.

◆ Previously

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF Previously

Definition at line 674 of file HISTORY.txt.

◆ production

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production

Initial value:

============================================================================
  V6.1.1 (Aqua)                                                     12/18/2008
  ============================================================================
  Changes from v6.0.1 which do not affect scientific output:
 
  1. Extended rvs ascii lut validation limitation from [-2.0E-4, 1.2] to
     [-4.0E-4, 2.4].
 
  ============================================================================
  V6.0.1 (Aqua)         NEVER USED FOR DATA PRODUCTION              05/23/2008
  ============================================================================
  Changes from v5.0.35 which affect scientific output:
 
  1.  Added a new QA LUT

Definition at line 206 of file HISTORY.txt.

◆ result

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a result

Definition at line 188 of file HISTORY.txt.

◆ SD_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific SD_500m

Definition at line 334 of file HISTORY.txt.

◆ SRCA_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific SRCA_250m

Definition at line 333 of file HISTORY.txt.

◆ SRCA_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific SRCA_500m

Definition at line 334 of file HISTORY.txt.

◆ SV_250m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific SV_250m

Definition at line 333 of file HISTORY.txt.

◆ SV_500m

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific SV_500m

Definition at line 334 of file HISTORY.txt.

◆ tables

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of tables

Definition at line 695 of file HISTORY.txt.

◆ term

PGE01 indicating that PGE02 PGE01 V6 for and PGE01 V2 for MOD03 were used to produce the granule By convention adopted in all MODIS Terra PGE02 code versions are The fourth digit of the PGE02 version denotes the LUT version used to produce the granule The source of the metadata environment variable ProcessingCenter was changed from a QA LUT value to the Process Configuration A sign used in error in the second order term was changed to already in place for MODIS TERRA was implemented for MODIS AQUA A time dependent LUT was added which gives coefficients for a detector specific crosstalk correction based on the aggregated Band radiances The Band scaled integers are adjusted by the Band correction term

Definition at line 439 of file HISTORY.txt.

◆ to

u5 which has been done in the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT production Changes from v6 which may affect scientific the sector rotation may actually occur during one of the scans earlier than the one where it is first reported As a the b1 values are about the LOCALGRANULEID metadata should have an extension NRT It is requested to identify the NRT to fill pixels affected by dead subframes with a special value Output the metadata of noisy and dead subframe Dead Subframe EV and Detector Quality Flag2 Removed the function call of Fill_Dead_Detector_SI to stop interpolating SI values for dead but also for all downstream products for science test only Changes from v5 which will affect scientific to conform to MODIS requirements Removed the Mixed option from the ScanType in the code because the L1A Scan Type is never Mixed Changed for ANSI C compliance and comments to better document the fact that when the HDF_EOS metadata is stricly the and products are off by and in the track respectively Corrected some misspelling of RCS swir_oob_sending_detector to the Reflective LUTs to enable the SWIR OOB correction detector so that if any of the sending detectors becomes noisy or non near by good detectors from the same sending band can be specified as the substitute in the new look up table Code change for adding an additional dimension of mirror side to the Band_21_b1 LUT to separate the coefficient of the two mirror sides for just like other thermal emissive so that the L1B code can calibrate Band scan to scan with mirror side dependency which leads better calibration result Changes which do not affect scientific when the EV data are not provided in this Crosstalk Correction will not be performed to the Band calibration data Changes which do not affect scientific and BB_500m in L1A Logic was added to turn off the or to spatial aggregation processes and the EV_250m_Aggr1km_RefSB and EV_500m_Aggr1km_RefSB fields were set to fill values when SDSs EV_250m and EV_500m are absent in L1A file Logic was added to skip the processing and turn off the output of the L1B QKM and HKM EV data when EV_250m and EV_500m are absent from L1A In this the new process avoids accessing and reading the and L1A EV skips and writing to the L1B and EV omits reading and subsampling SDSs from geolocation file and writing them to the L1B and omits writing metadata to L1B and EV and skips closing the L1A and L1B EV and SDSs Logic was added to turn off the L1B OBC output when the high resolution OBC SDSs are absent from L1A This is accomplished by skipping the openning the writing of metadata to

Definition at line 336 of file HISTORY.txt.

◆ Uncertainty

u5 Uncertainty

Initial value:

= sqrt(u1*u1+u2*u2+u3*u3+u4*u4+u5*u5)
 
     There are 6 new reflective LUTs added and 8 old LUTs made obsolete.
     The change will affect RSB UI (uncertainty index) field in L1B product.
 
  2. The algorithm to calculate uncertainties for Theramal Emissive bands 
     (TEB) is also updated. The perturbation method used to derive UI terms 
     in the current L1B is replaced with an analytical expression approach.
     There are 11 new emissive LUTs added and 5 old LUTs made obsolete.
     The change will affect TEB UI (uncertainty index) field in L1B product.
 
  3. The quadratic reflective solar bands (RSB) RVS is changed to 4th order.
 
  ============================================================================
  V6.1.9 (Aqua)                                                     11/15/2010
  ============================================================================
  Changes from v6.1.9 which do not affect scientific output:
  1. A fatal error occurs when both sides of PCLW electronics are on 
     simultaneously in the previous L1B code. The case is actually permissible
     according to the MODIS design. A change is made to drop the scan affected 
     instead of the whole granule.
 
  ============================================================================
  V5.0.39 (Aqua)                                                   02/25/2010
  ============================================================================
  Changes from v5.0.37 which may affect scientific output:
  1. Fixed the sector rotation anomaly

Definition at line 132 of file HISTORY.txt.

◆ v2

an array had not been initialized Several spelling and grammar corrections were which is read from the appropriate MCF the above metadata values were hard coded A problem calculating the average background DN for SWIR bands when the moon is in the space view port was corrected The new algorithm used to calculate the average background DN for all reflective bands when the moon is in the space view port is now the same as the algorithm employed by the thermal bands For non SWIR changes in the averages are typically less than Also for non SWIR the black body DNs remain a backup in case the SV DNs are not available For SWIR the changes in computed averages were larger because the old which used the black body suffered from contamination by the micron leak As a consequence of the if SV DNs are not available for the SWIR the EV pixels will not be the granule time is used to identify the appropriate tables within the set given for one LUT the first two or last two tables respectively will be used for the interpolation If there is only one LUT in the set of it will be treated as a constant LUT The manner in which Earth View data is checked for saturation was changed Previously the raw Earth View DNs and Space View DNs were checked against the lookup table values contained in the table dn_sat The change made is to check the raw Earth and Space View DNs to be sure they are less than the maximum saturation value and to check the Space View subtracted Earth View dns against a set of values contained in the new lookup table dn_sat_ev The metadata configuration and ASSOCIATEDINSTRUMENTSHORTNAME from the MOD02HKM product The same metatdata with extensions and were removed from the MOD021KM and MOD02OBC products ASSOCIATEDSENSORSHORTNAME was set to MODIS in all products These changes are reflected in new File Specification which users may consult for exact the pow functions were eliminated in Emissive_Cal and Emissive bands replaced by more efficient code Other calculations throughout the code were also made more efficient Aside from a few round off there was no difference to the product The CPU time decreased by about for a day case and for a night case A minor bug in calculating the uncertainty index for emissive bands was corrected The frame the required RAM for each execution is MB on the DEC ALPHA and MB on the SGI Octane v2

Initial value:

============================================================================
  (Principal changes)
  1. In previous versions

Definition at line 728 of file HISTORY.txt.

◆ V6

u5 which has been done in V6

Initial value:

============================================================================
  V6.1.7 (Aqua)                                                     12/15/2009
  ============================================================================
  Changes from v6.1.5 which do not affect scientific output:
  1. Excluded the fill value from the valid range check of LAST_VALID_SCAN in
     the function of Check_If_Sector_Rotated in Preprocess.c.  
 
  ============================================================================
  V6.1.5 (Aqua)                                                     08/28/2009
  ============================================================================
  Changes from v6.1.3 which do not affect scientific output:
  1. A bug from the output of dead and noisy subframe list in Metadata.c 
     is fixed. 
  2. Fixed a minor bug for the log message in a few header files.  
 
  ============================================================================
  V6.1.3 (Aqua)                                                     07/22/2009
  ============================================================================
  Changes from v6.1.1 which do not affect scientific output:
     (same change as V5.0.37)
  1. If the ReprocessingActual from pcf is "Near Real Time"

Definition at line 160 of file HISTORY.txt.

◆ Version

PGE01 indicating that PGE02 Version

Definition at line 396 of file HISTORY.txt.

Typedefs

Functions

Variables

Typedef Documentation

◆ code

Function Documentation

◆ Box()

◆ calibrated()

◆ details()

◆ even()

◆ File()

◆ files()

◆ index()

◆ scans()

◆ table()

Variable Documentation

◆ __pad0__

◆ __pad1__

◆ __pad2__

◆ __pad3__

◆ __pad4__

◆ __pad5__

◆ __pad6__

◆ a

◆ algorithm

◆ ASSOCIATEDSENSORSHORTNAME

◆ August

◆ average

◆ Band

◆ bands

◆ BB_250m

◆ calibration

◆ case

◆ change

◆ Contact

◆ correction

◆ creating

◆ Data

◆ data

◆ delivery

◆ dependency

◆ detector_quality_flag2_values_table

◆ detectors

◆ differences

◆ direction

◆ DNs

◆ documents

◆ file

◆ files

◆ flags

◆ functioning

◆ inaccurate

◆ interpreted

◆ keywords

◆ L1A

◆ late

◆ lists

◆ made

◆ March

◆ MOD01

◆ now

◆ of

◆ once

◆ opening

◆ orbit

◆ output

◆ personnel

◆ PGE02

◆ preprocessing

◆ Previously

◆ production

◆ result

◆ SD_500m

◆ SRCA_250m

◆ SRCA_500m

◆ SV_250m

◆ SV_500m

◆ tables

◆ term

◆ to

◆ pad0

◆ pad1

◆ pad2

◆ pad3

◆ pad4

◆ pad5

◆ pad6