ocssw
V2022
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L1B_Setup.h
Definition: Granule.h:1095
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: HISTORY.txt:695
Definition: Granule.h:773
Definition: Granule.h:745
Definition: Granule.h:956
PGSt_SMF_status Write_L1B_ScanMeta(L1B_Scan_Metadata_t *L1B_Scan_Meta, L1A_granule_t *L1A_Gran, QA_Data_t *QA, boolean skip_night_hi_res)
Definition: L1B_Setup.c:4810
Definition: L1B_Setup.h:59
Definition: Granule.h:856
Definition: L1B_Tables.h:952
PGSt_SMF_status Determine_Other_Missing_Scans(lookup_tables_t *tables, L1A_granule_t *L1A_Gran)
Definition: L1B_Setup.c:5242
PGSt_SMF_status L1B_Setup(lookup_tables_t *lookup_tables, L1A_granule_t *L1A_Gran, L1B_granule_t *L1B_Gran, L1A_Scan_t *L1A_Scan, L1B_Scan_t *L1B_Scan, QA_Data_t *QA, L1B_Scan_Metadata_t *L1B_Scan_Meta, boolean skip_night_hi_res)
Definition: L1B_Setup.c:218