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ocssw
V2022
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table_io_wrapper.h
double * table_read_r8(char *input_filename, int m, int n)
Definition: table_io.cpp:2536
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
