The first file should contain the 9 TIR channels of MAS image data, calibrated in units of milliWatts per square meter per steradian per micrometer. The second file should be the MAS TIR radiance to temperature lookup table for the spectral response calibration that is in effect for the date of data acquisition.
The output dataset will contain surface kinetic temperature for each of the
9 input channels, assuming the emissivities supplied in the EMIS parameter.
Output pixels are halfword (16 bit signed integer), in units of degrees
Celsius, scaled by a factor of 100.0
For example,
DN = 2531 denotes a temperature of 25.31 degrees Celsius.
The standard VICAR2 output size field. Default will process the entire data set. Example: SIZE = (1,1,200,716)
Starting line (same as SIZE(1)).
Starting sample (same as SIZE(2)).
Number of lines (same as SIZE(3)).
Number of samples (same as SIZE(4)).
These are the spectral emissivity values assumed when computing the amount of reflected downwelling radiance in the input, and when using the Planck function to convert from radiance to temperature. Nine values are required, one for each MAS channel from Channel 42 to 50.