Help for TEMIS
PURPOSE:
TEMIS is a program to generate spectral emissivity images from
calibrated radiance data. The input dataset should be the calibrated
(IRAD or GRAD) channels. The first output will contain the spectral
emittance images for each input band, while the second output will
contain the temperature image.
Three algorithms (MODEs) have presently been implemented. The first
method, called REFCHAN, sets a specified reference channel to a specified
constant emittance value. The default sets Channel 6 to 0.95. The temperature
is computed based upon the radiance and given emittance of the reference
channel, then the other five spectral emittances are computed, using this temperature.
The second method, called BBFIT, assumes that the highest spectral
emittance is at a user-specified level (default = 0.95). It then computes the
highest temperature consistent with this assumption, and the six spectral
emittances, based upon the computed temperature.
The third method, ALPHA, uses the alpha residuals method
PARAMETERS:
INP
input calibrated image (RAD)
OUT
(1) Spectral emittance image
(2) Temperature image
SIZE
The standard VICAR2 output
size field.
SL
Starting line
SS
Starting sample
NL
Number of lines
NS
Number of samples
REFCHAN
(For REFCHAN mode only)
The channel to be used as the
reference channel. Valid: (1:30)
E
The emittance assumed for the
reference channel (REFCHAN or
TWOCHAN mode); or the maximum
emittance (BBFIT mode)
MODE
REFCHAN, ALPHA, or BBFIT or BTEM
DATE
Date of data acquisition.
Used to get a TIMS filter.
FILFILE
file containing a filter
function
CWAVE
center wavelengths for
each band of the input file
See Examples:
Cognizant Programmer: