Help for MIVISTIR
PURPOSE:
MIVISTIR is a program that accepts as input MIVIS TIR brightness temperature
at sensor image data and outputs upwelling radiance at surface for the thermal
infrared channels. Also required as input are a valid MODTRAN input file, to
define the atmospheric model, the MIVIS TIR spectral response file, and the
MIVIS radiance lookup table.
OPERATION:
MIVITIR takes as input the 10 Channels of MIVIS TIR brightness temperature
at sensor data in units of degrees Celsius, multiplied by 10, a file
containing the the MIVIS TIR spectral response functions, and the MIVIS
temperature to radiance lookup table. The second file must be a VICAR labelled
file consisting of ten lines (one for each TIR channel) and 900 samples (one
for the spectral response at each wavenumber from 601 to 1500). The spectral
response functions must be normalized, i.e., the sum of all values on each line
must be 1.0. The third file must be a temperature to radiance lookup table
in the format common to MIVIS, MASTER, MAS, and TIMS.
The atmospheric model used is defined by a user supplied MODTRAN input
file. MIVISTIR uses these parameters to run MODTRAN twice; once with a
nadir looking geometry, and once for the case of viewing at maximum deflection
from nadir. From these two runs, the atmospheric transmittance, path
radiance, and downwelling sky radiance at surface are calculated for the ten
MIVIS TIR bandpasses. The downwelling sky radiance values are placed in
the VICAR label of the output dataset.
Values of transmittance and path radiance are calculated for each pixel
location in the scene by interpolation, where it is assumed that each
quantity varies linearly with path length.
The upwelling radiance at surface is then computed by the following
formula:
Rad(at sensor) = Rad(upwelling)*transmittance + Rad(path)
It should be noted that the output quantity (upwelling radiance) of MIVISTIR
differs from the output quantity of TIMSCAL2 (surface emitted radiance). It
it includes both the surface emitted component plus the surface reflected
component.
The output dataset consists of 10 channels of halfword (16 bit signed
integer) pixels, in units of milliWatts per square meter per steradian per
micrometer. Note that these units are 1000 times smaller than the input
units.
WRITTEN BY: Ron Alley November 68
COGNIZANT PROGRAMMER: Ron Alley
REVISION: New
PARAMETERS:
INP
(1) MIVIS TIR brightness
temperature image (10*deg C)
(2) MIVIS TIR calibration file
(3) MIVIS radiance lookup table
OUT
Output data set of the 10 MIVIS
TIR bands, for upwelling
radiance at surface.
SIZE
The standard VICAR output size
field.
SL
Starting line
SS
Starting sample
NL
Number of lines
NS
Number of samples
MODINP
Dataset name for the MODTRAN
input file, containing the
atmospheric data relevant to
this image.
MODOUT
Dataset name for MODTRAN
output report file.
MODTAB
Dataset name for MODTRAN
output tabular file.
See Examples:
Cognizant Programmer: