How to use the Radiation Model Program

The program diskh:[gllseq.software]background_rad_model.pro uses 
spice kernels to estimate the background radition levels during uvs 
observations.  The output file of this program lists the following:

(1) event-- observation command or voltage commmand (hv, f, n ,g)
(2) time-- The time of the event
(3) Rj-- The distance of Galileo from Jupiter
(4) Radiation-- The background radiation in count/sec
(5) Radiation dosage-- The dosage in counts
(6) Object-- The object being observed
(7) Observation Name-- The name of the observation

At the end of the data file, the observation times are totaled in rims and 
hours.  The total radition dosage in counts is given for each tube during the 
given orbit, separating objects from torus observations.

This list file is kept on line in diskk:[orbit_design.*.sef_products], where
the * represents the orbit (i.e. g1).  The file is name radiation_model_*.lis.

To run the program, type check.

The second program, diskh:[gllseq.software]Jupiter_rad_model.pro reads the 
output file from the the above file and adds in the counts from Jupiter 
sun-lit observations.   

To run the program, type check2.

This program will ask for the time that the viewed object was sun-lit and the 
percentage of the field of view the object covers.  This information must be 
found by gggs plots.  This program will also ask if any observations were
not asked about, such as a NIMS ride along.