SEE PRODUCTS / SEE Related Model & DB -
Ionizing
Radiation Environment
TRAPPED PROTON MODEL (TPM)
Description:
The model
determines the differential omnidirectional proton flux from
1–100MeV. At high altitudes the model is based on CRRESPRO,
developed by AFRL; at low altitudes, the model is based on
data from the TIROS/NOAA (POES) low-altitude polar-orbiting
satellites. The model contains a true solar cycle variation
and also contains sub-models for quiet and active
magnetospheric states.
The model
also contains an orbit generator which allows the user to
determine an orbit-averaged energy spectrum.
Language: FORTRAN
Operating System: Windows
95/98/1000/NT/XP
Hardware Requirements: m or greater; 32 Mb
Availability:
Input Description:
In order to determine
orbit-averaged energy spectra, the user must input the date
for which the spectra are desired and the orbital elements.
The
TPM-1 documentation report is currently in publication.
Point of Contact:
Stuart L. Huston
Science Applications International Corporation
Seal Beach, CA 90740
Phone: 562-594-7382
Fax: 562-594-7301
E-mail:
stuart.l.huston@saic.com
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