The number of segments is currently limited to 1 for the two last possibilities.
In order to run these models, a spacecraft trajectory is needed. If no
trajectory has been generated yet, the
should be run first.
The input parameters and options for the trapped particle radiation models are
described below. When the input form has been completed, pressing the
button will start the calculation and
bring up the "Results" page.
Note:The IGE-2006 model could only be selected for geostationary orbits.
The report file spenvis_trp.html contains the
input parameters and summary tables. The report files spenvis_ppeakfl.html and
spenvis_epeakfl.html contain data related to the proton and electron peak fluxes
respectively. The orbit averaged spectra for trapped
protons and electrons are stored in the spenvis_tri.txt file.
The spectrum files spenvis_spp.txt and
spenvis_spe.txt contain, for each orbital point, the full
spectra of trapped protons and electrons, respectively.
To generate plots, select the plot
type(s), options and
and click the or
The current page will be updated with the newly generated plot files.