Overview
SPENVIS can run
trapped particle radiation models for Jupiter
over a spacecraft trajectory. This feature is available for
advanced users
only.
In order to run these models, a spacecraft trajectory is needed. If no
trajectory has been generated yet, the
orbit generator
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.
The button calls up the
model selection page for consecutive runs of
multiple models.
Warning: using these buttons deletes all existing output from the
trapped radiation models and from any model that uses this output, in order to
ensure consistency in the outputs.
Input parameters
Model selection
Select a trapped proton and a trapped electron
model
by means of the respective selection menus.
Results
The radiation models produce the files listed in the table below.
A description of the file formats can be brought up by clicking on their
description in the table.
The report file spenvis_trp.html contains the
input parameters and summary tables. 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.
Note that when flux values are
extrapolated,
data are included in spenvis_tri.txt,
spenvis_spp.txt and spenvis_spe.txt files for later use.
However, these values are listed in grey in the report file spenvis_trp.html.
To generate plots, select the plot
type(s), options and
graphics format,
and click the or
button.
The current page will be updated with the newly generated plot files.
The button calls up the
output page for consecutive
runs of multiple models. This button only appears when the trapped radiation
models have been included in the
combined model run selection.