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The Energetic Particle Radiation Environment Module (EPREM) takes input
produced by the Input Parser and SPICE. The EPREM transport code currently
generates two types of primary output: a restart file in the NetCDF format,
which contains the entire computational grid together with various parameters
important for the run, and is used to restart the runs; and observer files,
which are time series of distribution function spectra for various positions in
the code, in ASCII internal EMMREM format.
EPREM solves for the propagation and acceleration of energetic particles in
the evolving magnetic fields of the inner heliosphere with input based on
observations from satellites.