Emission of Solar Protons (ESP) Model(MFS-31315-1)

environmental science earth air space exoplanet
Emission of Solar Protons (ESP) Model
The Emission of Solar Protons (ESP) Model is a computer model of the solar proton environment. The model predicts total solar proton fluence levels for interplanetary space in the energy range of 1 to 300 MeV, which is the range required for both solar cell and electronics applications.
Notes: More information can be found at https://see.msfc.nasa.gov/model-esp

Software Details

Environmental Science (Earth, Air, Space, Exoplanet)
Reference Number
Release Type
U.S. Release Only
Operating System
Windows 95/NT
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Marshall Space Flight Center
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