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Emission of Solar Protons (ESP) Model
A NASA software catalog entry available for reuse or request.
About this technology
Overview
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.
Release notes
More information can be found at https://see.msfc.nasa.gov/model-esp