Emission of Solar Protons (ESP) Model

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.
Internal Laboratory Ref #: 
MFS-31315-1
Patent Status: 
U.S. Release Only
Agency
NASA
Region
Southeast
State: 
Alabama
Phone: 
256-544-9151
Email: 
terry.taylor@nasa.gov
Lab Representatives
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