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-31315-1Patent Status:
U.S. Release OnlyLab Representatives
