A model for the differential energy spectra of galactic cosmic radiation as a function of solar activity is described. It is based on the standard diffusion-convection theory of solar modulation. Estimates of the modulation potential based on fitting this theory to observed spectral measurements from 1954 to 1989 are correlated to the Climax neutron counting rates and to the sunspot numbers at earlier times taking into account the polarity of the interplanetary magnetic field at the time of observations. These regression lines then provide a method for predicting the modulation at later times. The results of this model are quantitatively compared to a similar Moscow State University (MSU) model. These model cosmic ray spectra are used to predict the linear energy transfer spectra, differential energy spectra of light (charge less than or = 2) ions, and single event upsets rates in memeory devices. These calculations are compared to observations made aboard the Space Shuttle.
Galactic cosmic radiation model and its applications
Advances in Space Research ; 17 , 2
1996-01-01
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Englisch
Galactic Cosmic Radiation Model and its Applications
British Library Conference Proceedings | 1995
|Galactic Cosmic Radiation Model and its Applications
Online Contents | 1995
|Galactic Cosmic Radiation Model and its Applications
Online Contents | 1996
|Shuttle Measurements of Galactic Cosmic Radiation LET Spectra
Online Contents | 1996
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