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Transport of solar flare protons: Comparison of a new analytic model with spacecraft measurements (1971)

Stone, E. C. ; Lupton, J. E.

In: CASI

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Publication Date: 2019-06-27

Description: An analytic solution was obtained to the complete Fokker-Planck equation including the effects of convection, interplanetary deceleration and acceleration, corotation, and anisotropic diffusion. The solution yields a time to maximum for the particle flux of about 10 h and an exponential decay time of about 5 h. Several solar flare particle events were observed with the solar and galactic cosmic ray experiment on OGO-6. Comparisons of the calculated time dependence of the fluxes with these observations of 1 to 70 MeV protons show that the model adequately describes both the rise and decay times.

Keywords: SPACE RADIATION

Type: NASA-CR-128295 , SRL-71-3

Format: application/pdf

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