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Solar heavy ion Heinrich fluence spectrum at low earth orbit
Authors:DR Croley  GC Spitale
Institution:

*SYSCON Corporation, 2550, Honolulu Avenue, #201, Montrose, California 91020, U.S.A.

**Jet Propulsion Laboratory, 4800 Oak Grove Drive, 301-456, Pasadena, California 91109, U.S.A.

Abstract:Solar heavy ions from the JPL Solar Heavy Ion Model have been transported into low earth orbit using the Schulz cutoff criterion for L-shell access by ions of a specific charge to mass ratio. The NASA Brouwer orbit generator was used to get L values along the orbit at 60 second time intervals. Heavy ion fluences of ions 2≤Z≤92 have been determined for the LET range 1 to 130 MeV-cm2/mg by 60, 120 or 250 mils of aluminum over a period of 24 hours in a 425 km circular orbit inclined 51°. The ion fluence is time dependent in the sense that the position of the spacecraft in the orbit at the flare onset time fixes the relationship between particle flux and spacecraft passage through high L-values where particles have access to the spacecraft.
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