Physics
Scientific paper
Aug 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....1..408p&link_type=abstract
In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 1. (A76-26851
Physics
1
Cosmic Rays, Electron Energy, Energy Spectra, Interplanetary Medium, Negatrons, Positrons, Antiparticles, Diffusion Coefficient, Fokker-Planck Equation, Particle Production, Propagation Modes, Solar Wind
Scientific paper
Recently measured positron and negatron spectra are discussed with regard to the problem of solar modulation. At energies above 180 MeV, the spherically symmetric Fokker-Planck equation with a diffusion coefficient proportional to particle rigidity provides reasonable fits to both the positron and total electron data. At energies below 180 MeV, the data are consistent with a continuation of the same diffusion coefficient and a local source of negatrons or with a change in the diffusion coefficient to a constant value.
Hartman Robert C.
Pellerin Charles J.
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