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• W2094319726 abstract "The power spectrum of the interplanetary magnetic field were tested, as well as the power spectrum-cosmic diffusion ray coefficient relation at low energies. A first order perturbation solution of the Fokker-Planck equation governing the diffusion, convection, and adiabatic deceleration of galactic cosmic rays in the solar medium was found to relate intensity fluctuations of low energy cosmic rays to local changes in the propagation parameters. Diffusion coefficients and their day to day variations were calculated from interplanetary magnetic field data obtained by Pioneer 6 in 1965/1966. These are compared to simultaneous observations by IMP 3 of the proton flux in three energy channels (20 to 40, 40 to 60, 60 to 80 MeV)." @default.
• W2094319726 created "2016-06-24" @default.
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• W2094319726 date "1975-02-01" @default.
• W2094319726 modified "2023-09-26" @default.
• W2094319726 title "Modulation of low-energy cosmic rays" @default.
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• W2094319726 doi "https://doi.org/10.1029/ja080i004p00457" @default.
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