Modulation of the spectrum of galactic cosmic rays by solar wind

Details Modulation of the spectrum of galactic cosmic rays by solar wind Modulation of the spectrum of galactic cosmic rays by solar wind

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..176n&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, Jan.-Feb. 1981, p. 176-178. In Russian.

Computer Science

Cosmic Rays, Galactic Radiation, Radiation Spectra, Solar Wind, Diffusion Coefficient, Magnetic Rigidity, Photons

Scientific paper

A solution is presented for a diffusion equation which describes the distribution of galactic cosmic rays in spherically symmetric solar wind. Theoretical spectra of cosmic rays have been compared with experimental data on photon spectra in the energy range 10-100,000 MeV for various relationships between the diffusion coefficient and particle impulse. A relationship between the diffusion coefficient and the particle impulse is found which corresponds to the best agreement between theory and experimental data.

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