Spectral characteristics of solar protons during the initial anisotropic stage of their propagation

Details Spectral characteristics of solar protons during the initial anisotropic stage of their propagation Spectral characteristics of solar protons during the initial anisotropic stage of their propagation

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..583p&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, July-Aug. 1980, p. 583-587. In Russian.

Physics

Polar Caps, Proton Flux Density, Solar Cosmic Rays, Solar Protons, Angular Distribution, Anisotropy, Polar Regions, Proton Energy, Spatial Distribution, Spectral Energy Distribution

Scientific paper

An investigation was made of spatial distributions of spectral indices of solar cosmic rays with energies in the 5-40 MeV range in the polar cap during the anisotropic stage of angular distribution of protons in a series of events. A north-south asymmetry of spectral indices of proton fluxes was found in the deep polar cap region, contrasting with proton spectra detected in regions of polar peaks, cusps, and valleys.

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