Energy spectra and radial intensity gradients of low-energy protons in recurrent increases

Details Energy spectra and radial intensity gradients of low-energy protons in recurrent increases Energy spectra and radial intensity gradients of low-energy protons in recurrent increases

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25...35b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Jan.-Feb. 1985, p. 35-41. In Russian.

Physics

1

Energy Spectra, Interplanetary Space, Proton Energy, Solar Protons, Particle Acceleration, Radial Distribution, Solar Wind

Scientific paper

Proton energy spectra are calculated on the basis of an analytical solution of the transport equation in interplanetary space with allowance for the statistical acceleration of particles. Good agreement is obtained between calculated spectra and proton spectra (E = 1.4-10 MeV) measured in recurrent increases at 1 AU. It is shown that the hypothesis of statistical acceleration in the interplanetary medium can explain cases of a negative gradient of intensity at 1 AU.

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