Dependence of length of free path of flare particles on energy

Details Dependence of length of free path of flare particles on energy Dependence of length of free path of flare particles on energy

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr...5...46d&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-85-005) p 46-47 (SEE N86-14111 04-88) Transl. into ENGLISH from Kosmich. Issled. (Moscow),

Physics

Energy Spectra, Interplanetary Magnetic Fields, Particle Flux Density, Solar Cosmic Rays, Solar Flares, Solar Protons, Alpha Particles, Magnetic Variations, Power Spectra, Prognoz Satellites, Proton Flux Density, Temporal Distribution

Scientific paper

An analysis is made of the time profiles of fluxes of protons and alpha particles in the 0.1 to 100 MeV/nucleaon range, detected by Prognoz-6 in the solar-flare events of September 24, October 9 and 12, November 22, December 27, 1977. It is shown that a harmonic expansion of the measured field cannot be used to calculate the transport characteristics of solar cosmic rays (SCR). This is evidently due to the fact that the usual procedure for determining the power spectrum of IMF fluctuations does not make it possible to identify the type of inhomogeneity (wave, oscillation, or discontinuity) on which SCR-scattering occurs.

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