Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events

Details Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cosre..46...35d&link_type=abstract

Cosmic Research, Volume 46, Issue 1, pp.35-39

Physics

96.60.Vg, Particle Emission, Solar Wind

Scientific paper

Energetic solar proton events within the energy interval 1-48 MeV at the stage of their decay are considered over the period of 1974-2001. The dependence of the characteristic decay time on the proton energy in the assumed power-law representation τ( E) = E - n is analyzed for the events with an exponential decay form. The dependence of n on the heliolongitude of the flare (the particles source on the Sun) is studied.

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