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
- Neue Suche nach: Daibog, E. I.
- Neue Suche nach: Logachev, Yu. I.
- Neue Suche nach: Kecskemety, K.
- Neue Suche nach: Daibog, E. I.
- Neue Suche nach: Logachev, Yu. I.
- Neue Suche nach: Kecskemety, K.
Abstract 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.
Dokumentinformationen
Energy dependence of the characteristic decay time of proton fluxes in solar cosmic ray events
Cosmic Research ; 46 , 1 ; 35-39
2008-02-01
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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