We found a match
Your institution may have access to this item. Find your institution then sign in to continue.
- Title
Simulation of heavy ion spectra for the solar event of October 5, 2002.
- Authors
Lytova, M.; Ostryakov, V.
- Abstract
The results of numerical simulation of stochastic acceleration of the heavy ions (He, He, O, and Fe) are presented for the impulsive solar event of October 5, 2002. The energy spectra of the aforementioned particles have peculiarities (depressions) in the low-energy region (≤1 MeV nucleon). Coulomb losses in the flare plasma and adiabatic losses during interplanetary propagation are considered in the study as possible causes of such peculiarities.
- Subjects
IONS spectra; HEAVY ions; SOLAR spectra; SIMULATION methods &; models; SOLAR wind; NUMERICAL analysis; STOCHASTIC analysis
- Publication
Solar System Research, 2011, Vol 45, Issue 6, p557
- ISSN
0038-0946
- Publication type
Article
- DOI
10.1134/S003809461105008X