On the formation of relativistic particle fluxes in extended coronal structures

Details On the formation of relativistic particle fluxes in extended coronal structures On the formation of relativistic particle fluxes in extended coronal structures

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..374..140m&link_type=abstract

High energy solar physics. AIP Conference Proceedings, Volume 374, pp. 140-152 (1996).

Physics

3

Particle Emission, Solar Wind

Scientific paper

We analyze neutron monitor data of solar cosmic rays in order to obtain information about their sources. We use three methods for these data analysis. As result, we obtain a set of evidences for two separate solar cosmic rays sources that we call as prompt and delayed components. We attempt here to substantiate a two sources scenario for the generation of both components. For the prompt component source, we suggest regular acceleration in a neutral current sheet. For the delayed one, we propose acceleration by magnetosonic wave turbulence.

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