A model for enhancement of the flux of very high energy particles during large solar flares.

Details A model for enhancement of the flux of very high energy particles during large solar flares. A model for enhancement of the flux of very high energy particles during large solar flares.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hepnp..20.1068h&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 20, No. 12, p. 1068 - 1072

Physics

Cosmic Rays: Solar Flares, Cosmic Rays: Solar Modulation

Scientific paper

In recent years, some short time enhancements of cosmic ray particles during large solar flares (GLE) were recorded by a neutron monitor at sea level and an underground muon detector at different depths. The energy regions concerned were several hundred GeV, even a few TeV. The authors discuss how the flux enhancement in the TeV region may be due to the re-acceleration of the galactic cosmic rays in the period of large solar flares. Because of the very steep energy spectrum of cosmic rays, if only 10% of cosmic ray particles are re-accelerated with an energy increment of several hundred GeV, the cosmic ray flux in the TeV region could increase considerably.

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