Very high-energy particle emission from the solar cosmic ray flares.

Details Very high-energy particle emission from the solar cosmic ray flares. Very high-energy particle emission from the solar cosmic ray flares.

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hepnp..14..862h&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 14, No. 9, p. 862 - 864

Physics

Solar Cosmic Rays: Solar Flares

Scientific paper

The authors have analyzed and studied the time variation of the daily counting rates of the very high-energy events observed by a large cloud-chamber system during August 1972 at a mountain altitude of 3200 meters above sea-level. An obvious increase of the counting rates which occurred during the 4th and 7th, August, 1972 solar cosmic ray flares is found. These daily counting rates are higher than 3σ of the daily counting rate averaged from 10th to 26th, August. The average energy of the events corresponds to a primary cosmic-ray energy of 1013eV.

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