Investigation of the generation conditions of high-energy particles in solar flares

Details Investigation of the generation conditions of high-energy particles in solar flares Investigation of the generation conditions of high-energy particles in solar flares

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mvsfa..27...16l&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika Astronomiia (ISSN 0579-9392), vol. 27, Jan.-Feb. 1986, p. 16-22. In Russian.

Astronomy and Astrophysics

Astronomy

Energetic Particles, Solar Electrons, Solar Flares, Solar Protons, Satellite Observation, Solar X-Rays, Thermal Emission

Scientific paper

The generation conditions of high-energy electrons (E greater than 0.025 MeV) and protons and heavier nuclei (E greater than 0.30 MeV/nucleon) in solar flares are examined on the basis of Prognoz and Venera data. A good correlation is obtained between flux amplitudes of flare electrons and thermal X-ray emission. Two types of events were found to exist in solar cosmic rays: those accompanying and those not accompanying bursts of hard X-ray emission. A model explaining this phenomenon is discussed.

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