Physics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984kosis..22..906b&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 22, Nov.-Dec. 1984, p. 906-921. In Russian.
Physics
5
Energetic Particles, Satellite Observation, Solar Flares, Solar X-Rays, Electron Density (Concentration), Solar Cosmic Rays, Time Response, Type 3 Bursts, Venera Satellites
Scientific paper
Venera-13, 14 data obtained from November 1981 to April 1982 are used to examine the correlation between bursts of hard solar X-rays (energy exceeding 0.055 MeV) and solar-cosmic-ray (SCR) flares. Data on solar flares in H-alpha, thermal X-rays, and type III radio bursts were used in the analysis. It is shown that the amplitude of flare-electron intensity (energies exceeding 0.025 and 0.07 MeV) and flare-proton intensity (energy exceeding 1.0 MeV) is best correlated with flare importance in the thermal X-ray range (r = 0.8 + or - 0.03). The use of this importance makes it possible to construct solar-longitude dependences of flare electrons and to assess the solar-longitudinal interval of flares in which coronal-propagation effects can be neglected. A practically linear correlation is found between SCR electrons with energies of tens of keV and thermal X-rays.
Beliakov S. A.
Daibog E. I.
Diachkov A. P.
Iurovitskaia E. V.
Kurt Victoria G.
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