Other
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold...8...81c&link_type=abstract
Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/8, p. 81 - 85
Other
Solar Gamma-Ray Bursts: Solar Protons, Solar Gamma-Ray Bursts: Solar Microwave Bursts
Scientific paper
The paper critisizes the assertion that the γ-ray line emission unlike other types of the flare emission (hard X-rays, microwave bursts) reveals a highly poor relation or even an anticorrelation with proton fluxes in the interplanetary space. About 30 flares (1972 - 1985) have been analyzed with known values of the γ-ray line emission in the 4 - 7 NeV band (F4-7) and the intensity of >10 MeV proton fluxes (J10). It is shown that (1) a considerable positive correlation between F4-7 and J10 takes place for large nonimpulsive flares with a significant metric component; (2) the γ-ray emission F4-7 correlates well with the maximum flux density of microwave bursts at 15 GHz. It is concluded that the γ-ray line emission in relation to interplanetary protons behaves as well as other types of flare emission.
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