Physics
Scientist
Moskovskii Gosudarstvennyi Universitet, Moscow, USSR
Application of the solar plasma density investigation method based on the solar flare 2.223 MeV gamma-line time profile analysis to the experimental data
Contribution of 20.58 MeV gamma-line in E>20 MeV solar flare gamma emission, and He-3 concentration in the deep layers of the solar atmosphere.
Diffusional component of nonrelativistic solar electrons
Gamma-Ray Radiation with Energy 2.223 MeV and the Density Distribution in the Solar Atmosphere during Flares
Possible causes of the formation of two maxima in the time variation of the intensity of 2.22-MeV gamma radiation in solar flares
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