Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1022k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Sept.-Oct. 1990, p. 1022-1025. In Russian.
Astronomy and Astrophysics
Astronomy
2
Gamma Ray Spectra, Photosphere, Solar Flares, Solar Neutrons, Gamma Ray Astronomy, Solar Atmosphere, Solar Flux Density, Thermal Neutrons
Scientific paper
The paper presents an analysis of the temporal behavior of 2.2-MeV gamma rays from solar flares and the matter density in the capture region of thermal neutrons generated during the flare. It is shown that the matter density in the subphotospheric region during a flare might experience disturbances. It is concluded that solar flares appear not only in the corona and chromosphere but also in deep subphotospheric layers of the solar atmosphere.
Kogan-Laskina E. I.
Kuzhevskij Boris M.
No associations
LandOfFree
Solar gamma-radiation in connection with the absorption of neutrons and the evolution of the matter density in the subphotospheric region after a flare does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Solar gamma-radiation in connection with the absorption of neutrons and the evolution of the matter density in the subphotospheric region after a flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar gamma-radiation in connection with the absorption of neutrons and the evolution of the matter density in the subphotospheric region after a flare will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1302857