Computer Science
Scientific paper
Nov 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..906b&link_type=abstract
Kosmicheskie Issledovaniia, vol. 17, Nov.-Dec. 1979, p. 906-912. In Russian.
Computer Science
2
Distribution Functions, Electron Distribution, Electron Energy, Electron Flux Density, Solar Flares, Energy Spectra, Microwaves, Particle Acceleration, Proton Energy, Relativistic Particles, Solar Protons, X Rays
Scientific paper
The distribution of flare-induced electron events with respect to peak intensity is studied and is compared with the distribution functions of X-ray and microwave bursts. It is shown that the intensity distribution of electron events (for nonrelativistic electrons) is a power law distribution, whose exponent is close to that of the distribution functions for X-ray and microwave bursts. The distribution of flares with respect to the number of accelerated relativistic electrons is similar to the distribution of flares with respect to accelerated (below 10 MeV) protons, and that it differs markedly from the distribution of events with respect to the number of accelerated nonrelativistic electrons.
Belovskii M. N.
Kurt Victoria G.
Ochelkov Iu. P.
No associations
LandOfFree
Characteristics of the distribution of electron events associated with solar flares, with respect to intensity 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 Characteristics of the distribution of electron events associated with solar flares, with respect to intensity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of the distribution of electron events associated with solar flares, with respect to intensity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-975367