Physics
Scientific paper
Jul 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...53..157k&link_type=abstract
Solar Physics, vol. 53, July 1977, p. 157-178.
Physics
7
Coherent Radiation, Electron Flux Density, Solar Electrons, Electron Energy, Satellite Observation, Solar Flares, Solar Protons, Solar Wind
Scientific paper
An experimental study of the propagation of solar electrons with energy greater than 30 keV was carried out. Measurements were made during the period 1972-1974 using the 'Prognoz' satellite-borne instruments. A two-component structure of electron fluxes was found. The fast component, rather well-observed after solar flares of minor importance, consists of a compact beam of electrons propagating without scattering inside a narrow cone with an opening less than or equal to 10 deg along interplanetary magnetic field lines. Peculiarities of the slow or diffusive component of electron fluxes are compared with the diffusive component of solar protons. It is shown that the diffusion coefficient for nonrelativistic electrons is the function of the number of particles injected in the event. A model of coherent propagation of nonrelativistic electrons is offered, which takes into account the presence of the fast and slow components and their interaction with solar wind plasma oscillations.
Kurt Victoria G.
Logachev Iu. I.
Pissarenko N. F.
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