Physics
Scientific paper
Dec 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...89..391g&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 89, Dec. 1983, p. 391-402.
Physics
6
Electron Sources, Noise Storms, Solar Electrons, Solar Radio Bursts, Type 3 Bursts, Astronomical Models, Particle Acceleration, Solar Corona, Solar Magnetic Field, Solar Wind, Space Plasmas, Tearing Modes (Plasmas)
Scientific paper
The source model of the electrons (1-10 keV) responsible for the observed impulsive low energy electron flux events in the solar wind plasma and for type I and III noise storms is considered. The appearance of such a source is associated with the tearing mode instability of a neutral current sheet located above the bipolar region of the solar disk and immersed to a flux of solar wind plasma. Such an instability develops most favorably in the low corona layers at the heights h of about (0.5-1) solar radii, where the solar wind flux is rather small. In the upper corona layers the current sheet is stabilized by a strong flux of solar wind plasma. Disruptions of the current sheet produce accelerated particles with energy and flux enough for the generation of type I radio bursts at the base of the bipolar structure and of type III bursts in the solar wind plasma.
Gubchenko V. M.
Zaitsev Valerii V.
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