The laws of the evolution and destruction of solar prominences

Details The laws of the evolution and destruction of solar prominences The laws of the evolution and destruction of solar prominences

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65.1319a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Nov.-Dec. 1988, p. 1319-1321. In Russian.

Astronomy and Astrophysics

Astronomy

Evolution (Development), Magnetic Flux, Solar Prominences, Radio Emission, Solar Activity

Scientific paper

Possible scenarios for the evolution of solar prominences are proposed on the basis of observational data. These are autonomous loop evolution, evolution with mass exchange, and evolution with magnetic flux emergence. The latter is a preflare type of evolution which begins 4-5 hrs before the flare with prominence activation in the radio range over the active region. The flares initiate the restructuring of the prominences as well as their partial or total destruction.

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