Numerical modeling of the arch eruptive prominence on Dec. 20, 1982.

Details Numerical modeling of the arch eruptive prominence on Dec. 20, 1982. Numerical modeling of the arch eruptive prominence on Dec. 20, 1982.

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acasn..27...47h&link_type=abstract

Acta Astron. Sin., Vol. 27, No. 1, p. 47 - 52

Astronomy and Astrophysics

Astronomy

Solar Prominences:Models

Scientific paper

The present paper presents a numerical modeling of the eruptive prominence on Dec. 20, 1982, based on one-dimensional hydrodynamical equations. The effect of various factors, such as front deceleration, thermal conduction, radiation loss and heating, on the formation of the eruptive prominence is preliminarily discussed. The result shows that arch eruptive prominences have completely different dynamic characters from coronal arches.

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