Plasma ejection from the solar corona: Mechanism and numerical modeling

Details Plasma ejection from the solar corona: Mechanism and numerical modeling Plasma ejection from the solar corona: Mechanism and numerical modeling

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..608p&link_type=abstract

Astronomy Reports, Volume 43, Issue 9, September 1999, pp.608-614

Astronomy and Astrophysics

Astronomy

4

Scientific paper

A mechanism for the ejection of plasma based on local chromospheric evaporation during a solar flare is presented. Numerical MHD modeling demonstrates the development of a powerful post-flare loop and the subsequent ejection of a plasma jet, leading to the formation of a vertical current sheet. The sheet decays due to reconnection and thermal radiative instability.

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