Features of mass supply and flows related with reconnection in the solar corona

Details Features of mass supply and flows related with reconnection in the solar corona Features of mass supply and flows related with reconnection in the solar corona

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70..161s&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 161-166

Physics

Magnetic Fields, Prominences, Mhd Flows

Scientific paper

Symmetrical broadening in the emission spectral lines is the ultimate observational effect of magnetic reconnection in the solar corona. Reconnection can create plasmas of very different temperatures and, hence, very different electrical conductivities in the corona. The electrodynamical effect of such a mass supply is considered. Electromagnetic expulsion force, different from Parker's well-known magnetic buoyancy force, can effectively balance gravity in prominences and generate fast vortex flows in the vicinity of fine threads inside prominences. The possibility of observing this effect from SOHO is discussed.

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