Electrostatically unstable heat flow during solar flares and its consequences

Details Electrostatically unstable heat flow during solar flares and its consequences Electrostatically unstable heat flow during solar flares and its consequences

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...54..379s&link_type=abstract

Solar Physics, vol. 54, Oct. 1977, p. 379-385.

Physics

23

Conductive Heat Transfer, Electric Current, Solar Flares, Electrostatics, Ion Acoustic Waves, Magnetohydrodynamic Stability

Scientific paper

This paper examines some of the consequences of an electrostatically unstable return current associated with heat conduction during a solar flare. It is noted that an electrostatically unstable return current will lead to strong hydrodynamic effects and more rapid magnetic-field thermalization if reconnection is the source of primary energy release during a solar flare.

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