Flare loops heating by the 0.1 1.0 MeV proton beams

Details Flare loops heating by the 0.1 1.0 MeV proton beams Flare loops heating by the 0.1 1.0 MeV proton beams

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..168..219v&link_type=abstract

Solar Physics, Volume 168, Issue 1, pp.219-222

Physics

10

Scientific paper

The fast heating of coronal loops at the very beginning of solar flares is discussed as a first observable signature of downstreaming 0.1 1 MeV proton beams. We place emphasis on the produced by proton beams large-scale upward electric field, supporting beam-driven instability of the kinetic Alfvén waves (KAW). The considerable part of a beam kinetic energy may be converted into heat via intermediate KAW with heated region initially spreading from the top downward to footpoints of the loop-like coronal structures with velocity of about a few thousands km/s.

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