The Flux Tube Tectonics model for coronal heating

Details The Flux Tube Tectonics model for coronal heating The Flux Tube Tectonics model for coronal heating

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jastp..73..271p&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 73, Issue 2-3, p. 271-276.

Physics

Scientific paper

An account is presented of the Flux Tube Tectonics model for heating the
solar corona, in which a multitude of current sheets are continually
forming and dissipating. In addition, a model is summarised for the
time-dependent response of the corona to the sudden dissipation of one
such current sheet.

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