Coronal heating by reconnection

Details Coronal heating by reconnection Coronal heating by reconnection

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1853p&link_type=abstract

Advances in Space Research, vol. 19, p. 1853

Astronomy and Astrophysics

Astronomy

Solar Corona, Magnetic Field Reconnection, Solar Heating, Solar Flares, Plasma Jets, Solar X-Rays, Magnetic Flux, Astronomical Models

Scientific paper

Magnetic reconnection is presently noted to be an important mechanism in the heating or microflaring of the solar corona, especially in the creation of such small-scale phenomena as X-ray bright points and X-ray jets. The 'converging flux model' for X-ray bright points gives plausible explanations for key observations relating to bright points, especially with respect to the complex structures that arise in them.

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