Magnetic helicity in the solar corona

Details Magnetic helicity in the solar corona Magnetic helicity in the solar corona

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006asthe..99....7k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 99, No. 1, p. 7 - 17 (2006)

Astronomy and Astrophysics

Astronomy

Solar Corona, Magnetic Fields

Scientific paper

Magnetic helicity, which is a measure of the magnetic flux linking, is an important quantity for the magnetohydrodynamics. Recently, the new methodologies were developed to enable the measurement of magnetic helicity injection through the solar surface into the solar corona. This new measurement confirmed that magnetic helicity as well as the complexity in coronal magnetic structure plays a crucial role for the energy liberation activity in the solar corona. Based on the results, a new model of the solar flare onset mechanism so-called "reversed-shear flare model" has been proposed.

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