Magnetic fine structures in coronal loops

Details Magnetic fine structures in coronal loops Magnetic fine structures in coronal loops

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70...31v&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 31-35

Physics

1

Sun, Corona

Scientific paper

The formation of magnetic fine structures and associated electric currents is considered in the context of the coronal heating problem. The penetration of field-aligned electric currents into the lower atmosphere is discussed. It is argued that currents strong enough to heat the corona can persist only for short periods of time. The formation of thin current sheets is discussed. It is argued that photospheric magnetic structures (flux tubes) play an important role in the generation of coronal currents.

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