Observational constraint on the build-up and relaxation of magnetic fields in the solar atmosphere.

Details Observational constraint on the build-up and relaxation of magnetic fields in the solar atmosphere. Observational constraint on the build-up and relaxation of magnetic fields in the solar atmosphere.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996chjph..34....1c&link_type=abstract

Chin. J. Phys., Vol. 34, No. 1, p. 1 - 8

Physics

1

Solar Atmosphere: Magnetic Fields

Scientific paper

High-resolution data of the solar vector magnetogram can be used to examine the ways by which magnetic fields in the solar atmosphere are built up and relax. In a relaxed state, the α parameter should have approached a constant value over an extended region, therefore yielding a sharply peaked distribution of |α|. The authors present, for the first time, the discovery of power-law distributions for the |α| parameter. This finding suggests the existence of nontrivial build-up and relaxation mechanisms for the magnetic energy in the solar atmosphere.

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