Note on an apparent highly-sheared magnetic field structure

Details Note on an apparent highly-sheared magnetic field structure Note on an apparent highly-sheared magnetic field structure

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..131l&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 131-132 (SEE N89-24974 1

Computer Science

Magnetic Field Configurations, Magnetic Signatures, Solar Magnetic Field, Magnetic Measurement, Solar Activity

Scientific paper

Using vector magnetograms and a force-free model, the magnetic field structure of the active solar region BBR 18474 of 1982 July 15, and 1982 July 16 was investigated. Comparison of the azimuths of the current-free model of the magnetic field structure in the central part of this active region with the map of the azimuth values estimates from the observation slows good qualitative agreement. Earlier results show that the appearance of highly sheared magnetic field structure near the neutral line in the central part of this active region may be a simulated effect generated by subphotospheric current system.

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