An analysis of the magnetic inversion lines in solar active region NOAA 6891

Details An analysis of the magnetic inversion lines in solar active region NOAA 6891 An analysis of the magnetic inversion lines in solar active region NOAA 6891

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acasn..38..167l&link_type=abstract

Acta Astronomica Sinica, vol. 38, p. 167

Astronomy and Astrophysics

Astronomy

1

Solar Magnetic Field, Solar Activity, Sunspots, Magnetic Islands, Lines Of Force, Magnetic Field Configurations, Solar Flares, Topology

Scientific paper

The superactive region NOAA 6891 is an 'island' delta-sunspot. There are five magnetic inversion lines in it. Across the 2nd and 3rd inversion lines there are highly sheared field configurations, and at these two places a lot of flares occurred. Especially near the 2nd inversion line, two white-light flares were produced. Magnetic inversion lines have different characteristics. This is due to their different magnetic circumstances. So we should study three-dimensional magnetic fields, and this is a useful way to study the magnetic topology separatrices.

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