A possible explanation of reversed magnetic field features observed in NOAA AR 7321

Details A possible explanation of reversed magnetic field features observed in NOAA AR 7321 A possible explanation of reversed magnetic field features observed in NOAA AR 7321

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..158..249l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 158, no. 2, p. 249-258

Physics

10

Chromosphere, Polarity, Solar Magnetic Field, Solar Physics, Sun, Magnetic Flux, Magnetic Signatures, Photosphere, Solar Flares, Velocity Distribution

Scientific paper

Observations of reversed-polarity features in the chromosphere as well as in the photosphere in the form of magnetic gulfs or islands of opposite polarity have been reported recently. In this paper, we present a possible explanation for the appearance of reserved-polarity features observed in the chromospheric magnetograms of the NOAA AR 7321 observed during 25-27 Oct., 1992. It is suggested that the large-scale reversed-polarity features may occur due to the twisting of the smaller-scale magnetic flux tubes in the layer between the photosphere and the chromosphere.

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