Physics
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115..107h&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 115, no. 1, 1988, p. 107-124. USAF-supported research.
Physics
79
Electric Current, Solar Flares, Solar Magnetic Field, Solar Prominences, Current Density, Current Distribution, Error Analysis, H Alpha Line, Magnetic Field Inversions, Solar Atmosphere
Scientific paper
The author has analyzed the vector magnetic field of an active region at a location of repeated flaring to determine the nature of the currents flowing in the areas where the flares initiated. The component of electric current density crossing the photosphere along the line-of-sight was derived. The calculated distribution of current density at the flare sites suggested that currents were flowing out of an area of positive magnetic polarity and across the magnetic inversion line into two areas of negative polarity. In the vicinity of the flare sites, the calculated source field was very similar to the field produced by two arcades of currents crossing the inversion line at the locations of greatest magnetic shear with orientations of about 60° to the inversion line. The author estimated the currents in the two arcades by matching the source field derived from observations with that produced by a model of parallel loops of currents. Finally, the author found that the source field at the flare sites was produced almost entirely by the angular difference between the observed and potential field and not by the difference in field intensity.
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