Magnetic Fields in Flares and Active Prominences. I: The Flares in Active Region McMath No. 8818, May 21 and 23, 1967

Details Magnetic Fields in Flares and Active Prominences. I: The Flares in Active Region McMath No. 8818, May 21 and 23, 1967 Magnetic Fields in Flares and Active Prominences. I: The Flares in Active Region McMath No. 8818, May 21 and 23, 1967

Feb 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969soph....6..278m&link_type=abstract

Solar Physics, Volume 6, Issue 2, pp.278-289

Physics

3

Scientific paper

The locations of flares and chromospheric absorption features on May 21 and 23, 1967, are compared with a series of Hα magnetograms. Each of the four major flares included in the study developed as double emission ribbons lying at positions of steep field gradient on opposite sides of the boundary between regions of opposite magnetic polarity. At certain stages, the flare outlines followed closely the isogauss contours of the longitudinal field. A fluctuating field of 75 gauss was measured directly in the importance two flare of May 21. Modifications in the magnetic structure of the active region followed the flares of May 23.

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