On the outburst of flare activity of 26 November, 1973 |
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| Authors: | Robert Howard Zdeněk Švestka |
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| Institution: | (1) Mount Wilson and Las Campanas Observatories, Carnegie Institution of Washington, 91101 Pasadena, Calif., U.S.A.;(2) Space Research Laboratory of the Astronomical Institute, Utrecht, The Netherlands;(3) Center for Astrophysics and Space Science, C-011, University of California at San Diego, 92093 La Jolla, Calif., U.S.A. |
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| Abstract: | We draw attention of flare build-up observers to a strong 30 hour-long outburst of homologous flare activity and unusual growth and brightening of coronal loops, seen on Skylab. We suggest that these events might have been closely associated with newly emerging magnetic flux, in spite of the fact that the flux effects in H and EUV were first seen only late after the activity had started, and the flux emerged at the opposite end of the coronal loops from where the flares occurred. |
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