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Magnetic Field Configuration in Hα Flare Loops and Flaring Arches

Published online by Cambridge University Press:  12 April 2016

Arvind Bhatnagar  and
Nandita Srivastava
Arvind Bhatnagar
Affiliation:
Udaipur Solar Observatory Udaipur -313001India
Nandita Srivastava
Affiliation:
Udaipur Solar Observatory Udaipur -313001India

Abstract

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It is concluded from the observations of Hα flaring loops and flaring arches that these are two entirely different phenomena. From the reconstructed shape of flaring loops, it is suggested that the magnetic field lines revert to potential field configuration from sheared non-potential state.

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 351 - 354
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

1. Loughhead, R.E., Wang, J.L. and Blows, G., 1983, Ap. J., 274, 883 Google Scholar
2. Loughhead, R.E., Chen Chuan, Le and Wang, J.L., 1984, Solar Phys., 92, 53 Google Scholar
3. Kopp, R.A., and Pneuman, G.W., 1976, Solar Phys., 50, 85 Google Scholar
4. Svestka, Z., Stewart, R.T., Hoyng, P., Van Tend, W.,Acton, L.W., Gabriel, A.H. 1982, Solar Phys., 75, 305 Google Scholar