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A Large Filament and Flares in Active Region NOAA 5669 on September 2, 1989

Published online by Cambridge University Press:  12 April 2016

G.A. Porfir’eva ,
G.V. Yakunina  and
Z. Mouradian
G.A. Porfir’eva
Affiliation:
Sternberg Astronomical Institute, 119899 Moscow B-234, Russia
G.V. Yakunina
Affiliation:
Sternberg Astronomical Institute, 119899 Moscow B-234, Russia
Z. Mouradian
Affiliation:
Observatoire de Paris-Meudon, URA 326, France

Abstract

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The behaviour of extended filaments in the vicinity of a new emerging magnetic flux site has been investigated during the 2N/M5.8 flare on September 1 and several flares on September 2, 1989.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 74 - 77
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Mouradian, Z. and Soru-Escout, I. 1991, in Dynamics of Solar Flares, Schmieder, B. and Priest, E. (eds.), Observ. de Paris, DASOP, p. 139 Google Scholar
Porfir’eva, G.A. and Yakunina, G.V. 1995, Izvestia Academia Nauk., 59, 181 Google Scholar
Zhang, H., Ai, G., Li, W. and Chen, J. 1992, Sol. Phys., 146, 61 CrossRefGoogle Scholar