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Hα Impulsive Phase Flare Observations with-High Temporal Resolution

Published online by Cambridge University Press:  27 September 2017

J-P. Wülser ,
H. Marti ,
E. Schanda  and
A. Magun
J-P. Wülser
Affiliation:
University of Bern, Switzerland
H. Marti
Affiliation:
University of Bern, Switzerland
E. Schanda
Affiliation:
University of Bern, Switzerland
A. Magun
Affiliation:
University of Bern, Switzerland

Extract

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Hα observations with high temporal resolution allow a detailed analysis of the chromospheric response to thre primary energy release. The timing; relationship between Hα and hard X-rays gives information about the energy transport mechanism. Sites of massive injection of nonthermal electrons are identified by characteristic features in the the line profile (Canfield et al. 1984;. Canfield and Gayley 1987).

Type
Session II: Solar Flares
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 211 - 214
Copyright
Copyright © Kluwer 1989

References

Canfield, R.C., Gunkler, T. A., and Ricchiazzi, P. J. 1984, Ap. J., 282, 290.Google Scholar
Canfield, R.C., and Gayley, K. G. 1987, Ap. J., 322, 999.Google Scholar
Fisher, G.H., Canfield, R.C., and McClymont, A. N. 1985, Ap. J., 289, 434.Google Scholar
Wülser, J. P., and Marti, H. 1988, Ap. J., in press.Google Scholar