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Resistive Instabilities and Solar Flares

Published online by Cambridge University Press:  25 April 2016

G. G. Lister
G. G. Lister*
Affiliation:
School of Physical Sciences, Flinders University, S.A.
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Extract

The study of plasma instabilities described by the inclusion of a finite conductivity in the hydromagnetic equations has aroused considerable interest since the initial work of Furth, Killeen and Rosenbluth for a two-dimensional geometry. In particular, the so-called ‘tearing’ mode, which has been observed in laboratory plasmas, has been suggested as a possible source of energy for solar flares.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 4 , December 1968 , pp. 152 - 153
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Furth, H. P., Killeen, J. and Rosenbluth, M. N., Phys. Fluids, 6, 459 (1963).Google Scholar
2 Aitken, K. L., Hopkins, K. J., Bickerton, R. J., Hardcastle, R. A. and Reynolds, P., Nucl. Fusion, 5, 330 (1965).Google Scholar
3 Sturrock, P. A., in Plasma Astrophysics, Sturrock, P. A. (ed.), Academic Press, New York 1967, 168.Google Scholar
4 Petschek, H. E., Proc. of the AAS-NASA Symposium on the Physics of Solar Flares, Washington 1964, 161.Google Scholar
5 Coppi, B., Greene, J. M. and Johnson, J. L., Nucl. Fusion, 6, 101 (1966).Google Scholar