Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-13T10:52:43.902Z Has data issue: false hasContentIssue false
  • English
  • Français

Eruptions of Magnetohydrostatic Structures and Onsets of Flares*

Published online by Cambridge University Press:  27 September 2017

Kai Sun
Kai Sun*
Affiliation:
Geophysics Department, Beijing University, Beijing, China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Two kinds of MHS equilibrium are studied; isothermal and nonisothermal. The onsets of two - ribbon flares and flare - loops are explained by this study.

Type
Session III: Theory
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 301 - 304
Copyright
Copyright © Kluwer 1989

Footnotes

*

Project supported by NSFC of China.

References

Bluman, G.W. and Cole, J.D., Similarity Methods for Differential Equations, Springer-Ver1ag, (1974).Google Scholar
Brown, A., Ap. J. 128 (1958).Google Scholar
Heyvaerts, J., Lasry, J.M. and Witomskey, G., Lecture Notes Math. 782 (1980).Google Scholar
Jockers, K., Solar Phys. 58 (1978)Google Scholar
Melville, J.P., Hood, A.W. and Priest, E.R., Solar Phys. 92 ( 1984).CrossRefGoogle Scholar
Melville, J.P., Hood, A.W. and Priest, E.R., Geophys. Astrophys. Fluid Dynamics 39 (1987)Google Scholar
Priest, E.R. and Milne, A.M., Solar Phys. 65 (1980).CrossRefGoogle Scholar
Sun, K., Zhang, D. and Wang, Y., Kexue Tongbao 32 (1987).Google Scholar