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Dynamics of Coronal Transients: Two-Dimensional Non-Plane MHD Models
Published online by Cambridge University Press: 14 August 2015
Abstract
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Numerical results are obtained for non-plane MHD responses to a sudden energy release in a stratified model atmosphere. In agreement with observations, it is shown that after the energy release, the magnetic field affected by the energy release relaxes toward the potential configuration while the outer atmospheric fields increase its shear. Additional results suggest a new way of interpreting the energy storage and release in repeated flares.
- Type
- Part VI. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Theoretical Considerations
- Information
- Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 495 - 498
- Copyright
- Copyright © Reidel 1980
References
Hildner, E., Gosling, J. T., MacQueen, R. M., Munro, R. H., Poland, A. I., and Ross, C. L.: 1975, Solar Phys., 42, p. 163.Google Scholar
Nakagawa, Y., Wu, S. T., and Tandberg-Hanssen, E.: 1978b, Astron. Astrophys., 69, p. 43.Google Scholar