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Dynamics of Coronal Transients: Two-Dimensional Non-Plane MHD Models

Published online by Cambridge University Press:  14 August 2015

Y. Nakagawa ,
S. T. Wu  and
S. M. Han
Y. Nakagawa
Affiliation:
Space Sciences Laboratory/NASA Marshall Space Flight Center, AL 35812, U.S.A.
S. T. Wu
Affiliation:
The University of Alabama in Huntsville Huntsville, AL 35807, U. S. A.
S. M. Han
Affiliation:
The University of Alabama in Huntsville Huntsville, AL 35807, U. S. A.

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

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