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Radiative Hydrodynamics of Flares: Preliminary Results and Numerical Treatment of the Transition Region

Published online by Cambridge University Press:  14 August 2015

A.N. McClymont  and
R. C. Canfield
A.N. McClymont
Affiliation:
Department of Physics, C-011 University of California, San Diego La Jolla, California 92093 U.S.A.
R. C. Canfield
Affiliation:
Department of Physics, C-011 University of California, San Diego La Jolla, California 92093 U.S.A.

Extract

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We report on a comprehensive numerical simulation of flare dynamics, encompassing the corona, transition region and chromosphere. A coronal loop geometry, whose magnetic pressure dominates gas pressure, is assumed. These preliminary results assume optically thin radiation; we are currently incorporating optically thick radiative transfer in the chromosphere. We discuss difficulties in modelling the transition region under flare conditions, and suggest tentative solutions.

Type
Part IV. Solar Transient Phenomena Affecting the Corona and Interplanetary Medium: - Theoretical Considerations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 313 - 316
Copyright
Copyright © Reidel 1980 

References

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