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Computational Modeling of Solar Magnetic Fields

Published online by Cambridge University Press:  12 April 2016

Takashi Sakurai
Takashi Sakurai*
Affiliation:
National Astronomical Observatory Mitaka, Tokyo 181, Japan

Abstract

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Modeling techniques for solar magnetic fields are discussed. As an extension of the source surface model for large scale solar magnetic fields, a method based on the Green’s function approach to the Laplace equation is proposed. In the force-free field modeling, a proper definition of the boundary condition is an important but still unresolved problem. A condition based on the continuity of the Maxwell stress is newly proposed.

Type
Session 2. Theory of Active Region Structure
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 91 - 97
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Dulk, G.A. and McLean, D.J. 1978, Solar Phys., 57, 279 Google Scholar
Kopp, R.A. and Pneuman, G.W. 1976, Solar Phys., 50, 85 Google Scholar
Leroy, J.L. 1988 in Dynamics and Structures of Quiescent Solar Prominences, Priest, E.R. (ed.), Kluwer Academic Publishers, Dordrecht, p.77 Google Scholar
Poletto, G. and Kopp, R.A. 1988, Solar Phys., 116, 163 Google Scholar
Sakurai, T. 1982, Solar Phys., 76, 301 Google Scholar
Sakurai, T. 1989, Space Sci. Rev., 51, 11 Google Scholar
Wang, Y.M. and Sheeley, N.R. Jr. 1992, Astrophys. J., 392, 310 CrossRefGoogle Scholar