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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.

Information

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

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