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Energy Storage and Instability in Magnetic Flux Tubes

Published online by Cambridge University Press:  14 August 2015

Takashi Sakurai
Takashi Sakurai*
Affiliation:
Department of Astronomy, University of Tokyo

Extract

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Now it is known that the solar corona consists of many loops which are believed to represent the structure of the magnetic field. Since the plasma is very tenuous in the corona, the equilibrium of the magnetic field is approximated by the force-free field:

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. 291 - 294
Copyright
Copyright © Reidel 1980 

References

Kowalik, J., and Osborne, M. R. 1968, “Methods for Unconstrained Optimization Problems” (Americal Elsevier, New York), p.45.Google Scholar
Nakagawa, Y., and Raadu, M. A. 1972, Solar Phys. 25, 127.CrossRefGoogle Scholar
Sakurai, T. 1976, Publ. Astron. Soc. Japan 28, 177.Google Scholar
Sakurai, T. 1979, Publ. Astron. Soc. Japan 31, 209.Google Scholar
Strang, G., and Fix, G. J. 1973, “An Analysis of the Finite Element Method” (Prentice-Hall, Englewood Cliffs, New Jersey).Google Scholar