Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T12:20:52.974Z Has data issue: false hasContentIssue false
  • English
  • Français

A model of an isolated magnetic flux tube in a stratified atmosphere

Published online by Cambridge University Press:  13 March 2009

Wen-Rui Hu
Wen-Rui Hu
Affiliation:
Institute of Mechanics, Chinese Academy of Science, Beijing, China
Get access Rights & Permissions [Opens in a new window]

Abstract

A two-dimensional model of a magnetic flux tube confined in a gravitational stratified atmosphere is discussed. The magnetic field in the flux tube is assumed to be force-free. By using the approximation of large scale height, the problem of a free boundary with nonlinear conditions may be reduced to one involving a fixed boundary. The two-dimensional features are obtained by applying the perturbation method and adopting the Lüst–Schlüter model as the basic state. The results show that the configuration of a flux tube confined in a gravitational stratified atmosphere is divergent, and the more twisted the magnetic field, the more divergent is the flux tube.

Type
Research Article
Information
Journal of Plasma Physics , Volume 37 , Issue 3 , June 1987 , pp. 323 - 333
Copyright
Copyright © Cambridge University Press 1987

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Deinzer, W. G. 1965 Astrophys. J. 141, 548.CrossRefGoogle Scholar
Deinzer, W. G., Hensler, G., Schussler, M. & Weisshaar, E. 1984 Astron. Astrophys 139, 426.Google Scholar
Hu, W. R. 1981 Scientia Sinica, 24, 1680.Google Scholar
Hu, W. R. & Li, J. G. 1986 a Acta Astron. Sinica, 27, 303. (In Chinese.)Google Scholar
Hu, W. R. & Li, J. G. 1986 b Acta Astrophys. Sinica, 6, 254. (In Chinese.)Google Scholar
Hu, W. R. & Li, J. G. 1986 c Monthly J. Science, 31, 1780. (In Chinese.)Google Scholar
Lüst, R. & Schlüter, A. 1954 Zs. Astrophys. 34, 303.Google Scholar
Osherovich, V. A. 1984 Solar Phys. 94, 205.CrossRefGoogle Scholar
Parker, E. N. 1974 Astrophys. J. 191, 245.CrossRefGoogle Scholar
Parker, E. N. 1979 Cosmical Magnetic Fields. Oxford University Press.Google Scholar
Spruit, H. C. 1981 The Sun as a Star (ed. Jordan, S.), p. 385. NASA SP-450.Google Scholar
Wilson, P. R. 1977 Astrophys. J. 214, 611.CrossRefGoogle Scholar
Yun, H. S. 1970 Astrophys. J. 162, 975.CrossRefGoogle Scholar