Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-26T07:23:44.915Z Has data issue: false hasContentIssue false
  • English
  • Français

Solitons in Magnetic Flux Tubes

Published online by Cambridge University Press:  04 August 2017

B. Roberts
B. Roberts*
Affiliation:
Dept. Applied Mathematics, St. Andrews University Scotland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The highly inhomogeneous nature of the solar atmosphere leads us to suggest that solitons may occur in magnetic structures such as coronal loops or photospheric flux tubes. The theory is outlined for the simple case of a magnetic slab in a field-free atmosphere and shown to lead to the Benjamin-Ono equation.

Type
I. Magnetic Fields in Stellar Photospheres
Information
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 61 - 66
Copyright
Copyright © Reidel 1983 

References

Benjamin, T.B.: 1967, J. Fluid Mech. 29, p. 559.Google Scholar
Edwin, P.M. and Roberts, B.: 1982, Solar Phys. 76, p. 239.CrossRefGoogle Scholar
Edwin, P.M. and Roberts, B.: 1983, in preparation.Google Scholar
Miles, J.W.: 1980, Ann. Rev. Fluid Mech. 12, p. 11.Google Scholar
Ono, H.: 1975, J. Phys. Soc. Japan 39, p. 1082.Google Scholar
Roberts, B.: 1981, Solar Phys. 69, p. 39.Google Scholar
Roberts, B. and Mangeney, A.: 1982, Monthly Not. Roy. Astron. Soc. 198, p. 7p.Google Scholar
Roberts, B. and Webb, A.R.: 1978, Solar Phys. 56, p. 5.Google Scholar
Spruit, H.C.: 1983, these proceedings.Google Scholar
Zabusky, N.J. and Kruskal, M.D.: 1965, Phys. Rev. Letters 15, p. 240.Google Scholar