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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

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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

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