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Hydromagnetic flow about a curved neutral sheet

Published online by Cambridge University Press:  13 March 2009

M. Teske†
Affiliation:
Gas Dynamics Laboratory, Department of Aerospace and Mechanical Sciences, Princeton University
S. H. Lam
Affiliation:
Gas Dynamics Laboratory, Department of Aerospace and Mechanical Sciences, Princeton University

Abstract

The present paper examines the magnetic boundary layer along a curved interface between two opposing fluid streams carrying oppositely directed magnetic fields. This problem is known classically as the neutral sheet or X neutral-point problem. A formal two-dimensional theory is constructed that depends solely on the mechanism of magnetic diffusion and thus eliminates the need for any added MHD waves. This theory shows clearly the detailed structure of the neutral sheet boundary layer and, more importantly, the parametric dependence of the solution on free-stream parameters such as the magnetic Reynolds number and the Alfvén number. It is shown that a thin, powerful jet of high thermal and kinetic energy exists within the boundary layer. Sample numerical solutions are presented, and the various mathematical difficulties associated with this class of problems are discussed.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1972

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References

REFERENCES

Dungey, J. W. 1961 Interplanetary magnetic field and the auroral zones. Phys. Rev. Lett. 6, 47.CrossRefGoogle Scholar
Levy, R. H., Petschek, H. E. & Siscoe, G. L. 1964 Aerodynamic aspects of the magneto spheric flow. AIAA Journal, 2, 2065.CrossRefGoogle Scholar
Petschek, H. E. 1964 Magnetic field annihilation. AAS–NASA Symposium on olar Flares (ed. Hess, W. N.), p. 425, NASA SP-50.Google Scholar
Sonnerup, B. U. Ö. 1970 Magnetic-field re-connoxion in a highly conducting incompressible fluid. J. Plasma Phys. 4, 161.CrossRefGoogle Scholar
Spreiter, J. R. & Alksne, A. Y. 1970 Solar-wind flow past objects in the solar system. Annual Review of Fluid Mechanics vol. 2 (ed. Van Dyke, M., Vincenti, W. G. and Wehausen, J. V.), p. 313. Annual Reviews.Google Scholar
Willis, D. M. 1971 Structure of the magnetopause. Rev. Geophys. Space Phys. 9, 953.CrossRefGoogle Scholar
Yeh, T. & Axford, W. I. 1970 On the re-connexion of magnetic field lines in conducting fluids. J. Plasma Phys. 4, 207.CrossRefGoogle Scholar