Hostname: page-component-77c89778f8-n9wrp Total loading time: 0 Render date: 2024-07-22T11:58:20.518Z Has data issue: false hasContentIssue false
  • English
  • Français

Plan MHD flows in a hyperbolic magnetic field: implications for the problem of magnetic field line reconnexion

Published online by Cambridge University Press:  13 March 2009

Shadia Rifai Habbal  and
Tai-Fu Tuan
Shadia Rifai Habbal
Affiliation:
Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221
Tai-Fu Tuan
Affiliation:
Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221
Get access Rights & Permissions [Opens in a new window]

Abstract

This paper examines the nature of plane, steady, incompressible MHD flow in a purely hyperbolic magnetic field. It is shown that in such a magnetic field the MHD equations can yield exact analytic solutions for the plasma flow. The flow has the following properties. In the far region where the conductivity is assumed to be sufficiently high so that the plasma is effectively ‘ frozen ’ to the magnetic field, the flow pattern is radial. The plasma motion is directed towards the neutral line in the incident ‘ sectors ’ and away from it in the outgoing ‘ sectors ’ with a consequent reversal in direction across the magnetic separatrices where the solution becomes singular. The plasma pressure and density in this flow are calculated and it is shown that the latter remains constant along a streamline. It is further shown that a uniform finite conductivity is not compatible with a stagnation point at the magnetic null point. However, for a parabolic increase of conductivity with increasing distance from that point, plasma flow with uniform density along hyperbolic streamlines is shown to be possible. The relevance of these flows to the magnetic field merging problem is discussed.

Type
Research Article
Information
Journal of Plasma Physics , Volume 21 , Issue 1 , February 1979 , pp. 85 - 96
Copyright
Copyright © Cambridge University Press 1979

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

Baum, P. J., Bratenahl, A. & Cowan, M. 1976 J. Plasma Phys. 15, 259.Google Scholar
Cowley, S. W. H. 1975 J. Plasma Phys. 14, 475.CrossRefGoogle Scholar
Dungey, J. W. 1953 Phil. Mag. 44, 725.Google Scholar
Parker, E. N. 1973 J. Plasma Phys. 9, 49.CrossRefGoogle Scholar
Petschek, H. E., 1964, AAS-NASA Symposium on the Physics of Solar Flares, NASA SP-50, 425.Google Scholar
Sonnerup, B. U. ü, 1970, J. Plasma Phys. 4, 161.Google Scholar
Sonnerup, B. U. ü & Priest, E. R., 1975 J. Plasma Phys. 14, 283.Google Scholar
Syrovatskii, S. I., 1969, Solar Flares and Space Research (ed. Jager, C. do and Svestka, Z.), 346.Google Scholar
Vasylinas, V. M., 1975, Rev. Geophys. Space Phys. 13, 303.Google Scholar
Yeh, T. & Axford, W. I., 1970, J. Plasma Phys. 4, 207.Google Scholar