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The Relativistic Force-free Equation

Published online by Cambridge University Press:  05 March 2013

Leon Mestel
Leon Mestel*
Affiliation:
Astronomy Centre, University of Sussex, Falmer, Brighton BN1 9QJ, England
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Abstract

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This paper is a preliminary report on ongoing work, in collaboration with Drs S. P. Goodwyn, A. J. Mestel, and G. A. E. Wright. The non-dissipative force-free condition should be a good approximation to describe the electromagnetic field in much of the pulsar magnetosphere, but we may plausibly expect it to break down in singular domains. The detailed properties of the solutions will be affected critically by the choice of equatorial boundary condition beyond the light-cylinder.

Keywords

pulsar magnetosphere: force-free fields
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 18 , Issue 4 , 2001 , pp. 384 - 393
Copyright
Copyright © Astronomical Society of Australia 2001

References

Abramowitz, M., & Stegun, I. A. 1965, Handbook of Mathematical Functions (New York: Dover) (AS)Google Scholar
Beskin, V. S., Gurevich, A. V., & Istomin, Ya. N. 1993, Physics of the Pulsar Magnetosphere (Cambridge: Cambridge University Press)Google Scholar
Contopoulos, I. 1995, ApJ, 446, 67 Google Scholar
Contopoulos, I., Kazanas, D., & Fendt, C. 1999, ApJ, 511, 351 (CKF)Google Scholar
Fitzpatrick, R., & Mestel, L. 1988a, MNRAS, 232, 277 (FM)CrossRefGoogle Scholar
Fitzpatrick, R., & Mestel, L. 1988b, MNRAS, 232, 303 (FM)Google Scholar
Goldreich, P., & Julian, W. H. 1969, ApJ, 157, 869 (GJ)Google Scholar
Holloway, N. J., & Pryce, M. H. L. 1981, MNRAS, 194, 95 CrossRefGoogle Scholar
Jeffreys, H., & Jeffreys, B. S. 1972, Methods of Mathematical Physics, 3rd Edition (Cambridge: Cambridge University Press)Google Scholar
Lynden-Bell, D. 1996, MNRAS, 279, 389 CrossRefGoogle Scholar
Mestel, L. 1999, Stellar Magnetism (Oxford: Clarendon Press)Google Scholar
Mestel, L., & Pryce, M. H. L. 1992, MNRAS, 254, 355 (MP)Google Scholar
Mestel, L., & Shibata, S. 1994, MNRAS, 271, 621 (MS)Google Scholar
Mestel, L., & Spruit, H. C. 1987, MNRAS, 226, 57 CrossRefGoogle Scholar
Mestel, L., & Wang, Y.-M. 1979, MNRAS, 188, 799 (MW)Google Scholar
Mestel, L., Robertson, J. A., Wang, Y.-M., & Westfold, K. C. 1985, MNRAS, 217, 443 (MRWW)CrossRefGoogle Scholar
Michel, F. C. 1973, ApJ, 180, 207 CrossRefGoogle Scholar
Michel, F. C. 1974, ApJ, 192, 713 Google Scholar
Michel, F. C. 1991, Theory of Neutron Star Magnetospheres (Chicago: University of Chicago Press)Google Scholar
Scharlemann, E. T., & Wagoner, R. V. 1973, ApJ, 182, 951 Google Scholar
Smith, I. A., Michel, F. C., & Thacker, P. D. 2001, MNRAS, 322, 209 Google Scholar