Hostname: page-component-8448b6f56d-tj2md Total loading time: 0 Render date: 2024-04-20T06:57:36.043Z Has data issue: false hasContentIssue false

Alfvén resonance absorption in electron-positron plasmas

Published online by Cambridge University Press:  08 June 2011

N. F. Cramer*
Affiliation:
School of Physics, The University of Sydney, NSW 2006, Australia email: cramer@physics.usyd.edu.au
Rights & Permissions [Opens in a new window]

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.

Waves propagating obliquely in a magnetized cold pair plasma experience an approximate resonance in the wavevector component perpendicular to the magnetic field, which is the analogue of the Alfvén resonance in normal electron-ion plasmas. Wave absorption at the resonance can take place via mode conversion to the analogue of the short wavelength inertial Alfvén wave. The Alfvén resonance could play a role in wave propagation in the pulsar magnetosphere leading to pulsar radio emission. Ducting of waves in strong plasma gradients may occur in the pulsar magnetosphere, which leads to the consideration of Alfvén surface waves, whose energy is concentrated in the region of strong gradients.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Arons, J. & Barnard, J. J. 1986, ApJ, 302, 120CrossRefGoogle Scholar
Cramer, N. F. 2001, The Physics of Alfvén Waves (Berlin: Wiley-VCH)CrossRefGoogle Scholar
Iwamoto, N. 1993, Phys. Rev. E, 47, 604CrossRefGoogle Scholar
Luo, Q., Melrose, D. B., & Fussell, D. 2002, Phys. Rev. E, 66, 026405.CrossRefGoogle Scholar
Stewart, G. A. & Laing, E. W. 1992, J. Plasma Phys., 47, 295CrossRefGoogle Scholar
Weltevrede, P., Stappers, B. W., van den Horn, L. J., & Edwards, R.T. 2003, A&A, 412, 473Google Scholar
Zank, G. P. & Greaves, R. G. 1995, Phys. Rev. E, 51, 6079CrossRefGoogle Scholar