Drift-Kinetic Alfvén Waves Observed near a Reconnection X Line in the Earth’s Magnetopause

C. C. Chaston, T. D. Phan, J. W. Bonnell, F. S. Mozer, M. Acuńa, M. L. Goldstein, A. Balogh, M. Andre, H. Reme, and A. Fazakerley
Phys. Rev. Lett. 95, 065002 – Published 4 August 2005

Abstract

We identify drift-kinetic Alfvén waves in the vicinity of a reconnection X line on the Earth’s magnetopause. The dispersive properties of these waves have been determined using wavelet interferometric techniques applied to multipoint observations from the Cluster spacecraft. Comparison of the observed wave dispersion with that expected for drift-kinetic Alfvén waves shows close agreement. The waves propagate outwards from the X line suggesting that reconnection is a kinetic Alfvén wave source. Energetic O+ ions observed in these waves indicate that reconnection is a driver of auroral ion outflow.

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  • Received 26 January 2005

DOI:https://doi.org/10.1103/PhysRevLett.95.065002

©2005 American Physical Society

Authors & Affiliations

C. C. Chaston1, T. D. Phan1, J. W. Bonnell1, F. S. Mozer1, M. Acuńa2, M. L. Goldstein2, A. Balogh3, M. Andre4, H. Reme5, and A. Fazakerley6

  • 1Space Science Laboratory, University of California, Berkeley, California 94720, USA
  • 2NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
  • 3Imperial College, London, United Kingdom
  • 4Swedish Institute of Space Physics, Uppsala, Sweden
  • 5CESR, Toulouse, France
  • 6Mullard Space Science Laboratory, Dorking, United Kingdom

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Issue

Vol. 95, Iss. 6 — 5 August 2005

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