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AGU: Geophysical Research Letters

 

Index Terms

  • Magnetospheric Physics: Magnetic reconnection
  • Magnetospheric Physics: Magnetotail
  • Magnetospheric Physics: Plasma convection
  • Magnetospheric Physics: Plasma sheet

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 32, L16103, 4 PP., 2005
doi:10.1029/2005GL023585

On the formation of a plasma bubble

M. I. Sitnov

Institute for Research in Electronics and Applied Physics, University of Maryland, College Park, Maryland, USA

P. N. Guzdar

Institute for Research in Electronics and Applied Physics, University of Maryland, College Park, Maryland, USA

M. Swisdak

Icarus Research Inc., Bethesda, Maryland, USA

A simple self-consistent model is proposed, which describes properties of the tail current sheet after the formation of a small plasmoid on the closed field lines in the magnetotail and its quick tailward retreat. Using a theory of forced magnetic reconnection, it is shown that the flux tube that contained a plasmoid becomes a plasma bubble, with the plasmoid being replaced by a thin current sheet embedded within the original thicker sheet. The model allows for an estimate of the decrease of the plasma entropy per unit magnetic flux within the bubble. It predicts that the bubble structure may also include bifurcated current sheets.

Received 20 May 2005; accepted 2 August 2005; published 25 August 2005.

Citation: Sitnov, M. I., P. N. Guzdar, and M. Swisdak (2005), On the formation of a plasma bubble, Geophys. Res. Lett., 32, L16103, doi:10.1029/2005GL023585.

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