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Magnetic Field Reconnection in Cosmic Plasmas

Published online by Cambridge University Press:  04 August 2017

B. U. Ö. Sonnerup
B. U. Ö. Sonnerup*
Affiliation:
Dartmouth College, Hanover, NH 03755 U.S.A.

Abstract

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A brief review is presented of the concept of magnetic field reconnection or merging. This process occurs whenever an electric field is present along a separator line in the magnetic field. The basic properties of reconnection are discussed in the context of the classical MHD models by Sweet and Parker and by Petschek. Attention is then focussed on reconnection in collision-free plasmas. The energization of charged particles during their interaction with the current layers associated with the reconnection geometry is discussed and the nature of the processes occurring in the so-called diffusion region which surrounds the separator is considered. Finally, comments are made on the nonsteady aspects of reconnection at the earth's magnetopause.

Type
Session I
Information
Symposium - International Astronomical Union , Volume 107: Unstable Current Systems and Plasma Instabilities , 1985 , pp. 5 - 23
Copyright
Copyright © Reidel 1985 

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