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Tearing instability in the pulsar magnetosphere
Authors:P. K. Shukla  M. Y. Yu  V. N. Pavlenko
Affiliation:(1) Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, F.R.G.;(2) Institute for Nuclear Research, Academy of Sciences of the Ukrainian SSR, Kiev, U.S.S.R.
Abstract:Equations governing the coupling of the scalar and vector potentials for a resistive electron-positron plasma in a strong magnetic field are derived. It is shown that in the presence of magnetic shear, a tearing instability may occur. The latter can lead to magnetic field line reconnection and the formation of magnetic islands which could affect the dynamics of the pulsar magnetosphere.
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