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Fast magnetosonic waves in pulsar winds

Y. E. Lyubarsky
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Abstract

Fast magnetosonic waves in a magnetically-dominated plasma are investigated. In the pulsar wind, these waves may transport a significant fraction of the energy flux. It is shown that the nonlinear steepening and subsequent formation of multiple shocks is a viable mechanism for the wave dissipation in the pulsar wind. The wave dissipation both in the free pulsar wind and beyond the wind termination shock is considered.

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Y. E. Lyubarsky. 2002-11-04. Fast magnetosonic waves in pulsar winds. https://doi.org/10.1046/j.1365-8711.2003.06221.x

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