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Alfvén wave collapse and the stability of a relativistic electron beam in a magnetized astrophysical plasma
Journal article   Peer reviewed

Alfvén wave collapse and the stability of a relativistic electron beam in a magnetized astrophysical plasma

S. R Spangler and J. P Sheerin
The Astrophysical journal, Vol.272(1), pp.273-278
1983
DOI: 10.1086/161290

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Abstract

The generation of Alfven waves by magnetic field-aligned electron streams, and the evolution of such streams under the action of the self-generated waves, remains an important question in theoretical radio astronomy. In this paper a simple derivation is presented of a time scale on which a nonlinear Alfven wave packet collapses. This time scale is compared with the linear growth and quasi-linear relaxation time scales for conditions appropriate to an extragalactic radio source. The nonlinear time scale can be comparable to the linear and quasi-linear time scales, which suggests that nonlinear effects may stabilize this instability and permit the propagation of anisotropic electron streams.
Astronomy Earth, ocean, space Exact sciences and technology Fundamental aspects of astrophysics Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Magnetohydrodynamics and plasmas

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