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Astrophysics and Space Science

, Volume 137, Issue 2, pp 303–315 | Cite as

Kinetic Alfvén waves in extended radio sources

I. Reacceleration
  • L. C. Jafelice
  • R. Opher
Article

Abstract

We study a model of extended radio sources (ERS), in particular, extragalactic jets and radio lobes, which are inhomogeneous and where noncompressive Alfvén and surface Alfvén waves (and not shocks and magnetosonic waves) are primarily excited. We assume that a negligible thermal population exists (i.e., the ion density at the low-energy cut-off of the power law distribution is greater than the ion density of the thermal population, if present). Due to internal instabilities and/or the interaction of the ERS with the ambient medium, surface Alfvén waves (SAW) are created. We show that even very small amplitude SAW are mode converted to kinetic Alfvén waves (KAW) which produce large moving accelerating potentials π, parallel to the magnetic field. Neglecting nonlinear perturbations, and for typical physical parameters of ERS, we obtaineπ≳1 MeV. Wesuggest that these potentials are important in acceleration (e.g., injection energy) and reacceleration of electrons in ERS. We show that energy losses by synchrotron radiation can be compensated by reacceleration by KAW. The relation between KAW acceleration, and previously studied cyclotron-resonance acceleration by Alfvén waves, is discussed.

Keywords

Radiation Magnetic Field Energy Loss Physical Parameter Synchrotron Radiation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1987

Authors and Affiliations

  • L. C. Jafelice
    • 1
  • R. Opher
    • 1
  1. 1.Instituto Astronômico e GeofisicoUniversidade de São PauloBrazil

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