A pressure tensor description for the time-resonant Weibel instability
Abstract
We discuss a fluid model with inclusion of the complete pressure tensor dynamics for the description of Weibel-type instabilities in a counterstreaming beam configuration. Differently from the case recently studied in Sarrat et al. (Europhys. Lett., vol. 115, 2016, 45001), where perturbations perpendicular to the beams were considered, here we focus only on modes propagating along the beams. Such a configuration is responsible for the growth of two kinds of instabilities, the two-stream instability and the Weibel instability, which in this geometry becomes `time resonant', i.e. propagating. This fluid description agrees with the kinetic one and makes it possible e.g. to identify the transition between non-propagating and propagating Weibel modes, already evidenced by Lazar et al. (J. Plasma Phys., vol. 76 (1), 2010, p. 49) as a `slope breaking' of the growth rate, in terms of a merger of two non-propagating Weibel modes.
- Publication:
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Journal of Plasma Physics
- Pub Date:
- February 2017
- DOI:
- arXiv:
- arXiv:1610.02723
- Bibcode:
- 2017JPlPh..83a7003S
- Keywords:
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- astrophysical plasmas;
- plasma instabilities;
- space plasma physics;
- Physics - Plasma Physics
- E-Print:
- The old title has been replaced in order to avoid confusion between time and spatial resonances. This paper deals with the Time Resonant Weibel Instability