Plasma and Fusion Research
Volume 5, 007 (2010)
Regular Articles
- Laboratoire de Physique des Rayonnements et leurs interactions avec la Matière (PRIMALAB), Département de Physique, Faculté des Sciences, Université de Batna, Batna, 05000 DZ, Algeria
- 1)
- Commissariat à l'Energie Atomique, Centre de Recherche Nucléaire de Draria, Division de Sûreté Nucléaire et Radioprotection, Draria, Alger, Algeria
- 2)
- Laboratoire de Physique Energétique Appliquée, Département de Physique, Faculté des Sciences, Université de Batna, Batna, 05000 DZ, Algeria
Abstract
In this paper, the Weibel instability, driven by the plasma temperature anisotropy, in the corona of high intense laser fusion plasma is studied. The unperturbed electronic distribution function, f, of the anisotropic corona is supposed to be a bi-Maxwellian. That T∥ = T⊥ ± WO, where WO = ¼ mevO2 is the averaged electron quiver energy in the laser electric field. The first and the second anisotropies of f projected on the Legendre polynomials are calculated as a function of the scaling parameter, WO / T⊥. The Weibel instability parameters are explicitly calculated as a function of the scaling parameter. For typical parameters of the laser pulse and the fusion plasma, it has been shown that very unstable Weibel modes, γ ≳ 1011 s−1, can be excited in the corona.
Keywords
inertial fusion, laser created plasma, electron oscillation, Weibel instability, scaling law
Full Text
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This paper may be cited as follows:
Abdelaziz SID, Abdennasser GHEZAL, Azzeddine SOUDANI and Mohamed BEKHOUCHE, Plasma Fusion Res. 5, 007 (2010).