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The amplification of magnetic (Weibel) modes in laser-plasma interaction is investigated by use of unperturbed distribution functions given by Fokker-Planck simulations and a dispersion relation valid for all collisionality regimes. In the five cases studied, a strongly growing mode is found in the underdense plasma, where v̄ₓ²<1/2v̄_⊥², and the usual slowly growing one in the overdense plasma. The first mode grows convectively outwards by more than 10⁴. The convection velocities are found to be very different from Nernst values.
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Matte et al. (1987) studied this question.
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