Advanced methods for space simulations by edited by H. Usui and Y. Omura.

By edited by H. Usui and Y. Omura.

It is a selection of prolonged lecture notes of the tutorials given on the overseas tuition for area Simulations (ISSS)-7, March 2005, by way of the invited teachers who've been actively fascinated about desktop simulation strategies in house plasma physics.

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2 Equilibrium thermal fluctuations A plasma sustains fluctuations of various modes of oscillation in thermal equilibrium.

While technically simpler to implement and to run, PIC codes include and even exaggerate the course-graininess of a plasma by clustering a large number of real particles into artificially large and heavy macro-particles. Vlasov-codes directly address the free flowing character of the distribution without adding artificial noise. g, near resonances, which are smeared out by noisy PIC-codes. Also from the point of view of the numerical effort Vlasov codes successfully compete with PIC codes, if the same requirements concerning noise and phase space resolution are applied.

2002) obtained resistivity values exceeding the quasi-linear estimate by up to five orders of magnitude. Petkaki et al. e. for tails enhanced above the Maxwellian distribution. They confirmed a slight enhancement of the linear growth rate obtained by Meng (1992). The anomalous resistivity obtained by these calculations, exceeded by three to five orders the quasi-linear prediction. These results seem to be, however, either an artifact of the low mass ratio or of the method, used. After all these calculations were carried out for an artificially low mass ratio of Mi /m e = 25 Hellinger et al.

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