By edited by H. Usui and Y. Omura.
It is a choice of prolonged lecture notes of the tutorials given on the foreign institution for house Simulations (ISSS)-7, March 2005, by way of the invited academics who've been actively interested by laptop simulation innovations in area plasma physics.
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Extra resources for Advanced methods for space simulations
2006. B¨uchner, J. and N. Elkina, Vlasov code simulation of anomalous resistivity, Space Sci. , 121, No. 1-4, 237–252, 2006a. 1007/s11214-006-6542-6) B¨uchner, J. and N. Elkina, Anomalous resistivity of current-driven isothermal plasmas due to phase space structuring, Phys. Plasmas, 13, 082304-1–082304-9, 2006b. , Vlasov simulations of ion acoustic double layers, in Computer simulation of Space Plasmas, edited by H. Matsumoto and T. Sato, Terra Scientific Publishing Company, Tokyo, Japan, pp.
Acknowledgments. The author gratefully acknowledges discussions with P. Bertrand, N. Elkina, F. Jenko, I. Silin, R. Sydora, Th. Wiegelmann and thanks the referee for his/her comments. References Arber, T. D. and R. G. Vann, A critical comparison of Eulerian-grid-based Vlasov solvers, J. Comput. , 180, 339–357, 2002. Armstrong, T. , R. C. Harding, G. Knorr, and D. Montgomery, Solution of Vlasov’s equation by transform methods, in Methods of Computational Physics, vol. 9, edited by B. Alder, S. Fernbach, M.
14) δ f Particle-in-Cell Plasma Simulation Model ∗n+1/2 n+1/2 • Obtain Ri used. x n+1/2 , vi n+1/2 , F ∗n+1/2 where vi n+1/2 • Advance weights(corrector step): wi ∗n+1/2 where win ≈ wi n−1/2 n−1/2 = wi 51 ≈ vin+1 + vin /2 is ∗n+1/2 − t 1 − win Ri n−1/2 +Ri 2 /2 is used. + wi The perturbed charge density is obtained from the δ f weights, wi , using ρ˜ = qi wi S (x − xi ) (19) i where S is the spatial shape factor associated with the phase space volume element of the marker particles. The perturbed charge density is formed at discrete grid points using interpolation, and then Eq.
Advanced methods for space simulations by edited by H. Usui and Y. Omura.
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