Advanced methods for space simulations - download pdf or read online

By edited by H. Usui and Y. Omura.

ISBN-10: 4887041381

ISBN-13: 9784887041387

It is a number of prolonged lecture notes of the tutorials given on the foreign institution for area Simulations (ISSS)-7, March 2005, through the invited teachers who've been actively interested in desktop simulation concepts in house plasma physics.

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This external, average current balances the average magnetic field (∇× < B >=< J >= Jext ) such that ∂/∂t < E >= 0 (Horne and Freeman, 2001). ∂ fα ∂ fα 1 ∂ fα +v + =0 ∂t ∂x Cα ∂v ∂E = −J + Jext ∂t (37) To complete the code one has to formulate a Vlasov–solver discretization of the elecn+ 1 trostatic Amp`ere equation (37). Since the electric field enters the flux G i, j±2 1 it is 2 appropriate to determine E also at each half-time step t n+1/2 . Hence, E i, j±1/2 should be calculated as n+ 1 n− 1 E i, j±2 1 = E i, j±2 1 − 2 2 t · Ji,n j± 1 (38) 2 while the current Ji,n j± 1 should be calculated synchronously with the advancement of 2 the distribution function.

Freeman, Ion-acoustic resistivity in plasmas with similar ion and electron temperatures, Geophys. Res. , 29, 1002, 2002. Wiegelmann, T. and J. B¨uchner, Evolution of magnetic helicity in the course of kinetic magnetic reconnection, Nonlin. Proc. , 8, 127–140, 2001. Yee, K. , Numerical solution of initial boundary value problems involving Maxwell’s equations in isotropic media, IEEE Trans. Electromagn. , AP-14, 302–307, 1966. Zalesak, S. , Fully multidimensional flux-corrected transport algorithms for fluids, J.

Sydora where α=electron and ion species. The second velocity moment gives the total energy conservation relation α mα 2 N 2 vαi wαi (t) + i=1 1 8π | E|2 d x = 0 (23) if the particle weights and fields are zero initially. 2 Equilibrium thermal fluctuations A plasma sustains fluctuations of various modes of oscillation in thermal equilibrium.

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

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