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@ARTICLE{Masek:11901,
author = {Masek, M. and Gibbon, P.},
title = {{M}esh-{F}ree {M}agnetoinductive {P}lasma {M}odel},
journal = {IEEE Transactions on Plasma Science},
volume = {38},
issn = {1939-9375},
address = {New York, NY},
publisher = {IEEE},
reportid = {PreJuSER-11901},
pages = {2377 - 2382},
year = {2010},
note = {Manuscript received December 1, 2009; revised May 6, 2010;
accepted May 28, 2010. Date of publication July 26, 2010;
date of current version September 10, 2010. This work was
supported by the Alliance Program of Helmholtz Association
(HA216/EMMI). Simulations were performed with computing
resources granted by the VSR of Research Center Julich under
project JZAM04.},
abstract = {To study the transport phenomena of energetic particles in
plasmas, a new type of mesh-free plasma simulation model is
introduced. The model is implemented within the parallel
tree code Pretty Efficient Parallel Coulomb-solver, which
uses an O(N logN) Barnes-Hut tree algorithm to speed up the
force calculation. In this paper, we present an extension of
this approach to include magnetic fields within the
so-called Darwin or magnetoinductive approximation, which
neglects the transverse part of the displacement current in
Ampere's law. This effectively omits radiation, which means
that the timestep is no longer limited by the Courant
condition, as in the fully electromagnetic case. The ability
of the model to give a valid description of an N-body system
with self-consistently evolving E- and B-fields is
demonstrated by preliminary tests.},
keywords = {J (WoSType)},
cin = {JSC},
ddc = {530},
cid = {I:(DE-Juel1)JSC-20090406},
pnm = {Scientific Computing (FUEK411) / 411 - Computational
Science and Mathematical Methods (POF2-411)},
pid = {G:(DE-Juel1)FUEK411 / G:(DE-HGF)POF2-411},
shelfmark = {Physics, Fluids $\&$ Plasmas},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000283252500039},
doi = {10.1109/TPS.2010.2052071},
url = {https://juser.fz-juelich.de/record/11901},
}