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000011901 0247_ $$2DOI$$a10.1109/TPS.2010.2052071
000011901 0247_ $$2WOS$$aWOS:000283252500039
000011901 0247_ $$2ISSN$$a0093-3913
000011901 0247_ $$2ISSN$$a1939-9375
000011901 037__ $$aPreJuSER-11901
000011901 041__ $$aeng
000011901 082__ $$a530
000011901 084__ $$2WoS$$aPhysics, Fluids & Plasmas
000011901 1001_ $$0P:(DE-HGF)0$$aMasek, M.$$b0
000011901 245__ $$aMesh-Free Magnetoinductive Plasma Model
000011901 260__ $$aNew York, NY$$bIEEE$$c2010
000011901 300__ $$a2377 - 2382
000011901 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article
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000011901 440_0 $$02527$$aIEEE Transactions on Plasma Science$$v38$$x0093-3913$$y9
000011901 500__ $$aManuscript 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.
000011901 520__ $$aTo study the transport phenomena of energetic particles in plasmas, a new type of mesh-free plasma simulation model is introduced. The model is implemented within the parallel tree code Pretty Efficient Parallel Coulomb-solver, which uses an O(N logN) Barnes-Hut tree algorithm to speed up the force calculation. In this paper, we present an extension of this approach to include magnetic fields within the so-called Darwin or magnetoinductive approximation, which neglects the transverse part of the displacement current in Ampere's law. This effectively omits radiation, which means that the timestep is no longer limited by the Courant condition, as in the fully electromagnetic case. The ability of the model to give a valid description of an N-body system with self-consistently evolving E- and B-fields is demonstrated by preliminary tests.
000011901 536__ $$0G:(DE-Juel1)FUEK411$$2G:(DE-HGF)$$aScientific Computing (FUEK411)$$cFUEK411$$x0
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000011901 588__ $$aDataset connected to Web of Science
000011901 65320 $$2Author$$aDarwin approximation
000011901 65320 $$2Author$$ahierarchical tree code
000011901 650_7 $$2WoSType$$aJ
000011901 7001_ $$0P:(DE-Juel1)132115$$aGibbon, P.$$b1$$uFZJ
000011901 773__ $$0PERI:(DE-600)2025402-7$$a10.1109/TPS.2010.2052071$$gVol. 38, p. 2377 - 2382$$p2377 - 2382$$q38<2377 - 2382$$tIEEE Transactions on Plasma Science$$v38$$x1939-9375$$y2010
000011901 8567_ $$uhttp://dx.doi.org/10.1109/TPS.2010.2052071
000011901 909CO $$ooai:juser.fz-juelich.de:11901$$pVDB
000011901 9141_ $$y2010
000011901 9132_ $$0G:(DE-HGF)POF3-511$$1G:(DE-HGF)POF3-510$$2G:(DE-HGF)POF3-500$$aDE-HGF$$bKey Technologies$$lSupercomputing & Big Data$$vComputational Science and Mathematical Methods$$x0
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000011901 9201_ $$0I:(DE-Juel1)JSC-20090406$$gJSC$$kJSC$$lJülich Supercomputing Centre$$x0
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