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| 001 | 11901 | ||
| 005 | 20210129210550.0 | ||
| 024 | 7 | _ | |2 DOI |a 10.1109/TPS.2010.2052071 |
| 024 | 7 | _ | |2 WOS |a WOS:000283252500039 |
| 024 | 7 | _ | |2 ISSN |a 0093-3913 |
| 024 | 7 | _ | |2 ISSN |a 1939-9375 |
| 037 | _ | _ | |a PreJuSER-11901 |
| 041 | _ | _ | |a eng |
| 082 | _ | _ | |a 530 |
| 084 | _ | _ | |2 WoS |a Physics, Fluids & Plasmas |
| 100 | 1 | _ | |0 P:(DE-HGF)0 |a Masek, M. |b 0 |
| 245 | _ | _ | |a Mesh-Free Magnetoinductive Plasma Model |
| 260 | _ | _ | |a New York, NY |b IEEE |c 2010 |
| 300 | _ | _ | |a 2377 - 2382 |
| 336 | 7 | _ | |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |a Journal Article |
| 336 | 7 | _ | |2 DataCite |a Output Types/Journal article |
| 336 | 7 | _ | |0 0 |2 EndNote |a Journal Article |
| 336 | 7 | _ | |2 BibTeX |a ARTICLE |
| 336 | 7 | _ | |2 ORCID |a JOURNAL_ARTICLE |
| 336 | 7 | _ | |2 DRIVER |a article |
| 440 | _ | 0 | |0 2527 |a IEEE Transactions on Plasma Science |v 38 |x 0093-3913 |y 9 |
| 500 | _ | _ | |a 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. |
| 520 | _ | _ | |a 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. |
| 536 | _ | _ | |0 G:(DE-Juel1)FUEK411 |2 G:(DE-HGF) |x 0 |c FUEK411 |a Scientific Computing (FUEK411) |
| 536 | _ | _ | |0 G:(DE-HGF)POF2-411 |a 411 - Computational Science and Mathematical Methods (POF2-411) |c POF2-411 |f POF II |x 1 |
| 588 | _ | _ | |a Dataset connected to Web of Science |
| 650 | _ | 7 | |2 WoSType |a J |
| 653 | 2 | 0 | |2 Author |a Darwin approximation |
| 653 | 2 | 0 | |2 Author |a hierarchical tree code |
| 700 | 1 | _ | |0 P:(DE-Juel1)132115 |a Gibbon, P. |b 1 |u FZJ |
| 773 | _ | _ | |0 PERI:(DE-600)2025402-7 |a 10.1109/TPS.2010.2052071 |g Vol. 38, p. 2377 - 2382 |p 2377 - 2382 |q 38<2377 - 2382 |t IEEE Transactions on Plasma Science |v 38 |x 1939-9375 |y 2010 |
| 856 | 7 | _ | |u http://dx.doi.org/10.1109/TPS.2010.2052071 |
| 909 | C | O | |o oai:juser.fz-juelich.de:11901 |p VDB |
| 913 | 2 | _ | |0 G:(DE-HGF)POF3-511 |1 G:(DE-HGF)POF3-510 |2 G:(DE-HGF)POF3-500 |a DE-HGF |b Key Technologies |l Supercomputing & Big Data |v Computational Science and Mathematical Methods |x 0 |
| 913 | 1 | _ | |0 G:(DE-HGF)POF2-411 |1 G:(DE-HGF)POF2-410 |2 G:(DE-HGF)POF2-400 |a DE-HGF |b Schlüsseltechnologien |l Supercomputing |v Computational Science and Mathematical Methods |x 3 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF2 |
| 914 | 1 | _ | |y 2010 |
| 920 | 1 | _ | |0 I:(DE-Juel1)JSC-20090406 |g JSC |k JSC |l Jülich Supercomputing Centre |x 0 |
| 970 | _ | _ | |a VDB:(DE-Juel1)123284 |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a ConvertedRecord |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a I:(DE-Juel1)JSC-20090406 |
| 980 | _ | _ | |a UNRESTRICTED |
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