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Phase Space Modulations in Magnetised Plasmas by a Mildly Relativistic Two-Stream Instability
Theoretische Physik IV, Ruhr-Universität Bochum, Bochum, Germany.
Theoretische Physik IV, Ruhr-Universität Bochum, Bochum, Germany.ORCID iD: 0000-0003-4055-0552
Theoretische Physik IV, Ruhr-Universität Bochum, Bochum, Germany.
2007 (English)In: Applied Parallel Computing. State of the Art in Scientific Computing: 8th International Workshop, PARA 2006, Umeå, Sweden, June 18-21, 2006, Revised Selected Papers / [ed] Bo Kågström, Erik Elmroth, Jack Dongarra, Jerzy Waśniewski, Springer Berlin/Heidelberg, 2007, 361-370 p.Conference paper, Published paper (Refereed)
Abstract [en]

A kinetic particle-in-cell simulation and 3D point-rendering visualisation are used to investigate a two-stream plasma instability, possibly found in the accretion disc of black holes. A plasma in an oblique external magnetic field is considered. The instability gives rise to a quasi-electrostatic wave able to trap electrons and accelerate them by cross-field transport. The results of the simulation show an acceleration of the electrons to speeds similar to the bulk speed of microquasar jets.

Place, publisher, year, edition, pages
Springer Berlin/Heidelberg, 2007. 361-370 p.
Series
Lecture Notes in Computer Science, ISSN 0302-9743 (print), 1611-3349 (online) ; 4699
Keyword [en]
collisionless plasma, oblique magnetic field, astrophysical jets, electron surfing acceleration, PIC simulation, visualisation
National Category
Engineering and Technology
Identifiers
URN: urn:nbn:se:liu:diva-39445DOI: 10.1007/978-3-540-75755-9_44ISI: 000250904900044Local ID: 48425ISBN: 978-3-540-75754-2 (print)ISBN: 978-3-540-75755-9 (print)OAI: oai:DiVA.org:liu-39445DiVA: diva2:260294
Conference
8th International Workshop, PARA 2006, Umeå, Sweden, June 18-21, 2006
Available from: 2009-10-10 Created: 2009-10-10 Last updated: 2017-11-03Bibliographically approved

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Dieckmann, Mark E

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CiteExportLink to record
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Citation style
  • apa
  • harvard1
  • ieee
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  • nn-NB
  • sv-SE
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