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Electron acceleration by a relativistic two stream instability with oblique B
Linköpings universitet, Institutionen för teknik och naturvetenskap, Visuell informationsteknologi och applikationer. Linköpings universitet, Tekniska högskolan.ORCID-id: 0000-0003-4055-0552
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Institute of Theoretical Physics IV Ruhr-University Bochum, Germany.
Vise andre og tillknytning
2006 (engelsk)Inngår i: 33rd European Physical Society Conference on Plasma Physics,2006, Rome: European Physical Society , 2006, s. P4.071-Konferansepaper, Publicerat paper (Fagfellevurdert)
Abstract [en]

Electrons that are trapped by a quasi-electrostatic wave move, on average, with the phase speed of the wave. In the presence of a magnetic field B, the trapped electrons could, in principle, be accelerated to cosmic ray energies through cross-field transport. We model this cross-field transport with a particle-in-cell (PIC) simulation for an oblique B. The electron energies at the simulation's end exceed 5 MeV for all pitch angles and they can reach GeV energies along the wavevector. We discuss environments, in which such conditions may exist and for which such an acceleration would be relevant.

sted, utgiver, år, opplag, sider
Rome: European Physical Society , 2006. s. P4.071-
Emneord [en]
plasma physics
HSV kategori
Identifikatorer
URN: urn:nbn:se:liu:diva-35709Lokal ID: 28209OAI: oai:DiVA.org:liu-35709DiVA, id: diva2:256557
Merknad
ISBN 2-914771-40-1Tilgjengelig fra: 2009-10-10 Laget: 2009-10-10 Sist oppdatert: 2017-11-03

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http://eps2006.frascati.enea.it/papers/start.htm

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Dieckmann, Mark EYnnerman, Anders

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