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Three-dimensional flow near a reconnection site at the dayside magnetopause: analytical solutions coupled with MHD simulations: 3D solar wind flow
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Fluid and Experimental Mechanics.ORCID iD: 0000-0001-5294-1855
Umeå university.
Swedish Institute of Space Physics / Institutet för rymdfysik.
2007 (English)In: Journal of Plasma Physics, ISSN 0022-3778, E-ISSN 1469-7807, Vol. 73, no 6, 811-819 p.Article in journal (Refereed) Published
Abstract [en]

We present a coupling between an analytical three-dimensional model covering the plasma flow behaviour through the magnetopause transition layer near a reconnection site, with results from a global MHD simulation describing the plasma flow in the magnetosheath. The structure of the plasma flow near a reconnection site at the dayside terrestrial magnetopause is investigated, together with the development of the magnetopause transition region.

Place, publisher, year, edition, pages
2007. Vol. 73, no 6, 811-819 p.
National Category
Fluid Mechanics and Acoustics
Research subject
Fluid Mechanics
Identifiers
URN: urn:nbn:se:ltu:diva-7746DOI: 10.1017/S0022377806006325Local ID: 628d8ec0-9449-11dc-b13a-000ea68e967bOAI: oai:DiVA.org:ltu-7746DiVA: diva2:980636
Note
Validerad; 2007; 20071116 (lgwe)Available from: 2016-09-29 Created: 2016-09-29 Last updated: 2017-11-28Bibliographically approved

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Westerberg, Lars-GöranÅkerstedt, Hans
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