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A modelling approach to infer the solar wind dynamic pressure from magnetic field observations inside Mercury's magnetosphere
Swedish Institute of Space Physics.
École nationale supérieure de mécanique et d’aérotechnique.
Umeå University, Faculty of Science and Technology, Department of Physics. Swedish Institute of Space Physics.
Umeå University, Faculty of Science and Technology, Department of Physics.ORCID iD: 0000-0002-5765-2806
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2018 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746Article in journal (Refereed) Accepted
Place, publisher, year, edition, pages
2018.
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Fusion, Plasma and Space Physics
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URN: urn:nbn:se:umu:diva-147410OAI: oai:DiVA.org:umu-147410DiVA, id: diva2:1203487
Available from: 2018-05-03 Created: 2018-05-03 Last updated: 2018-06-09

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Lindkvist, Jesper

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