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  Magnetopause Thickness at the Dawn and Dusk Flanks

Keyser, J. D., Maes, L., Maggiolo, R., & Haaland, S. (2017). Magnetopause Thickness at the Dawn and Dusk Flanks. In S. Haaland, A. Runov, & C. Forsyth (Eds.), Dawn-Dusk Asymmetries in Planetary Plasma Environments (pp. 85-93). Hoboken: Wiley.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0000-431C-6 Version Permalink: https://hdl.handle.net/21.11116/0000-0007-1C2F-7
Genre: Book Chapter

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 Creators:
Keyser, Johan De, Author
Maes, Lukas, Author
Maggiolo, Romain, Author
Haaland, Stein1, Author           
Affiliations:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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 MPIS_PROJECTS: Cluster
 Abstract: This paper examines how the magnetic field rotation across the magnetopause influences the fine structure of the layer and its thickness. The situation is examined at noon, dawn, and dusk using a one-dimensional kinetic Vlasov-Maxwell model. The findings indicate that intrinsic physical properties of the Chapman-Ferraro layer may play a role in creating a dawn-dusk asymmetry in the magnetopause thickness.

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Language(s): eng - English
 Dates: 2018-01-312017
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1002/9781119216346.ch7
 Degree: -

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Title: Dawn-Dusk Asymmetries in Planetary Plasma Environments
Source Genre: Book
 Creator(s):
Haaland, Stein, Editor
Runov, Andrei, Editor
Forsyth, Colin, Editor
Affiliations:
-
Publ. Info: Hoboken : Wiley
Pages: 376 Volume / Issue: - Sequence Number: - Start / End Page: 85 - 93 Identifier: ISBN: 978-1-119-21632-2