• Login
     
    View Item 
    •   ORFEO Home
    • Royal Belgian Institute for Space Aeronomy
    • BIRA-IASB publications
    • View Item
    •   ORFEO Home
    • Royal Belgian Institute for Space Aeronomy
    • BIRA-IASB publications
    • View Item
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Magnetopause Thickness at the Dawn and Dusk Flanks

    View/Open
    DeKeyser(2017a).pdf (321.0Kb)
    Authors
    De Keyser, J.
    Maes, L.
    Maggiolo, R.
    Haaland, S.
    Show allShow less
    Discipline
    Physical sciences
    Audience
    Scientific
    Date
    2017
    Metadata
    Show full item record
    Description
    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.
    Citation
    De Keyser, J.; Maes, L.; Maggiolo, R.; Haaland, S. (2017). Magnetopause Thickness at the Dawn and Dusk Flanks. (Haaland, S., Ed.), Dawn-Dusk Asymmetries in Planetary Plasma Environments, 85-93, DOI: 10.1002/9781119216346.ch7.
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/6313
    doi: http://dx.doi.org/10.1002/9781119216346.ch7
    Type
    Book chapter
    Peer-Review
    Yes
    Language
    eng
    Links
    NewsHelpdeskBELSPO OA Policy

    Browse

    All of ORFEOCommunities & CollectionsBy Issue DateAuthorsTitlesDisciplinesThis CollectionBy Issue DateAuthorsTitlesDisciplines
     

    DSpace software copyright © 2002-2016  DuraSpace
    Send Feedback | Cookie Information
    Theme by 
    Atmire NV