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    The role of plasma interchange motion for the formation of a plasmapause

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    Authors
    Lemaire, J.
    Kowalkowski, L.
    Discipline
    Physical sciences
    Audience
    Scientific
    Date
    1981
    Metadata
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    Description
    Mcllwain's electric and magnetic field distributions (E3H and M2) have been used to calculate the drift path of plasma density irregularities taking into account plasma interchange motion driven by the gravitational and inertial forces acting on the whole mass of the plasma elements. It has been shown that there is a region in the magnetosphere which is unstable with respect to the interchange motion of the cold plasma element. Any plasma hole in the background density drifts ultimately toward an asymptotic trajectory. Along this trajectory the inward gravitational force is balanced by the outward inertial force averaged over one revolution around the Earth. This asymptotic trajectory, along which all plasma holes ultimately accumulate, is identified with the equatorial plasmapause. The maximum velocity for the interchange motion is proportional to the excess (or defect) of density in the plasma element, and inversely proportional to the integrated Pedersen conductivity. Plasma detachment is shown to occur preferentially in the post-midnight sector.
    Citation
    Lemaire, J.; Kowalkowski, L. (1981). The role of plasma interchange motion for the formation of a plasmapause. , Planetary and Space Science, Vol. 29, Issue 4, 469-478, DOI: 10.1016/0032-0633(81)90090-8.
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/6169
    doi: http://dx.doi.org/10.1016/0032-0633(81)90090-8
    scopus: 2-s2.0-19944368870
    Type
    Article
    Peer-Review
    Yes
    Language
    eng
    Links
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