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    The magnetospheric driver of subauroral ion drifts

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    DeKeyser(1998b).pdf (349.5Kb)
    Authors
    De Keyser, J.
    Roth, M.
    Lemaire, J.
    Discipline
    Physical sciences
    Subject
    Electric fields
    Ionosphere
    Ions
    Computer simulation
    Electric fields
    Ionosphere
    Magnetosphere
    Thermoelectricity
    Combined effect
    Ion drifts
    Magnetospheric currents
    Subauroral ion drifts
    Substorms
    Magnetosphere
    Atmospheric composition
    Magnetospheric current sheet
    Subauroral ion drifts (SAID)
    Audience
    Scientific
    Date
    1998
    Metadata
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    Description
    Subauroral ion drifts (SAID) are narrow layers of intense westward ionospheric flow observed during substorms. We present numerical simulations showing that the combined effect of thermo-electric and convection electric fields in a magnetospheric current sheet - when mapped down to the ionosphere - can account for the westward direction of the ion drift, the width and intensity of the drift speed peak, and the lifetime of SAID. The model can also explain why SAID occur mainly in the pre-midnight sector.
    Citation
    De Keyser, J.; Roth, M.; Lemaire, J. (1998). The magnetospheric driver of subauroral ion drifts. , Geophysical Research Letters, Vol. 25, Issue 10, 1625-1628, DOI: 10.1029/98GL01135.
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/5400
    doi: http://dx.doi.org/10.1029/98GL01135
    scopus: 2-s2.0-0032069781
    Type
    Article
    Peer-Review
    Yes
    Language
    eng
    Links
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