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  • American Geophysical Union (AGU)  (2)
  • 1980-1984  (2)
Medientyp
Verlag/Herausgeber
  • American Geophysical Union (AGU)  (2)
Sprache
Erscheinungszeitraum
  • 1980-1984  (2)
Jahr
  • 1
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 1982
    In:  Journal of Geophysical Research: Space Physics Vol. 87, No. A8 ( 1982-08), p. 5949-5962
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 87, No. A8 ( 1982-08), p. 5949-5962
    Kurzfassung: We present preliminary results of applying the Rice convection model to the early main phase of the magnetic storm of July 29, 1977. The computer model self‐consistently computes electric fields and currents, as well as plasma distributions and velocities, in the inner‐magnetosphere/ionosphere system. In the equatorial plane, the region modeled includes geocentric distances less than about the magnetopause standoff distance. Particle loss, parallel electric fields, and neutral winds are neglected. On the basis of solar wind parameters and the AL index as input, the model predicts the injection of plasma‐sheet plasma to form a substantial storm time ring current. The total strength of the model‐predicted ring current agrees accurately with the observed Dst index. Comparison of the model results with electric fields and Birkeland currents measured by S3‐3 shows qualitative agreement but interesting quantitative discrepancies. During this event, region 1 currents, which in standard convection theory would connect to the outer magnetosphere, are observed as low as 60° invariant latitude at dawn and dusk. We examine the possibility that the magnetic field might be so highly inflated that 60° field lines extend to the outer magnetosphere. In the model, distortion of the inner edge of the plasma sheet by the magnetospheric compression associated with the sudden commencement temporarily disturbs the normal Birkeland‐current pattern. The normal tendency for the plasma sheet's inner edge to shield low L values from the convection electric field is also temporarily disrupted. Normal Birkeland currents and shielding reassert themselves after about an hour. Time‐integrated Joule heating in the model ionosphere over the first 5.5 hours of the storm main phase is about half the increase in model ring‐current energy.
    Materialart: Online-Ressource
    ISSN: 0148-0227
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 1982
    ZDB Id: 2033040-6
    ZDB Id: 3094104-0
    ZDB Id: 2130824-X
    ZDB Id: 2016813-5
    ZDB Id: 2016810-X
    ZDB Id: 2403298-0
    ZDB Id: 2016800-7
    ZDB Id: 161666-3
    ZDB Id: 161667-5
    ZDB Id: 2969341-X
    ZDB Id: 161665-1
    ZDB Id: 3094268-8
    ZDB Id: 710256-2
    ZDB Id: 2016804-4
    ZDB Id: 3094181-7
    ZDB Id: 3094219-6
    ZDB Id: 3094167-2
    ZDB Id: 2220777-6
    ZDB Id: 3094197-0
    SSG: 16,13
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 2
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 1984
    In:  Journal of Geophysical Research: Space Physics Vol. 89, No. A4 ( 1984-04), p. 2169-2179
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 89, No. A4 ( 1984-04), p. 2169-2179
    Kurzfassung: The configuration of the tail plasma sheet in earth's magnetotail has been calculated in connection with a three‐dimensional magnetospheric B field model. This model is based on the idea that thermal plasma, tail currents, and magnetic field be in magnetohydrostatic equilibrium during time periods of magnetically quiet conditions. The tail configuration is generated by a separation method assuming a cylindrical magnetotail boundary with constant radius. The separation method restricts self‐consistency to planes perpendicular to the tail axis. The computed tail plasma sheet is flexible and reacts to changes of the earth's dipole tilt angle and changes of the solar wind pressure. Consequences for the plasma sheet configuration with respect to the assumed tail magnetopause shape and the separation method are the following: (1) the plasma sheet thickness increases in Y GSM direction toward the flanks of the tail; (2) the plasma sheet becomes thicker and more diffuse with increasing distance from the earth; (3) during the northern hemisphere summer, the neutral sheet is raised above the magnetospheric equatorial plane around local midnight but crosses this plane and is depressed below it near the flanks of the tail. The latter result agrees qualitatively with Fairfield's empirical neutral sheet model which he derived from spacecraft measurements of the tail field polarity. This agreement between theory and observational material provides a further piece of evidence that the magnetohydrostatic theory is an appropriate level for describing quantitatively the quiet state of the magnetosphere.
    Materialart: Online-Ressource
    ISSN: 0148-0227
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 1984
    ZDB Id: 2033040-6
    ZDB Id: 3094104-0
    ZDB Id: 2130824-X
    ZDB Id: 2016813-5
    ZDB Id: 2016810-X
    ZDB Id: 2403298-0
    ZDB Id: 2016800-7
    ZDB Id: 161666-3
    ZDB Id: 161667-5
    ZDB Id: 2969341-X
    ZDB Id: 161665-1
    ZDB Id: 3094268-8
    ZDB Id: 710256-2
    ZDB Id: 2016804-4
    ZDB Id: 3094181-7
    ZDB Id: 3094219-6
    ZDB Id: 3094167-2
    ZDB Id: 2220777-6
    ZDB Id: 3094197-0
    SSG: 16,13
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
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