Results 201 to 210 of about 1,155 (215)
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Recent Research on the Magnetospheric Plasmapause
Radio Science, 1968The plasmapause is a three‐dimensional field aligned boundary that divides the closed field‐line portion of the earth's magnetosphere into two physically distinct regions. The boundary is asymmetric, usually exhibiting a minimum geocentric range near dawn and a maximum near dusk under conditions of moderate but steady geomagnetic agitation (Kp = 2 − 4).
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The ‘Roche-Limit’ of ionospheric plasma and the formation of the plasmapause
Planetary and Space Science, 1974Abstract The plasmapause position is determined by the innermost equipotential surface which is tangent to the ‘Roche-Limit’ surface of the ionospheric plasma filling the magnetosphere. When the thermal particles corotate with the Earth's angular velocity, the ‘Roche-Limit’ equatorial distance is L c =5.78 [ R E ].
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Plasmapause effects in the top side ionosphere
Journal of Geophysical Research, 1976Values of plasma temperature and O+/H+ ion transition height, obtained from 60,000 Alouette 1 electron density profiles, are used to study changes associated with the plasmapause. An ionospheric plasmapause can be defined by (1) the latitude at which peak temperatures occur, (2) the latitude down to which the ion transition height remains high, showing
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Snake-based technique for plasmapause tracking
Proceedings of the 17th International Conference on Pattern Recognition, 2004. ICPR 2004., 2004Ram M. Kandimalla +2 more
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Epoch‐Based Model for Stormtime Plasmapause Location
Journal of Geophysical Research: Space Physics, 2019J Goldstein, W S Kurth, S De Pascuale
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Statistical storm time examination of MLT‐dependent plasmapause location derived from IMAGE EUV
Journal of Geophysical Research: Space Physics, 2015D L Gallagher +2 more
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Plasmapause response to geomagnetic storms: CRRES results
Journal of Geophysical Research, 2003Mark B Moldwin +2 more
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A new solar wind‐driven global dynamic plasmapause model: 2. Model and validation
Journal of Geophysical Research: Space Physics, 2017Fei He, Xiaoxin Zhang, M -C Fok
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