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Recent Research on the Magnetospheric Plasmapause

Radio Science, 1968
The 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, 1974
Abstract 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, 1976
Values 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., 2004
Ram M. Kandimalla   +2 more
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Epoch‐Based Model for Stormtime Plasmapause Location

Journal of Geophysical Research: Space Physics, 2019
J Goldstein, W S Kurth, S De Pascuale
exaly  

Statistical storm time examination of MLT‐dependent plasmapause location derived from IMAGE EUV

Journal of Geophysical Research: Space Physics, 2015
D L Gallagher   +2 more
exaly  

Plasmapause response to geomagnetic storms: CRRES results

Journal of Geophysical Research, 2003
Mark B Moldwin   +2 more
exaly  

A new solar wind‐driven global dynamic plasmapause model: 2. Model and validation

Journal of Geophysical Research: Space Physics, 2017
Fei He, Xiaoxin Zhang, M -C Fok
exaly  

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