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- W3010063590 abstract "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 ]. When the angular convection velocity is evaluated from the quiet time electric field distribution E3 of McIIwain (1972), L c depends on the local time. Its minimum value is then L C =4.5Near 2400 LT, and the plasmapause shape and position satisfactorily fit the observations. The diffusive equilibrium dnesity distribution appropriated inside the plasmasphere, becomes convectively unstable beyond L = L c , where the collisions type of model satisfactorily represents the observations. In the intermediate region between the plasmapause and the last closed magnetic field line, contimues ionization fluxes are expected to flow out of the midlatitude ionosphere" @default.
- W3010063590 created "2020-03-13" @default.
- W3010063590 creator A5031754993 @default.
- W3010063590 date "2018-01-30" @default.
- W3010063590 modified "2023-09-23" @default.
- W3010063590 title "The ROCHE-LIMIT of ionospheric plasma and the formation of the plasmapause" @default.
- W3010063590 doi "https://doi.org/10.18758/a_122" @default.
- W3010063590 hasPublicationYear "2018" @default.
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