Results 1 to 10 of about 2,961 (224)
Plasmapause surface wave oscillates the magnetosphere and diffuse aurora [PDF]
Theoretical studies suggested that plasmapause surface waves related to the sharp inhomogeneity exist and act as a source of geomagnetic pulsations.
Fei He +15 more
doaj +2 more sources
Prediction of Dynamic Plasmapause Location Using a Neural Network
As a common boundary layer that distinctly separates the regions of high‐density plasmasphere and low‐density plasmatrough, the plasmapause is essential to comprehend the dynamics and variability of the inner magnetosphere.
Deyu Guo +11 more
doaj +2 more sources
Empirical plasmapause models from magnetic indices [PDF]
We use a database of CRRES in situ observations of plasmapause crossings to build empirical models of the plasmapause location as a function of geomagnetic indices. Previous models used the maximum value in Kp during the hours to days leading up to the plasmapause crossing.
Thomas Obrien
exaly +3 more sources
We present observational support for whistler mode waves guidance by the plasmapause gradients based on a case study and statistical analyses. Due to the combined effects of inhomogeneous magnetic fields and plasma densities, whistler mode waves near the
Rui Chen +4 more
doaj +1 more source
The Plasmasphere Boundary Layer [PDF]
As an inner magnetospheric phenomenon the plasmapause region is of interest for a number of reasons, one being the occurrence there of geophysically important interactions between the plasmas of the hot plasma sheet and of the cool plasmasphere. There
D. L. Carpenter, J. Lemaire, J. Lemaire
doaj +1 more source
Improving Predictions of the 3D Dynamic Model of the Plasmasphere
In this perspective paper, we review and discuss different ways that can be used to improve the predictions of the models of the plasmaspheric region. The density of the background cold plasma and the plasmapause position are very important to determine ...
Viviane Pierrard +3 more
doaj +1 more source
The plasmapause marks the limit of the plasmasphere and is characterized by a sudden change in plasma density. This can influence the other regions of the magnetosphere, including due to different waves circulating inside and outside the plasmasphere. In
V. Pierrard +8 more
doaj +1 more source
Plasmapause formation at Saturn [PDF]
AbstractCassini observations during a rapid, high‐latitude, dawnside pass from Saturn's lobe to inner magnetosphere on 25 June 2009 provide strong evidence for the formation of a “plasmapause” at Saturn by Vasyliunas‐type nightside reconnection of previously mass‐loaded flux tubes.
M. F. Thomsen +5 more
openaire +4 more sources
Van Allen Probes Observations of Oxygen Ions at the Geospace Plume
The geospace plume couples the ionosphere, plasmasphere, and magnetosphere from sub-auroral regions to the magnetopause, on polar field lines, and into the magnetotail.
John C. Foster, Philip J. Erickson
doaj +1 more source
Ionospheric and magnetospheric “plasmapauses” [PDF]
Abstract During August 1972, Explorer 45 orbiting near the equatorial plane with an apogee of ∼5.2 R e traversed magnetic field lines in close proximity to those simultaneously traversed by the topside ionospheric satellite ISIS 2 near dusk in the L range 2.0–5.4.
Joseph M. Grebowsky +2 more
openaire +1 more source

