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Presence of cavity resonances in the inner magnetosphere

2020
<p>In the inner magnetosphere there are sharp plasma boundaries that can cause resonance cavities. The four Cluster satellites move in a string-of-pearls configuration at perigee (at L=4-5) so that they are spatially well separated but their separation is still short that at least some of them are simultaneously at different ...
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Solar Particle Access into the Inner Magnetosphere

1974
There are four modes of access of energetic particles into the inner magnetosphere, defined here as the region of ‘closed’ field lines, i.e. regions of latitude below, for instance, the 40 keV electron boundary. These are direct entry to all latitudes above the cut-off, longitudinal drift from the nightside to the dayside pseudotrapping region, radial ...
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Simulation of Centrifugally Driven Convection in Jovian Inner Magnetosphere Using the Rice Convection Model

Journal of Geophysical Research: Space Physics, 2023
Yuxian Wang, Jian Yang, X C Guo
exaly  

Electric and magnetic field observations of Pc4 and Pc5 pulsations in the inner magnetosphere: A statistical study

Journal of Geophysical Research, 2009
Wenlong Liu, Xinlin Li, S R Elkington
exaly  

Relativistic electron dynamics in the inner magnetosphere — a review

Journal of Atmospheric and Solar-Terrestrial Physics, 2002
R H W Friedel, G D Reeves, T Obara
exaly  

How the Earth's inner magnetosphere works: An evolving picture

Journal of Atmospheric and Solar-Terrestrial Physics, 2007
R A Wolf, S Sazykin, F R Toffoletto
exaly  

Source and loss processes in the inner magnetosphere

Space Science Reviews, 1999
M. Blanc   +8 more
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