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The connection between the radio emission from “lightningsproduced by the absorption of high-energy photons from the cosmic gamma-ray background in a neutron star magnetosphere and radio bursts from...
There is a constant flow of electrons ions and into and out of the magnetosphere and the intricacies of the magnetosphere determine the paths that these particles take through it. Although the plasma ...
An optimal approach reducing the population of MeV electrons in the magnetosphere is presented. Under a double resonance condition, whistler wave is simultaneously in cyclotron resonance with keV and ...
The Imaging Proton Spectrometer (IPS) and the Imaging Electron Spectrometer (IES) on the Polar satellite have measured temporary deviations in the isotropy of the pitch angle distributions (PADs) of c...
The possibility of quasi-stable trapping of charged particles of hundreds keV to MeV energy on the frontside Earth magnetosphere is explored in by numerical modeling of the single particle orbits in t...
The variation of the charge state of iron [Fe] ions is used to trace volume elements of plasma in the solar wind into the magnetosphere and to determine the time scales associated with the entry into ...
The RAPID/CLUSTER is an advanced ion spectrometer with a position sensitive time-of-flight (T) and energy (E) detection system which determines the mass of incident energetic ions. The energy range ex...
A possible cusp acceleration mechanism has been investigated during a major geomagnetic storm on May 4, 1998 when the magnetosphere was compressed and eroded. At 5:00–12:05 UT, the WIND spacecraft was...
A statistical study of butterfly pitch angle distributions (PADs) in the outer magnetosphere was carried out using data from the medium energy particle experiment (MEPE) on-board ISEE 1. Protons rangi...
The Charge and Mass Magnetospheric Ion Composition Experiment (CAMMICE) on board the Polar spacecraft observed 75 energetic particle events in 1996 while the satellite was at apogee. All of these even...

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