Entropy mapping of the outer electron radiation belt between the magnetotail and geosynchronous orbit
- 28 June 2011
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 116 (A6)
Abstract
No abstract availableKeywords
This publication has 124 references indexed in Scilit:
- Tracing solar wind plasma entry into the magnetosphere using ion‐to‐electron temperature ratioGeophysical Research Letters, 2009
- Simulation of the outer radiation belt electrons near geosynchronous orbit including both radial diffusion and resonant interaction with Whistler‐mode chorus wavesGeophysical Research Letters, 2005
- Solar wind stream interaction regions without sector boundariesJournal of Geophysical Research, 2004
- Solar wind electron characteristics inside and outside coronal mass ejectionsJournal of Geophysical Research, 2000
- On the determination of electron polytrope indices within coronal mass ejections in the solar windJournal of Geophysical Research, 1999
- Identification of trailing edge solar wind stream interfaces: A comparison of Ulysses plasma and composition measurementsJournal of Geophysical Research, 1999
- Central plasma sheet ion properties as inferred from ionospheric observationsJournal of Geophysical Research, 1998
- Plasma sheet polytropic index as inferred from the FPE measurementsGeophysical Research Letters, 1990
- The variation of the plasma sheet polytropic index along the midnight meridian in a finite width magnetotailGeophysical Research Letters, 1990
- Particle acceleration during substorm growth and onsetGeophysical Research Letters, 1990