Abundances and spectra of suprathermal H+, He++ and heavy ions in a fast moving plasma structure (plasmoid) in the distant Geotail
- 1 June 1984
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 11 (6), 603-606
- https://doi.org/10.1029/gl011i006p00603
Abstract
No abstract availableThis publication has 18 references indexed in Scilit:
- Energetic ion regimes in the deep geomagnetic tail: ISEE‐3Geophysical Research Letters, 1984
- Structure of the magnetotail at 220 RE and its response to geomagnetic activityGeophysical Research Letters, 1984
- Plasma regimes in the deep geomagnetic tail: ISEE 3Geophysical Research Letters, 1983
- Plasma behavior during energetic electron streaming events: Further evidence for substorm‐associated magnetic reconnectionGeophysical Research Letters, 1982
- A new trajectory concept for exploring the earth's geomagnetic tailJournal of Guidance and Control, 1981
- Observed distribution functions of H, He, C, O, and Fe in corotating energetic particle streams - Implications for interplanetary acceleration and propagationThe Astrophysical Journal, 1979
- Transient phenomena in the magnetotail and their relation to substormsSpace Science Reviews, 1979
- The Nuclear and Ionic Charge Distribution Particle Experiments on the ISEE-1 and ISEE-C SpacecraftIEEE Transactions on Geoscience Electronics, 1978
- Solar wind heavy ion abundancesSolar Physics, 1975
- Energy spectra and angular distributions of particles in the plasma sheet and their comparison with rocket measurements over the auroral zoneJournal of Geophysical Research, 1971