Observations of ions of ionospheric origin in the storm‐time ring current
- 1 October 1977
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 4 (10), 403-406
- https://doi.org/10.1029/gl004i010p00403
Abstract
No abstract availableThis publication has 13 references indexed in Scilit:
- Observation of an ionospheric acceleration mechanism producing energetic (keV) ions primarily normal to the geomagnetic field directionJournal of Geophysical Research, 1977
- A search for helium ions in the recovery phase of a magnetic stormJournal of Geophysical Research, 1977
- The inconsistency between proton charge exchange and the observed ring current decayJournal of Geophysical Research, 1976
- Evidence that the recovery phase ring current consists of helium ionsJournal of Geophysical Research, 1976
- Satellite observations of an ionospheric acceleration mechanismGeophysical Research Letters, 1976
- The morphology of energetic O+ions during two magnetic storms: Temporal variationsJournal of Geophysical Research, 1976
- Ring current proton decay by charge exchangeJournal of Geophysical Research, 1976
- Protons as the prime contributors to storm time ring currentJournal of Geophysical Research, 1975
- Satellite observations of energetic heavy ions during a geomagnetic stormJournal of Geophysical Research, 1972
- Solar wind ions:56Fe+8to56Fe+12,28Si+7,28Si+8,28Si+9, and16O+6Journal of Geophysical Research, 1970