New sources for the hot oxygen geocorona: Solar cycle, seasonal, latitudinal, and diurnal variations
Open Access
- 20 September 1995
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 100 (A9), 17377-17388
- https://doi.org/10.1029/95ja00895
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- Sounding rocket observation of a hot atomic oxygen geocoronaJournal of Geophysical Research, 1993
- Reevaluation of the O+(²P) reaction rate coefficients derived from Atmosphere Explorer C observationsJournal of Geophysical Research, 1993
- On the escape of oxygen and hydrogen from MarsGeophysical Research Letters, 1993
- Energy distribution of energetic O+ precipitation into the atmosphereJournal of Geophysical Research, 1992
- The generation of O(1S) from the dissociative recombination of O+2The Journal of Chemical Physics, 1991
- The fast atomic oxygen corona extent of MarsGeophysical Research Letters, 1990
- Hot oxygen geocorona as inferred from neutral exospheric models and mass spectrometer measurementsJournal of Geophysical Research, 1989
- MSIS‐86 Thermospheric ModelJournal of Geophysical Research, 1987
- The quenching rate of O(1D) by O(3P)Planetary and Space Science, 1986
- The role of energetic O+ precipitation in a mid‐latitude auroraJournal of Geophysical Research, 1986