Spatial and temporal variations of Jupiter's H3+ emission deduced from image analysis
- 1 July 1999
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 26 (13) , 1789-1792
- https://doi.org/10.1029/1999gl900372
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Thermal structure of Jupiter's atmosphere near the edge of a 5‐μm hot spot in the north equatorial beltJournal of Geophysical Research, 1998
- JIM: A time‐dependent, three‐dimensional model of Jupiter's thermosphere and ionosphereJournal of Geophysical Research, 1998
- Mid-to-Low Latitude H+3Emission from JupiterIcarus, 1997
- A Baseline Spectroscopic Study of the Infrared Auroras of JupiterIcarus, 1997
- Emission Source Model of Jupiter's H+3Aurorae: A Generalized Inverse Analysis of ImagesIcarus, 1996
- Interpretation of Auroral “Lightcurves” with Application to Jovian H+3EmissionsIcarus, 1996
- Solar Wind Control of Jupiter's H+3AurorasIcarus, 1996
- Four micron high-resolution spectra of Jupiter in the North Equatorial Belt: H3+ emissions and the 12C/13C ratioPlanetary and Space Science, 1994
- Latitudinal Temperature Variations of Jovian H+3Icarus, 1994
- Electron precipitation and related aeronomy of the Jovian thermosphere and ionosphereJournal of Geophysical Research, 1983