Jupiter's dayglow H Ly α emission line profile
- 1 November 1991
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 18 (11), 1935-1938
- https://doi.org/10.1029/91gl02091
Abstract
No abstract availableThis publication has 10 references indexed in Scilit:
- An unusual change in the Jovian Lyman‐alpha bulgeGeophysical Research Letters, 1991
- The center to limb variation in Jupiter's H Ly α emissionJournal of Geophysical Research, 1990
- UV resonance line dayglow emissions on Earth and JupiterJournal of Geophysical Research, 1988
- The excitation of the far ultraviolet electroglow emissions on Uranus, Saturn, and JupiterJournal of Geophysical Research, 1987
- An explanation for the H Ly α longitudinal asymmetry in the equatorial spectrum of Jupiter: An outcrop of paradoxical energy deposition in the exosphereJournal of Geophysical Research, 1985
- IUE monitoring of the spatial distribution of the H Ly-alpha emission from JupiterThe Astrophysical Journal, 1981
- The Jovian hydrogen bulge: Evidence for co-rotating magnetospheric convectionPlanetary and Space Science, 1981
- Equatorial anomaly in the Jovian ionosphereGeophysical Research Letters, 1981
- Copernicus measurements of the Lyman-alpha albedo of JupiterThe Astrophysical Journal, 1980
- Search for Jovian auroral hot spotsThe Astrophysical Journal, 1977