The distribution of hot hydrogen atoms produced by electron and proton precipitation in the Jovian aurora
- 25 September 1996
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 101 (E9) , 21157-21168
- https://doi.org/10.1029/96je01952
Abstract
No abstract availableKeywords
This publication has 51 references indexed in Scilit:
- Line profile of H Lyman α from dissociative excitation of H2 with application to JupiterJournal of Geophysical Research, 1995
- Kinetic Energy Distribution ofAtoms from Dissociative Excitation ofPhysical Review Letters, 1995
- A kinetic model of the formation of the hot oxygen geocorona: 2. Influence of O+ion precipitationJournal of Geophysical Research, 1995
- Optically thin H Lyman alpha production on outer planets: Low‐energy proton Acceleration in parallel electric fields and neutral H atom precipitation from ring currentJournal of Geophysical Research, 1993
- Doppler shifted H Ly α Emission from Jupiter's auroraGeophysical Research Letters, 1989
- Ultraviolet Spectrometer Observations of UranusScience, 1986
- Studies of extreme-ultraviolet emission from Rydberg series ofby electron impactPhysical Review A, 1984
- Observations from earth orbit and variability of the polar aurora on JupiterThe Astrophysical Journal, 1980
- Extreme Ultraviolet Observations from Voyager 1 Encounter with JupiterScience, 1979
- Transport properties of atomic hydrogenAtomic Data and Nuclear Data Tables, 1971