Balmer profiles in the geocorona and interstellar space: I. Asymmetries due to fine structure
- 30 June 1987
- Vol. 70 (3) , 476-482
- https://doi.org/10.1016/0019-1035(87)90089-3
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Geocoronal structure: 3. Optically thin, Doppler-broadened line profilesJournal of Geophysical Research, 1987
- Simultaneous Hα line profile and radar measurements at AreciboJournal of Geophysical Research, 1986
- Measurements of the spectral profile of Balmer alpha emission from the hydrogen geocoronaGeophysical Research Letters, 1980
- Interpretation of OGO-5 line shape measurements of Lyman-α emission from terrestrial exospheric hydrogenPlanetary and Space Science, 1978
- Spectral line profiles for a planetary coronaJournal of Geophysical Research, 1976
- Direct measurement of hydrogen density at exobase level and exospheric temperatures from Lyman α line shape and polarization, 1. Physical background and first results on day sideJournal of Geophysical Research, 1975
- Doppler profile measurements of the geocoronal hydrogen Balmer alpha lineJournal of Geophysical Research, 1975
- Interpretation of Ogo 5 Lyman alpha measurements in the upper geocoronaJournal of Geophysical Research, 1973
- Planetary coronae and atmospheric evaporationPlanetary and Space Science, 1963
- Interplanetary Gas. I. Hydrogen Radiation in the Night Sky.The Astrophysical Journal, 1959