Interpretation of OGO-5 line shape measurements of Lyman-α emission from terrestrial exospheric hydrogen
- 31 May 1978
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 26 (5), 431-447
- https://doi.org/10.1016/0032-0633(78)90065-x
Abstract
No abstract availableThis publication has 14 references indexed in Scilit:
- Charge exchange in a planetary corona: Its effect on the distribution and escape of hydrogenJournal of Geophysical Research, 1977
- Spectral line profiles for a planetary coronaJournal of Geophysical Research, 1976
- Apollo 16 Lyman alpha imagery of the hydrogen geocoronaJournal 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
- Observed variations of the exospheric hydrogen density with the exospheric temperatureJournal of Geophysical Research, 1975
- Excitation of the Low-Luminosity Balmer Emissions in the GeocoronaThe Astrophysical Journal, 1973
- Interpretation of Ogo 5 Lyman alpha measurements in the upper geocoronaJournal of Geophysical Research, 1973
- Geomagnetic effect on the neutral temperature of theFregion during the magnetic storm of September 1969Journal of Geophysical Research, 1972
- Planetary coronae and atmospheric evaporationPlanetary and Space Science, 1963
- Non-Coherent Scattering: I. The Redistribution Function with Doppler BroadeningMonthly Notices of the Royal Astronomical Society, 1962