Exospheric temperatures deduced from 7320‐ to 7330‐Å (O+(²P) ‐ O+(²D)) twilight observations
- 1 February 1982
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 87 (A2) , 913-918
- https://doi.org/10.1029/ja087ia02p00913
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- The O II(7320‐7330Å) airglow: A morphological studyJournal of Geophysical Research, 1981
- Airglow measurements of the variation of the O+(²P) ionization frequency during solar cycle 21Geophysical Research Letters, 1980
- Ionization frequencies for major thermospheric constituents as a function of solar cycle 21Geophysical Research Letters, 1979
- Changes in thermospheric composition inferred from twilight O+(2P) emissionPlanetary and Space Science, 1979
- Intercalibration of airglow observatories with the atmosphere explorer satellitePlanetary and Space Science, 1977
- The neutral‐atmosphere temperature instrumentRadio Science, 1973
- A Technique for Recovering Doppler Line Profiles from Fabry-Perot Interferometer Fringes of Very Low IntensityApplied Optics, 1971
- Fluorescence of solar ionizing radiationPlanetary and Space Science, 1963
- Relative [o II] Intensities in Gaseous Nebulae.The Astrophysical Journal, 1957
- Atmospheric Winds and Temperatures to 50-Kilometers Altitude as Determined by Acoustical Propagation StudiesThe Journal of the Acoustical Society of America, 1952