On determining the ozone number density distribution from OAO-2 stellar occultation measurements
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference6 articles.
1. Distribution of atomic oxygen in the upper atmosphere deduced from OGO-6 airglow observations;Donahue;J. geophys. Res.,1973
2. Observation of mesospheric ozone at low latitudes;Hays;Planet. Space Sci.,1973
3. Atomic oxygen densities in the lower thermosphere as derived from in situ 5577-A night airglow and mass spectrometer measurements;Offermann;J. geophys. Res.,1973
4. A technique for recovering the vertical number density profile of atmospheric gases from planetary occultation data;Roble;Planet. Space Sci.,1972
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1. Oxygen and Air Density Retrieval Method for Single-Band Stellar Occultation Measurement;Remote Sensing;2024-06-03
2. Satellite observations of daytime and nighttime ozone in the mesosphere and lower thermosphere;Journal of Geophysical Research: Atmospheres;2003-05-07
3. The long-term trend of ozone at heights from 80 to 100 km at the mid-latitude mesopause for the nocturnal conditions;Physics and Chemistry of the Earth, Parts A/B/C;2002-01
4. Radiative transfer of atomic and molecular resonant emissions in the upper atmospheres. II. The 9.6 micrometer emission of atmospheric ozone.;Journal of geomagnetism and geoelectricity;1977
5. Ozone measurements between 90 and 110 km altitude by mass spectrometer;Geophysical Research Letters;1975-03
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