2003
DOI: 10.1016/j.jastp.2003.08.002
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Rocket observations of atomic oxygen density and airglow emission rate in the WAVE2000 campaign

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Cited by 14 publications
(18 citation statements)
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“…The WAVE2000 campaign was carried out over Kagoshima, Japan, in January 2000. This campaign was planned to study the formation process of wave structures in the airglow image from both dynamical and chemical perspectives [ Iwagami et al , 2002, 2003]. The second campaign, WAVE2004, was conducted at the same place, Kagoshima, in January 2004.…”
Section: Wave Campaignsmentioning
confidence: 99%
“…The WAVE2000 campaign was carried out over Kagoshima, Japan, in January 2000. This campaign was planned to study the formation process of wave structures in the airglow image from both dynamical and chemical perspectives [ Iwagami et al , 2002, 2003]. The second campaign, WAVE2004, was conducted at the same place, Kagoshima, in January 2004.…”
Section: Wave Campaignsmentioning
confidence: 99%
“…Model calculations of chemical species represent characteristics of large‐scale global distributions. Rocket observations of atomic oxygen indicate that the density of the atomic oxygen was often significantly perturbed by the passage of an atmospheric gravity wave or tide, and by the subsequent convective or dynamical instabilities induced by superposition of that wave [ Iwagami et al , 2003; Howlett et al , 1980; Melo et al , 1996; Hecht et al , 2004]. So, the density of atomic oxygen used in the temperature retrieval can be quite different from the local oxygen profile over the lidar site or rocket trajectory.…”
Section: Database Used and Analysis Proceduresmentioning
confidence: 99%
“…2.2 557.7-nm all-sky camera and Fabry-Perot interferometer An all-sky CCD imager for measuring OI 557.7-nm airglow in the lower thermosphere has been operated at Shigaraki to obtain two-dimensional airglow intensity maps (512×512 pixels) every 5.5 min with an exposure time of 105 s (Shiokawa et al, 1999). As the 557.7-nm emission occurs mostly at altitudes of 90-100 km with its peak intensity at around 96 km (McDade et al, 1986;Iwagami et al, 2003), we assume the emission altitude of 96 km in this paper. A Fabry-Perot interferometer (FPI) has also been operated at Shigaraki to measure the Doppler shift of 557.7-nm emission at zenith angles of 50 • ±4.75 • and at four azimuthal directions of N, S, E, and W, every 15 min, and to obtain neutral wind speed for the first and second fringes independently (Shiokawa et al, 2001).…”
Section: The Mu Radarmentioning
confidence: 99%