2005
DOI: 10.1016/j.asr.2005.02.022
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Waves in airglow structures experiment 2004: Overview and preliminary results

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Cited by 8 publications
(10 citation statements)
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“…In fact, ripple structures were observed in the all‐sky image of the OI 558 nm line at Sata and also appeared in the all‐sky images of the OI 558 nm line and the O 2 atmospheric (0,1) band at Yamagawa. From the volume emission rate measurements of the OI 558 nm line, the O 2 atmospheric (0,0) band at 762 nm, and the OH (6,2) band at 836 nm by Airglow photometer (AGL) on board the rocket [ Iwagami et al , 2005], the main peaks of the OI emission and the O 2 atmospheric band emission are at 97 and 95 km, respectively. The ripple structure is not observed by the all‐sky image of the OH Meinel band, whose main peak is at 90 km.…”
Section: Discussionmentioning
confidence: 99%
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“…In fact, ripple structures were observed in the all‐sky image of the OI 558 nm line at Sata and also appeared in the all‐sky images of the OI 558 nm line and the O 2 atmospheric (0,1) band at Yamagawa. From the volume emission rate measurements of the OI 558 nm line, the O 2 atmospheric (0,0) band at 762 nm, and the OH (6,2) band at 836 nm by Airglow photometer (AGL) on board the rocket [ Iwagami et al , 2005], the main peaks of the OI emission and the O 2 atmospheric band emission are at 97 and 95 km, respectively. The ripple structure is not observed by the all‐sky image of the OH Meinel band, whose main peak is at 90 km.…”
Section: Discussionmentioning
confidence: 99%
“…The second campaign, WAVE2004, was conducted at the same place, Kagoshima, in January 2004. An overview and the initial results of the WAVE2004 campaign have been presented by Iwagami et al [2005], and Kubota et al [2006] presented the result of the detailed data analysis and discussed the source of the AGW.…”
Section: Wave Campaignsmentioning
confidence: 99%
“…This wavelength is quite large as compared to the AGW usually observed by the ASI. According to the rocket‐borne measurement, peak altitude of the emission rate of the OI 557.7‐nm airglow was 97 km at this time [ Iwagami et al , 2005]. Therefore wave parameters obtained from the OI 557.7‐nm airglow observation by the ASI indicate the status of the AGW at around 97 km altitude.…”
Section: Resultsmentioning
confidence: 98%
“…The ground‐based instruments described above were operated simultaneously. An overview and the preliminary results of this experiment have been presented by Iwagami et al [2005].…”
Section: Resultsmentioning
confidence: 99%
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