OMTI Spectral Airglow Temperature Imager (SATI) at Shigaraki, Japan

2014-09-22 01:00:00

Optical Mesosphere Thermosphere Imagers (OMTIs) Spectral Airglow Temperature Imager (SATI) Data. The SATI measures airglow rotational temperature and airglow intensity in the mesopause region at 80-100km altitudes through the OH and O2 airglow emission lines. For more information, see http://stdb2.isee.nagoya-u.ac.jp/omti/. Digital data are available upon request to PI.

PI: Kazuo Shiokawa, Institute for Space-Earth Environmental Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601, Japan Rules of the Road for OMTI FPI Data Use: 1. Please contact the Principal Investigator (PI), K. Shiokawa (shiokawa at isee.nagoya-u.ac.jp), ISEE, Nagoya University before using the data at any publications and/or presentations. 2. Please cite Shiokawa et al. (2004) in the publication. The detailed citation is: *Shiokawa, K., Y. Otsuka, T. Ogawa, H. Takahashi, T. Nakamura, and T. Shimomai, Comparison of OH rotational temperatures measured by the Spectral Airglow Temperature Imager (SATI) and by a tilting-filter photometer, J. Atmos. Solar-Terr. Phys., 66, 891-897, 2004.

	Role	Person	StartDate	StopDate	Note
1.	PrincipalInvestigator	spase://IUGONET/Person/Kazuo.Shiokawa
2.	CoInvestigator	spase://IUGONET/Person/Yuichi.Otsuka
3.	MetadataContact	spase://IUGONET/Person/ISEE.Metadata.Management.Group

Online

Open

GIF

P4M

34.8

34.8

34.8

136.1

136.1

136.1

OH and O2 rotational temperature

Rotational temperature in the mesopause region measured by the OH and O2 airglow emission lines.

K

OH and O2 airglow intensity

OH and O2 airglow intensities in the mesopause region at altitudes of 80-90km and 90-100km, respectively.

Rayleighs