The tilting photometer (No.1) settled at Shigaraki Observatory, which is a part of the Optical Mesosphere Thermosphere Imagers (OMTIs), meaures airglow emissions at OH (846.5 nm and 843 nm) lines in every 10-minutes and OI (557.7 nm) line in every 1-minute. This meridian-scanning is for five zenith angles from -74.88 (deg., northward) to +74.88 (deg., southward). Line spectra at the scan angle of 0 (deg., zenith) is also obtained every hour. It starts observation in 1998 and continues observation. The OMTIs were developed at the Institute for Space-Earth Environmental Research, Nagoya University, in order to investigate the dynamics of the upper atmosphere through nocturnal airglow emissions.
Version:2.5.0
The tilting photometer (No.1) settled at Shigaraki Observatory, which is a part of the Optical Mesosphere Thermosphere Imagers (OMTIs), meaures airglow emissions at OH (846.5 nm and 843 nm) lines in every 10-minutes and OI (557.7 nm) line in every 1-minute. This meridian-scanning is for five zenith angles from -74.88 (deg., northward) to +74.88 (deg., southward). Line spectra at the scan angle of 0 (deg., zenith) is also obtained every hour. It starts observation in 1998 and continues observation. The OMTIs were developed at the Institute for Space-Earth Environmental Research, Nagoya University, in order to investigate the dynamics of the upper atmosphere through nocturnal airglow emissions.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | PrincipalInvestigator | spase://IUGONET/Person/Kazuo.Shiokawa | |||
| 2. | CoInvestigator | spase://IUGONET/Person/Yuichi.Otsuka | |||
| 3. | MetadataContact | spase://IUGONET/Person/Akiyo.Yatagai | |||
| 4. | MetadataContact | spase://IUGONET/Person/ISEE.Metadata.Management.Group |
Detailed description of OMTIs and quick-look data are available. All the plotted data and images are just for browsing purpose and are not fully calibrated. Please do not use the data at any presentations and publications without contacting the PI.