Ozone monitoring instrument
This article includes a list of references, related reading or external links, but its sources remain unclear because it lacks inline citations. (October 2012) (Learn how and when to remove this template message)
The ozone monitoring instrument (OMI) is a visual and ultraviolet spectrometer aboard the NASA Aura spacecraft. OMI can distinguish between aerosol types, such as smoke, dust, and sulfates, and can measure cloud pressure and coverage, which provide data to derive tropospheric ozone. OMI follows in the heritage of TOMS, SBUV, GOME, SCIAMACHY, and GOMOS. It is a wide-field-imaging spectrometer with a 114° across-track viewing angle range that provides a 2600 km wide swath, enabling measurements with a daily global coverage. OMI is continuing the TOMS record for total ozone and other atmospheric parameters related to ozone chemistry and climate.
The OMI project was carried out under the direction of the NIVR and financed by the Ministries of Economic Affairs, Transport and Public Works and the Ministry of Education and Science. The instrument was built by Dutch Space in co-operation with Netherlands Organisation for Applied Scientific Research Science and Industry and Netherlands Institute for Space Research. The Finnish industry supplied the electronics. The scientific part of the OMI project is managed by KNMI (principal investigator Prof. Dr. P. F. Levelt), in close co-operation with NASA and the Finnish Meteorological Institute.
- OMI webpage at NASA.gov
- OMI webpage at KNMI.nl
- Tropospheric Emission Monitoring Internet Service (TEMIS)
|This article about one or more spacecraft of the United States is a stub. You can help Wikipedia by expanding it.|
|This climatology/meteorology–related article is a stub. You can help Wikipedia by expanding it.|