The Ozone Monitoring Instrument (OMI) was launched on 15 July 2004 on NASA’s EOS AURA satellite. The OMI instrument is an ultraviolet-visible imaging spectrograph that uses two-dimensional CCD detectors to register both the spectrum and the swath perpendicular to the flight direction with a 115 degrees wide swath, which enables global daily ground coverage with high spatial resolution. This paper presents a number of in-flight radiometric and spectral instrument performance and calibration results.
MR Dobber, R Dirksen, PF Levelt, GHJ van den Oord, R Voors, Q Kleipool, G Jaross, M Kowalewski. Ozone Monitoring Instrument in-flight performance and calibration
Conference: Optical Systems Design 2005, Organisation: SPIE, Place: Jena, Germany, Year: 2005, First page: 0, Last page: 0