Abstract
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.
| Original language | English |
|---|---|
| Article number | 59621L |
| Journal | Proceedings of SPIE - The International Society for Optical Engineering |
| Volume | 5962 |
| Issue number | 2 |
| DOIs | |
| State | Published - 2005 |
| Event | Optical Design and Engineering II - Gena, Germany Duration: Sep 13 2005 → Sep 16 2005 |
Keywords
- Calibration
- Charge coupled devices
- Remote sensing
- Ultraviolet spectroscopy