Abstract
The Ozone Monitoring Instrument is an UV-Visible imaging spectrograph using two-dimensional CCD detectors to register both the spectrum and the swath perpendicular to the flight direction. This allows having a wide swath (114 degrees) combined with a small ground pixel (nominally 13×24 km 2). The instrument is planned for launch on NASA's EOS-AURA satellite in January 2004. The on-ground calibration measurement campaign of the instrument was performed May-October 2002, data is still being analyzed to produce the calibration key data set. The paper highlights selected topics from the calibration campaign, the radiometric calibration, spectral calibration including a new method to accurately calibrate the spectral slitfunction and results from the zenith sky measurements and gas cell measurements that were performed with the instrument.
| Original language | English |
|---|---|
| Pages (from-to) | 400-410 |
| Number of pages | 11 |
| Journal | Proceedings of SPIE - The International Society for Optical Engineering |
| Volume | 5234 |
| DOIs | |
| State | Published - 2004 |
| Event | Sensors, Systems and Next-Generation Satellites VII - Barcelona, Spain Duration: Sep 8 2003 → Sep 10 2003 |
Keywords
- Calibration
- Imaging spectrograph
- Remote sensing
- Trace gases
- UV-Visible