Paper
13 September 1994 Global Ozone Monitoring Experiment (GOME): spectrometer for ozone monitoring from space
Andrea Mariani, Enrico Corpaccioli, M. Fibbi, R. Veratti, Achim R. Hahne, Joerg Callies, Alain Lefebvre
Author Affiliations +
Abstract
Global Ozone Monitoring Experiment (GOME) is a grating spectrometer designed to monitor from the ESA satellite ERS-2 absorption by ozone and trace gases in the earth atmosphere. The instrument works in the spectral range 240-790 nm, with a spectral resolution of 0.2 nm and a spatial resolution of 40 X 40 km2. GOME makes use of high density holographic gratings as dispersing elements, and cooled photodiode arrays of 1024 pixels as detectors. Its characteristics, as well as the in flight calibration means, permit to use both differential optical absorption spectrometry and backscattering in the ultra-violet as retrieval methods. This paper describes the main features of the instrument, the results of the test campaign performed on the engineering model and the concepts adopted for ground and in- flight calibration.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrea Mariani, Enrico Corpaccioli, M. Fibbi, R. Veratti, Achim R. Hahne, Joerg Callies, and Alain Lefebvre "Global Ozone Monitoring Experiment (GOME): spectrometer for ozone monitoring from space", Proc. SPIE 2209, Space Optics 1994: Earth Observation and Astronomy, (13 September 1994); https://doi.org/10.1117/12.185298
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Calibration

Sensors

Ozone

Lamps

Spectroscopy

Diffusers

Sun

RELATED CONTENT

GOME 2 the ozone instrument onboard the...
Proceedings of SPIE (December 12 2003)
New generation of GOME instruments
Proceedings of SPIE (February 08 2002)
GOME-2 ozone instrument onboard the European METOP satellites
Proceedings of SPIE (September 15 2004)
Slit function measurement optical stimulus
Proceedings of SPIE (April 08 2003)
First results from GLI’s solar calibration
Proceedings of SPIE (November 10 2003)

Back to Top