5 September 2017 The Sentinel-4 detectors: architecture and performance
Author Affiliations +
Abstract
The Sentinel-4 instrument is an imaging spectrometer, developed by Airbus under ESA contract in the frame of the joint European Union (EU)/ESA COPERNICUS program. SENTINEL-4 will provide accurate measurements of trace gases from geostationary orbit, including key atmospheric constituents such as ozone, nitrogen dioxide, sulfur dioxide, formaldehyde, as well as aerosol and cloud properties. Key to achieving these atmospheric measurements are the two CCD detectors, covering the wavelengths in the ranges 305 nm to 500 nm (UVVIS) and 750 to 775 nm (NIR) respectively. The paper describes the architecture, and operation of these two CCD detectors, which have an unusually high full-well capacity and a very specific architecture and read-out sequence to match the requirements of the Sentinel- 4 instrument. The key performance aspects and their verification through measurement are presented, with a focus on an unusual, bi-modal dark signal generation rate observed during test.
Conference Presentation
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael P. Skegg, Michael P. Skegg, Markus Hermsen, Markus Hermsen, Rüdiger Hohn, Rüdiger Hohn, Christian Williges, Christian Williges, Charles Woffinden, Charles Woffinden, Yves Levillain, Yves Levillain, Ralf Reulke, Ralf Reulke, } "The Sentinel-4 detectors: architecture and performance", Proc. SPIE 10402, Earth Observing Systems XXII, 1040218 (5 September 2017); doi: 10.1117/12.2274362; https://doi.org/10.1117/12.2274362
PROCEEDINGS
8 PAGES + PRESENTATION

SHARE
RELATED CONTENT

SAGE III measurements
Proceedings of SPIE (September 23 2002)
Overview of the SAGE III experiment
Proceedings of SPIE (October 19 1999)

Back to Top