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Characterisation of the analogue read-out chain for the CCDs onboard the Mesospheric Airglow/Aerosol Tomography and Spectroscopy (MATS)
KTH, School of Engineering Sciences (SCI), Physics.
KTH, School of Engineering Sciences (SCI), Physics.
KTH, School of Engineering Sciences (SCI), Physics.
Chalmers Univ Technol, Gothenburg, Sweden..
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2018 (English)In: SPACE TELESCOPES AND INSTRUMENTATION 2018: OPTICAL, INFRARED, AND MILLIMETER WAVE / [ed] Lystrup, M MacEwen, HA Fazio, GG, SPIE-INT SOC OPTICAL ENGINEERING , 2018, article id 106984YConference paper, Published paper (Refereed)
Abstract [en]

The MATS satellite aims at observing airglow and noctilucent clouds in the mesosphere. The main instrument consists of a six channels limb imager in the near-ultraviolet and near-infrared. A high signal-to-noise ratio is required for detecting these mesospheric phenomena: 100 and 500 for ultraviolet and infrared, respectively. This is achieved by an optical design minimizing stray-light, but also with a dedicated design of the read-out analogue chain for the CCD on each channel. The requirements and expected light level on the imaging channels are briefly discussed before focusing on the CCD read-out analogue chain, for which the design and performances are presented.

Place, publisher, year, edition, pages
SPIE-INT SOC OPTICAL ENGINEERING , 2018. article id 106984Y
Series
Proceedings of SPIE, ISSN 0277-786X ; 10698
Keywords [en]
CCD, read-out electronics, noise, dark current, MATS
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-240046DOI: 10.1117/12.2313732ISI: 000450864600128Scopus ID: 2-s2.0-85054818871ISBN: 978-1-5106-1950-0 (print)OAI: oai:DiVA.org:kth-240046DiVA, id: diva2:1269215
Conference
Conference on Space Telescopes and Instrumentation - Optical, Infrared, and Millimeter Wave, JUN 10-15, 2018, Austin, TX
Note

QC 20181210

Available from: 2018-12-10 Created: 2018-12-10 Last updated: 2018-12-10Bibliographically approved

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