DocumentCode
1142473
Title
High-performance detector read-out at very low temperatures
Author
Eggel, H. ; Schaap, H.P.
Author_Institution
ESA/ESTEC, Noordwijk, Netherlands
Volume
4
Issue
3
fYear
1992
fDate
6/1/1992 12:00:00 AM
Firstpage
103
Lastpage
106
Abstract
An infra-red detection system must be physically colder than the objects it needs to observe. As some of the objects to be observed by the European Space Agency´s Infra-red Space Observatory (ISO) might be as cold as a few tens of degrees Kelvin, it is essential that the ISO´s detectors should themselves operate at temperatures close to absolute zero. To avoid problems with electromagnetic interference, it is also necessary that detector read-out (i.e. first-stage signal amplification) be located as close as possible to the detectors. As conventional amplifiers cannot work at temperatures close to absolute zero, special techniques had to be used for the ISO´s detectors
Keywords
artificial satellites; astronomical instruments; infrared astronomy; infrared detectors; instrumentation; low-temperature techniques; ESA; European Space Agency; ISO; Infra-red Space Observatory; detector read-out; electromagnetic interference; first-stage signal amplification; infra-red detection system; very low temperatures;
fLanguage
English
Journal_Title
Electronics & Communication Engineering Journal
Publisher
iet
ISSN
0954-0695
Type
jour
Filename
149841
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