DocumentCode
474008
Title
Terahertz heterodyne technology for astronomy and planetary science
Author
Wild, Wolfgang
Author_Institution
SRON Netherlands Inst. for Space Res., Groningen
fYear
2007
fDate
2-9 Sept. 2007
Firstpage
323
Lastpage
325
Abstract
Heterodyne detection techniques play an important role in high-resolution spectroscopy in astronomy and planetary science. In particular, heterodyne technology in the Terahertz range has rapidly evolved in recent years. Cryogenically cooled receivers approaching quantum-limited sensitivity have been developed up to 2 THz for large astronomy projects like ESA´s Herschel Space Observatory and the Atacama Large Millimeter Array (ALMA) as well as other observing facilities. Future space- and ground-based submillimeter observatories require heterodyne detectors and receivers up to 6 THz and beyond. Recent developments in superconducting mixer as well as local oscillator technology bring such receivers into reach. This short article summarizes the main technological achievements of Terahertz heterodyne technology, and gives an outlook into future developments.
Keywords
astronomical spectra; astronomical techniques; submillimetre wave receivers; submillimetre wave spectroscopy; astronomy; cryogenically cooled receivers; heterodyne detection techniques; heterodyne detectors; high-resolution spectroscopy; planetary science; quantum-limited sensitivity; terahertz heterodyne technology; Astronomy; Detectors; Frequency; Local oscillators; Millimeter wave technology; Observatories; Space heating; Space technology; Submillimeter wave technology; Superconducting photodetectors; Astronomy; heterodyning; submillimeter wave detectors; submillimeter wave receivers;
fLanguage
English
Publisher
ieee
Conference_Titel
Infrared and Millimeter Waves, 2007 and the 2007 15th International Conference on Terahertz Electronics. IRMMW-THz. Joint 32nd International Conference on
Conference_Location
Cardiff
Print_ISBN
978-1-4244-1438-3
Type
conf
DOI
10.1109/ICIMW.2007.4516517
Filename
4516517
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