1994
DOI: 10.1006/jmsp.1994.1132
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Precision broadband Spectroscopy in the Terahertz Region

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Cited by 123 publications
(69 citation statements)
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“…Individual transitions have been recorded with the Cologne Terahertz Spectrometer (CTS) which has been described in detail by Winnewisser et al (1994). It uses broadband tunable, phase-locked backward-wave oscillators (BWOs) as powerful sources, and a magnetically tuned, liquid helium cooled hotelectron InSb bolometer as detector.…”
Section: Methodsmentioning
confidence: 99%
“…Individual transitions have been recorded with the Cologne Terahertz Spectrometer (CTS) which has been described in detail by Winnewisser et al (1994). It uses broadband tunable, phase-locked backward-wave oscillators (BWOs) as powerful sources, and a magnetically tuned, liquid helium cooled hotelectron InSb bolometer as detector.…”
Section: Methodsmentioning
confidence: 99%
“…For details of the spectrometer see e. g. [4], A 4.4 m long free-space cell of Duran glass was filled with the sample gas of about 3 Pa. The transmission intensity was measured by a liquid-He-cooled InSb detector.…”
mentioning
confidence: 99%
“…
We have employed the Cologne terahertz spectrometer [ 1,2] to observe Lamb dip and crossover phenomena in rotational spectra at 572 GHz. Because of the large power output of the backward wave oscillators used in the system, no special means are required to induce this saturation effect; the coincidentally reflected radiation from the bolometer present in our quasi-optical absorption cell is sufficient to saturate the v, = 0 sub-group.
…”
mentioning
confidence: 99%
“…We have met the Lamb dip requirements in our submillimeterwave laboratory using the backward wave oscillator (BWO)-based spectrometer system described in previous publications [1,2], The high power provided by the BWOs employed is suffi cient at 570 GHz to saturate rotational transitions of ammonia without the use of resonant cavities. The backward-traveling radiation is caused by reflections from various optical surfaces of the spectrometer, and it seems clear that the majority of the reflected power comes from the detector.…”
mentioning
confidence: 99%
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