Supersonic-jet cryogenic-resonator coaxially oriented beam-resonator arrangement Fourier transform microwave spectrometer

Research output: Contribution to journalArticleResearchpeer review

Authors

  • Jens Uwe Grabow
  • E. Samuel Palmer
  • Michael C. McCarthy
  • Patrick Thaddeus

External Research Organisations

  • Harvard University
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Details

Original languageEnglish
Article number093106
JournalReview of scientific instruments
Volume76
Issue number9
Publication statusPublished - Sept 2005

Abstract

The design and performance of a cryogenic (T=77 K) microwave spectrometer are reported. This instrument, being a time domain experiment in microwave molecular spectroscopy, consists of three basic components: a near-confocal Fabry-Perot-type resonator, a pulsed microwave excitation Fourier transform system, and a pulsed molecular-beam source in a coaxially oriented beam-resonator arrangement. With the recently developed spectrometer, which employs confocal reflectors cooled to liquid-nitrogen temperature, we were able to reduce the system noise of the instrument significantly. The high sensitivity of this next generation spectrometer allows the detection of transient species produced in a dc-discharge nozzle, other short-lived molecules and complexes at low abundance, or nearly nonpolar molecules. We will discuss the spectrometer design with respect to critical considerations of the resonator theory in the context of cryogenic operation, as well as important aspects of classical circuit theory applied to excitation and detection of molecular systems in a resonator. Following the description of the dc-discharge source, the performance of the instrument is demonstrated.

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Supersonic-jet cryogenic-resonator coaxially oriented beam-resonator arrangement Fourier transform microwave spectrometer. / Grabow, Jens Uwe; Palmer, E. Samuel; McCarthy, Michael C. et al.
In: Review of scientific instruments, Vol. 76, No. 9, 093106, 09.2005.

Research output: Contribution to journalArticleResearchpeer review

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N1 - Funding Information: The authors like to thank the members of their group for help and discussion and their workshop for the numerous mechanical parts. They are especially indebted to Elaine W. Gottlieb for development of the spectrometer software and Carl A. Gottlieb for helpful discussions. Support by the Deutsche Forschungsgemeinschaft (DFG), the Land Niedersachsen, the Department of Energy (DOE), and the National Air and Space Administration (NASA) is gratefully acknowledged.

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