Phillips, T. G. (1994) THz source requirements for astrophysics receivers. In: Nonlinear Optics for High-Speed Electronics and Optical Frequency Conversion. Proceedings of SPIE. No.2145. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 230-238. ISBN 0-8194-1440-9. https://resolver.caltech.edu/CaltechAUTHORS:20161019-143102015
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Abstract
A discussion is given of current and projected needs for local oscillators for submillimeter and terahertz receivers used in astrophysical and astrochemical applications. Arguments are given for frequency range, tunability, power, and noise specifications for local oscillators in various applications. The receivers will generally employ SIS or Schottky diode mixers, and these may be used in single elements, receiver arrays or aperture synthesis interferometry, each of which has differing requirements. The platforms may be ground-based, probably on high mountain sites, balloons, air or space-based, again each demanding somewhat varying local oscillator capabilities.
Item Type: | Book Section | |||||||||
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Alternate Title: | Terahertz source requirements for astrophysics receivers | |||||||||
Additional Information: | © 1994 The International Society for Optical Engineering, SPIE. | |||||||||
Series Name: | Proceedings of SPIE | |||||||||
Issue or Number: | 2145 | |||||||||
DOI: | 10.1117/12.177147 | |||||||||
Record Number: | CaltechAUTHORS:20161019-143102015 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20161019-143102015 | |||||||||
Official Citation: | Thomas G. Phillips; Terahertz source requirements for astrophysics receivers. Proc. SPIE 2145, Nonlinear Optics for High-Speed Electronics and Optical Frequency Conversion, 230 (June 2, 1994); doi:10.1117/12.177147. | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 71293 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | Ruth Sustaita | |||||||||
Deposited On: | 19 Oct 2016 22:17 | |||||||||
Last Modified: | 11 Nov 2021 04:42 |
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