Design and fabrication of a 800-900 GHz Pb-alloy SIS mixing device incorporating an on-substrate tuning element

Tame, Keith and Price, Mark C. and Little, L.T. (1998) Design and fabrication of a 800-900 GHz Pb-alloy SIS mixing device incorporating an on-substrate tuning element. In: Phillips, Thomas G., ed. Advanced Technology MMW, Radio, and Terahertz Telescopes. Proceedings of the Society of Photo-Optical InstrumentationNSTRUMENTATION ENGINEERS (SPIE), 3357. Spie-Int Soc Optical Engineering, Bellingham, USA pp. 63-74. ISBN 0-8194-2804-3. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided)

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Official URL
http://dx.doi.org/10.1117/12.317394

Abstract

The use of SIS (Superconductor-Insulator-Superconductor) devices as the mixing element in ultra-sensitive heterodyne receivers for use in radio astronomy is well established. In attempting to exploit the last main submillimetre atmospheric window we are developing a Pb-alloy SIS mixer to work in the frequency band 800-900 GHz. In this paper we address some of the problems with working at frequencies above the energy gap of a superconducting alloy. We also present initial results obtained from Pb-alloy SIS junctions fabricated at the University of Kent at Canterbury (UKC).

Item Type: Conference or workshop item (Paper)
Additional information: Proceedings paper.
Uncontrolled keywords: SIS receiver; quasiparticle mixer; submillimetre waves; radio astronomy; superconducting microstrip
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculties > Science Technology and Medical Studies > School of Engineering and Digital Arts
Faculties > Science Technology and Medical Studies > School of Physical Sciences > Optics
Depositing User: Tara Puri
Date Deposited: 04 Jun 2009 09:27
Last Modified: 04 Jun 2014 08:42
Resource URI: https://kar.kent.ac.uk/id/eprint/17186 (The current URI for this page, for reference purposes)
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