JCMT receiver A2-a 210-280 GHz SIS receiver

Author

Davies, S.R. ; Cunningham, C.T. ; Little, L.T. ; Matheson, D.N.

Author_Institution

Electron. Eng. Lab., Kent Univ., Canterbury

fYear

1992

fDate

33879

Firstpage

42522

Lastpage

42525

Abstract

The most sensitive receivers constructed for short millimetre and sub-millimetre wavelengths use superconductor-insulator-superconductor (SIS) tunnel junctions as the mixing elements. The authors describe the design and performance of a 210-280 GHz SIS heterodyne receiver, which was commissioned on the James Clerk Maxwell Telescope, Hawaii in March 1992. A prototype version of this receiver was tested on the JCMT in May 1992, which was then modified for permanent use on the telescope as a facility instrument

Keywords

mixers (circuits); radio receivers; radiotelescopes; solid-state microwave circuits; submillimetre wave devices; superconducting junction devices; 210 to 280 GHz; EHF; Hawaii; JCMT receiver A2; James Clerk Maxwell Telescope; SIS heterodyne receiver; SIS tunnel junctions; mixing elements; superconductor-insulator-superconductor;

fLanguage

English

Publisher

iet

Conference_Titel

Millimetre and Sub-Millimetre Wave Heterodyne Receivers, IEE Colloquium on

Conference_Location

London

Type

conf

Filename

193596

Link To Document

https://search.isc.ac/dl/search/defaultta.aspx?DTC=49&DC=281078