DocumentCode :
62758
Title :
Wideband SIS Receivers Using Series Distributed SIS Junction Array
Author :
Tong, Cheuk-Yu Edward ; Grimes, Paul ; Blundell, Raymond ; Ming-Jye Wang ; Noguchi, Takashi
Author_Institution :
Harvard-Smithsonian Center for Astrophys., Cambridge, MA, USA
Volume :
3
Issue :
4
fYear :
2013
fDate :
Jul-13
Firstpage :
428
Lastpage :
432
Abstract :
We have developed an SIS mixer based on a 3-junction series distributed array. In this mixer layout, the three junctions are connected together by passive network elements, such that each junction is subjected to different local oscillator (LO) drive, and slightly different DC bias voltages. This design helps to reduce the output capacitance of the mixer at the intermediate frequency (IF) so as to achieve a wider IF bandwidth, while maintaining adequate RF bandwidth. The receiver performance of this type of mixer was evaluated in the 220 GHz band. The lowest noise temperature measured was ~30 K, and the noise temperature remains below 50 K over the IF range from 3 to 11 GHz. Receivers incorporating this new mixer design are currently in routine operation at the Submillimeter Array.
Keywords :
millimetre wave mixers; millimetre wave receivers; superconducting arrays; superconducting microwave devices; superconductor-insulator-superconductor mixers; DC bias voltages; IF bandwidth; LO drive; SIS mixer; frequency 220 GHz; frequency 3 GHz to 11 GHz; intermediate frequency; local oscillator drive; mixer layout; noise temperature; passive network elements; series distributed SIS junction array; submillimeter array; supercon-ductor-insulator-superconductor junction; wideband SIS receivers; Distributed mixers; submillimeter receivers; superconductor–insulator–superconductor (SIS) mixers; ultra wideband receivers;
fLanguage :
English
Journal_Title :
Terahertz Science and Technology, IEEE Transactions on
Publisher :
ieee
ISSN :
2156-342X
Type :
jour
DOI :
10.1109/TTHZ.2013.2259624
Filename :
6516592
Link To Document :
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