DocumentCode :
664611
Title :
Low-noise sub-millimeter wave local oscillators for ALMA
Author :
Bryerton, Eric ; Saini, Kelly ; Muehlberg, Jim ; Vaselaar, Dustin ; Thacker, Dorsey
Author_Institution :
Nat. Radio Astron. Obs., Charlottesville, VA, USA
fYear :
2013
fDate :
2-7 June 2013
Firstpage :
1
Lastpage :
3
Abstract :
High signal-to-noise ratio sub-millimeter wave local oscillators (LOs) were developed and produced for the Atacama Large Millimeter Array (ALMA). They cover fractional bandwidths of 15-25% from 92 to 942 GHz. The LOs were designed and tested for high signal-to-noise ratio since they are used to drive single-ended mixers. Integrated millimeter-wave multi-chip MMIC modules, employing custom and commercial MMICs, were designed to yield the required power and SNR performance. 73 modules of the LO have been produced for each of the six bands to date, with two more bands currently under construction.
Keywords :
MMIC; mixers (circuits); multichip modules; oscillators; signal processing; ALMA; Atacama large millimeter array; SNR performance; bandwidth 92 GHz to 942 GHz; commercial MMIC; high signal to noise ratio submillimeter wave local oscillators; integrated millimeter wave multichip MMIC modules; low noise submillimeter wave local oscillators; single ended mixers; Local oscillators; MMICs; Mixers; Power amplifiers; Receivers; Signal to noise ratio; ALMA; sub-millimeter wave;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Microwave Symposium Digest (IMS), 2013 IEEE MTT-S International
Conference_Location :
Seattle, WA
ISSN :
0149-645X
Print_ISBN :
978-1-4673-6177-4
Type :
conf
DOI :
10.1109/MWSYM.2013.6697622
Filename :
6697622
Link To Document :
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