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A G-band cryogenic MMIC heterodyne receiver module for astronomical applications

Published online by Cambridge University Press:  12 March 2012

Patricia Voll ,
Lorene Samoska ,
Sarah Church ,
Judy M. Lau ,
Matthew Sieth ,
Todd Gaier ,
Pekka Kangaslahti ,
Mary Soria ,
Sami Tantawi  and
Dan Van Winkle
Patricia Voll*
Affiliation:
Department of Physics, Stanford University, Stanford, CA 94305, USA. Phone: +1 650 725 9796. Kavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94309, USA.
Lorene Samoska
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Sarah Church
Affiliation:
Department of Physics, Stanford University, Stanford, CA 94305, USA. Phone: +1 650 725 9796. Kavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94309, USA.
Judy M. Lau
Affiliation:
Department of Physics, Stanford University, Stanford, CA 94305, USA. Phone: +1 650 725 9796. Kavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94309, USA.
Matthew Sieth
Affiliation:
Department of Physics, Stanford University, Stanford, CA 94305, USA. Phone: +1 650 725 9796. Kavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94309, USA.
Todd Gaier
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Pekka Kangaslahti
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Mary Soria
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Sami Tantawi
Affiliation:
SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA.
Dan Van Winkle
Affiliation:
SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA.
*
Corresponding author: P. Voll Email: [email protected]
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Abstract

We report cryogenic noise temperature and gain measurements of a prototype heterodyne receiver module designed to operate in the atmospheric window centered on 150 GHz. The module utilizes monolithic microwave integrated circuit (MMIC) InP high electron mobility transistor (HEMT) amplifiers, a second harmonic mixer, and bandpass filters. Swept local oscillator (LO) measurements show an average gain of 22 dB and an average noise temperature of 87 K over a 40 GHz band from 140 to 180 GHz when the module is cooled to 22 K. A spot noise temperature of 58 K was measured at 166 GHz and is a record for cryogenic noise from HEMT amplifiers at this frequency. Intermediate frequency (IF) sweep measurements show a 20 GHz IF band with less than 94 K receiver noise temperature for a fixed LO of 83 GHz. The compact housing features a split-block design that facilitates quick assembly and a condensed arrangement of the MMIC components and bias circuitry. DC feedthroughs and nano-miniature connectors also contribute to the compact design, so that the dimensions of the moduleare approximately 2.5 cm per side.

Keywords

Multi-Chip ModulesLow Noise Amplifier (LNA)Low Noise ReceiverMMICHEMT
Type
Research Papers
Information
International Journal of Microwave and Wireless Technologies , Volume 4 , Special Issue 3: European Microwave Week 2011 , June 2012 , pp. 283 - 289
Copyright
Copyright © Cambridge University Press and the European Microwave Association 2012

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References

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