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Low Noise Amplifiers for 140 Ghz Wide-Band Cryogenic ReceiversWe report S-parameter and noise measurements for three different Indium Phosphide 35-nanometer-gate-length High Electron Mobility Transistor (HEMT) Low Noise Amplifier (LNA) designs operating in the frequency range centered on 140 gigahertz. When packaged in a Waveguide Rectangular-6.1 waveguide housing, the LNAs have an average measured noise figure of 3.0 decibels - 3.6 decibels over the 122-170 gigahertz band. One LNA was cooled to 20 degrees Kelvin and a record low noise temperature of 46 Kelvin, or 0.64 decibels noise figure, was measured at 152 gigahertz. These amplifiers can be used to develop receivers for instruments that operate in the 130-170 gigahertz atmospheric window, which is an important frequency band for ground-based astronomy and millimeter-wave imaging applications.
Document ID
20150007401
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Larkoski, Patricia V.
(Stanford Univ. Stanford, CA, United States)
Kangaslahti, Pekka
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Samoska, Lorene
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lai, Richard
(Northrop Grumman Corp. Redondo Beach, CA, United States)
Sarkozy, Stephen
(Northrop Grumman Corp. Redondo Beach, CA, United States)
Date Acquired
May 6, 2015
Publication Date
June 2, 2013
Subject Category
Electronics And Electrical Engineering
Instrumentation And Photography
Engineering (General)
Astronomy
Meeting Information
Meeting: International Microwave Symposium (IMS)
Location: Seattle, WA
Country: United States
Start Date: June 2, 2013
End Date: June 7, 2013
Sponsors: Institute of Electrical and Electronics Engineers
Distribution Limits
Public
Copyright
Other
Keywords
High Electron Mobility Transistors (HEMTs)
noise measurement
cryogenic electronics

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