The rapid advances recently achieved by cryogenically cooled high electron mobility transistor (HEMT) low-noise amplifiers (LNA's) in the 1- to 10-GHz range are making them extremely competitive with maser amplifiers. In order to address future spacecraft navigation, telemetry, radar, and radio science needs, the Deep Space Network is investing both maser and HEMT amplifiers for its Ka-band (32-GHz) downlink capability. This article describes the current state cryogenic HEMT LNA development at Ka-band for the DSN. Noise performance results at S-band (2.3 GHz) and X-band (8.5 GHz) for HEMT's and masers are included for completeness
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
A total system noise temperature of 6.6 K was demonstrated with an 8.4-GHz traveling wave maser and ...
Two broadband very low-noise amplifiers operating in the frequency range from 4 to 12 GHz at cryogen...
Exploration of the Solar System with automated spacecraft that are more than ten astronomical units ...
A prototype 2.3 GHz (S band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
A prototype 8.4 GHz (X-band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
New low-noise cryogenic input transmission lines have been developed for the Deep Space Network (DSN...
The cryogenic noise temperature performance of a two-stage and a three-stage 32 GHz High Electron Mo...
A cryogenically cooled Ka-band (33.6-GHz), seven-element front-end array for the DSN was built and t...
The highlights of 20 years of maser use and development are presented. Masers discussed include cavi...
The research of the Advanced Radio Instrumentation Group (ARIG) is focused on the design and develop...
Significant advances in the development of high electron-mobility field-effect transistors (HEMT's) ...
Indium phosphide high electron mobility transistors (InP HEMTs), are today the best transistors for ...
Monolithic (MMIC) and discrete transistor (MIC) low noise amplifiers are compared on the basis of pe...
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorp...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
A total system noise temperature of 6.6 K was demonstrated with an 8.4-GHz traveling wave maser and ...
Two broadband very low-noise amplifiers operating in the frequency range from 4 to 12 GHz at cryogen...
Exploration of the Solar System with automated spacecraft that are more than ten astronomical units ...
A prototype 2.3 GHz (S band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
A prototype 8.4 GHz (X-band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
New low-noise cryogenic input transmission lines have been developed for the Deep Space Network (DSN...
The cryogenic noise temperature performance of a two-stage and a three-stage 32 GHz High Electron Mo...
A cryogenically cooled Ka-band (33.6-GHz), seven-element front-end array for the DSN was built and t...
The highlights of 20 years of maser use and development are presented. Masers discussed include cavi...
The research of the Advanced Radio Instrumentation Group (ARIG) is focused on the design and develop...
Significant advances in the development of high electron-mobility field-effect transistors (HEMT's) ...
Indium phosphide high electron mobility transistors (InP HEMTs), are today the best transistors for ...
Monolithic (MMIC) and discrete transistor (MIC) low noise amplifiers are compared on the basis of pe...
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorp...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
A total system noise temperature of 6.6 K was demonstrated with an 8.4-GHz traveling wave maser and ...
Two broadband very low-noise amplifiers operating in the frequency range from 4 to 12 GHz at cryogen...