A prototype 8.4 GHz (X-band) high electron mobility transistor (HEMT) amplifier/closed cycle refrigerator system was installed in the Deep Space Station 13 feedcone in August 1987. The amplifier is cryogenically cooled to a physical temperature of 12 K and provides 31 K antenna noise temperature (zenith) and 35 dB of gain at a frequency of 8.2 to 8.6 GHz. Antenna system noise temperature is less than 50 K from 7.2 to 9.4 MHz. The low noise HEMT amplifier system is intended for use as a radio astronomy or space communications receiver front end
We present a way to design a high-frequency low-temperature pHEMT-based balanced amplifier. The desi...
We have realized receiving - amplifying circuits for a frequency range of 21.0-23.0 GHz using freque...
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...
A prototype 2.3 GHz (S band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
A cryogenically cooled Ka-band (33.6-GHz), seven-element front-end array for the DSN was built and t...
The rapid advances recently achieved by cryogenically cooled high electron mobility transistor (HEMT...
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...
Exploration of the Solar System with automated spacecraft that are more than ten astronomical units ...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
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) ...
This PhD thesis presents the work that was done developing radioastronomy instrumentation. The first...
Contains report on one research project.National Aeronautics and Space Administration (Contract NAG3...
instrumentation activities, several low noise, low power consumption cryogenic amplifiers were devel...
We present a way to design a high-frequency low-temperature pHEMT-based balanced amplifier. The desi...
We have realized receiving - amplifying circuits for a frequency range of 21.0-23.0 GHz using freque...
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...
A prototype 2.3 GHz (S band) high electron mobility transistor (HEMT) amplifier/closed cycle refrige...
A cryogenically cooled Ka-band (33.6-GHz), seven-element front-end array for the DSN was built and t...
The rapid advances recently achieved by cryogenically cooled high electron mobility transistor (HEMT...
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...
Exploration of the Solar System with automated spacecraft that are more than ten astronomical units ...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
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) ...
This PhD thesis presents the work that was done developing radioastronomy instrumentation. The first...
Contains report on one research project.National Aeronautics and Space Administration (Contract NAG3...
instrumentation activities, several low noise, low power consumption cryogenic amplifiers were devel...
We present a way to design a high-frequency low-temperature pHEMT-based balanced amplifier. The desi...
We have realized receiving - amplifying circuits for a frequency range of 21.0-23.0 GHz using freque...
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...