The development and performance of X-band traveling-wave maser (TWM) systems with effective input noise temperature of 3.5 K and bandwidths varying from 65 to 108 MHz is discussed. These TWMs are used on the 64-meter antennas at Deep Space Stations 14, 43 and 63 at 8420 MHz to meet the requirements of the Voyager-Saturn encounter. The TWMs use shortened and cooled signal input waveguide to reduce noise and are equipped with superconducting magnets and solid-state pump sources to provide the required stability performance
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...
The Deep Space Network (DSN) 64-meter antenna in Spain (DSN 63) has been calibrated prior to its upg...
A 33.68-GHz dual-cavity ruby maser was built to support the Ka-Band Link Experiment (KABLE) conducte...
The highlights of 20 years of maser use and development are presented. Masers discussed include cavi...
The development of an X-band exciter, for use in the X-Band Uplink Subsystem, was completed. The exc...
A 2.3 GHz traveling-wave maser/closed-cycle refrigeration system was installed on the 64 m antenna a...
Improved pump source assemblies and new 8.4-GHz low noise traveling-wave masers (TWMs) were installe...
A wideband low noise preamplifier system will be utilized for the A TS series of satellites at the M...
A 2.3 GHz traveling-wave maser/closed-cycle refrigerator (TWM/CCR) that is used in the DSN was insta...
The rapid advances recently achieved by cryogenically cooled high electron mobility transistor (HEMT...
A document discusses a multi-Gigabit-per-second, Ka-band transceiver with a software-defined modem (...
A total system noise temperature of 6.6 K was demonstrated with an 8.4-GHz traveling wave maser and ...
An eight stage, 32 GHz reflected wave ruby maser was built. The maser operates in a 3 watt closed cy...
The results of the reliability and availability analyses of the individual S- and X-band traveling-w...
The design concepts and measured performance characteristics are summarized of an X band (7162 MHz/8...
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...
The Deep Space Network (DSN) 64-meter antenna in Spain (DSN 63) has been calibrated prior to its upg...
A 33.68-GHz dual-cavity ruby maser was built to support the Ka-Band Link Experiment (KABLE) conducte...
The highlights of 20 years of maser use and development are presented. Masers discussed include cavi...
The development of an X-band exciter, for use in the X-Band Uplink Subsystem, was completed. The exc...
A 2.3 GHz traveling-wave maser/closed-cycle refrigeration system was installed on the 64 m antenna a...
Improved pump source assemblies and new 8.4-GHz low noise traveling-wave masers (TWMs) were installe...
A wideband low noise preamplifier system will be utilized for the A TS series of satellites at the M...
A 2.3 GHz traveling-wave maser/closed-cycle refrigerator (TWM/CCR) that is used in the DSN was insta...
The rapid advances recently achieved by cryogenically cooled high electron mobility transistor (HEMT...
A document discusses a multi-Gigabit-per-second, Ka-band transceiver with a software-defined modem (...
A total system noise temperature of 6.6 K was demonstrated with an 8.4-GHz traveling wave maser and ...
An eight stage, 32 GHz reflected wave ruby maser was built. The maser operates in a 3 watt closed cy...
The results of the reliability and availability analyses of the individual S- and X-band traveling-w...
The design concepts and measured performance characteristics are summarized of an X band (7162 MHz/8...
The Very Large Array (VLA) is being equipped to receive telemetry from Voyager 2 during the Neptune ...
The Deep Space Network (DSN) 64-meter antenna in Spain (DSN 63) has been calibrated prior to its upg...
A 33.68-GHz dual-cavity ruby maser was built to support the Ka-Band Link Experiment (KABLE) conducte...