The Galileo mission was originally designed to investigate Jupiter and its moons utilizing a high-rate, X-band (8415 MHz) communication downlink with a maximum rate of 134.4 kb/sec. However, following the failure of the high-gain antenna (HGA) to fully deploy, a completely new communication link design was established that is based on Galileo's S-band (2295 MHz), low-gain antenna (LGA). The new link relies on data compression, local and intercontinental arraying of antennas, a (14,1/4) convolutional code, a (255,M) variable-redundancy Reed-Solomon code, decoding feedback, and techniques to reprocess recorded data to greatly reduce data losses during signal acquisition. The combination of these techniques will enable return of significant sc...
The Galileo low-gain antenna mission will be supported by a coding system that uses a (14,1/4) inner...
Uplink optical communication to a deep-space vehicle was demonstrated. In the Galileo Optical Experi...
Reducing the Time To First Fix (TTFF) and improving the resilience of future Galileo signals are two...
The Galileo mission operations concept is undergoing substantial redesign, necessitated by the deplo...
The Galileo spacecraft is currently on its way to Jupiter and its moons. In April 1991, the high gai...
The Galileo Jupiter orbital mission using the Low Gain Antenna (LGA) requires a higher degree of spa...
On day of the year 062, 1994, a prototype of the Deep Space Communications Complex Galileo Telemetry...
On April 11, 1991, the Galileo spacecraft executed a sequence that would open the spacecraft's High ...
The Galileo low-gain antenna mission has a severely rate-constrained channel over which we wish to s...
Full-spectrum combining (FSC) and complex-symbol combining (CSC) are two antenna-arraying techniques...
Due to the hardware design of Galileo's Command and Data Subsystem (CDS), the channel code usable in...
The Galileo mission to Jupiter is now faced with extreme limitations in its communication downlink c...
Work is in progress to determine the feasibility of using the Very Large Array (VLA) radio telescope...
The Galileo mission to Jupiter is now faced with extreme limitations in its communication downlink c...
Cost efficiency is becoming a major driver in future space missions. Because of the constraints on t...
The Galileo low-gain antenna mission will be supported by a coding system that uses a (14,1/4) inner...
Uplink optical communication to a deep-space vehicle was demonstrated. In the Galileo Optical Experi...
Reducing the Time To First Fix (TTFF) and improving the resilience of future Galileo signals are two...
The Galileo mission operations concept is undergoing substantial redesign, necessitated by the deplo...
The Galileo spacecraft is currently on its way to Jupiter and its moons. In April 1991, the high gai...
The Galileo Jupiter orbital mission using the Low Gain Antenna (LGA) requires a higher degree of spa...
On day of the year 062, 1994, a prototype of the Deep Space Communications Complex Galileo Telemetry...
On April 11, 1991, the Galileo spacecraft executed a sequence that would open the spacecraft's High ...
The Galileo low-gain antenna mission has a severely rate-constrained channel over which we wish to s...
Full-spectrum combining (FSC) and complex-symbol combining (CSC) are two antenna-arraying techniques...
Due to the hardware design of Galileo's Command and Data Subsystem (CDS), the channel code usable in...
The Galileo mission to Jupiter is now faced with extreme limitations in its communication downlink c...
Work is in progress to determine the feasibility of using the Very Large Array (VLA) radio telescope...
The Galileo mission to Jupiter is now faced with extreme limitations in its communication downlink c...
Cost efficiency is becoming a major driver in future space missions. Because of the constraints on t...
The Galileo low-gain antenna mission will be supported by a coding system that uses a (14,1/4) inner...
Uplink optical communication to a deep-space vehicle was demonstrated. In the Galileo Optical Experi...
Reducing the Time To First Fix (TTFF) and improving the resilience of future Galileo signals are two...