Future communication systems will move toward the 20 to 30 GHz frequency range for wider bandwidth and reduced interference, and will use small earth terminals. The ESA satellite OLYMPUS is scheduled for launch this June and will be ready for use in October. OLYMPUS has 12, 20, and 30 GHz beacons. Virginia Tech and Michigan Tech are working with NASA/JPL on an OLYMPUS experiment and hardware development program. OLYMPUS beacons provide coverage of the east coast of the US sufficient for attenuation measurements. The planned hardware for the OLYMPUS experiments is illustrated. The components of the experiment are summarized. A block diagram level overview of a typical channel is given and one of the four RF front ends is shown
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
Virginia Tech is performing a comprehensive set of propagation measurements using the Olympus satell...
Virginia Tech is performing a comprehensive set of propagation measurements using the OLYMPUS satell...
The OLYMPUS and ACTS satellites both provide opportunities for 10 to 30 GHz propagation measurements...
Virginia Polytechnic Institute has been carrying out a comprehensive set of propagation measurements...
Virginia Tech has developed two types of receivers to monitor the Olympus beacons, as well as a cust...
Virginia Tech has performed a comprehensive propagation experiment using the Olympus satellite beaco...
Rapidly growing demand for channel capacity and limitations in satellite power and frequency spectru...
Rapidly growing demand for channel capacity and limitations in satellite power and frequency spectru...
A medium-size Beacon Receiving System for reception and processing of the B1 (20 GHz) and B2 (30 GHz...
Measurements of attenuation of the 20 and 30 GHz beacons onboard the OLYMPUS satellite are compared ...
The outline of a design of a system using ultra small earth stations (picoterminals) for data traffi...
An overview of the organization of the OLYMPUS propagation experimenters group (OPEX) is given. Prep...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
Virginia Tech is performing a comprehensive set of propagation measurements using the Olympus satell...
Virginia Tech is performing a comprehensive set of propagation measurements using the OLYMPUS satell...
The OLYMPUS and ACTS satellites both provide opportunities for 10 to 30 GHz propagation measurements...
Virginia Polytechnic Institute has been carrying out a comprehensive set of propagation measurements...
Virginia Tech has developed two types of receivers to monitor the Olympus beacons, as well as a cust...
Virginia Tech has performed a comprehensive propagation experiment using the Olympus satellite beaco...
Rapidly growing demand for channel capacity and limitations in satellite power and frequency spectru...
Rapidly growing demand for channel capacity and limitations in satellite power and frequency spectru...
A medium-size Beacon Receiving System for reception and processing of the B1 (20 GHz) and B2 (30 GHz...
Measurements of attenuation of the 20 and 30 GHz beacons onboard the OLYMPUS satellite are compared ...
The outline of a design of a system using ultra small earth stations (picoterminals) for data traffi...
An overview of the organization of the OLYMPUS propagation experimenters group (OPEX) is given. Prep...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...
A multifrequency antenna system for future propagation experiments, at 12.5, 20, and 30 GHz with the...