Selected critical microwave components for a 400-kW very-long-pulse (several hours) X-band radar system are discussed from theoretical and practical viewpoints. Included are the special-sized waveguide and flanges, hybrid power combiner, couplers, switches, polarizer, rotary joints, feedhorn, and radome. The system is installed on the National Aeronautics and Space Administration/Jet Propulsion Laboratory 64-m-diam reflector antenna at Goldstone, CA.
The high-power X-band planetary radar at Goldstone - Design, development, and early results
1976-12-01
Miscellaneous
No indication
English
Recent Results from Goldstone Orbital Debris Radar
British Library Conference Proceedings | 1999
|Recent Results from Goldstone Orbital Debris Radar
British Library Conference Proceedings | 1999
|Goldstone Solar System Radar (GSSR)
NTRS | 1991
|Goldstone Solar System Radar (GSSR)
NTIS | 1991
|CHAPTER 1 -- RADAR AND OPTICAL OBSERVATIONS - Recent Results from Goldstone Orbital Debris Radar
Online Contents | 1999
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