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The High-Power X-Band Planetary RADAR at Goldstone: Design, Development, and Early Results
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 ra...
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Published in: | IEEE transactions on microwave theory and techniques 1976-12, Vol.24 (12), p.958-963 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | 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. |
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ISSN: | 0018-9480 1557-9670 |
DOI: | 10.1109/TMTT.1976.1129007 |