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A short history of geophysical radar at Arecibo Observatory

机译:阿雷西博天文台的地球物理雷达简史

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As Arecibo Observatory (AO) approaches its 50th anniversary, it isappropriate to review the many radars and ionospheric heaters that have beendeployed on or near the 305 m dish and to summarize some of the innovativeradar-based geophysical research that has resulted. The reasons William E.(Bill) Gordon developed the 305 m Arecibo dish are well known but arebriefly reviewed. The early and then more recent radar/feed designs arereviewed as geophysical uses of Arecibo have evolved and as the fullpotential of the dish and nearby facilities was and is being realized fromHF through S-band frequencies. This history surely has some gaps and thereare a few mysteries. The community is encouraged to fill these gaps and tohelp complete the history.
机译:随着阿雷西博天文台(AO)成立50周年,宜对在305 m皿上或附近部署的许多雷达和电离层加热器进行回顾,并总结一些由此产生的基于雷达的创新地球物理研究。威廉·比尔·戈登(William E.(Bill)Gordon)开发305 m阿雷西博(Arecibo)碟的原因众所周知,但简要回顾一下。随着对Arecibo的地球物理用途的发展,以及从HF到S波段频率的碟形天线和附近设施的全面潜力的研究,人们对早期/最近的雷达/馈送设计进行了审查。这个历史肯定有一些空白,并且有一些奥秘。鼓励社区填补这些空白并帮助完善历史。

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