Genesis of the 1000-foot Dish at Arecibo

Details Genesis of the 1000-foot Dish at Arecibo Genesis of the 1000-foot Dish at Arecibo

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.7104c&link_type=abstract

American Astronomical Society, AAS Meeting #211, #71.04; Bulletin of the American Astronomical Society, Vol. 39, p.862

Astronomy and Astrophysics

Astronomy

Scientific paper

The Arecibo dish was conceived early in 1958 by William E. Gordon, a Professor of Electrical Engineering at Cornell University. The objective was to design and build a radar sensitive enough to measure the backscattered signal from free electrons in the high ionosphere, the so-called incoherent scatter (IS) signal. Gordon calculated the required size of the antenna by assuming that the thermal velocity of the electrons controlled the width of the spectrum of the echo. Six months later Kenneth L. Bowles, a Cornell graduate now working at NBS in Boulder, Colorado, did a radar experiment that confirmed part of Gordon's ideas. Bowles showed that the strength of the IS signal is roughly as calculated by Gordon, but the spectral width of the echo is much narrower than that calculated by Gordon. This meant that a substantially smaller, cheaper, dish could be used. A year later, however, ARPA gave the money to start the project, still at the original size, 1000 feet. By this time the goals of the project had widened considerably, to include radio and radar astronomy, and most of the new goals did require the 1000 foot diameter. Note that this project went from conception to funding in a year and a half, far quicker than it would at present. The IGY in 1957-1958, and the launch of the Sputnik and Explorer satellites during this period, fueled a great deal of interest in the high ionosphere in both military and civilian circles. I speculate on how this affected the Arecibo project.

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