Abstract
Thank you for the article “The Arecibo Observatory: Fifty astronomical years” by Daniel Altschuler and Chris Salter (Physics Today, November 2013, page 43). I’d like to add a historical note.The first publication to discuss using a spherical reflector set in the ground and steered by a line source, as illustrated in the article’s figure 2, was published in May 1951 by engineers at the Air Force Cambridge Research Laboratories (AFCRL).11. R. C. Spencer, C. J. Sletten, J. E. Walsh, Correction of Spherical Aberration by a Phased Line Source, Air Force Cambridge Research Laboratories, Cambridge, MA (1951);http://www.dtic.mil/dtic/tr/fulltext/u2/a800275.pdf The Department of Defense was interested in using what would become the world’s largest antenna to better understand the ionosphere for long-range radar and communications. Thus in 1959 officials from the AFCRL and Cornell University, home to Arecibo designer William Gordon, signed a contract to build the observatory. The project was funded by the Advanced Research Projects Agency, with Philipp Blacksmith of the AFCRL named as the project officer.REFERENCESSection:ChooseTop of pageREFERENCES <<1. R. C. Spencer, C. J. Sletten, J. E. Walsh, Correction of Spherical Aberration by a Phased Line Source, Air Force Cambridge Research Laboratories, Cambridge, MA (1951);http://www.dtic.mil/dtic/tr/fulltext/u2/a800275.pdf, Google Scholar© 2014 American Institute of Physics.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.