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Image courtesy of Doc Ewen
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Introduction
Harvard Cyclotron: 1948-1951
Detection of HI Line: 1951
Harvard 24ft and 60ft and NRAO founding: 1952-1956
1950s and 1960s: Two Roads that Crossed
Microwave & Millimeter Wave Applications in the 1970s and 1980s
Mm Wave Radiometry in the 1990s
May 2001 visit to NRAO Green Bank
Bibliography
Permissions
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Image courtesy of Doc Ewen |
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Doc Ewen: The Horn, HI, and Other Events in US Radio Astronomy
by Doc Ewen, © 2003
Slide 11: Detecting the Interstellar Hydrogen Line, 1951
The design of the horn antenna was based on descriptive information presented in the Rad Lab book on Antennas by Sam Silver [Microwave Antenna Theory and Design, edited by Samuel Silver. MIT Radiation Laboratory Series 12, published by McGraw-Hill, 1949; reprinted by P. Peregrinus on behalf of the Institution of Electrical Engineers, 1984]. The maximum size was determined by the geometric constraints of the fourth floor parapet at Lyman Lab. I sent my calculations and sketches to Sam for a sanity check, before sending the build order to the Physics Dept. Model Shop. It was up on the parapet in about three weeks. [Diagrom courtesy of Doc Ewen]
Slide 12
Modified on Monday, 06-Sep-2004 14:06:02 EDT by Ellen Bouton
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