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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
Millimeter Wave Radiometry in the 1990s: RAVIN-SL5 slide 7
The RAVIN-SL5 temperature calibration unit (TCU), mounted on the RF head. The TCU is a unique feature of the RAVIN-SL5 radio telescope. It allows direct calibration of the recorded antenna temperature while observing a target. The TCU is controlled directly from the telescope control panel. A three position switch allows selection of the target signal, the ambient temperature, or an automatic repetitive sequence between the target signal and ambient temperature. It is particularly useful for rocket plume measurements during the launch phase, since it provides a direct measurement of the sky noise background temperature over the extent of the launch profile, prior to launch. When used with the remote focusing unit (RFU), it provides a direct measure of aperture focusing and efficiency, using the moon as a target. TCU and RFU capabilities are essential to the accumulation and analysis of short term phenomena, typical of rocket launches and kinetic kill events. Credit: Photo courtesy of Doc Ewen.
Modified on Tuesday, 07-Jun-2005 16:43:28 EDT by Ellen Bouton
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