Astronomical site evaluation in the visible and radio range

Astronomical site evaluation in the visible and radio range

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Annotation This collection from the November 2000 workshop reviews the state of the art in observatory site testing methods and instruments across the entire ground-based optical, infrared, and (sub)mm wavelength ranges. The 72 papers investigate the physical mechanisms of atmospheric turbulence, measuring instruments in the visible range, site characterization and atmospheric transparency in the (sub)mm range, tropospheric phase stability, forecasting, site surveys, astroclimatic stations, and phase correction. Specific topics include site monitoring for extremely large telescopes, atmospheric turbulence profiles deduced from solar limb observations, and a comparison of the Pampa La Bola and Llano de Chajnator sites in northern Chile. No index. Annotation (c)2003 Book News, Inc., Portland, OR (booknews.com)It has the advantages of using a single down conversion stage and a direct estimate of the phase difference (Hiriart, priv. comm.). ... beacon signal having a 3 MHz bandwidth is received by two commercial 80cm satellite dishes. ... 5 presents a block diagram of the implemented system. ... Low noise direct TV broadcasting receivers amplify the Ku band signal. ... from the antennas to the processing electronics through thermally stable cables to reduce the phase drift of the instrument.


Title:Astronomical site evaluation in the visible and radio range
Author: Jean Vernin, Zouhair Benkhaldoun, Casiana Muñoz-Tuñón, International Astronomical Union
Publisher:Astronomical Society of the pacific - 2002
ISBN-13:

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