Radio Astronomy at Long Wavelengths

Format Electronic
Publication InfoWashington : American Geophysical Union Somerset : John Wiley & Sons, Incorporated [Distributor]
Description372 p.
Supplemental ContentFull text available from AGU Digital Library - Books Series

Other author/creatorStone, Robert G. Editor
Other author/creatorWeiler, Kurt W. Editor
Other author/creatorGoldstein, Melvyn L. Editor
Other author/creatorBougeret, Jean-Louis Editor
SeriesGeophysical Monograph Ser. 119
Summary Annotation Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 119.The spectacular success of Earth-based radio astronomy is due to several factors. A broad atmospheric window of more than four orders-of-magnitude in frequency extends from ~30 MHz (wavelength 10 m), where ionospheric distortions and opacity begin to become a problem, to ~300 GHz (wavelength 1 mm), where atmospheric absorption becomes excessive, even from high mountain sites. This radio window reveals a rich variety of astrophysical phenomena. Also key to the success of radio astronomy has been the development of interferometry which provides high resolution, even at long wavelengths, without the construction of impossibly large and expensive single dish radio telescopes.
Access restrictionAvailable only to authorized users.
Technical detailsMode of access: World Wide Web
Genre/formElectronic books.
ISBN9781118668368
ISBN1118668367 (Online Resource) Active Record
Stock number00001265

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