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Astronomical optical interferometry: Astronomical interferometer, Mount Wilson Observatory, Betelgeuse, Astronomical seeing, Keck Interferometer, Palomar Testbed Interferometer - Softcover
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. One of the first astronomical interferometers was built on the Mount Wilson Observatory''s reflector telescope in 1920 in order to measure the diameters of stars. The red giant star Betelgeuse was among the first to have its diameter determined in this way. This method was extended to measurements using separated telescopes by Johnson, Betz and Towns (1974) in the infrared and by Labeyrie (1975) in the visible. In the late 1970s improvements in computer processing allowed for the first fringe-tracking" interferometer, which operates fast enough to follow the blurring effects of astronomical seeing, leading to the Mk I,II and III series of interferometers. Similar techniques have now been applied at other astronomical telescope arrays, including the Keck Interferometer and the Palomar Testbed Interferometer. "
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. One of the first astronomical interferometers was built on the Mount Wilson Observatory''s reflector telescope in 1920 in order to measure the diameters of stars. The red giant star Betelgeuse was among the first to have its diameter determined in this way. This method was extended to measurements using separated telescopes by Johnson, Betz and Towns (1974) in the infrared and by Labeyrie (1975) in the visible. In the late 1970s improvements in computer processing allowed for the first fringe-tracking" interferometer, which operates fast enough to follow the blurring effects of astronomical seeing, leading to the Mk I,II and III series of interferometers. Similar techniques have now been applied at other astronomical telescope arrays, including the Keck Interferometer and the Palomar Testbed Interferometer. "
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Astronomical optical interferometry
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Astronomical optical interferometry | Astronomical interferometer, Mount Wilson Observatory, Betelgeuse, Astronomical seeing, Keck Interferometer, Palomar Testbed Interferometer
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Taschenbuch. Condition: Neu. Astronomical optical interferometry | Astronomical interferometer, Mount Wilson Observatory, Betelgeuse, Astronomical seeing, Keck Interferometer, Palomar Testbed Interferometer | Frederic P. Miller (u. a.) | Taschenbuch | Englisch | 2026 | OmniScriptum | EAN 9786132539786 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu Print on Demand. Seller Inventory # 134701508
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Astronomical optical interferometry : Astronomical interferometer, Mount Wilson Observatory, Betelgeuse, Astronomical seeing, Keck Interferometer, Palomar Testbed Interferometer
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Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Please note that the content of this book primarily consists of articlesavailable from Wikipedia or other free sources online. One of the firstastronomical interferometers was built on the Mount Wilson Observatory'sreflector telescope in 1920 in order to measure the diameters of stars.The red giant star Betelgeuse was among the first to have its diameterdetermined in this way. This method was extended to measurements usingseparated telescopes by Johnson, Betz and Towns (1974) in the infraredand by Labeyrie (1975) in the visible. In the late 1970s improvements incomputer processing allowed for the first 'fringe-tracking'interferometer, which operates fast enough to follow the blurringeffects of astronomical seeing, leading to the Mk I,II and III series ofinterferometers. Similar techniques have now been applied at otherastronomical telescope arrays, including the Keck Interferometer and thePalomar Testbed Interferometer. Seller Inventory # 9786132539786
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Astronomical optical interferometry
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Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Please note that the content of this book primarily consists of articlesavailable from Wikipedia or other free sources online. One of the firstastronomical interferometers was built on the Mount Wilson Observatory'sreflector telescope in 1920 in order to measure the diameters of stars.The red giant star Betelgeuse was among the first to have its diameterdetermined in this way. This method was extended to measurements usingseparated telescopes by Johnson, Betz and Towns (1974) in the infraredand by Labeyrie (1975) in the visible. In the late 1970s improvements incomputer processing allowed for the first 'fringe-tracking'interferometer, which operates fast enough to follow the blurringeffects of astronomical seeing, leading to the Mk I,II and III series ofinterferometers. Similar techniques have now been applied at otherastronomical telescope arrays, including the Keck Interferometer and thePalomar Testbed Interferometer.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 128 pp. Englisch. Seller Inventory # 9786132539786
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