Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
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Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
Condition: New.
Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
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Seller: Revaluation Books, Exeter, United Kingdom
Hardcover. Condition: Brand New. 1st edition. 450 pages. 9.00x6.10x1.40 inches. In Stock.
Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
Seller: GreatBookPricesUK, Woodford Green, United Kingdom
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Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
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Condition: As New. Unread book in perfect condition.
Seller: Revaluation Books, Exeter, United Kingdom
Hardcover. Condition: Brand New. 1st edition. 450 pages. 9.00x6.10x1.40 inches. In Stock. This item is printed on demand.
Language: English
Published by Jenny Stanford Publishing, 2015
ISBN 10: 9814613274 ISBN 13: 9789814613279
Seller: AHA-BUCH GmbH, Einbeck, Germany
Buch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Interferometric observations need snapshots of very high time resolution of the order of (i) frame integration of about 100 Hz or (ii) photon-recording rates of several megahertz (MHz). Detectors play a key role in astronomical observations, and since the explanation of the photoelectric effect by Albert Einstein, the technology has evolved rather fast. The present-day technology has made it possible to develop large-format complementary metal oxide-semiconductor (CMOS) and charge-coupled device (CCD) array mosaics, orthogonal transfer CCDs, electron-multiplication CCDs, electron-avalanche photodiode arrays, and quantum-well infrared (IR) photon detectors. The requirements to develop artifact-free photon shot noise-limited images are higher sensitivity and quantum efficiency, reduced noise that includes dark current, read-out and amplifier noise, smaller point-spread functions, and higher spectral bandwidth. This book aims to address such systems, technologies and design, evaluation and calibration, control electronics, scientific applications, and results.One of the fastest growing applications is signal sensing, especially wavefront sensing for adaptive optics and fringe tracking for interferometry, which is important for long-baseline optical interferometry. The coherence time of the atmosphere is a highly variable parameter. Depending upon the high velocity wind, it varies from.