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Titlebook: Electronic Imaging in Astronomy; Detectors and Instru Ian S. McLean Textbook 2008Latest edition Springer-Verlag Berlin Heidelberg 2008 Adap

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發(fā)表于 2025-3-21 19:14:16 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Electronic Imaging in Astronomy
副標(biāo)題Detectors and Instru
編輯Ian S. McLean
視頻videohttp://file.papertrans.cn/307/306330/306330.mp4
概述Collects all the fundamental astronomical observing techniques and methods into a single reference work.Unlike competing books, written at a level that will serve both advanced undergraduate and gradu
叢書(shū)名稱Springer Praxis Books
圖書(shū)封面Titlebook: Electronic Imaging in Astronomy; Detectors and Instru Ian S. McLean Textbook 2008Latest edition Springer-Verlag Berlin Heidelberg 2008 Adap
描述.The second edition of Electronic Imaging in Astronomy: Detectors and Instrumentation describes the remarkable developments that have taken place in astronomical detectors and instrumentation in recent years – from the invention of the charge-coupled device (CCD) in 1970 to the current era of very large telescopes, such as the Keck 10-meter telescopes in Hawaii with their laser guide-star adaptive optics which rival the image quality of the Hubble Space Telescope. ..Authored by one of the world’s foremost experts on the design and development of electronic imaging systems for astronomy, this book has been written on several levels to appeal to a broad readership. Mathematical expositions are designed to encourage a wider audience, especially among the growing community of amateur astronomers with small telescopes with CCD cameras. The book can be used at the college level for an introductory course on modern astronomical detectors and instruments, and as a supplement for a practical or laboratory class..
出版日期Textbook 2008Latest edition
關(guān)鍵詞Adaptive Optics; Astronomical Detectors; Astronomical Instrumentation; CCDs; Textbook; image processing; o
版次2
doihttps://doi.org/10.1007/978-3-540-76583-7
isbn_softcover978-3-642-09532-0
isbn_ebook978-3-540-76583-7
copyrightSpringer-Verlag Berlin Heidelberg 2008
The information of publication is updating

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Beating the atmosphere,ects, the spreading of the image is determined by the diffraction of light. In practice, for ground-based observatories, the light must pass through the atmosphere, which has a major impact on image quality because of turbulence.
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Charge-coupled devices,at the dominant detector in modern astronomy is the charge-coupled device (CCD), it is important to consider these remarkable detectors in more detail. We begin with a brief historical review of CCDs from invention to present day, an amazing story by itself, and then cover the basic principles of ho
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Characterization and calibration of array instruments,tand how the properties of the detector can be measured and how the behavior of the detector affects photometric and spectroscopic analyses. This chapter describes important steps in these calibrations in terms of CCDs, but the same considerations apply to other array detectors. Signal-to-noise expr
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