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Titlebook: Detection and Spectrometry of Faint Light; John Meaburn Book 1976 Springer Science+Business Media B.V. 1976 spectrometry

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發(fā)表于 2025-3-21 18:00:20 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Detection and Spectrometry of Faint Light
編輯John Meaburn
視頻videohttp://file.papertrans.cn/270/269198/269198.mp4
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Detection and Spectrometry of Faint Light;  John Meaburn Book 1976 Springer Science+Business Media B.V. 1976 spectrometry
描述The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these devices are identified and the designs of a wide variety of practical instruments are illustrated working on topical problems. The author has spent 14 years designing and applying spectrometers in the visible and near infra-red domains predominantly to investigate gaseous nebulae. Most recently he has designed for instance a large (15 x IS-in.) Ha interference filter for the SRC, 48-in. Schmidt camera, insect-eye Fabry-Perot spectrographs, image tube filter cameras, a SISAM monochromator, a three-beam Fabry-Perot monochromator (collaboratively) for the ISO-in. Anglo-Australian telescope and a two-etalon PEPSIOS type monochromator. Consequently emphasis in this book is placed on devices useful from the ultra-violet to the infra-red. Likewise many of the illustrations are drawn from astronomy. However most of the ideas that are presented invariably have applications in other branches of science and wavelength domains.
出版日期Book 1976
關(guān)鍵詞spectrometry
版次1
doihttps://doi.org/10.1007/978-94-015-6914-9
isbn_softcover978-90-277-1198-4
isbn_ebook978-94-015-6914-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media B.V. 1976
The information of publication is updating

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發(fā)表于 2025-3-21 21:44:22 | 只看該作者
0067-0057 from the ultra-violet to the infra-red. Likewise many of the illustrations are drawn from astronomy. However most of the ideas that are presented invariably have applications in other branches of science and wavelength domains.978-90-277-1198-4978-94-015-6914-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
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N.C.T. Van Grieken,G.A. Meijer,E.J. KuipersA critical component of any spectrometer is obviously the system employed to detect the radiation. The parameters which describe the performance of this detector then invariably determine many of those which specify the overall performance of the spectrometer itself.
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https://doi.org/10.1007/978-3-642-69511-7Until the development of all-dielectric multi-layer reflection coatings, which have low light-loss coefficients, the Fabry-Pérot interferometer had very little application to the spectrometry of faint light sources, although it was used by Fabry and Buisson as early as 1911 on the relatively bright Orion nebula, though with lossy metallic layers.
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W. R?dl,K. Hofmann-Preiss,H. WorlicekThere are a variety of interferometers whose output is the inverse Fourier transformation of the spectrum being investigated.
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