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標(biāo)題: Titlebook: Electronic Imaging in Astronomy; Detectors and Instru Ian S. McLean Textbook 2008Latest edition Springer-Verlag Berlin Heidelberg 2008 Adap [打印本頁(yè)]

作者: 復(fù)雜    時(shí)間: 2025-3-21 19:14
書目名稱Electronic Imaging in Astronomy影響因子(影響力)




書目名稱Electronic Imaging in Astronomy影響因子(影響力)學(xué)科排名




書目名稱Electronic Imaging in Astronomy網(wǎng)絡(luò)公開度




書目名稱Electronic Imaging in Astronomy網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Electronic Imaging in Astronomy被引頻次




書目名稱Electronic Imaging in Astronomy被引頻次學(xué)科排名




書目名稱Electronic Imaging in Astronomy年度引用




書目名稱Electronic Imaging in Astronomy年度引用學(xué)科排名




書目名稱Electronic Imaging in Astronomy讀者反饋




書目名稱Electronic Imaging in Astronomy讀者反饋學(xué)科排名





作者: alabaster    時(shí)間: 2025-3-21 23:33
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.
作者: 防御    時(shí)間: 2025-3-22 03:28

作者: scrutiny    時(shí)間: 2025-3-22 08:14

作者: AFFIX    時(shí)間: 2025-3-22 11:21

作者: 使厭惡    時(shí)間: 2025-3-22 13:19

作者: 使厭惡    時(shí)間: 2025-3-22 20:38
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
作者: 燈絲    時(shí)間: 2025-3-22 21:23

作者: condescend    時(shí)間: 2025-3-23 04:54
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
作者: 樹膠    時(shí)間: 2025-3-23 07:56

作者: 縮短    時(shí)間: 2025-3-23 12:21

作者: Aerophagia    時(shí)間: 2025-3-23 15:13

作者: 優(yōu)雅    時(shí)間: 2025-3-23 20:25

作者: 正常    時(shí)間: 2025-3-24 01:29
Future developments,arize plans for some future new facilities. Despite all the advances since the invention of the CCD, many important questions about the Universe remain to be answered, and the experiments needed to study these questions will spur the development of new technology. Larger telescopes, better detectors
作者: 調(diào)整    時(shí)間: 2025-3-24 06:20
Textbook 2008Latest editionstronomical 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 Hubbl
作者: bourgeois    時(shí)間: 2025-3-24 06:57
level that will serve both advanced undergraduate and gradu.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 char
作者: 向前變橢圓    時(shí)間: 2025-3-24 11:00
Rolf F?re,Shawna Grosskopf,R. Robert Russelln the telescope dome are important steps in obtaining good images. Following a brief historical review of telescope development, we consider some basic optical properties and their applications to telescope design.
作者: 和平    時(shí)間: 2025-3-24 17:02

作者: 組成    時(shí)間: 2025-3-24 21:18

作者: 嫻熟    時(shí)間: 2025-3-25 02:21
Finanzierungstheoretische Grundlagen, as FITS. Astronomical software is a vast subject beyond the scope of a single chapter. Our goal here is to introduce some well-known software packages but focus more on basic concepts including image visualization, high-pass and low-pass filtering, false color and image restoration by deconvolution.
作者: Decimate    時(shí)間: 2025-3-25 03:40
https://doi.org/10.1007/978-3-030-96818-2ion of infrared facilities. In contrast to UV, X-ray, and gamma-ray astronomy, there are extensive opportunities to make infrared observations from ground-based sites, as well as from the stratosphere and from space.
作者: CRAMP    時(shí)間: 2025-3-25 10:03

作者: 他姓手中拿著    時(shí)間: 2025-3-25 15:40
https://doi.org/10.1057/9781137367105n to be answered, and the experiments needed to study these questions will spur the development of new technology. Larger telescopes, better detectors, and more efficient instruments are a few of the driving factors.
作者: 浪費(fèi)物質(zhì)    時(shí)間: 2025-3-25 19:20

作者: 尖酸一點(diǎn)    時(shí)間: 2025-3-25 22:54

作者: 蒼白    時(shí)間: 2025-3-26 02:51

作者: Synthesize    時(shí)間: 2025-3-26 05:17

作者: parsimony    時(shí)間: 2025-3-26 09:03
Charge-coupled devices,. 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 how CCDs work. Practical details will follow in the next chapter.
作者: 動(dòng)物    時(shí)間: 2025-3-26 13:49
Image processing and analysis, as FITS. Astronomical software is a vast subject beyond the scope of a single chapter. Our goal here is to introduce some well-known software packages but focus more on basic concepts including image visualization, high-pass and low-pass filtering, false color and image restoration by deconvolution.
作者: JIBE    時(shí)間: 2025-3-26 18:08
Electronic imaging at infrared wavelengths,ion of infrared facilities. In contrast to UV, X-ray, and gamma-ray astronomy, there are extensive opportunities to make infrared observations from ground-based sites, as well as from the stratosphere and from space.
作者: ICLE    時(shí)間: 2025-3-26 22:19
Electronic imaging at ultraviolet, X-ray, and gamma-ray wavelengths, will be explained. High-energy photons with extremely small (sub-atomic) wavelengths require different kinds of detectors, and even the telescope design must change. Within the scope of this text, we can only illustrate some of the most important innovations and advances that have made imaging possible in these exciting fields.
作者: gruelling    時(shí)間: 2025-3-27 02:45

作者: BUCK    時(shí)間: 2025-3-27 09:19

作者: 單挑    時(shí)間: 2025-3-27 12:34

作者: 主動(dòng)脈    時(shí)間: 2025-3-27 15:34
978-3-642-09532-0Springer-Verlag Berlin Heidelberg 2008
作者: 無底    時(shí)間: 2025-3-27 18:33
https://doi.org/10.1007/978-3-540-76583-7Adaptive Optics; Astronomical Detectors; Astronomical Instrumentation; CCDs; Textbook; image processing; o
作者: Heretical    時(shí)間: 2025-3-28 00:06
E. A. Selvanathan,D. S. Prasada Rao realized that careful astronomical observations were important to survival because such observations enabled them to predict seasonal events, such as when to plant and when to harvest. Observational astronomy was also one of the earliest scientific activities.
作者: conduct    時(shí)間: 2025-3-28 05:29

作者: 臭名昭著    時(shí)間: 2025-3-28 06:44
Rolf F?re,Shawna Grosskopf,R. Robert Russellollected and focused, but telescopes must do more than gather light. Providing excellent telescope optics, good tracking, and minimum air turbulence in the telescope dome are important steps in obtaining good images. Following a brief historical review of telescope development, we consider some basi
作者: 傻瓜    時(shí)間: 2025-3-28 14:04
International Council of Opthalmologytor. To motivate a more detailed study of detectors and instrumentation, this chapter provides a limited review of the kinds of measurements that can be made. In the space available only a small and incomplete sampling is possible. Subsequent chapters cover the underlying principles of instruments a
作者: 軍火    時(shí)間: 2025-3-28 17:29
Index der Krystallformen der MineralienIn this chapter each class of instrument is examined in more detail. For optical instruments, typical layouts are shown and the basic relationships involving spatial and spectral resolution are given. Each major type of detector is introduced and the basic properties of semiconductors are also prese
作者: Grievance    時(shí)間: 2025-3-28 20:19

作者: 感激小女    時(shí)間: 2025-3-29 00:44
Index der Krystallformen der Mineralienat 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
作者: 雄偉    時(shí)間: 2025-3-29 04:04

作者: 蛛絲    時(shí)間: 2025-3-29 10:20

作者: Basal-Ganglia    時(shí)間: 2025-3-29 12:29
Finanzierungstheoretische Grundlagen,s, numerical simulations, and more. In this chapter we present some important terminology and explain the standard astronomical data file format known as FITS. Astronomical software is a vast subject beyond the scope of a single chapter. Our goal here is to introduce some well-known software package
作者: Priapism    時(shí)間: 2025-3-29 17:23

作者: 胎兒    時(shí)間: 2025-3-29 22:23





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