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Detection of Light: From the Ultraviolet to the Submillimeter 2nd Revised edition [Pehme köide]

(University of Arizona)
  • Formaat: Paperback / softback, 376 pages, kõrgus x laius x paksus: 246x175x22 mm, kaal: 838 g, 18 Tables, unspecified; 11 Halftones, unspecified; 112 Line drawings, unspecified
  • Ilmumisaeg: 17-Oct-2002
  • Kirjastus: Cambridge University Press
  • ISBN-10: 0521017106
  • ISBN-13: 9780521017107
  • Formaat: Paperback / softback, 376 pages, kõrgus x laius x paksus: 246x175x22 mm, kaal: 838 g, 18 Tables, unspecified; 11 Halftones, unspecified; 112 Line drawings, unspecified
  • Ilmumisaeg: 17-Oct-2002
  • Kirjastus: Cambridge University Press
  • ISBN-10: 0521017106
  • ISBN-13: 9780521017107
A course text or self-study tutorial that bridges between general physics and the advanced detection of photons. Students are assumed to have completed a semester or two of college-level physics with calculus; the necessary radiometry and solid state physics are reviewed in the first chapter. The first edition was published in 1994. Annotation c. Book News, Inc., Portland, OR (booknews.com)

A comprehensive overview of important approaches to photon detection from ultraviolet to submillimeter spectral regions.

Detection of Light provides a comprehensive overview of the important approaches to photon detection from the ultraviolet to the submillimeter spectral regions. This expanded and fully updated second edition discusses recently introduced types of detector: superconducting tunnel junctions, hot electron bolometer mixers, and fully depleted CCDs. It also includes historically important devices such as photographic plates. Material from many disciplines is combined into a comprehensive and unified treatment of the detection of light, with emphasis on the underlying physical principles.

Arvustused

'Although on the face of it a hard science volume, this book is still quite readable. This is due to the progressive style in which each topic is approached this book does provide a complete introduction and reference volume to the world of photon detection.' Alex Colburn, Webb Society Reviews 'The book is well laid out and covers most of the basic solid state physics required to understand how the various types of detectors work. I found the diagrams very clear and the examples well thought through. It is certainly a book that I wish I had had available as an undergraduate when studying detection systems in astronomy.' Owen Brazell, Astronomy Now 'In summary this is a must for anyone involved in millimetre-to-ultraviolet instrumentation, and will also be of interest to the non-specialist who wants to keep abreast of photo-detection technology.' Observatory ' This book is clearly and authoritatively written, and should appeal to astronomers, engineers and physicists, and prove particularly useful to the advanced university student.' Irish Astronomical Journal ' providing in a single source a comprehensive, up-to-date overview of the field. Whether used as a text or as a reference, an invaluable addition.' Physics Today 'In my view, this book is a 'must' for any laboratory where experimental work involves the detection of electromagnetic radiation - which means pretty well any laboratory this is an excellent reference work.' Contemporary Physics

Muu info

A comprehensive overview of important approaches to photon detection from ultraviolet to submillimeter spectral regions.
Preface ix
Introduction
1(30)
Radiometry
1(7)
Detector types
8(1)
Performance characteristics
8(9)
Solid state physics
17(7)
Superconductors
24(1)
Examples
25(2)
Problems
27(4)
Notes
29(1)
Further reading
29(2)
Intrinsic photoconductors
31(26)
Basic operation
32(7)
Limitations and optimization
39(11)
Performance specification
50(3)
Example: design of a photoconductor
53(1)
Problems
54(3)
Notes
56(1)
Further reading
56(1)
Extrinsic photoconductors
57(21)
Basics
58(3)
Limitations
61(7)
Variants
68(8)
Problems
76(2)
Note
77(1)
Further reading
77(1)
Photodiodes and other junction-based detectors
78(38)
Basic operation
79(5)
Quantitative description
84(12)
Photodiode variations
96(7)
Quantum well detectors
103(6)
Superconducting tunnel junctions (STJs)
109(4)
Example
113(1)
Problems
113(3)
Further reading
115(1)
Amplifiers and readouts
116(29)
Building blocks
116(3)
Load resistor and amplifier
119(1)
Transimpedance amplifier (TIA)
120(5)
Integrating amplifiers
125(9)
Performance measurement
134(5)
Examples
139(3)
Problems
142(3)
Further reading
143(2)
Arrays
145(42)
Overview
146(1)
Infrared arrays
147(4)
Charge coupled devices (CCDs)
151(24)
CMOS imaging arrays
175(1)
Direct hybrid PIN diode arrays
176(1)
Array properties
176(5)
Example
181(2)
Problems
183(4)
Notes
185(1)
Further reading
185(2)
Photoemissive detectors
187(30)
General description
187(6)
Photocathode behavior and photon detection limits
193(2)
Practical detectors
195(16)
Vacuum tube television-type imaging detectors
211(2)
Example
213(2)
Problems
215(2)
Further reading
216(1)
Photography
217(21)
Basic operation
217(2)
Underlying processes
219(5)
Characteristic curve
224(2)
Performance
226(9)
Example
235(1)
Problems
236(2)
Further reading
237(1)
Bolometers and other thermal detectors
238(37)
Basic operation
239(1)
Detailed theory of semiconductor bolometers
240(10)
Superconducting bolometers
250(4)
Bolometer construction and operation
254(10)
Other thermal detectors
264(4)
Operating temperature
268(3)
Example: design of a bolometer
271(2)
Problems
273(2)
Note
274(1)
Further reading
274(1)
Visible and infrared coherent receivers
275(27)
Basic operation
275(4)
Visible and infrared heterodyne
279(7)
Performance attributes of heterodyne receivers
286(10)
Test procedures
296(1)
Examples
297(3)
Problems
300(2)
Notes
301(1)
Further reading
301(1)
Submillimeter- and millimeter-wave heterodyne receivers
302(29)
Basic operation
302(4)
Mixers
306(14)
Performance characteristics
320(2)
Local oscillators
322(4)
Problems
326(5)
Notes
327(3)
Further reading
330(1)
Summary
331(11)
Quantum efficiency and noise
331(1)
Linearity and dynamic range
332(1)
Number of pixels
332(1)
Time response
333(1)
Spectral response and bandwidth
334(1)
Practical considerations
334(1)
Overview
335(1)
Problems
335(3)
Note
336(1)
Further reading
336(2)
Appendices
A Physical constants
338(1)
B Answers to selected problems
339(3)
References 342(14)
Index 356


George Rieke is a Professor of Astronomy and Planetary Sciences at the University of Arizona.