Observational Astrophysics

by ; ; ;
Edition: 2nd
Format: Hardcover
Pub. Date: 1999-01-01
Publisher(s): Springer Verlag
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Summary

Written specifically for physicists and graduate students, this textbook focuses on fundamental and sometimes practical limitations on the ultimate performance that an astronomical system may reach, rather than presenting particular systems in detail. This second edition has been entirely restructured and almost doubled in size, in order to improve its clarity and to account for the great progress achieved in the last 15 years. It deals with ground-based and space-based astronomy and their respective fields. It presents the new generation of giant ground-based telescopes, with the new methods of optical interferometry and adaptive optics. But it also presents the ambitious concepts behind space missions aimed for the next decades. Avoiding particulars, it covers the whole of the electromagnetic spectrum, and touches upon the "new astronomies" becoming possible with gravitational waves and neutrinos.

Table of Contents

1. Astrophysical Information
1(30)
1.1 Carriers of Information
2(7)
1.2 Collecting and Analysing Information
9(17)
1.2.1 The Main Characteristics of Photons
9(1)
1.2.2 Observing Systems
10(16)
1.2.3 Reaching a Systematic Description of Observation
26(1)
1.3 Strategies and Costs
26(5)
2. The Earth's Atmosphere and Space
31(48)
2.1 Physical and Chemical Structure of the Atmosphere
32(4)
2.1.1 Vertical Structure
32(1)
2.1.2 Constituents of the Atmosphere
33(3)
2.2 Absorption of Radiation
36(5)
2.3 Atmospheric Emission
41(7)
2.3.1 Fluorescent Emission
41(3)
2.3.2 Thermal Emission
44(3)
2.3.3 Differential Measurement Techniques
47(1)
2.4 Scattering of Radiation
48(4)
2.5 Atmospheric Refraction and Dispersion
52(1)
2.6 Turbulence Structure of the Earth's Atmosphere
52(8)
2.6.1 Turbulence in the Lower and Middle Atmosphere
53(7)
2.6.2 Ionospheric Turbulence
60(1)
2.7 Terrestrial Observing Sites
60(5)
2.7.1 Visible, Infrared and Millimetre Observations
60(3)
2.7.2 Centimetre Radioastronomy and Beyond
63(1)
2.7.3 Man-Made Pollution and Interference
63(1)
2.7.4 The Antarctic
64(1)
2.8 Observation from Space
65(9)
2.8.1 The Advantages of Observation from Space
66(1)
2.8.2 Sources of Perturbation
66(6)
2.8.3 Choice of Orbits
72(2)
2.9 The Moon as an Astronomical Site
74(1)
2.10 Exercises
75(4)
3. Radiation and Photometry
79(28)
3.1 Radiometry
80(4)
3.2 Aspects of Radiation
84(6)
3.2.1 Blackbody Radiation
84(1)
3.2.2 Coherence
85(5)
3.3 Magnitudes
90(2)
3.4 Photometry Through the Atmosphere
92(1)
3.5 Calibration and Intensity Standards
93(12)
3.5.1 Radiofrequencies (Lambda is greater than 1 mm)
94(1)
3.5.2 Submillimetre, Infrared and Visible
95(5)
3.5.3 Ultraviolet and X-Rays (0.1 nm is less than Lambda is less than 300 nm)
100(2)
3.5.4 Gamma Radiation
102(1)
3.5.5 Some Examples of Spectrophotometry
102(3)
3.6 Exercises
105(2)
4. Telescopes and Images
107(90)
4.1 Image and Object in Astronomy
108(7)
4.1.1 Geometrical Images
109(5)
4.1.2 Gravitational Optics
114(1)
4.2 Diffraction and Image Formation
115(18)
4.2.1 The Zernike-van Cittert Theorem
115(5)
4.2.2 Diffraction at Infinity. Pupils
120(5)
4.2.3 Pupils and Spatial Filtering
125(6)
4.2.4 Waveguides and Fibre Optics
131(2)
4.3 Telescopes
133(34)
4.3.1 Radiotelescopes (Beyond the Submillimetre Range)
133(13)
4.3.2 Ground-Based Optical Telescopes (Visible and Infrared)
146(3)
4.3.3 Aperture Synthesis in the Visible and Infrared
149(8)
4.3.4 Space Telescopes, from Ultraviolet to Submillimetre
157(2)
4.3.5 X-Ray Telescopes (0.1-10 keV)
159(1)
4.3.6 Gamma-Ray Telescopes (Greater than 10 keV)
160(7)
4.4 Image Degradation by the Atmosphere
167(17)
4.4.1 Perturbations of the Wavefront
168(3)
4.4.2 Image Formation
171(1)
4.4.3 Short-Exposure Images and Speckle Interferometry
172(3)
4.4.4 Adaptive Optics
175(7)
4.4.5 Phase Perturbations in Aperture Synthesis
182(2)
4.5 Image Processing
184(4)
4.5.1 The Principal Solution
185(1)
4.5.2 Methods of Information Restitution
186(2)
4.6 Exercises
188(9)
5. Spectral Analysis
197(58)
5.1 Astrophysical Spectra
198(17)
5.1.1 Formation of Spectra
198(6)
5.1.2 Information in Spectrometry
204(6)
5.2 General Features of Spectrometers
210(5)
5.3 Interferometric Spectrometers
215(29)
5.3.1 General Criteria
215(1)
5.3.2 Interference Filters
216(1)
5.3.3 Grating Spectrometers
217(15)
5.3.4 Fourier Transform Spectrometers
232(7)
5.3.5 The Fabry-Perot Spectrometers
239(2)
5.3.6 The Bragg Crystal Spectrometer (X-ray Region)
241(3)
5.4 Radiofrequency Spectrometer
244(6)
5.4.1 Multichannel Spectrometers
246(1)
5.4.2 The Acoustic Spectrometer
247(1)
5.4.3 The Autocorrelation Spectrometer
247(1)
5.4.4 Submillimetre Developments
248(2)
5.5 Resonance Spectrometers
250(2)
5.6 Exercises
252(3)
6. The Signal in Astronomy
255(34)
6.1 The Signal and Its Fluctuations
256(16)
6.1.1 Observing System and Signal
256(1)
6.1.2 Signal and Fluctuations. Noise
257(6)
6.1.3 Elementary Signal Processing
263(8)
6.1.4 A Specific Example of Data Processing
271(1)
6.2 Fundamental Fluctuations
272(10)
6.2.1 Quantum Noise
276(3)
6.2.2 Thermal Noise
279(3)
6.3 Exercises
282(7)
7. Detectors
289(96)
7.1 General Properties
290(8)
7.1.1 Amplitude Detectors. Quadratic Detectors
290(2)
7.1.2 Spatial Structure of Detectors
292(3)
7.1.3 Temporal Response
295(1)
7.1.4 Detector Noise
296(1)
7.1.5 Characterisation of Detectors
297(1)
7.2 Physical Principles of the Detection of Electromagnetic Radiation
298(14)
7.2.1 Detection of Quanta
299(10)
7.2.2 Detection of the Electromagnetic Field
309(3)
7.3 The Main Astronomical Detectors
312(46)
7.3.1 Photographic Plates
312(4)
7.3.2 Photomultipliers and Classical Cameras (X-Ray, UV and Visible)
316(8)
7.3.3 Solid-State Imagers
324(14)
7.3.4 Detectors for the Visible and Ultraviolet
338(2)
7.3.5 Other Infrared Detectors (1-1 000 Mum)
340(5)
7.3.6 General Features of Radiofrequency Detection
345(7)
7.3.7 Radiofrequency Detectors
352(6)
7.4 High-Energy Detectors (X- and Gamma-Ray)
358(13)
7.4.1 X-Ray Detection (0.1-10 keV)
358(4)
7.4.2 Gamma-Ray Detection (Greater than 10 keV)
362(9)
7.5 Neutrino Detection
371(3)
7.5.1 Inelastic Reaction Detectors
371(2)
7.5.2 Momentum Transfer Detectors
373(1)
7.6 Gravitational Wave Detection
374(5)
7.7 Exercises
379(6)
8. Space-Time Reference Frames
385(34)
8.1 Spatial Reference Systems
385(12)
8.1.1 Definitions of Spatial Frames
385(2)
8.1.2 A List of Astronomical Reference Frames
387(6)
8.1.3 Change of Frame
393(4)
8.2 Practical Realisation of Spatial Frames
397(11)
8.2.1 Celestial Reference Systems
397(1)
8.2.2 Fundamental Catalogues
398(1)
8.2.3 The Extra-Galactic System
399(4)
8.2.4 The Hipparcos Frame
403(5)
8.3 Temporal Reference Systems
408(11)
8.3.1 Time Scales
408(2)
8.3.2 Atomic Time
410(4)
8.3.3 Coordinated Universal Time (CUT or UTC)
414(1)
8.3.4 Dynamical Time Scales
415(2)
8.3.5 Dates and Epochs
417(2)
Appendix A. Fourier Transforms
419(16)
A.1 Definitions and Properties
419(11)
A.1.1 Definitions
419(1)
A.1.2 Some Properties
420(1)
A.1.3 Important Special Cases in One Dimension
421(3)
A.1.4 Important Special Cases in Two Dimensions
424(1)
A.1.5 Important Theorems
425(5)
A.2 Physical Quantities and Fourier Transforms
430(3)
A.3 Wavelets
433(2)
Appendix B. Random Processes and Variables
435(22)
B.1 Random Variables
435(7)
B.2 Random or Stochastic Processes
442(7)
B.3 Physical Measurements and Estimates
449(8)
B.3.1 An Example of Estimation: Law of Large Numbers
450(1)
B.3.2 Estimating the Moments of a Process
451(2)
B.3.3 Estimation and Bias
453(4)
Appendix C. Physical and Astronomical Constants
457(2)
Appendix D. Tables of Space Missions
459(4)
Appendix E. Astronomy on the World Wide Web
463(18)
Appendix F. Acronyms and Abbreviations
481(4)
Bibliography 485(16)
Index 501

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