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9780521828727

An Introduction to Optical Stellar Interferometry

by
  • ISBN13:

    9780521828727

  • ISBN10:

    0521828724

  • Format: Hardcover
  • Copyright: 2006-07-24
  • Publisher: Cambridge University Press

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Summary

During the last two decades, optical stellar interferometry has become an important tool in astronomical investigations requiring spatial resolution well beyond that of traditional telescopes. This is the first book to be written on the subject. The authors provide an extended introduction discussing basic physical and atmospheric optics, which establishes the framework necessary to present the ideas and practice of interferometry as applied to the astronomical scene. They follow with an overview of historical, operational and planned interferometric observatories, and a selection of important astrophysical discoveries made with them. Finally, they present some as-yet untested ideas for instruments both on the ground and in space which may allow us to image details of planetary systems beyond our own.

Author Biography

Antoine Labeyrie is Professor at the College de France Stephen G. Lipson is Chair of Electro-Optics and Professor of Physics at Technion - Israel Institute of Technology, Haifa Peter Nisenson sutudied physics and optics before becoming a professional astronomer at the Harvard Smithsonian Center for Astrophysics

Table of Contents

List of Illustrations
xii
Preface xxviii
Introduction
1(8)
Historical introduction
1(6)
About this book
7(2)
References
7(2)
Basic concepts: a qualitative introduction
9(14)
A qualitative introduction to the basic concepts and ideas
9(4)
Young's experiment (1801--3)
9(2)
Using Young's slits to measure the size of a light source
11(2)
Some basic wave concepts
13(6)
Plane waves
15(1)
Huygens' principle
15(2)
Superposition
17(2)
Electromagnetic waves and photons
19(4)
References
22(1)
Interference, diffraction and coherence
23(41)
Interference and diffraction
23(17)
Interference and interferometers
24(4)
Diffraction using the scalar wave approximation
28(3)
Fraunhofer diffraction patterns of some simple apertures
31(6)
The point spread function
37(2)
The optical transfer function
39(1)
Coherent light
40(4)
The effect of uncertainties in the frequency and wave vector
40(1)
Coherent light and its importance to interferometry
41(1)
Partial coherence
41(1)
Spatial coherence
42(1)
Temporal coherence
43(1)
A quantitative discussion of coherence
44(8)
Coherence function
45(1)
The relationship between the coherence function and fringe visibility
45(1)
Van Cittert--Zernike theorem
46(6)
Fluctuations in light waves
52(12)
A statistical model for quasimonochromatic light
52(3)
The second-order coherence function
55(1)
Photon noise
56(2)
Photodetectors
58(4)
References
62(2)
Aperture synthesis
64(24)
Aperture synthesis
64(7)
The optics of aperture synthesis
64(2)
Sampling the (u, v) plane
66(3)
The optimal geometry of multiple telescope arrangements
69(2)
From data to image: the phase problem
71(4)
Phase closure
73(2)
Image restoration and the crowding limitation
75(3)
Algorithmic image restoration methods
76(1)
The crowding limitation
77(1)
Signal detection for aperture synthesis
78(3)
Wave mixing and heterodyne recording
78(3)
A quantum interpretation of aperture synthesis
81(2)
A lecture demonstration of aperture synthesis
83(5)
References
87(1)
Optical effects of the atmosphere
88(32)
Introduction
88(2)
A qualitative description of optical effects of the atmosphere
90(3)
Quantitative measures of the atmospheric aberrations
93(3)
Kolmogorov's (1941) description of turbulence
93(2)
Parameters describing the optical effects of turbulence: Correlation and structure functions. B(r) and D(r).
95(1)
Phase fluctuations in a wave propagating through the atmosphere
96(6)
Fried's parameter r0 describes the size of the atmospheric correlation region
99(1)
Correlation between phase fluctuations in waves with different angles of incidence: the isoplanatic patch
100(2)
Temporal fluctuations
102(6)
The wind-driven ``frozen turbulence'' hypothesis
102(1)
Frequency spectrum of fluctuations
102(1)
Intensity fluctuations: twinkling
103(5)
Dependence on Height
108(1)
Dependence of atmospheric effects on the wavelength
108(1)
Adaptive optics
109(6)
Measuring the wavefront distortion
111(2)
Deformable mirrors
113(1)
Tip--tilt correction
114(1)
Guide stars
114(1)
Short exposure images: speckle patterns
115(5)
A model for a speckle image
116(3)
References
119(1)
Single-aperture techniques
120(21)
Introduction
120(3)
Masking the aperture of a large telescope
123(3)
Using the whole aperture: speckle interferometry
126(8)
Theory of speckle interferometry
128(2)
Experimental speckle interferometry
130(3)
Some early results of speckle interferometry
133(1)
Speckle imaging
134(7)
The Knox--Thompson algorithm
135(1)
Speckle masking, or triple correlation
136(3)
Spectral speckle masking
139(1)
References
139(2)
Intensity interferometry
141(17)
Introduction
141(1)
Intensity fluctuations and the second-order coherence function
142(5)
The classical wave interpretation
142(4)
The quantum interpretation
146(1)
Estimating the sensitivity of fluctuation correlations
147(2)
The Narrabri intensity interferometer
149(3)
The electronic correlator
150(2)
Data analysis
152(2)
Double stars
152(2)
Stellar diameters
154(1)
Limb darkening
154(1)
Astronomical results
154(1)
Retrieving the phase
155(1)
Conclusion
156(2)
References
157(1)
Amplitude interferometry: techniques and instruments
158(54)
Introduction
158(3)
The Michelson stellar interferometer
159(1)
The Narrabri Intensity Interferometer
160(1)
Aperture masking
161(1)
What do we demand of an interferometer?
161(1)
The components of modern amplitude interferometers
162(22)
Subapertures and telescopes
163(2)
Beam lines and their dispersion correction
165(2)
Correction of angular dispersion
167(1)
Path-length equalizers or delay lines
168(2)
Beam-reducing optics
170(1)
Beam combiners
170(2)
Semireflective beam-combiners
172(2)
Optical fiber and integrated optical beam-combiners
174(1)
Star tracking and tip--tilt correction
175(4)
Fringe dispersion and tracking
179(1)
Estimating the fringe parameters
180(3)
Techniques for measuring in the photon-starved region
183(1)
Modern interferometers with two subapertures
184(13)
Heterodyne interferometers
185(1)
Interferometre a 2 Telescopes (I2T)
186(1)
Grand interferometre a deux telescopes (GI2T)
186(3)
The Mark III Interferometer
189(1)
Sydney University stellar interferometer (SUSI)
189(2)
The large binocular telescope (LBT)
191(2)
The Mikata optical and infrared array (MIRA-I.2)
193(1)
Palomar testbed interferometer (PTI)
193(3)
Keck interferometer
196(1)
Interferometers with more than two subapertures
197(15)
The Cambridge optical aperture synthesis telescope (COAST)
197(3)
Center for High Angular Resolution Astronomy (CHARA)
200(2)
Infrared optical telescope array (IOTA)
202(1)
Navy prototype optical interferometer (NPOI)
203(2)
The Berkeley infrared spatial interferometer (ISI)
205(3)
Very large telescope interferometer (VLTI)
208(2)
References
210(2)
The hypertelescope
212(20)
Imaging with very high resolution using multimirror telescopes
212(2)
The physical optics of pupil densification
214(7)
A random array of apertures
214(5)
A periodic array of apertures
219(2)
The field of view of a hypertelescope and the crowding limitation
221(3)
Hypertelescope architectures
224(4)
Michelson's stellar interferometer as a hypertelescope, and multi-aperture extensions
224(1)
Hypertelescope versions of multitelescope interferometers
224(1)
Carlina hypertelescopes
224(2)
A fiber-optical version of the hypertelescope
226(2)
Experiments on a hypertelescope system
228(4)
References
231(1)
Nulling and coronagraphy
232(30)
Searching for extrasolar planets and life
232(1)
Planet detection methods
233(3)
The relative luminosities of a star and planet
234(1)
Requirements for imaging planet surface features
235(1)
Apodization
236(4)
Apodization using binary masks
238(1)
Apodization using phase masks
239(1)
Nulling methods in interferometers
240(7)
Bracewell's single-pixel nulling in nonimaging interferometers
241(1)
Bracewell nulling in imaging interferometers
242(1)
Achromatic nulling in Bracewell interferometers
243(2)
Starlight leakage in nulling interferometers
245(2)
Imaging coronagraphy
247(9)
The Lyot coronagraph in its original and stellar versions
248(3)
The Roddier--Roddier phase-dot coronagraph
251(1)
Four-quadrant phase-mask and phase-spiral coronagraphs
251(1)
The achromatic interference coronagraph
252(1)
Elementary modeling of mask coronagraphs
252(1)
Mirror bumpiness tolerance calculated with Marechal's equation
253(3)
High contrast coronagraphy and apodization
256(6)
Adaptive coherent correction of mirror bumpiness
256(1)
Adaptive hologram within the coronagraph
257(2)
Incoherent cleaning of recorded images
259(1)
Comparison of coherent and incoherent cleaning
259(1)
References
260(2)
A sampling of interferometric science
262(16)
Interferometric science
262(1)
Stellar measurements and imaging
262(9)
Stellar diameters and limb darkening
262(3)
Star-spots, hot spots
265(1)
Pulsating stars
266(1)
Miras
267(1)
Young stellar object disks and jets
268(1)
Dust shells, Wolf--Rayets
268(2)
Binary stars
270(1)
Galactic and extragalactic sources
271(3)
SN1987a
271(1)
R136a
272(1)
The galactic center
273(1)
Astrometry
273(1)
Solar system
274(1)
The Galilean satellites
274(1)
Asteroid imaging
274(1)
Pluto--Charon
275(1)
Brown dwarfs
275(1)
Solar feature imaging and dynamics measurements
275(3)
References
276(2)
Future ground and space projects
278(17)
Future ground-based projects
278(6)
New ground-based long-baseline interferometers
279(1)
The optical very large array (OVLA)
280(1)
Toward large Carlina hypertelescopes
281(1)
Comparison of OVLA and Carlina concepts
281(1)
Comparing compact and exploded ELTs
282(1)
Coupling telescopes through fibers: the OHANA project at Mauna Kea
283(1)
Future space projects
284(6)
Flotillas of mirrors
285(1)
Darwin
285(2)
Terrestrial planet finder (TPF)
287(1)
Space interferometry mission (SIM)
288(1)
The exo-Earth imager (EEI)
289(1)
Simulated Exo-Earth-Imager images
290(2)
Some speculations on identifying life from colored patches
291(1)
Extreme baselines for a Neutron Star Imager
292(3)
References
294(1)
Appendix A
295(21)
Electromagnetic waves: a summary
295(3)
Plane and spherical electromagnetic waves
296(1)
Energy and momentum in waves
297(1)
Geometrical phase in wave propagation
298(2)
Fourier theory
300(11)
The Fourier transform
301(1)
Some simple examples
302(3)
Convolution
305(2)
Sampling and aliasing
307(4)
Fraunhofer diffraction
311(5)
Random objects and their diffraction patterns: speckle images
313(3)
Appendix B
316(1)
References 317(2)
Index 319

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