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Diffraction-limited Imaging With Large And Moderate Telescopes [Kietas viršelis]

(Indian Inst Of Astrophysics, India)
  • Formatas: Hardback, 636 pages
  • Išleidimo metai: 21-Jun-2007
  • Leidėjas: World Scientific Publishing Co Pte Ltd
  • ISBN-10: 9812707778
  • ISBN-13: 9789812707772
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 636 pages
  • Išleidimo metai: 21-Jun-2007
  • Leidėjas: World Scientific Publishing Co Pte Ltd
  • ISBN-10: 9812707778
  • ISBN-13: 9789812707772
Kitos knygos pagal šią temą:
This book deals with the fundamentals of wave optics, polarization, interference, diffraction, imaging, and the origin, properties, and optical effects of turbulence in the Earth's atmosphere. Techniques developed during the last few decades to overcome atmospheric image degradation (including passive methods, speckle interferometry in particular, and active methods such as adaptive optics), are highlighted. Also discussed are high resolution sensors, image processing, and the astronomical results obtained with these techniques.
Preface vii
Principal symbols xiii
List of acronyms
xvii
Introduction to electromagnetic theory
1(26)
Introduction
1(1)
Maxwell's equations
1(6)
Charge continuity equation
3(2)
Boundary conditions
5(2)
Energy flux of electromagnetic field
7(3)
Conservation law of the electromagnetic field
10(4)
Electromagnetic wave equations
14(13)
The Poynting vector and the Stokes parameter
16(5)
Harmonic time dependence and the Fourier transform
21(6)
Wave optics and polarization
27(54)
Electromagnetic theory of propagation
27(8)
Intensity of a light wave
28(2)
Harmonic plane waves
30(4)
Harmonic spherical waves
34(1)
Complex representation of monochromatic light waves
35(9)
Superposition of waves
37(3)
Standing waves
40(1)
Phase and group velocities
41(3)
Complex representation of non-monochromatic fields
44(13)
Convolution relationship
47(2)
Case of quasi-monochromatic light
49(2)
Successive wave-trains emitted by an atom
51(3)
Coherence length and coherence time
54(3)
Polarization of plane monochromatic waves
57(24)
Stokes vector representation
61(4)
Optical elements required for polarimetry
65(6)
Degree of polarization
71(3)
Transformation of Stokes parameters
74(3)
Polarimeter
77(2)
Imaging polarimeter
79(2)
Interference and diffraction
81(46)
Fundamentals of interference
81(1)
Interference of two monochromatic waves
81(15)
Young's double-slit experiment
86(4)
Michelson's interferometer
90(4)
Mach-Zehnder interferometer
94(2)
Interference with quasi-monochromatic waves
96(6)
Propagation of mutual coherence
102(4)
Propagation laws for the mutual coherence
102(2)
Wave equations for the mutual coherence
104(2)
Degree of coherence from an extended incoherent source: partial coherence
106(6)
The van Cittert-Zernike theorem
107(3)
Coherence area
110(2)
Diffraction
112(15)
Derivation of the diffracted field
114(3)
Fresnel approximation
117(2)
Fraunhofer approximation
119(2)
Diffraction by a rectangular aperture
121(2)
Diffraction by a circular pupil
123(4)
Image formation
127(32)
Image of a source
127(14)
Coherent imaging
132(2)
Incoherent imaging
134(1)
Optical transfer function
135(4)
Image in the presence of aberrations
139(2)
Imaging with partially coherent beams
141(8)
Effects of a transmitting object
141(2)
Transmission of mutual intensity
143(3)
Images of trans-illuminated objects
146(3)
The optical telescope
149(10)
Resolving power of a telescope
154(2)
Telescope aberrations
156(3)
Theory of atmospheric turbulence
159(52)
Earth's atmosphere
159(2)
Basic formulations of atmospheric turbulence
161(18)
Turbulent flows
162(2)
Inertial subrange
164(2)
Structure functions of the velocity field
166(1)
Kolmogorov spectrum of the velocity field
167(3)
Statistics of temperature fluctuations
170(2)
Refractive index fluctuations
172(4)
Experimental validation of structure constants
176(3)
Statistical properties of the propagated wave through turbulence
179(8)
Contribution of a thin layer
180(2)
Computation of phase structure function
182(2)
Effect of Fresnel diffraction
184(1)
Contribution of multiple turbulent layers
185(2)
Imaging in randomly inhomogeneous media
187(10)
Seeing-limited images
188(4)
Atmospheric coherence length
192(3)
Atmospheric coherence time
195(1)
Aniso-planatism
196(1)
Image motion
197(14)
Variance due to angle of arrival
198(2)
Scintillation
200(1)
Temporal evolution of image motion
201(1)
Image blurring
202(2)
Measurement of r0
204(1)
Seeing at the telescope site
205(2)
Wind shears
207(1)
Dome seeing
207(2)
Mirror seeing
209(2)
Speckle imaging
211(48)
Speckle phenomena
211(9)
Statistical properties of speckle pattern
213(2)
Superposition of speckle patterns
215(1)
Power-spectral density
216(4)
Speckle pattern interferometry with rough surface
220(7)
Principle of speckle correlation fringe formation
220(4)
Speckle correlation fringes by addition
224(1)
Speckle correlation fringes by subtraction
225(2)
Stellar speckle interferometry
227(19)
Outline of the theory of speckle interferometry
229(3)
Benefit of short-exposure images
232(1)
Data processing
233(2)
Noise reduction using Wiener filter
235(3)
Simulations to generate speckles
238(2)
Speckle interferometer
240(3)
Speckle spectroscopy
243(1)
Speckle polarimetry
244(2)
Pupil-plane interferometry
246(7)
Estimation of object modulus
246(2)
Shear interferometry
248(5)
Aperture synthesis with single telescope
253(6)
Phase-closure method
253(2)
Aperture masking method
255(2)
Non-redundant masking interferometer
257(2)
Adaptive optics
259(52)
Basic principles
259(5)
Greenwood frequency
260(2)
Thermal blooming
262(2)
Wavefront analysis using Zernike polynomials
264(7)
Definition of Zernike polynomial and its properties
264(3)
Variance of wavefront distortions
267(2)
Statistics of atmospheric Zernike coefficients
269(2)
Elements of adaptive optics systems
271(40)
Steering/tip-tilt mirrors
273(1)
Deformable mirrors
274(1)
Segmented mirrors
275(1)
Ferroelectric actuators
276(2)
Deformable mirrors with discrete actuators
278(2)
Bimorph deformable mirror (BDM)
280(1)
Membrane deformable mirrors
281(3)
Liquid crystal DM
284(1)
Deformable mirror driver electronics
285(1)
Wavefront sensors
286(1)
Shack Hartmann (SH) wavefront sensor
287(4)
Curvature sensing
291(2)
Pyramid WFS
293(2)
Wavefront reconstruction
295(1)
Zonal and modal approaches
296(2)
Servo control
298(2)
Accuracy of the correction
300(4)
Reference source
304(4)
Adaptive secondary mirror
308(1)
Multi-conjugate adaptive optics
309(2)
High resolution detectors
311(50)
Photo-electric effect
311(20)
Detecting light
312(2)
Photo-detector elements
314(4)
Detection of photo-electrons
318(5)
Photo-multiplier tube
323(4)
Image intensifiers
327(4)
Charge-coupled device (CCD)
331(12)
Readout procedure
334(2)
Characteristic features
336(1)
Quantum efficiency
336(1)
Charge Transfer efficiency
337(1)
Gain
337(1)
Dark current
338(1)
Calibration of CCD
339(2)
Intensified CCD
341(2)
Photon-counting sensors
343(10)
CCD-based photon-counting system
345(1)
Digicon
346(1)
Precision analog photon address (PAPA) camera
347(1)
Position sensing detectors
348(1)
Special anode cameras
349(4)
Solid state technologies
353(5)
Electron multiplying charge coupled device (EMCCD)
353(4)
Superconducting tunnel junction
357(1)
Avalanche photo-diodes
357(1)
Infrared sensors
358(3)
Image processing
361(36)
Post-detection image reconstruction
361(21)
Shift-and-add algorithm
362(2)
Selective image reconstruction
364(1)
Speckle holography
365(1)
Cross-spectrum analysis
366(1)
Differential speckle interferometry
367(1)
Knox-Thomson technique (KT)
368(3)
Triple-correlation technique
371(4)
Deciphering phase from bispectrum
375(4)
Relationship between KT and TC
379(3)
Iterative deconvolution techniques
382(8)
Fienup algorithm
383(1)
Blind iterative deconvolution (BID) technique
384(3)
Richardson-Lucy algorithm
387(1)
Maximum entropy method (MEM)
388(1)
Pixon
389(1)
Miscellaneous iterative algorithms
390(1)
Phase retrieval
390(7)
Phase-unwrapping
392(2)
Phase-diversity
394(3)
Astronomy fundamentals
397(78)
Black body radiation
397(12)
Cavity radiation
398(2)
Planck's law
400(3)
Application of blackbody radiation concepts to stellar emission
403(2)
Radiation mechanism
405(1)
Atomic transition
406(2)
Hydrogen spectra
408(1)
Astronomical measurements
409(36)
Flux density and luminosity
409(3)
Magnitude scale
412(1)
Apparent magnitude
413(1)
Absolute magnitude
413(1)
Bolometric corrections
414(1)
Distance scale
415(3)
Extinction
418(1)
Interstellar extinction
418(2)
Color excess
420(2)
Atmospheric extinction
422(1)
Instrumental magnitudes
423(1)
Color and magnitude transformation
424(1)
UBV transformation equations
425(2)
Stellar temperature
427(1)
Effective temperature
427(1)
Brightness temperature
428(1)
Color temperature
428(1)
Kinetic temperature
429(1)
Excitation temperature
430(1)
Ionization temperature
431(1)
Stellar spectra
432(3)
Hertzsprung-Russell (HR) diagram
435(3)
Spectral classification
438(4)
Utility of stellar spectrum
442(3)
Binary stars
445(14)
Masses of stars
445(1)
Types of binary systems
446(1)
Visual binaries
447(1)
Spectroscopic binaries
447(3)
Eclipsing binaries
450(2)
Astrometric binaries
452(1)
Binary star orbits
453(1)
Apparent orbit
454(2)
Orbit determination
456(3)
Conventional instruments at telescopes
459(9)
Imaging with CCD
460(1)
Photometer
461(3)
Spectrometer
464(4)
Occultation technique
468(7)
Methodology of occultation observation
469(3)
Science with occultation technique
472(3)
Astronomical applications
475(78)
High resolution imaging of extended objects
475(22)
The Sun
476(1)
Solar structure
477(7)
Transient phenomena
484(5)
Solar interferometric observations
489(2)
Solar speckle observation during eclipse
491(2)
Jupiter
493(2)
Asteroids
495(2)
Stellar objects
497(50)
Measurement of stellar diameter
497(3)
Variable stars
500(1)
Pulsating variables
500(3)
Eruptive variables
503(1)
Cataclysmic variables
504(2)
Young stellar objects
506(8)
Circumstellar shell
514(4)
Planetary nebulae
518(5)
Supernovae
523(3)
Close binary systems
526(3)
Multiple stars
529(2)
Extragalactic objects
531(3)
Active galactic nuclei (AGN)
534(7)
Quasars
541(1)
Impact of adaptive optics in astrophysics
542(5)
Dark speckle method
547(6)
Appendix A Typical tables
553(4)
Appendix B Basic mathematics for Fourier optics
557(20)
Fourier transform
557(10)
Basic properties and theorem
558(3)
Discrete Fourier transform
561(1)
Convolution
561(2)
Autocorrelation
563(1)
Parseval's theorem
564(1)
Some important corollaries
565(1)
Hilbert transform
566(1)
Laplace transform
567(2)
Probability, statistics, and random processes
569(8)
Probability distribution
569(4)
Parameter estimation
573(2)
Central-limit theorem
575(1)
Random fields
575(2)
Appendix C Bispectrum and phase values using triple-correlation algorithm
577(2)
Bibliography 579(16)
Index 595