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目录

Prefacepagexi
1.Elementarycoherencephenomena
1.1Interferenceandstatisticalsimilarity
1.2Temporalcoherenceandthecoherencetime
1.3Spatialcoherenceandthecoherencearea
1.4Thecoherencevolume
Problems
2.Mathematicalpreliminaries
2.1Elementaryconceptsofthetheoryofrandomprocesses
2.2Ergodicity
2.3Complexrepresentationofarealsignalandtheenvelopeofanarrow-bandsignal
2.4Theautocorrelationandthecross-correlationfunctions
2.4.1Theautocorrelationfunctionofafinitesumofperiodiccomponentswithrandomamplitudes
2.5ThespectraldensityandtheWiener-Khintchinetheorem
Problems
3.Second-ordercoherencephenomenainthespace-timedomain
3.1Interferencelawforstationaryopticalfields.Themutualcoherencefunctionandthecomplexdegreeofcoherence
3.2Generationofspatialcoherencefromanincoherentsource.ThevanCittert-Zerniketheorem
3.3Illustrativeexamples
3.3.1Michelson"smethodformeasuringstellardiameters
3.3.2Michelson"smethodfordeterminingenergydistributioninspectrallines
3.4Propagationofthemutualintensity
3.5Waveequationsforthepropagationofmutualcoherenceinfreespace
Problems
4.Second-ordercoherencephenomenainthespace-frequencydomain
4.1Coherent-moderepresentationandthecross-spectraldensityasacorrelationfunction
4.2Thespectralinterferencelawandthespectraldegreeofcoherence
4.3Anillustrativeexample:spectralchangesoninterference
4.4Interferenceofnarrow-bandlight
Problems
5.Radiationfromsourcesofdifferentstatesofcoherence
5.1Fieldsgeneratedbysourceswithdifferentcoherenceproperties
5.2Correlationsandthespectraldensityinthefarfield
5.3Radiationfromsomemodelsources
5.3.1Schell-modelsources
5.3.2Quasi-homogeneoussources
5.4Sourcesofdifferentstatesofspatialcoherencewhichgenerateidenticaldistributionsoftheradiantintensity
5.5CoherencepropertiesofLambertiansources
5.6Spectralchangesonpropagation.Thescalinglaw
Problems
6.Coherenceeffectsinscattering
6.1Scatteringofamonochromaticplanewaveonadeterministicmedium
6.2Scatteringofpartiallycoherentwavesonadeterministicmedium
6.3Scatteringonrandommedia
6.3.1Generalformulas
6.3.2Examples
6.3.3Scatteringonaquasi-homogeneousmedium
Problems
7.Higher-ordercoherenceeffects
7.1Introduction
7.2Intensityinterferometrywithradiowaves
7.3TheHanburyBrown-Twisseffectandintensityinterferometrywithlight
7.4Einstein"sformulaforenergyfluctuationsinblackbodyradiationandthewave-particleduality
7.5Mandel"stheoryofphotoelectricdetectionoflightfluctuations
7.5.1Mandel"sformulaforphotocountstatistics
7.5.2Thevarianceofcountsfromasinglephotodetector
7.5.3Correlationbetweencountfluctuationsfromtwodetectors
7.6Determinationofstatisticalpropertiesoflightfromphotocountmeasurements
Problems
8.Elementarytheoryofpolarizationofstochasticelectromagneticbeams
8.1The2_2equal-timecorrelationmatrixofaquasi-monochromaticelectromagneticbeam
8.2Polarized,unpolarizedandpartiallypolarizedlight.Thedegreeofpolarization
8.2.1Completelypolarizedlight
8.2.2Natural(unpolarized)light
8.2.3Partiallypolarizedlightandthedegreeofpolarization
8.2.4Thegeometricalsignificanceofcompletepolarization.TheStokesparametersofcompletelypolarizedlight.ThePoincarésphere
Problems
9.Unifiedtheoryofpolarizationandcoherence
9.1The2×2cross-spectraldensitymatrixofastochasticelectromagneticbeam
9.2Thespectralinterferencelaw,thespectraldegreeofcoherenceandthespectraldegreeofpolarizationofstochasticelectromagneticbeams
9.3Determinationofthecross-spectraldensitymatrixfromexperiments
9.4Changesinrandomelectromagneticbeamsonpropagation
9.4.1Propagationofthecross-spectraldensitymatrixofastochasticelectromagneticbeam-generalformulas
9.4.2Propagationofthecross-spectraldensitymatrixofanelectromagneticGaussianSchell-modelbeam
9.4.3Examplesofcorrelation-inducedchangesinstochasticelectromagneticbeamsonpropagation
9.4.4Coherence-inducedchangesofthedegreeofpolarizationinYoung"sinterferenceexperiment
9.5GeneralizedStokesparameters
Problems
Appendices
ⅠCellsofphasespaceandthedegeneracyparameter
(a)Cellsofphasespaceofaquasi-monochromaticlightwave(Section1.4)
(b)Cellsofphasespaceofradiationinacavity(Sections7.4and7.5)
(c)Thedegeneracyparameter
ⅡDerivationofMandel"sformulaforphotocountstatistics[Eq.(2)ofSection7.5.1]
ⅢThedegreeofpolarizationofanelectromagneticGaussianSchell-modelsource
ⅣSomeimportantprobabilitydistributions
(a)Thebinomial(orBernoulli)distributionandsomeofitslimitingcases
(b)TheBose-Einsteindistribution
Authorindex
Subjectindex

作者简介

(美)沃尔夫（E.Wolf），美国罗彻斯特大学教授。

内容简介

所有的光场都是随机涨落的，有些光场的随机涨落很小，例如许多激光器输出的光；有些光场的随机涨落相当大，例如从热光源辐射的光。描述涨落光场的基础理论是相干理论。部分偏振现象就是涨落的重要表现。实际上，相干理论所能处理的问题不有且只有于涨落。与常规的处理方法不同，相干理论是依据可观测量描述光场，并解释这些可观测量，例如光的光谱以及它在传输中如何变化的。
本书给出了光的相干与偏振现象的统一处理方法。适合光通信、激光光束在光纤中和通过湍流大气传输、光学成像，尤其在显微镜成像（例如医学诊断）的物理界和工程界的研究者阅读。

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