Add to ORKGIt has been known for some time that the spectrum of light may change on propagation, even in free space. The theory of this phenomenon was developed within the framework of scalar theory. We generalize it to electromagnetic beams, generated by planar, secondary, stochastic sources. We also derive an electromagnetic analog of the so-called scaling law. When this law is satisfied the normalized spectrum of the beam is the same throughout the far zone and across the source
Taking the stochastic electromagnetic J0-correlated Schell-model pulsed (JSMP) beam as a typical ex...
We report analytic formulas for the elements of the e 2 X 2 cross-spectral density matrix of a stoch...
It has been known for some time that the degree of polarization of a light beam may change on propag...
It has been known for some time that the spectrum of light may change on propagation, even in free s...
A generalization from random scalar fields to random electromagnetic fields is obtained, of the phen...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
We present a detailed investigation, qualitative and quantitative, on how the atmospheric turbulence...
We develop a scaling law for a class of statistically nonstationary scalar optical fields, which ens...
A very useful theoretical tool for investigating coherence properties of stochastic scalar sources a...
A very useful theoretical tool for investigating coherence properties of stochastic scalar sources a...
We discuss fourth-order correlation properties of wide-sense statistically stationary, quasi-monochr...
We discuss fourth-order correlation properties of wide-sense statistically stationary, quasi-monochr...
It was shown some years ago that the spectrum of a stochastic scalar field depends not only on the s...
It is well known that in general the spectrum of a beam that is generated by a partially coherent so...
Taking the stochastic electromagnetic J0-correlated Schell-model pulsed (JSMP) beam as a typical ex...
We report analytic formulas for the elements of the e 2 X 2 cross-spectral density matrix of a stoch...
It has been known for some time that the degree of polarization of a light beam may change on propag...
It has been known for some time that the spectrum of light may change on propagation, even in free s...
A generalization from random scalar fields to random electromagnetic fields is obtained, of the phen...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
We present a detailed investigation, qualitative and quantitative, on how the atmospheric turbulence...
We develop a scaling law for a class of statistically nonstationary scalar optical fields, which ens...
A very useful theoretical tool for investigating coherence properties of stochastic scalar sources a...
A very useful theoretical tool for investigating coherence properties of stochastic scalar sources a...
We discuss fourth-order correlation properties of wide-sense statistically stationary, quasi-monochr...
We discuss fourth-order correlation properties of wide-sense statistically stationary, quasi-monochr...
It was shown some years ago that the spectrum of a stochastic scalar field depends not only on the s...
It is well known that in general the spectrum of a beam that is generated by a partially coherent so...
Taking the stochastic electromagnetic J0-correlated Schell-model pulsed (JSMP) beam as a typical ex...
We report analytic formulas for the elements of the e 2 X 2 cross-spectral density matrix of a stoch...
It has been known for some time that the degree of polarization of a light beam may change on propag...