
- •Chapter 1
- •Introduction to linear singular optics
- •I.I. Mokhun
- •Chapter 1
- •Introduction to linear singular optics
- •I.I. Mokhun
- •1.1. IntRoduction
- •1.2. Basic notions of scalar singular optics
- •1.2.1. Phase vortices
- •1.2.2. Topological charge and topological index of singular points. Elementary topological reactions
- •1.2.2.1. Topological charge
- •1.2.2.2. Topological index
- •1.2.2.3. Conservation law for topological charge
- •1.2.2.4. Elementary topological reactions
- •1.2.3. Experimental observation and identification of vortices into scalar fields
- •1.2.4. Generation of vortices using computer-generated holograms
- •1.3. Vortices and phase structure of a scalar field
- •1.3.1. Sign principle
- •1.3.2. Phase speckles. “breathing” of phase speckles
- •1.3.3. Birth of vortices
- •1.3.4. Appearance of wave front dislocations as a result of interference of waves with simple phase surfaces
- •1.3.5. Topological indices of the field of intensity. Extrema of phase and intensity. “correlation” of phase and intensity
- •1.3.6. Vortex nets. Phase skeleton of a scalar field
- •1.3.6.1. Reconstruction of the field’s phase on the basis of shifted vortex nets
- •1.3.6.2. Image reconstruction using a regular sampling found from analysis of the parameters of vortices in random field
- •1.3.6.3. Some remarks on the field reconstruction by the use of nets of the intensity sTationary points
- •1.4. Singularities of a vector field
- •1.4.1. Disclinations. Polarization singularities
- •1.4.2. Vortices of phase difference. Sign principle for a vector field
- •1.4.2.1. Field decomposition into orthogonally linearly polarized components
- •1.4.2.2. Principle of the vortex analysis of vector fields
- •1.4.2.3. Vortices of orthogonally polarized field components. Technique for study of polarizatioN singularities
- •1.4.3. “Correlation” of intensity and polariszation of the vector field
- •1.4.4. Interconnection of the component vortices and -points
- •1.4.5. Elementary polarization structures and elementary polarization singularities of vector fields
- •1.4.5.1. Polarization structures resulting from interference of orthogonally linearly polarized beams
- •1.4.5.2. Elementary polarization singularities resulting from interference of circularly polarized beams
- •1.4.5.3. Experimental mOdeling of elementary polarization singularities
- •1.4.6. Fine structure and averaged polarization characteristics of inhomogeneous vector fields
- •1.4.6.1. Avaraged stokes parameters
- •1.4.6.2. Analysis of the averaged parameters for decomposition of the field into linearly polarized components
- •1.4.6.3. Computer simulation of the vector field’s parameters
- •1.4.6.4. Analysis of the averaged parameters for the field decomposition into circular basis
- •1.4.6.5. Comparison of the experimental results and the data of computer simulation
- •1.4.7. “Stokes-formalism” for polarization singularites. “stokes-vortices”
- •1.5. Singularities of the Poynting vector and the structure of optical fields
- •1.5.1. General assumptions. Components of the poynting vector
- •1.5.2. Singularities of the poynting vector in scalar fields
- •1.5.2.1. Instantaneous singularities of a scalar field
- •1.5.2.2. Averaged singularities of the poynting vector of scalar field
- •1.5.3. Singularities of the Poynting vector at vector fields
- •1.5.3.1. Instantaneous singularities of vector field
- •1.5.3.2. Behavior of the Poynting vector in areas of elementary polarization singularities
- •1.5.3.2.1. Symmetric distributions of amplitude and phase of the interfering beams
- •1.5.3.2.2. Non-symmetrical distributions of amplitudes and phases of the interfering beams
- •1.5.3.2.3. Experimental proving of the existence of the orbital momentum in the vicinity of -point
- •1.5.3.3. The averaged Poynting vector of the vector field
- •Instantaneous singularities of the Poynting vector
- •Appendix 1.1. Wave fronts approximation
- •104. I.Mokhun, r.Brandel and Ju.Viktorovskaya, “Angular momentum of electromagnetic field in areas of polarization singularities”, ujpo, Vol. 7, pp. 63-73, (2006).
1.4.6.3. Computer simulation of the vector field’s parameters
It has been noted above that our consideration is performed at far zone, and the paraxial approximation is valid, while the field is analyzed within small solid angle. Under these conditions, correlation length of the field does not depend on the structure of the scattering object, being depending on the relation of the field-of-view of the object (for the specified scattering angle) and the wave length alone.
To consider the problem in general setting, one must provide the algorithm of computer simulation allowing formation of arbitrary set of Stokes parameters. Note, however, that the second Stokes parameter equals zero, if the condition (1.114) is satisfied. Remember also, the first normalized Stokes parameter equals zero by definition. That is why the requirements to the simulation algorithm are reduced to the only requirement of formation of arbitrary third and fourth Stokes parameters.
At far
zone, for the specified scattering angle and under assumption of
statistical homogeneity of the field, the direct connection between
the characteristics of the scattered field and the scattering object
is lost. In part, it is not important, what specific object forms the
field with the measured Stokes parameters. The same statement is true
for the structure of the each of the orthogonally linearly polarized
components of the scattered field. Thus, the simulation algorithm
must provide obtaining arbitrary magnitude of the correlation
coefficient,
,
for two components, what requirement is the equal strength as
specifying the desirable magnitudes of the third and the fourth
Stokes parameters.
Under
paraxial approximation, the far-zone field,
,
is the Fourier transformation from the boundary object field,
[92]. Taking into account that the field structure at far field is
not connected directly with the object’s structure (excluding the
requirement for the field
to be random), one can form the field
for the orthogonal components as the set of randomly distributed
point sources with the unitary amplitudes and random phases:
,
(1.140)
where
is the total number of point sources,
,
are phase and coordinates of the
th
source. The only difference in forming the “input” sampling of
point sources of the orthogonal components is that the positions and
the phases of sources are quite different for two samplings
associated with the orthogonally polarized components.
In this case, the components of equal intensities are formed at far zone, and the correlation coefficient for them is determined by the following simple ratio:
,
(1.141)
where
is the number of point sources with the same characteristics in both
orthogonal components.
T
he
degree of “integral depolarization“,
,
is the polarization parameter characterizing the averaged
polarization characteristics of a vector field. Note, the field
remains to be completely polarized at the each point.
It is known that if the condition (1.114) is fulfilled, then integral depolarization is connected directly with the correlation coefficient of the orthogonal components, [28]:
.
(1.142)
F
Figure
1.46
characterizes the level of polarization in assumption that the
condition (1.114) is fulfilled. The ratios of the distance between
the adjacent component vortices,
,
to the correlation length,
–
,
have been obtained, as well as the maps of phase difference and the
averaged Stokes parameters, for different levels of integral
depolarization.
Figure 1.46 shows dependence of the phase difference dispersion, , on a mean distance between the adjacent component vortices .
Figure 1.47
illustrates the maps of a phase difference for the magnitudes of the
prevailing phase difference,
,
0 and
.
Note, the character
of
behavior of a phase difference does not depend on
,
while the phase
differences
in both cases are different by a constant at arbitrary point of the
a b
Figure
1.47.
Maps of the phase difference between the orthogonal components of an
optical field for 40% depolarization; effective phase differences are
(a) and
=0
(b). For clearness, the phase difference is given within to
.
The phase differences different by
are depicted by the same level of grey. The boundaries of white and
black colors are
-contours;
the points of gathering of the lines of all colors correspond to the
phase difference vortices; the points at the centers of the
like
regions are the saddle points of phase difference.
а b
c d
Figure 1.48. Intensity distribution of non-uniformly polarized field. Intensity distributions for 5% (а), 10% (b), 30% (c), 50% (d) depolarization of the field (correlation coefficient of the orthogonal components is 0.95, 0.9, 0.7, 0.5, respectively).
field. It results in changing of the form, size and localization of -contours, while the saddle points and the phase difference vortices do not change their positions. One can see from the figure that -contours are small and almost all are concentrated within the area of figure, when = .
The results of computer simulation of the parameters of a vector field for different correlation coefficients are represented in Figures 1.48 and 1.49. Circular polarization was chosen as the prevailing one. In this case, the areas with rapidly changed polarization coincide with the size of -contours [81,82].
Intensity distribution of the field slightly differs for various degrees of depolarization, cf. Figure 1.48). One can see in Figure 1.49 that both the size of -contours and a mean distance between the adjacent vortices of the same sign grow, as the level of depolarization increases. -contours are small in comparison with an average speckle size, being the closed domains with one type of polarization (clockwise or counterclockwise), when the correlation coefficient exceeds 0.5.
а b
c d
Figure
1.49. Maps
of a phase difference between the orthogonal components. Phase
difference between the orthogonal components for 5% (а), 10% (b),
30% (c), 50% (d) depolarization of the field (correlation coefficient
of the orthogonal components is 0.95, 0.9, 0.7, 0.5, respectively);
–
-component
vortices,
–
-component
vortices.
These domains are located just in the vicinity of the component vortices. The size of -contours grows and the localization of the domains with large polarization changes becomes random, when the correlation coefficient is less than 0.5.