The present invention relates to an interferometer apparatus.
Interferometers are widely used both in academia and industry for a great variety of applications. They can be used to measure the spectral component of the light, measure the speed of light, evaluate imperfections of transparent materials such as optical elements, measure lengths and more.
Michelson's interferometers and their variations are the most used. In this device, two replicas are created employing a beam splitter, and they travel along different paths. The path travelled by one of the two replicas can be varied and the two are then recombined into one output beam making interference possible. Since the two replicas travel along two distinct paths, they can experience different perturbations and this can negatively affect the quality of the interference. It is a technological challenge to maintain interferometric stability between the two different interferometer arms due to environmental vibrations and perturbations. Indeed, for this approach to work, the path length difference must not fluctuate more than λ/10, where λ is the radiation wavelength. This is the main reason why this technique is de facto restricted to the infrared spectral region and cannot be easily used outside laboratory environments.
To overcome this limitation several common path interferometers were developed in past years. In particular, by using a birefringent material it is possible to divide the two replicas based on their polarization. The optical path difference is given by the different velocities of the replica polarizations travelling through a birefringent material and depends on the thickness of the material.
Differently from a double-beam interferometer, the two replicas travel along the same path and experience the same perturbations, so they are phase locked. This assures great delay stability and interference quality and these devices can work well even with shorter wavelengths down to the visible and ultraviolet range. Moreover, these devices are compact and robust and can be applied also in industrial environments and under harsh conditions.
Documents U.S. Pat. Nos. 3,849,001 and 5,157,458 identify as a possible solution the use of a Babinet-Soleil compensator between two polarizers. The Babinet-Soleil based interferometer has been used in a large variety of applications such as fluorescence spectroscopy (document U.S. Pat. No. 11,181,423), spectral imaging (document U.S. Pat. No. 11,346,719), circular dichroism (document WO2018/115446) and more. This device uses a first birefringent element made of two birefringent wedges to create a variable delay between two replicas having orthogonal polarization. A modified version of a Babinet-Soleil compensator interferometer is described in document US20213/329228 adding other birefringent elements to compensate for the group velocity dispersion and to lock the propagation delay of one of the two polarizations, useful for pump-probe spectroscopy.
However, the Applicant has noticed that the Babinet-Soleil based interferometers of the above cited documents are very sensitive to the light travelling direction inside the interferometer. The Applicant noticed that this light direction sensitivity is because the birefringence of the used material and the path length inside the crystals is angle-dependent and since such interferometers use two birefringent optical crystals (the second one to permit also negative delays) the dependency is even worsened.
Said dependency severely affects the usage of the interferometer as a spectrometer as the light entering the interferometer needs to be collimated and makes the device suitable only for point-like sources and performs poorly with extended light sources.
In this latter case (i.e. extended light sources), the light cannot be collimated and consists of beams travelling having a multitude of angular directions.
In this case, the interfering output beam shows several spatial fringes alternating high and low intensity for constructive and destructive interference, respectively. The Applicant observes that these fringes are present because the light propagates inside the interferometer with different angular directions and the interferometer delay depends strongly depends on them. So, for certain directions, there is a constructive interference condition and the intensity is high while in others there is destructive interference and the intensity is low.
Moreover, the Applicant has noticed that a single pixel detector spatially integrates the intensity profiles of the output beam and this decreases the interference contrast. To obtain high interferometric contrast the beam size must be reduced by using a small aperture selecting only the portion of the output beam corresponding to a single fringe. The angle dependency of the optical delay is particularly problematic in using the common-path interferometer in imaging such as for spectral imaging or microscopy as described in document U.S. Pat. No. 11,346,719.
In this case, an imaging lens is used which collects the light coming from each point of a large scene of interest. Each ray bundle coming from a specific point comprises a collection of rays propagating with different angles inside the interferometer. This is especially accentuated in imaging closer objects since, for each point of the scene, the range of angles of the collected rays by the lens is bigger.
Another example of a scanning common path interferometer is shown in publication “Birefringent Fourier-transform imaging spectrometer”, Vol. 12, Issue 22, pp. 5368-5374 (2004) by A. R Harvey et Al. The interferometer is based on two Wollaston prisms placed in between two polarizers. The first prism separates angularly the replicas and the second one is used to make the two beams collinear again but separated by a distance that depends on the distance between the two Wollaston prisms. A lens is used to recombine spatially the beams and let them interfere with a detector. The second prism is scanned across the beam and due to its configuration, this introduces an optical path difference between the two replicas. The two light replicas interfere at the detector coming from different directions; therefore, also the wavefront of the two beams are inclined accordingly and this causes a loss of the interferometric modulation at the detector that reduces the signal-to-background ratio. Moreover, the Wollaston prisms separate angularly the different spectral components of the light and this further reduces the interferometric modulation at the detector, because the same colour of the two orthogonally polarized replicas impinges on a slightly different position of the camera, thus reducing the interferometric signal.
Moreover, this known interferometer introduces strongly angular dependent delays and this limits the performance of the system for non-point like sources. It is important to note that these two problems increase when the two Wollaston prisms are made bigger in order to increase the maximum interferometric delay and therefore the maximum resolution.
Document US20215/355027 describes an interferometer based on two Wollaston prisms provided in addition with a relay optical system to have the same optical delay for all the points in the object field. However, the Applicant notices that this is true only for light entering the interferometer parallel to the optical axis of the system. Therefore, this approach is severely limited to objects located at infinity or to the use of other optical elements to put the object at infinity. The interferometer of this document has still a strong dependency on the propagating angle inside the system and this severely limits the interferometric contrast hence the light throughput, sensitivity, and field of view of the system.
The present invention addresses the problem of providing an interferometer apparatus, of the type comprising an adjustable birefringent device producing replicas with orthogonal polarizations, in which the radiation direction dependency is eliminated or reduced so increasing the interference quality and, as an example, obtaining an apparatus that effectively work for single-point radiation sources as well as extended radiation sources.
Further characteristics and advantages will be more apparent from the following description of a preferred embodiment and of its alternatives given as an example with reference to the enclosed drawings in which:
The interferometer apparatus 100 comprises a first adjustable birefringent device 110 and a first compensation optical device 120, which is optically coupled with the first adjustable birefringent device 110.
Moreover, according to an example, the interferometer apparatus 100 comprises a source module 130 which can be an electromagnetic radiation source or an optical imaging system.
Referring to the case in which the source module 130 is an electromagnetic radiation source, it is configured to generate a radiation (also called “light”, without limitation to visible light wavelengths) propagating along the first adjustable birefringent device 110 and the first compensation optical device 120. The electromagnetic radiation source 130 can be a coherent source (e.g. a laser) or an incoherent source (e.g. a lamp). The electromagnetic radiation source 130 can generate polychromatic radiation or monochromatic radiation of either linear or other types of polarizations.
The source module 130 can be even a sample emitting, reflecting or scattering light. In imaging application, an optical imaging system is added in front and/or after the interferometer apparatus 100 and the image of the sample is formed on a bi-dimensional detector.
Particularly, the interferometer apparatus 100 can be configured to operate in one of the wavelength ranges selected from: 180-3500 nm, 500-5000 nm, 400-20000 nm.
In both cases, as schematically represented in
The first adjustable birefringent device 110 is configured to receive an input radiation INR and produce corresponding replicas having reciprocally orthogonal polarizations. Such replicas are delayed from each other by an adjustable time delay depending on a configuration assumed by the first adjustable birefringent device 110.
Moreover, as it will be further clarified later, the first adjustable birefringent device 110 introduces an additional time delay between said replicas.
Such additional dependent on an angle of incidence of said radiation on the adjustable birefringent device which is function of a structural thickness and an ordinary and extraordinary refractive indexes of the adjustable birefringent device.
In accordance with the example of
The adjustable wedge pair BL1 comprises a first optical wedge 101 and a second optical wedge 102. Both first 101 and second 102 optical wedges are made of a birefringent material. As an example, the first 101 and second 102 optical wedges have corresponding optical axis o1 of the birefringence material parallel to each other. Particularly, the first optical wedge 101 and the second optical wedge 102 are optical prisms, having, preferably, the same apex angle. The first optical wedge 101 coupled to the second optical wedge 102 is equivalent to an optical plate having variable thickness.
At least one of the two optical wedges 101 and 102 is movable (e.g. it can be translated) along a direction transversal to the main direction 2 by means of an actuator 104, schematically represented in
The adjustable time delay introduced by the adjustable wedge pair BL1 is dependent on the variable position of the first optical wedge 101. Moreover, as an example, the actuator 104 may be connected to a computer-controlled precision translation stage.
It is noticed that the first 101 and the second optical wedges 102 can be arranged to be very close to each other in order to reduce chromatic dispersion and spatial separation of the replicas. As an example, the first optical wedge 101 and the second optical wedge 102 can be at a distance between the corresponding adjacent tilted faces of 0-1 mm.
In accordance to an example, optical element BL2 is a birefringent plate (e.g. with fixed thickness) having a respective optical axis o2 of the birefringent material perpendicular to the optical axis o1 of adjustable wedge pair BL1 and the main direction 2. The optical element BL2 is coupled with the adjustable wedge pair BL1 and, according to the considered example, is configured to introduce a fixed phase delay between the radiations having reciprocally orthogonal polarizations.
The adjustable wedge pair BL1 (i.e. first optical wedge 101 and second optical wedge 102) is made by a birefringence material having a first ordinary index no and a first extraordinary index ne and has an adjustable thickness t1v. In the following description, one specific value t1 that the variable thickness t1v can assume during the movement of the first optical wedge 101 is considered.
The optical element BL2 is a plate having a thickness t2 equal to the specific thickness t1 of the adjustable wedge pair BL1 and is made by a birefringence material having the same first ordinary index no and first extraordinary index ne defined for the adjustable wedge pair BL1. Preferably, the adjustable wedge pair BL1 and the optical element BL2 are made by the same material such as an example: α-BBO.
Particularly, considering the first ordinary index no and the first extraordinary index ne that characterizes the first adjustable birefringent device 110 it is observed that a first birefringence range Δn can be defined as the difference ne-no, that can have a positive or a negative sign.
The first compensation optical device 120 is optically coupled to said first adjustable birefringent device 110 and configured to have a respective structural thickness and respective ordinary and extraordinary refractive indexes so as to introduce a compensation time delay between said replicas having a sign opposite to a sign of the additional time delay, so as to reduce the dependence on said angle of incidence in said interferometer apparatus.
According to an example, the first compensation optical device 120 comprises a polarization flipper 121, a first compensation birefringent plate BL3 and a second compensation birefringent plate BL4.
The polarization flipper 121 is an optical device that converts the vertical polarization to a horizontal polarization and vice-versa. As an example, the polarization flipper 121 can be made with a half-wave plate at 45° or with a Fresnel romb. According to the shown example, an input port of the polarization flipper 121 optically coupled with an output of the optical element BL2.
The first compensation birefringent plate BL3 has an input port optically coupled to an output port of the polarizing flipper 121 and second compensation birefringent plate BL4 has an input port optically coupled to an output port of the first compensation birefringent plate BL.
According to an example, the first compensation birefringent plate BL3 is designed to compensate for the angular dependence introduced by optical element BL2 and the second compensation birefringent plate BL4 is designed to compensate for the angular dependence introduced by the In accordance with this example, the first compensation birefringent plate BL3 and the second compensation birefringent plate BL4 are designed so as to satisfy the following conditions:
It is noticed that a condition more general than the conditions E) and F) is that the interferometer apparatus 100 of
According to specific examples, the interferometer apparatus 100 is further equipped with an input polarizer 105 (particularly, placed between the source module 130 and the first adjustable birefringent device 110) to provide an output radiation of linear polarization transversal to the optical axes o1 and o2 of the first adjustable birefringent device 110 and, preferably, having tilt of 45° with respect to such axes.
With reference to an example, the interferometer apparatus 100 also includes an output polarizer 106 placed, as an example, at the output of the second compensation birefringent plate BL4 and designed to project the two replicas into a common polarization state so as they can interfere.
Moreover, the interferometer apparatus 100 can be equipped with a detector 107 and an analysis device 108. The detector 107 receive the radiation exiting the output polarizer 106 and convert such interfering radiation into an electrical signal that is provided to the analysis device 108 that performs elaborations depending on the particular application.
As the skilled person can recognize, the order of the elements of the interferometer apparatus 00 can be different from the one shown in the drawings. Optionally, some of the above described components may be glued together. Moreover, it is observed that the first adjustable birefringent device 110 and the first compensation optical device 120 may be inserted into an interferometer apparatus different from the one depicted in
With reference to the operation of the interferometer apparatus 100 of
The optical element BL2 introduces a fixed time delay between the two orthogonally polarized components of the radiation having a sign opposite to the one introduced by the adjustable wedge pair BL1.
The combination of the adjustable wedge pair BL1 and the optical element BL2 allows setting time delays ranging from positive to negative values.
It is observed that the delay introduced by the first adjustable birefringent device 110 is different for each propagation angle and the delay also depends both on an azimuthal and polar angles of the radiation that enters the first adjustable birefringent device 110, as will further described later.
The polarizations of the two replicas (i.e. the two orthogonally polarized components) exiting the first adjustable birefringent device 110 are exchanged by the polarization flipper 121.
The corresponding components exit the first adjustable birefringent device 110 and pass through the compensation optical device 120. Considering the specific described example, the first compensation birefringent plate BL3 acts on the radiation passing through it by at least partially compensating the time delay amount due to the angular dependence introduced by the optical element BL2. The second compensation birefringent plate BL4 acts on the radiation passing through it by at least partially compensating the time delay amount due to the angular dependence introduced by the adjustable wedge pair BL1. As it will be clarified in the following, the compensation is due to the selection of the birefringence index values and the thickness for the plates BL3 and BL4 with respect that of the first adjustable birefringent device 110.
According to the example described, the compensated radiation, which is under the form of two replicas, exits the first compensation optical device 120 and reaches the output polarizer 106 that projects the two replicas into a common polarization state to cause interference. The interfering replicas are converted into a corresponding electrical signal by the detector 107 and said electrical signal is analyzed by the analysis device 108. It is noticed that the reduction or elimination of the angular dependence from the interfering replicas significantly improves the quality of the obtained interference positively affecting the subsequent analysis of the corresponding electrical signal especially for big detector areas and/or large emitting sources.
The following section provides a description of the operation of the interferometer apparatus 100 with reference to the reduction of the angular dependence and proves, theoretically and by numerical simulations, said compensation effect.
The birefringent materials employable for the components of the interferometer apparatus 100 are, as an example, selectable from the following group: barium borate (BaB2O4), alpha-barium borate (x-BaB2O4), lithium niobate (LiNbO3), Calomel (Hg2Cl2), beryl (Be3Al2 (SiO3) 6), calcite (CaCO3), magnesium fluoride (MgF2), quartz (SiO2), ruby (Al2O3), rutile (TiO2), sapphire (Al2O3), silicon carbide (SiC), tourmaline (complex silicate), high zircon (ZrSiO4), low zircon.
It is noticed that the interferometer apparatus 100 of
In a uniaxial birefringent crystal there is a single direction known as the optical axis that represents a centre of symmetry for the material.
Namely, rotating the material around this axis does not change its optical behavior. Each direction with a specific angle with respect to this axis is optically equivalent. No matter its polarization state, the light propagating parallel to the optic axis is governed by a refractive index no known as the ordinary refractive index. Considering any other propagation direction, it is always possible to decompose the incoming light polarization into two orthogonal polarizations: one linear polarization that is perpendicular to the optic axis which is called the ordinary ray and experiences a refractive index value no, and another polarization propagating in the same direction will be oriented partly in the direction of the optic axis. This polarization is called the extraordinary ray and is governed by a different, direction-dependent refractive index.
The propagation of the ordinary ray is simply described by no as if there were no birefringence involved. The extraordinary ray propagates differently from any wave in an isotropic optical material. This beam has an effective refractive index which has a value in between no and ne. Its power flow is not in the same direction as the wave vector which is called also wave normal. Notably, while the power flow does not respect Snell's law and behaves extraordinarily the direction of the wave vector follows it.
Particularly,
Inside the crystal element BL, the light is split into two rays with different angles: a first ray r and a second f. After the crystal element BL the ordinary ray “o” (the first ray r) and extraordinary ray “e” (the second F) travels substantially parallelly with the same angle as the incident ray INr but having a lateral offset CD.
With reference to
The extraordinary beam “e” experiences an effective refractive index
Or equivalently:
Considering the light beam INr impinging on the crystal BL with the angle i as in
With the help of these equations, it is possible to evaluate the path difference ΔP between the extraordinary and ordinary waves when they propagate at an angle i into the crystal element BL.
Following
Therefore
and using equations (1.3) and (1.4) it is obtained:
which is equivalent to:
From which the term cot(r) can be evaluated by considering that:
and using equation (1.3) it is obtained
leading to:
The term cot(T) can be written as:
Evaluating the term sin(
Where equation (1.2) can be considered to evaluate the 1 term 1/
The term cos(θ)2 of the last equation cab be evaluated by considering
So, it is possible to write cos(0)=ô·{circumflex over (t)} where
{circumflex over (t)}=cos(
Substituting this value in equation (1.8) and solving for sin(
Inserting this expression into 1.7, it is obtained:
Finally, the path difference is:
It is evident that the above path difference introduces time delay between the replicas that is proportional to the quantity of equation (1.11).
The above equation (1.11) can be used to design the adjustable wedge pair BL1 since the gap in between the two wedges 101 and 102 can be made by design very small, as an example from 0 to 1 mm; 0-0, 6 mm. Therefore its role in term of the path difference between the extraordinary and ordinary waves is just an offset with no contribution to the angular dependency and can be neglected.
Let us consider the optical path difference between the horizontal h and vertical v polarization entering the adjustable wedge pair BL1. With reference to
This optical path difference ΔPh-v is displayed, for an exemplary case, as a function of ω and i in
The map of
With reference to the path difference ΔP introduced by the optical element BL2, this is identical to that of the adjustable wedge pair BL1 but, since the two have an orthogonal optical axis, to model the optical element BL2 it is necessary to use equation (1.11) with the following substitution ω=ω+π/2.
It is noticed that the optical element BL2 has the optical axis o2 rotated by 90 degrees with respect to optical axis o1. In this case, the vertical polarization is the extraordinary ray “e” while the horizontal is the ordinary “o”. Therefore, the optical path difference between the horizontal and vertical polarization is:
This optical path difference is displayed in
The total amount of the path difference (corresponding to an undesired addition time delay between the two replicas) is given by the sum of the amount of equation (1.12) and the amount of equation (1.13).
While the combined amount of the first adjustable birefringent device 110 is displayed in
Considering the interfering radiation exiting a polarizer, the obtained interference at a particular wavelength has the fringe pattern shown in
It is noticed that the fringe pattern, like that of
This is especially true for shorter wavelengths when these fringes have a higher spatial frequency. Moreover, in imaging mode the interference signal as detected by each pixel has a different phase, hence zero-path difference. Each common fluctuation, as an example due to a perturbed illumination that happens in a particular moment of the scan of the moving element, will have a different phase and the result is that this fluctuation is translated as intensity noise following the same pattern.
As already indicated, the first compensation optical device 120 has an opposite effect with respect to that of the first adjustable birefringent device 110.
In the embodiment above described, the first compensation optical device 120 is provided with the polarization flipper 121 (to swap the vertical with the horizontal polarization) and the first and second compensation birefringent plates BL3 and BL4, which are two plates with equal thickness with respect to the adjustable wedge pair BL1 and the optical element BL2.
The first and the second compensation birefringent plates BL3 and BL4 have the same thickness in order to not vary the optical path difference between the two replicas, hence polarizations.
After the polarization flipper 121, the vertical polarization becomes horizontal and vice-versa.
The optical path difference considered in the following computing is the path difference between the originally horizontal and vertical polarizations, as indicated before.
Inside the first compensation birefringent plate BL3 the originally horizontal polarization is oriented along the vertical axis (i.e. along the optical axis o3 of
This optical path difference is displayed as a function of ω and i in
Inside the second compensation birefringent plate BL4 the originally horizontal polarization is still oriented along the vertical axis (i.e. perpendicularly to the plane of
For this reason, the optical path difference introduced by the second compensation birefringent plate BL4 is:
This optical path difference is displayed as a function of ω and i in
The total path difference introduced by the first compensation birefringent plate BL3 and the compensation birefringent plate BL4, after the polarization flipper 121, is given by the sum of the amount expressed by equations (1.14) and (1.15). An example, of said delay is shown
The effect is as desired: indeed, the first compensation birefringent plate BL3 and the compensation birefringent plate BL4 causes a path difference with the same magnitude and with an opposite sign as the one generated by first adjustable birefringent device 110, so as to reduce or eliminate the angular dependence.
The total effect of the first adjustable birefringent device 110 and the first compensation optical device 120 is given by the sum of the amount expressed by the equations (1.12), (1.13), (1.14) and (1.15). This total effect is shown, as an example, in
The corresponding interference signal across the field is shown in
It is noticed that through the interferometer apparatus 100 of
In this gap the vertical and horizontal polarization replicas travels along different direction angle. This angle is 0=asin(no sinα)−asin(ne sin(α)) where alpha is the apex angle of component 101. This value is very small, considering a-BBO at 400 nm this lead to a value of 1.28°. This small angular deviation lead to an offset between the vertical and horizontal beam given by: Offset=tan(0) leading to a very small value ranging from 0 to 22 μm for an air gap with a thickness from 0 to 1 mm respectively. This low value is not a problem for many of applications. However, it can be compensated by tilting one of the plate comprised in the interferometer. As an example, by turning counter-clockwise the optical element BL2 in
2. Second Embodiment (
The second adjustable birefringent device 140 comprises the adjustable wedge pair BL1 identical or analogous to the one of
The optical element BL2 of
As already noticed the interferometer apparatus 100 of
Instead, the second embodiment described with reference to
Indeed, while scanning the first wedge 101, increasing its thickness, it is possible to scan also the third optical wedge 111, decreasing its thickness. In this way, the increased angular dependency of adjustable wedge pair BL1 is compensated by the decreasing angular dependency of the optical element BL2.
By looking at
Moreover, considering the second embodiment shown in
This can be very beneficial to increase the spectral resolution of the measurement. It is important to note that the angular dependence as shown in
In this configuration, by scanning the moving wedge of the adjustable wedge pair BL1, the optical element BL2 as shown in
As an example, the optical path difference has a maximum change varying the propagating angles from ω=[0; 2π]rad and i=[0;0.14]rad of less than 110 nm. This calculation is performed by considering a radiation with 400 nm wavelength, hence the change is smaller than half of the considered light wavelength.
It is observed that fact that the change is smaller than half of the considered light wavelength is a feature valid for all the described embodiments.
As an example, considering an interferometer with the same conditions for BL1 and BL2 but without the compensating elements BL3 and BL4, we obtain a maximum change for the optical path differences close to 7 μm. Therefore, the angular dependency of the delay has been decreased by almost two orders of magnitude.
The optical path difference for t1=0.007m, t2=0.001m and t4=t3=0.004m is shown in
Therefore, the configuration of the second embodiment (
With reference to
This thickness-sum condition refers to the situation in which the adjustable wedge pair BL1, the optical element BL2, the first compensation birefringent plate BL3 and second compensation birefringent plate BL4 are made by the same birefringent material.
The third embodiment of the interferometer apparatus 100 is a variant of the first embodiment of
With reference to
Particularly, it is further noticed that the material used for the first compensation birefringent plate BL3 and the second compensation birefringent plate BL4 shows a transmission range at least partially overlapping that of the material of the first adjustable birefringent device 110.
According to conditions b) and d), if the birefringence range of the material of the first adjustable birefringent device 110 is negative Δn=ne−no<0 (such as for α-BBO) the birefringence range of the material employed in second compensation optical device 150 is positive Δn=ne−no>0.
Indeed, equation (1.11) expressing the difference of path for the first adjustable birefringent device 110, as rewritten below for convenience, is:
Applying a Taylor expansion considering that √{square root over ((1+x))}≈1+1/2x it is obtained:
The combined effect of the adjustable wedge pair BL1 and the optical element BL2 is, considering t1=t2=t (as already done before):
In order to compensate the first and the second compensation birefringent plates BL3 and BL4 should have a thickness t2=t3=t′ and an ordinary and extraordinary refractive index no′ and ne′ such that ΔP=−ΔP′. This is possible only if ne-no has an opposite sign with respect to ne′-no′ and the thickness
Therefore, the value t′ of the thickness of the first compensation birefringent plate BL3 (equal to the one of the second compensation birefringent plate BL4) is given by the product of the value t of the thickness of the adjustable wedge pair BL1 (when in a specific position) for a factor which depends on the first indexes no and ne and the second indexes no′ and ne′.
As an example, considering the light wavelength to be 400 nm and the material for adjustable wedge pair BL1 and the optical element BL2 is a-BBO with t1=t2=t=0.004m. If we consider TeO2 as positive birefringent material having ne′=2.6266 and no′=2.4412, we obtain a thickness t′ is given by: t′=1.5092t=0.006037m.
In this further noticed that, analogously to what expressed for
4. Fourth embodiment (
With reference to the embodiment of
5. Further embodiments (
According to the embodiment of
Moreover, according to the embodiment of
The first adjustable compensation wedge pair BLW3 (which can be analogous to one of the previous described wedge pairs) includes a fifth optical wedge 113 and a sixth optical wedge 114. The first adjustable compensation wedge pair BLW3 defines the thickness t3.
The second adjustable compensation wedge pair BLW4 includes a seventh optical wedge 115 and an eight optical wedge 116. The second adjustable compensation wedge pair BLW4 defines the thickness t4.
As described for the embodiments of
It is noticed that, advantageously, all the movable optical elements of
The embodiment of
Considering the embodiment of
According to a first implementation shown in
Moreover, in the third compensation optical device 160 of
The interferometer apparatuses 100 including the components of
It is noticed that the described embodiments of the interferometer apparatus 100 allows producing delayed replicas having orthogonal polarizations wherein the delay is not strongly influenced by the propagating angle and by the entering position of the input radiation with respect to the propagation axis travelling in the center of each optical element of the interferometer. Moreover, the two obtained replicas are substantially (according to the meaning already described) parallel having no separating angle.
Symbols employed in the drawings
Number | Date | Country | Kind |
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102023000005346 | Mar 2023 | IT | national |