DEVICES AND METHODS FOR OPTICAL IMAGING BY MEANS OF OFF-AXIS DIGITAL HOLOGRAPHY
20200233378 · 2020-07-23
Assignee
- Centre National De La Recherche Scientifique (Cnrs) (Paris, FR)
- ECOLE SUPÉRIEURE DE PHYSIQUE ET DE CHIMIE INDUSTRIELLES DE LA VILLE DE PARIS (Paris, FR)
Inventors
Cpc classification
G03H2001/005
PHYSICS
G03H1/0443
PHYSICS
G03H1/041
PHYSICS
International classification
Abstract
According to one aspect, the invention concerns an optical imaging device (20) for an object (OBJ) by off-axis holography comprising a light source (21) adapted for emitting an illumination wave (E.sub.I) on the object, in transmission or reflection, and an assembly formed by one or more thick Bragg gratings (22) for receiving a wave (E.sub.O) coming from the object thus illuminated and for deflecting a first component (E.sub.R) of the wave coming from the object, called the reference wave, and to allow a second component (E.sub.S) of the wave coming from the object, called the signal wave, to pass without deflection in such a way that the deflected reference wave presents predetermined deflection angles with respect to the non-deflected signal wave defined in two perpendicular planes. The imaging device according to the first aspect further comprises a two-dimensional detection device (23) for acquiring an interferogram resulting from the interference between said deflected reference wave and said signal wave and a computing unit for determining, from said interferogram, an amplitude and phase distribution of the signal wave in the plane of the object (hologram).
Claims
1. An optical imaging device of an object by off-axis holography comprising: a light source for emitting an illumination wave on the object, in transmission or reflection; an assembly formed of one or more thick Bragg gratings arranged to receive a wave coming from the illuminated object and to deflect by compliance to the Bragg's law a first component undisturbed by the object of said wave coming from the object, referred to as reference wave, and to let pass without deflection, because of the non-compliance to the Bragg's law, a second component of said wave coming from the object, called the signal wave, so that the deflected reference wave presents predetermined deflection angles defined in two perpendicular planes with respect to the non-deflected signal wave, a two-dimensional detection device for acquiring an interferogram resulting from the interference between said deflected reference wave and said non-deflected signal wave; and a computing unit for determining, from said interferogram, an amplitude and phase distribution of the signal wave in the plane of the object.
2. The optical imaging device according to claim 1, wherein said assembly formed of one or more thick Bragg grating(s) comprises at least one first thick Bragg grating with multiplexed index strata, having index strata arranged in two perpendicular directions, with a given pitch in each of the directions.
3. The optical imaging device according to claim 2, wherein said assembly formed of one or more thick Bragg grating(s) further comprises a second thick Bragg grating with multiplexed index strata, having index strata arranged in two perpendicular directions, with a given pitch in each direction, such that the total deflection angle of the deflected reference wave, measured in each of said perpendicular planes, is equal to the difference in the deflection angles introduced by each of said multiplexed thick Bragg gratings.
4. The optical imaging device according to claim 1, wherein said assembly formed of one or more thick Bragg grating(s) comprises at least one first thick Bragg grating with index strata arranged in a first direction, with a first given pitch and at least one second thick Bragg grating with index strata arranged in a second direction, perpendicular to the first direction, with a second given pitch.
5. The optical imaging device according to claim 1, further comprising a microscope lens for forming an image of a limited field of the object with a given magnification.
6. A method for optical imaging of an object by off-axis holography comprising: the illumination of the object in transmission or reflection by means of an illumination wave coming from a light source; the sending on an assembly formed of one or more thick Bragg gratings of a wave coming from the illuminated object; the deflection by compliance to the Bragg's law of a first component not disturbed by the object of said wave coming from the object, called the reference wave, while a second component of the wave coming from the object, called the signal wave, due to non-compliance with the Bragg's law, passes through said assembly formed of one or more Bragg gratings without being deflected, the deflected reference wave having predetermined deflection angles defined in two perpendicular planes relative to the non-deflected signal wave, the acquisition by means of a two-dimensional detection device of an interferogram resulting from the interference between said deflected reference wave and said signal wave; and the calculation, from said interferogram, of an amplitude and phase distribution of the signal wave in the plane of the object.
Description
BRIEF DESCRIPTION OF THE FIGURES
[0030] Other advantages and characteristics of the invention will appear upon reading the description, illustrated by the figures below, wherein:
[0031]
[0032]
[0033]
[0034]
[0035]
[0036]
[0037]
DETAILED DESCRIPTION
[0038]
[0039] The imaging device 20 includes a light source 21 adapted for emitting an illumination wave of the object OBJ, whose the electromagnetic field is noted E.sub.I. Although represented in transmission in
[0040] The imaging device 20 also includes an assembly 22 of one or more thick Bragg gratings to receive a wave coming from the object, with an electromagnetic field E.sub.O. The wave coming from the object includes a first component formed by a wave coming from the object, or signal wave, of electromagnetic field E.sub.S and a second component formed by a wave coming from the source and not disturbed by the object, or reference wave, of electromagnetic field E.sub.R. The wave coming from the object is in practice a wave resulting from the diffraction of the illumination wave by all the microstructures of the object, the microstructures being able to result for example from the inhomogeneities of the refractive index in an object observed in transmission. Under certain conditions of incidence of the reference wave, known as Bragg's law conditions, the reference wave is deflected by the thick Bragg grating 22 in a given direction and spatially filtered due to the intrinsic properties of the thick Bragg gratings. The signal wave, emitted by the object in an angular cone defined by the optogeometric characteristics of the imaging device, is always transmitted without being deflected due to the non-respect of the Bragg's law. The reference wave E.sub.R deflected and filtered by the thick Bragg grating 22 therefore interferes with the signal wave E.sub.S transmitted by the Bragg grating without being deflected. The result is an interference signal formed in a detection plane of a two-dimensional detection device 23; the two-dimensional detection device thus allows the acquisition of an interferogram resulting from said interference signal. A calculation unit 24 then makes it possible to determine, from said interferogram, an amplitude and phase distribution of the signal wave in the plane of the object.
[0041] The imaging device is therefore an off-axis digital holography device whose characteristics, particularly in terms of fringe pitch of the interference signal, fringe orientation in the plane of the detector, angular spectrum width of the reference wave, are given by the characteristics of the thick Bragg grating(s), as explained below. The reconstruction of the signal wave coming from the interferogram includes, for example, a Fresnel transformation in a known way, and can be done in the same way as that performed in known off-axis digital holography techniques.
[0042] It is of course possible to acquire a series of interferograms if, for example, dynamic imaging of the object (video) is desired. In this case, a reconstruction of the signal wave is performed for each interferogram.
[0043] For the acquisition of the interferogram(s), the two-dimensional detection device is, for example, a matrix detector of a CCD (Charge-coupled device) or CMOS (Complementary metal-oxide-semiconductor) camera.
[0044]
[0045] In this description, a thick Bragg grating with so-called horizontal or vertical index strata is referred to as a thick Bragg grating with index modulation in a single preferred direction, allowing a set of parallel index strata to be defined. The terms horizontal and vertical are used arbitrarily and simply mean in this description that the two sets of strata of the two respective Bragg gratings are perpendicular. A thick Bragg grating with so-called multiplexed index strata is a thick Bragg grating with index modulation extending in two privileged directions, allowing to form two sets of multiplexed strata extending in two perpendicular directions.
[0046] According to an example, the refractive index n(x,y) in a Bragg grating can be written, in each of the perpendicular directions x and y:
n(x,y)=n.sub.0+n.sub.x sin(2x/.sub.x)+n.sub.y sin(2y/.sub.y) (3)
[0047] Where n.sub.0 is the average index, .sub.x and .sub.y the pitches (or periods) of the refractive index modulations along the two perpendicular directions x and y respectively and n.sub.x and n.sub.y the amplitudes of the refractive index modulations along the two perpendicular directions x and y respectively.
[0048] In practice, to obtain a two-dimensional image of the object, a thick Bragg grating with multiplexed index strata can be used as a first example or, as a second example, two thick Bragg gratings arranged one behind the other, with perpendicular index strata between them. In both examples, this makes it possible to define a direction of the deflected wave with respect to the signal wave by two angles defined in planes perpendicular to each other.
[0049] Thus, in an example of two successive gratings with horizontal and vertical index strata, for the first Bragg grating with horizontal index strata (
[0050] In addition, in an example of a thick Bragg grating with multiplexed index strata (
[0051] In practice, thick Bragg gratings with index strata characterized by an angle of inclination with respect to a normal direction at the entrance face of the grating can be used. This makes it easier to mount the Bragg grating(s) in the device by working with an incident wave that is always normal to the input face of the grating while respecting the Bragg's law(s).
[0052] In both the first and second examples, a deflection of the reference wave with respect to the propagation direction of the signal wave may occur provided that the angles (.sub.B, .sub.B) verify the Bragg's law conditions of the grating(s), as described for example in Kogelnik et al. (Coupled wave theory for thick hologram gratings. Bell Labs Technical Journal 48, no. 9 (1969): 2909-2947) and recalled below with reference to
[0053] In
[0054] Bragg angles .sub.B and .sub.B satisfy the following relationships in a known way:
2 sin(.sub.B)=/.sub.x (4)
2 sin(.sub.B)=/.sub.y (5)
[0055] Or, in the approximation of small angles:
2.sub.B/.sub.x (4)
2.sub.B/.sub.y (5)
[0056] Therefore, it is possible, for a given wavelength of the illumination wave of the object, to choose pitches (or periods) .sub.x and .sub.y of the refractive index modulations in two mutually perpendicular directions (horizontal and vertical strata), respectively, in order to determine the angle (2.sub.B,2.sub.B) formed between the reference wave and the signal wave.
[0057] The four electromagnetic fields E.sub.00, E.sub.10, E.sub.01, and E.sub.11 correspond to light beams detectable by a matrix detector arranged downstream of the Bragg grating(s), as shown in
[0058] More precisely,
[0059] The incident wave is a wave coming from an object (a sight) illuminated in transmission by means of a laser source emitting at =660 nm. A camera with 20482048 elementary detectors (or pixels) allows the acquisition of images. Images 41-44 represented in
[0060]
[0061] Thus, the total field E.sub.t is the sum of the four transmitted fields:
E.sub.t=E.sub.00+E.sub.10 e{circumflex over ()}{i k.sub.x x}+E.sub.01 e{circumflex over ()}{i k.sub.y y}+E.sub.11 e{circumflex over ()}{i k.sub.x x+i k.sub.y y}(6)
Where:
[0062]
k.sub.x=4.sub.B/(7)
k.sub.y=4.sub.B/(8)
[0063] The interferogram is given by the intensity of the total field strength:
I=|E.sub.t|e{circumflex over ()}2(9)
[0064] The cross-interference term E.sub.00 E.sub.11* of the interferogram thus calculated represents the useful signal for hologram reconstruction.
[0065] Image 47 corresponds to the amplitude of the spatial Fourier transform of the interferogram shown in image 45. The useful component of this signal, corresponding to the cross-interference term E.sub.00 E.sub.11*, appears in the upper right corner on the calculated amplitude of the spatial Fourier transform of the interferogram, shown in image 47 of
[0066] Image 48 is the hologram calculated in the plane of the object by a discrete Fresnel transform of the interferogram; a calculation method is described for example in the article by N. Verrier et al. (Off-axis digital hologram reconstruction: some practical considerations. Applied optics 50, no. 34 (2011): H136-H146). The hologram region in the upper right corner of image 48 corresponds to the amplitude of the discrete Fresnel transform of the cross-interference term E.sub.00 E.sub.11* calculated in the plane of the object. The phase of this hologram corresponds to the phase difference between field E.sub.00 and field E.sub.11 calculated in the plane of the object.
[0067] In practice, for the implementation of the off-axis digital holography method according to this description, the choice of pitches .sub.x and .sub.y of the horizontal and vertical strata may be made taking into account the sampling rules dictated by the Nyquist-Shannon theorem. The angles of deflection 2.sub.B and 2.sub.B between the electromagnetic field waves E.sub.11 (deflected reference wave) and E.sub.00 (transmitted signal wave) advantageously satisfy conditions 2.sub.B[.sub.S/2, .sub.S/2] and 2.sub.B[.sub.S/2, .sub.S/2], with:
2.sub.S/d.sub.x (10)
2.sub.S/d.sub.y (11)
[0068] Where .sub.S and .sub.S are called coherent detection acceptance angles, and d.sub.x and d.sub.y, respectively, the pitches between the elementary detectors (or pixels) of the two-dimensional detector, in the x and y directions, respectively.
[0069] The applicants showed that the use of thick Bragg gratings for the formation of signal and reference waves in an off-axis digital holography assembly is very robust, especially since the reference wave is formed from the object wave. Thus, the phase of the hologram corresponds strictly to the phase difference between field E.sub.00 and field E.sub.11 calculated in the plane of the object. In other words, phase fluctuations that may be present in separate arm interferometry assemblies are avoided here.
[0070] In addition, it is remarkable to note that a thick Bragg grating generates a spatial filtering of the deflected wave, which contributes to forming an angularly low-pass filtered reference wave and therefore, a very good quality hologram.
[0071] More precisely, the angular width of the beams deflected by thick Bragg gratings, respectively with horizontal index strata (
.sub.1n.sub.0.sub.x/d (12)
.sub.1n.sub.0.sub.y/d (13)
[0072] The thickness d of a Bragg grating is defined by the thickness through which the incident wave will pass. In a thick Bragg grating designed to work at normal incidence with respect to the grating entry face (index strata inclined at an angle F with respect to a normal direction at the entry face of the grating), the thickness d of the thick Bragg grating can simply be the distance between the entry and exit faces.
[0073] Thus, for example, for a thickness of each Bragg grating thick 9 mm, an average index n.sub.01.5 (average index of glass) and pitch values .sub.x18.9 m et .sub.y18.3 m, .sub.1=.sub.13.3 mrad are obtained, which is equivalent, in an interferometer of the point diffraction interferometer type as described in the reference Smartt, R. N. et al. (Point-Diffraction Interferometer. Journal of the Optical Society of America. 62: 737 (1972)) to filtering by a 330 m diameter pupil, placed in the focus of a 10 cm focal lens.
[0074] It is therefore possible to adapt the pitches of the index strata .sub.x and .sub.y and the grating thickness d according to the angular width (.sub.1,.sub.1) required for the deflected reference wave.
[0075]
[0076] In the example of
.sub.0=.sub.0=2 arcsin(NA) (14)
[0077]
[0078] In the first case, the angular bandwidth (.sub.0,.sub.0) of the wave coming from the object is defined by
.sub.0D.sub.x/L (15)
.sub.0D.sub.y/L (16)
[0079] Where D.sub.x and D.sub.y are the dimensions of the image field defined by the detector, respectively along the x and y axes, and L is the distance between the plane of the object and the detector.
[0080] In the second case, the angular bandwidth (.sub.0,.sub.0) of the wave coming from the object is defined by
.sub.0a.sub.x/(17)
.sub.0a.sub.y/(18)
[0081] Where a.sub.x and a.sub.y are the dimensions of the field diaphragm 52, respectively along the x and y axes, and l is the distance between the plane of the object and the field diaphragm.
[0082] In practice, as described above, for the implementation of the off-axis holography method according to this description and illustrated in
[0083] As will be described in relation to
[0084] In particular,
[0085] This configuration has the advantage of ensuring greater angular selectivity (.sub.1, .sub.1) of the wave E.sub.11, for given grating thicknesses. Indeed, in a single thick Bragg grating, the search for small deflection angles between the reference wave and the object wave results in important index strata pitches (see equations (3) and (4)). To benefit from a good filtering power of the reference wave (equations (12), (13)), it is then necessary to increase the thickness d of the grating, which is not desirable beyond a certain limit. The configuration with split Bragg gratings allows to work with gratings that remain thin.
[0086] For example, two successive gratings of periods .sub.1=1.5 microns and .sub.2=1.9 microns each 2.25 mm thick, with orientation angles of the strata .sub.1.sub.280 degrees, allow an angular selectivity in the order of .sub.01 mrad, and a deflection angle between the reference wave and the object wave of about 1.5 degree. To obtain an angular selectivity in the order of .sub.01 mrad and a deflection angle between the reference wave and the object wave of about 1.5 degrees with a single grating, its pitch must be about 20 microns and its thickness must be about 30 mm. The distance between the object and the detector in a device as shown in
[0087] Although
[0088] Although described through a number of detailed exemplary embodiments, the off-axis digital holography optical imaging method and device according to this description comprise different alternative embodiments, modifications and improvements which will be obvious to those skilled in the art, it being understood that these different alternative embodiments, modifications and improvements fall within the scope of the invention as defined in the following claims.