1. Technical Field
This invention broadly relates to methods, instruments and apparatus for use in the characterization of optical systems, devices and elements. It is applicable to the determination of reflective and refractive characteristics of figured optical elements such as lenses, mirrors and even complex optical systems such as natural or model eyes and optical instruments.
One use of such methods and apparatus is mapping or spatially resolving refractive power over the area of a lens, which is sometimes referred to as the determination of wave-front aberrations of the lens. The instruments or apparatus concerned include wave-front sensors that can be used with the human eye, with isolated lenses, sets of lenses, mirrors and figured reflective or refractive surfaces (collectively referred to herein as ‘optical system(s)’). Of particular practical interest is mapping the refractive power of ophthalmic lenses, and more specifically of soft contact lenses for the purpose of quality control in production, experimental use and prescription.
The reflective and refractive characteristics of interest are data-sets here—referred to as ‘power maps’ indicating the variation of sphere, prism, cylinder and/or axis components, Zernike descriptors for higher and lower order aberrations, optical mean transfer functions, averaged power profiles, or the like, over an optical surface of the optical system of interest. Visualization of the variation of selected characteristics over an optical surface provides a valuable way of checking the performance of an optical system. This allows efficient assessment of the various refractive, blending and peripheral zones of soft contact lenses, for example. The methods and apparatus of the present invention may also be applied to mapping the optical characteristics of the intact human eye onto—say—the surface of the cornea by making use of light reflected or scattered from the retina or another surface of the eye.
For convenience, therefore, such data-sets and their generation will be herein referred to as ‘power maps’ and ‘power mapping’ without intending to suggest that either visualization is essential or that simple refractive power is the only characteristic of interest.
2. Description of Related Art
A variety of wave-front sensing methods are used for assessment of optical aberrations of lenses. An overview of these methods has been given by J. M. Geary. ‘Introduction to Wave-front Sensors’ SPIE 1995, ISBN-13: 978-0819417015. Hartmann-Shack and ray-tracing techniques are commonly used for mapping the optical aberrations of lenses and are suited to mapping the complex optical characteristics of the natural eye. These techniques were explained and compared by E. Moreno-Barriuso and R. Navarro in a paper entitled, ‘Laser Ray Tracing versus Hartmann-Shack sensor for measuring optical aberrations in the human eye’ [J. Opt. Soc. Am. A/Vol. 17, No. 6/June 2000].
In the Hartmann-Shack technique, a plate consisting of a uniform array of micro-lenslets is positioned in the optical path after the lens under test so that a corresponding array of image spots is projected onto the objective plane, the departure of the image array from uniformity indicating aberration (or local variation in optical power). In this technique, it is not necessary to know the precise distance of an optical surface or axis from the instrument or target for good results.
In ray-tracing, a narrow laser beam is scanned over the surface of the lens to build up a similar image array, one spot at a time. While ray-tracing allows a more finely detailed power map to be generated because spot sizes can be less than for Hartmann-Shack, the Hartmann-Shack technique allows rapid assessment since all rays/spots are processed at once rather than serially. It should also be noted that ray-tracing methods assume that the position of a lens surface along the optical axis of the instrument is known with precision, which is problematic in the case of optical devices with small, strongly curved or figured surfaces, or which are flexible like soft contact lenses. Wave-front aberrations are commonly described by means of Zernike Polynomials. These polynomials can mathematically be converted into refractive power maps to visualize the lower order aberrations within the plain view of the optical device.
An example of a ray-tracing technique for measuring refractive aberration in the human eye is disclosed by U.S. Pat. No. 6,932,475 to Molebny et al [and by Molebny et al in “Principles of Ray Tracing Aberrometry” J. Refractive Surgery, Vol 6 S572-S575 (2000). See also U.S. Pat. Nos. 7,311,400, 7,303,281 and 6,409,345 to Molebny]. In U.S. Pat. No. 6,932,475, for example, an image of a spot reflected from the retina is directed to two linear CCD detectors arranged at the same effective distance from the retina in such a way that the x-coordinate of the spot is recorded by one detector and the y-coordinate of the same spot is simultaneously recorded by the other. In this way, an aberration map can be built by showing the manner in which spots are shifted with respect to the interrogating beam.
Campbell and Hughes [Vision Res. Vol 21 pp 1229-1148, 1981], Glasser and Campbell [Vision Res. Vol 38 No. 2 pp 209-229, 1988] and Roorda and Glasser [Journal of Vision (2004) 4, 250-261] disclosed methods of measuring wave aberrations in isolated animal eye lenses in which the trajectories of an array of narrow incident and refracted laser beams are photographed laterally or from the side. In these methods, a mounted lens is located in a tank of a milky solution that makes visible the incident and emergent rays. The incident rays can be scanned laser beams or a bundle of incident beams directed parallel to the optical axis of the lens under test. The number of rays that can be employed is strictly limited by the need to visualize and distinguish them in side view. However, the slope of each ray was estimated (if crudely) and a contour map of wave-front aberration was constructed. Though not disclosed, it is noted that the refractive power at a spot on the lens can be estimated from the slope of the beam emerging from that spot and, therefore, it should be possible to construct a power map of the lens. The accuracy and resolution of such a map would leave a lot to be desired and the crudeness and laboriousness of the technique makes it quite impractical as a method for generating useful power maps of contact lenses for production quality control. The technique cannot, of course, be applied to eyes in vivo.
Chase et al [Chase R, Keleti S, Norman B R, A Scanning Hartmann Instrument. Proceedings of SPIE Volume 1618, Large Optics II (1991) pp 89-96] presented a method for slope determination of large mirrors whereby a laser beam is scanned across the mirror in a pivoting motion and the reflected beam is captured with a photodetector mounted on an x-y stage. From the lateral position of the detected reflected beam, the slope of the mirror can be determined for each raster spot. The position detection unit can move only in the lateral x-y plane and its axial location is in close proximity to the incoming beam steering scanner to achieve optimum resolution and measurement range.
A concept of using spot detection at two axial planes has been disclosed in U.S. Pat. No. 6,406,146 B1. The apparatus is essentially a Hartmann-Shack ocular wave-front sensor with a beam splitter added after the lenslet array so that a second photodetector can be added at a different axial position to the first one. This second detector helps to extend the measurement range by reducing the ambiguity of overlapping spots, which is the limiting factor with single detector Hartmann-Shack systems.
From one aspect, this invention involves directing an incident beam onto spots on an optical surface so as to generate an emergent beam for each spot, determining the lateral location of each emergent beam at first and second optical distances from the surface and deriving the optical power at each spot therefrom. Normally this will involve calculating the emergent angle of the emergent beam at each spot. The resulting data can then be used to determine the optical characteristics of the system. Normally, the scanning of the incident beam, the computation of emergent beam angles, the generation of the data-set and its visual presentation will be computer-controlled or mediated. This will allow a wide variety of optical characteristics of the optical system to be generated and, if desired, to be visually mapped onto a representation of the optical surface.
The lateral locations of the emergent beam are preferably determined by employing detector means that includes at least one photodetector array that can be arranged to intercepting at least a portion of the emergent beam at each optical distance and to output the lateral spatial coordinates of the beam at each distance to processor means. The lateral coordinates of an emergent beam at two distances will generally be sufficient to allow the angle of emergent beam to be determined with sufficient precision and, when related to the corresponding incident angle of the beam, the refractive power of the optical system at each spot to be readily computed. The set of such measurements and/or computations over the optical surface then provides a data-set from which as noted above many important optical characteristics of the optical system can be derived and, if desired, displayed or mapped onto the surface.
It is convenient but not essential to ensure that each incident beam is parallel with is a fixed axis of the optical system. Normally, this will be the central optical axis of the system but the fixed axis can be arbitrarily designated. If all incident beams are parallel with one another—and preferably parallel with the optical axis of the system—then variation of the angles of the emergent beams can be used as a proxy for power variation of the optical system over the designated optical surface. If the angle of the incident beam varies from spot to spot, as would be the case where the incident beams are conically scanned from a common point source, then it is necessary to record or calculate the angle of each incident beam with respect to a common datum such as the optical axis and to employ both the incident and the emergent angles for each spot to calculate the ‘spot power’.
It is convenient to use two-dimensional photodetector arrays (for example CCDs or CMOS detectors of the types commonly used in digital cameras) to detect and output, determine and/or derive the intersection coordinates of the emergent beam at each optical distance or plane so that the angle and/or position of the emergent beam can be determined. Various arrangements are envisaged. For example, a single detector array can be moved from one plane to another and beam coordinates can be derived at each location. A single fixed array can be used at one location with one or more beam-dividers that direct portions of the emergent beam to an array via different optical distances; the various portions of the emergent beam being distinguished from one another by encoding, time-division or other forms of multiplexing. Multiple photodetector arrays can be used in-line if selected arrays are moved into or out of the beam path to intercept the emergent beam at a desired distance. Alternatively, it may be possible to obtain photodetector arrays that are sufficiently transparent to allow one to be fixedly located in-line behind the other. Multiple fixed arrays that are not in-line can be employed by using beam-dividers to direct portions of the same emergent beam to each.
Any convenient beam-divider known in the art may be employed, such as partially silvered mirrors, dichroic or polarizing or non-polarizing cubic or pelliclular beam-splitters, rotating or oscillating mirrors, cubes, prisms that act as beam switchers, or beam multiplexers that make use of encoding, variation of optical properties or time-division multiplexing.
While the detector arrays are preferably of the planar two-dimensional ‘area’ type so that each can immediately output the lateral coordinates of the emergent beam at its location, narrow linear detector arrays can also be employed if intersections along specific meridians only are of interest. Otherwise, such linear detector arrays can be rotated or crossed at a location to effectively act as full or partial area arrays.
It will be appreciated from the above that the detector means embraces both the detector arrays and any beam-divider.
In one application, the method may include the step of supporting a hydrated soft contact lens horizontally and directing the incident light beam vertically downward through the lens and dividing the emergent beam at a location below the lens to direct different portions of the refracted emergent beam to respective fixed detectors arranged at different optical distances from the lens. In this case, the contact lens constitutes the optical system and, conveniently, its upper surface constitutes the optical surface over which optical characteristics are to be mapped. As some contact lenses do not have circular peripheral boundaries, have multiple optical zones, are designed to be used in a particular orientation, and/or have minute orientation markings, it is desirable for the incident beam to be scanned over the entire surface of the lens, beyond its peripheral boundary and for the computer software to identify and reproduce the orientation mark.
The use of more than two detectors at different distances can enhance the precision with—or the range over—which the coordinates of the emergent beam can be determined at a given plane or location. The additional detector or detectors can be positioned intercept emergent beams that are deflected more or less normal. For example, when a more powerful lens than normal is being mapped, the emergent beam may be ‘super-deflected’ to such a degree that it misses the more remote of two ‘standard’ detectors. A third detector could thus be positioned to intercept the super-deflected emergent beam. An additional beam-divider may be used to deflect portion of the emergent beam to the additional detector. Alternatively, (as indicated above) the ‘standard’ remote detector could be moved to intercept the super-deflected beam. Conversely, if a weaker lens than normal is being characterized, the ‘standard’ near detector may be positioned too close to read the emergent beam coordinates with sufficient accuracy and the near detector might be moved further away or a third, more remote detector, with an associated beam-divider may be used for that purpose. Many other arrangements are possible within the scope of the present invention.
As already noted, the method may involve the step of scanning the interrogating beam beyond the edge of the lens so that the edge can be detected and the periphery of the lens can be precisely and automatically determined. This not only allows the entire lens to be mapped but also ensures that the power map is correctly and automatically aligned where the lens does not have a circular periphery or is otherwise asymmetric. Thus, the method can also include the step of determining the edge/boundary, the optical axis, the physical or optical center of the optical system. Similarly, where the lens bears an orientation mark, the method may include the step of detecting and recognizing such a mark. This allows the orientation mark, as well as the peripheral contour to be reproduced with the power map. In the specific case of multi-focal optical systems (such as bifocal ophthalmic lenses), the method may also include the step of detecting the junction/boundary between adjacent optical power zones.
In another variant, the method may include the step of adjusting the angle of the incident beam with respect to the optic axis of the lens being mapped, with concomitant adjustments of the angles and positions of the detectors, as required. This is of particular value with ophthalmic lenses that have a central optic zone surrounded by a peripheral optic zone adapted to adjust the peripheral curvature of field in the manner taught in U.S. Pat. No. 7,025,460 to Smith et al.
From another aspect, the invention includes apparatus, an instrument or a system for use in characterizing an optical system with respect to an optical surface of the system, the apparatus including:
The detector means may include separate photodetector arrays located at first and second optical distances from the optical system, each detector array being adapted to output the lateral coordinates of the intersection of an emergent beam with the array. To avoid one array occluding the other, the array(s) closer to the optical system might be moveable to allow the emergent beam to strike a more remote array. Alternatively, the arrays need not be positioned in-line (so that one occludes another) but, instead, the detector means may include beam-divider means that direct a different portion of the emergent beam to each array. In another arrangement, the detector means may include only one photodetector array that can be moved between the first and second optical distances so that the same array is used to determine the lateral coordinates of the emergent beam at each distance or position. As already indicated, the detector means may include more than two separate detector arrays and beam-divider means to direct at least portion of the emergent beam to each.
In one embodiment, the apparatus may be an instrument for mapping the power and/or aberrations of an eye lens (such as a contact lens or spectacle lens). Where the lens is a soft contact lens, it is preferable that it be mounted in a hydrated state—possibly within an aqueous bath—so that it sits upright with its plane horizontal without substantial distortion due to gravity or surface tension, the scanning means may direct the incident beam vertically downwards through the lens, the detector means with its photodetectors and beam-divider (if used) being arranged below the lens. Techniques for mounting and locating soft contact lenses are known in the art and are, for example, employed with Hartmann-Shack instruments.
It will be convenient to employ lasers to generate the incident beams, as is common in the art. The incident beam or beams can be monochromatic with a wavelength selected to suit the purpose of the investigation. More usually, beams with a range of wavelengths that approximate white light in the visible spectrum are appropriate where the lens being characterized is intended for use in association with eyes. However, the use of bi- or poly-chromatic beams is also envisaged to obtain specific spectral characteristics of the device under test.
Having portrayed the nature of the present invention, particular examples will now be described with reference to the accompanying drawings. However, those skilled in the art will appreciate that many variations and modifications can be made to the examples provided without departing from the scope of the invention as outlined above and as claimed below. Also, many other examples are possible within the scope of the invention.
In the accompanying drawings:
In
Scanner unit 17 is connected to and operates under the control of a computer “PC”. Scanner 17 includes a laser light source, an electromechanical scanning device as well as a scanner driver adapted to interface with computer PC, these components not being show as such scanner units are known in the art.
The emergent beam 20 is intercepted by a partially reflective beam-splitter 22 (which serves as a beam-divider) that transmits one portion 20a of emergent beam 20 to a first detector array 24 and reflects a second portion 20b to a second detector array 26, arrays 24 and 26 being located by mounts 24a and 26a that are fixed relative to lens 12 and beam-splitter 22. [Thus, in this example, the detector means comprises beam-splitter 22 and detector arrays 24 and 26.] For convenience, the plane of first detector array 24 is shown orthogonal to axis 14 and optically closer to lens 12 while the plane of array 26 is shown parallel to axis 14 and optically further away from lens 12 than array 24. While this particular arrangement is not essential, it is important that arrays 24 and 26 are positioned at different optical distances from lens 12; one array (say array 24) being at the first optical distance and the other (say array 26) being positioned at the second.
In
The data set or power map thus generated can be used in many ways known in the art. For example, to compare the designed and measured power profiles to monitor the quality of manufactured lenses, or to compute corrective optics, optical improvements or modifications. This is of considerable importance where an ophthalmic lens is being figured or customized to match and correct the aberrations of a particular human eye. Such a figured surface may be applied to a corrective lens by a machine, indicated at 28. Alternatively, where the optical system is the eye (as described with reference to
It will be appreciated by those skilled in the art that the basic optical configuration of instrument 10 of
A first variant 30 of the instrument of the first example is diagrammatically illustrated by
A second variant 34 of the instrument of
In the third variant 40 of the first example shown in
The fifth variant 60 of the first example shown in
In instrument 100 the single detector array 112 is fixed at a location indicated by broken line 114, array 112 being drawn in solid lines at this position. Wet cell 104, together with soft contact lens 102 that serves as the optical system under investigation, is moveable up and down along optical axis 106 between two positions, indicated at 116 and 118, position 116 being a shorter optical distance from detector array 112 than position 118. If desired, cell 104 can be moved to one or more intermediate positions for scanning by incident beam 108 to exploit the advantages mentioned in connection with instrument 50 of
In a second configuration of instrument 100, array 112 can be moved up and down along axis 106 so as to be closer to or further away (optically) from lens 102 in wet cell 104, as indicated by arrow 122. For simplicity, it is assumed that only two positions, indicated at 114 and 124 are required, though one or more intermediate positions can be readily employed with the advantages mentioned in connection with instrument 50 of
While this example of an instrument for characterizing an optical system such as a contact lens eliminates the need for a beam-divider, the need to accurately move the detector array(s) and/or the optical system in one or two dimensions will add cost and complication.
The third example of a measurement instrument or system formed in accordance with the present invention is shown in
It is convenient to map the optical characteristics of eye 152 onto the surface of cornea 161 rather than retina 125 because the cornea is readily visualized and, in procedures involving the reshaping of the cornea, the contour or profile of the cornea surface prior to the reshaping procedure is determined with considerable accuracy. The combination of mapping the power of the eye onto the cornea with determination of the profile of the cornea provides near-complete information necessary for cornea modification as well as the provision of tailored corrective ophthalmic lenses. However, the optical characteristics of the eye could be mapped onto the surface of the retina, or any other interface that can be visualized within the eye, if desired.
The fourth exemplary embodiment of the invention is instrument 200 shown in
Emergent beam 204 is split by beam-splitter 208 into two portions. A first portion 204a travels direct to array 207 over a short optical distance via a second beam-splitter 210 and a second portion 204b travels indirectly over a longer optical distance to array 207, also via second beam-splitter 210. The greater optical distance for beam portion 204b is achieved by reflecting beam 204b laterally in splitter 208 to a first mirror 214, from which it is reflected to a second mirror 216 that reflects it back to second beam-splitter 210 from which it is finally reflected to array 207 along with the first beam portion 204a.
Confusion between beam portions 204a and 204b at array 207 can be avoided in a number of ways, the most convenient being discrimination by optical properties, time multiplexing or pulse-encoding. Discrimination by optical properties can be implemented using a first optical filter 218 in the path of beam portion 204a and a second filter 220 in the path of beam portion 204b. Filters 218 and 220 can be polarizing, chromatic or intensity; the choice depending upon the characteristics of detector array 207. Thus, if array 207 is color sensitive, filter 218 might be a chromatic red filter and filter 220 might be a chromatic green filter so that beam portions 204a and 204b can be readily distinguished by array 207. Time multiplexing can be implemented by introducing a first mechanical or opto-electronic chopper 222 into the path of beam portion 204a and a similar chopper 224 into the path of beam portion 204b. Choppers 222 and 224 are operated so that beams 204a and 204b are alternately blocked so that they are presented alternately to array 207, a form of time-division multiplexing. This requires the computer system (not shown here) to keep track of which beam is present in each time-slot, a matter that those skilled in the art will be able to implement. Pulse encoding can be implemented by using only one of choppers 222 or 224, say chopper 222 in the path of beam 204a. This chopper is operated significantly faster than the scanning of incident beam 202 from spot to spot on lens 206 so that the signal from beam 204a appears as AC while that from beam 204b appears as DC during the time interval that incident beam 202 remains on spot P0. These two signals will then be readily distinguished by well known electronic filtering techniques.
Another optional refinement of instrument 200 allows the path length of beam portion 204b to be lengthened as desired so as to greatly increase the sensitivity of the instrument where the optical system being characterized either has unusually low refractive power or aberrations. In this option, the sub-assembly indicated by box 226 comprising mirrors 214 and 216 can be moved laterally towards and away from beam-splitters 208 and 210 to alter the optical distance between the optical system [lens 206 in this case] being characterized and detector array 207 for beam portion 204b only. This variation of instrument 200 can be extended to include more than two optical path lengths. More beam-dividers can be added to generate several optical path lengths, before recombining them to be detected by a single detector. The use of other variations described in the previous examples—such as the substitution of a moving-mirror beam-divider for beam-splitter 208 and/or 210—is also envisaged.
Number | Date | Country | Kind |
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2007900710 | Feb 2007 | AU | national |
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/AU08/00183 | 2/14/2008 | WO | 00 | 4/15/2010 |