Known systems for precision alignment or displacement measurements have a number of common drawbacks. In particular, such systems are generally complex and expensive. Additionally, many such systems are inflexible in requirements, e.g., space and/or isolation requirements, making implementations awkward or impossible in many applications. Many require specific patterns such as grating patterns to be laid-down on the object being measured to produce moiré or diffraction patterns. Such patterns can be highly regular, so that spatial-uniqueness (or false matches) can become an issue. Also many precision measurement systems that are accurate at small dimensions are specifically designed for alignment sensing and cannot track movement or provide quantitative displacement information. Further, the systems that do provide quantitative displacement information are often unable to do so in real-time because of required scanning processes or significant post-processing.
Current measurement systems for tracking of an object can be broadly categorized as being optical or non-optical measurement systems. An interferometer is one example of an optical measurement system that can precisely measure the position or velocity of an object by interfering or comparing a beam reflected from the object with a reference beam. Other optical interference based measurement systems are known that track object movement by measuring the movement of diffraction patterns that gratings mounted on the object generate. Some other optical measurement systems use image correlations to detect the alignment or movement of known geometric patterns. Non-optical techniques are also available or proposed for tracking object movement. Examples of non-optical systems for precise measurements of small displacements include a Scanning Electron Microscope (SEM), an Atomic Force Microscope (AFM), or a capacitance sensing system.
An advantage of optical measurement systems when compared to the non-optical systems is the availability of precise and relatively inexpensive beam sources and optical elements. Accordingly, optical systems for alignment or tracking have been implemented at scales ranging from tracking astronomical bodies to tracking missiles to tracking integrated circuit structures.
One specific optical technique for measuring a displacement uses Fourier transforms of consecutive images of an object. A well-known property of Fourier transforms is that a position shift in an image results in a phase delay in the Fourier transform of the image. This property for a two-dimensional Fourier transform is expressed in Equation 1, where functions ƒ(x,y) and ƒ(x−x0, y−y0) can respectively represent intensity variations of an image and a shifted image and a function F(ωx,ωy) represents the Fourier transform of function ƒ(x,y). In the Fourier transform of Equation 1, the phase (ωxx0+ωyy0) is a linear function of frequencies (ωx,ωy) having slopes equal to the displacements (x0, y0) of the image. However, determination of the displacement vector through phase delays in measurement systems have generally required transformations back to the spatial domain because comparisons of phases of transformed functions in the frequency domain correspond to subtractions of measurements that are believed to increase the effects of measurement noise.
Optical systems for tracking movement with nanometer scale accuracies are desired, particularly for manufacturing of nanometer-scale devices.
In accordance with an aspect of the invention, a system or method for measuring a displacement of an object transforms data derived from images of an object to generate frequency domain data; determines phases corresponding to the frequency domain data, assigns weights to phases according known properties of the frequencies, and uses the phases and the weights to determine one or more slopes corresponding to change in the phases with change in frequency. The slopes indicate the displacements and can provide accuracies down a fraction of a pixel size, thereby providing nanometer scale precision using conventional digital imaging systems.
Use of the same reference symbols in different figures indicates similar or identical items.
In accordance with an aspect of the invention, displacements much smaller than image pixels and smaller than the wavelength of illumination used for imaging can be observed from phases measured in transformed images. In particular, a slope of the phase as a function of the domain of the transformed space indicates a magnitude of a shift in the untransformed space. Determination of the slope in the transformed domain, e.g., the frequency domain, allows selection of data for reduction of measurement error. In particular, values associated with frequencies expected to be noisy, for example, frequencies corresponding to vibrations of the imaging system, spatial variations in illumination, or patterned sensor noise, can be ignored or given less weight in the measurement. Data associated with frequencies at which the transform is small can be similarly ignored given less weight.
An imaging system 130 captures images of object 110 and provides the images to a processing system 140 for analysis. Imaging system 130 can generally be any type of system capable of generating an image that can be divided into pixels corresponding to the portions of object 110 having a known size (or known sizes). Some specific implementations of imaging system 130 include video or still, digital or analog, color or black-and-white cameras. In the illustrated embodiment, imaging system 130 includes a lens 132, a light source 134, and a sensor array 136. Objective lens 132, which can be a microscope objective lens providing a magnification, is focused to form an image of object 110 on sensor array. Light source 134 illuminates object 110 during image capture and generally can be a conventional white light.
Sensor array 136, which can be a conventional CCD or CMOS sensor array captures and digitizes each image of object 110 for transmission to processing system 140. Generally, the image data from sensor array 136 is in the form of a pixel map containing pixel values, with each pixel value corresponding to an area of known size, e.g., 10 μm by 10 μm on object 110. The size and depth of the pixel map is generally not critical provided that the pixel map provides sufficient image data for analysis.
In one specific embodiment of imaging system 130, image sensor 136 is a monochrome digital camera such as the Pulnix™-1400CL has a 1.4M pixels CCD that provides 8-bit pixel values, a pixel size of 4.65 μm in the image plane, and a maximum frame rate of 30 Hz. Lens 132 is a system of two alternative lenses such as Neo S Plan 20x/0.40NA (Numerical Aperture) and 50x/0.80NA available from Olympus, and light source 134 is a power regulated light source from Schott fitted with a standard broadband white light (e.g., a Phillips 150W Focusline). Alternatively, a narrow band light source could reduce the chromatic aberration and hence allow for a better focus, resulting in a higher displacement resolution. However, measurement accuracies less than a pixel, e.g., less than 10 nm can be achieved using white light, so white light may be preferred for system simplicity and lower cost.
Processing system 140 analyzes the images from digital imaging system 130 and quantifies the displacement of object 110 from one image to the next. Processing system 140 can be implemented in any desired manner including but not limited to implementations as hardwired logic that performs the desired analysis or as a general-purpose computer executing software or firmware that performs the desired analysis.
The initial step 310 of process 300 performs a transform such as a Fourier transform (or a Discrete Fourier transform) on the pixel data ƒ1(x,y) of the first image to generate a transformed function F1(ωx,ωy). Transformed function F1(ωx,ωy) like the pixel data in the spatial domain consists of discrete values, but the discrete values in the frequency domain are indexed by discrete values of angular frequencies ωx and ωy. As an illustrative embodiment, the following description of process 300 assumes that transformed function F1(ωx,ωy) is the Fourier transform (or the Discrete Fourier transform) of pixel data ƒ1(x,y), but as described further below, transforms other than Fourier transforms could alternatively be used.
Step 320 transforms the pixel data ƒ2(x,y) of the second image to generate a transformed function F2(ωx,ωy). Since the second image is theoretically the same as the first image after a shift operation, the Fourier transformed functions F1(ωx,ωy) and F2(ωx,ωy) theoretically should satisfy Equation 2. Since transformed functions F1(ωx,ωy) and F2(ωx,ωy) are determined from measured pixel data ƒ1(x,y) and ƒ2(x,y), Equation 2 will generally be only an approximation.
Step 330 determines the phase θ(ωx,ωy) of the ratio of transformed functions F1(ωx,ωy) and F2(ωx,ωy) for the range of frequencies ωx and ωy. As shown in Equation 3, phase θ(ωx,ωy) is approximately equal to ωxx0+ωyy0. Accordingly, displacements x0 and y0 can be determined from the slopes of phase θ(ωx,ωy).
Slopes of phase θ(ωx,ωy) can be determined using conventional analysis techniques such as a least square fit on all of the phase values associated with all of the discrete values of frequencies ωx and ωy. However, in accordance with an aspect of the invention, a step 340 assigns weightings to values of the phase θ(ωx,ωy) based on known properties of frequencies ωx and ωy. In the illustrated embodiment, step 340 includes a step 342 that identifies ranges of frequencies ωx and ωy that are expected to be noisy, based on known characteristics of the measurement system, and a step 344 then assigns weights to phase values corresponding to the identified frequencies. Noisy frequencies may, for example, correspond to a mode of vibration of the measurement system, a frequency of the illumination pattern used when capturing images, or periodic sensor noise to name a few examples. The frequencies identified in step 342 depend on the properties of the measurement system and hence may be known before the start of any particular measurement using process 300.
Step 346 uses measurement data to identify noisy frequencies or frequencies having any other known property. These identified frequencies may be unique to specific measurements and in particular may depend on the features of the object being measured. In an exemplary embodiment of the invention, step 346 uses the magnitudes of transformed functions F1(ωx,ωy) and/or F2(ωx,ωy) to detect frequency ranges where measurement error may be a more significant factor. For example, when either transformed function is particularly small, i.e., having a magnitude approaching the error, the determined phase θ(ωx,ωy) may be undependable. Step 346 more generally can identify the numerical problem areas such as noisy frequencies with low SNR in magnitude response as well as aliasing. Step 346 can be, but is not required to be, performed on-the-fly or in real time during measurement process 300.
Steps 344 and 348 assign weights to the frequencies identified in steps 342 and 346. The two types of noisy frequencies are fundamentally different types, so that steps 344 and 348 may use different types of masks/weightings. In a simple example of weighting, values of phase θ(ωx,ωy) corresponding to ranges of frequencies ωx and ωy identified in step 342 or 346 can be assigned zero weight. Alternatively, fractional weightings may be assigned based on measurement, e.g., transformed functions F1(ωx,ωy) and F2(ωx,ωy), or as required for the particular slope determination technique employed in step 350.
Step 350 uses the weightings and the phase θ(ωx,ωy) to determine slopes that indicate displacements x0 and y0. For example, step 350 can ignore zero-weighted or masked values when fitting the phases to a linear function or otherwise determining slopes that indicate displacements x0 and y0. Any desired fitting technique can be employed. For example, step 350 could employ a general maximum likelihood method or a least-square fit.
A plot 420 in
A line 416 illustrates a best-fit line based on the weightings of phase values 412 that are not eliminated from the fitting process. More generally, values for the full range of frequencies ωx and ωy can be fit to a plane, where line 416 is in the plane and corresponds to a fixed value of frequency ωy. Slopes of the plane along ωx- and ωy-directions in the frequency domain respectively indicate the displacements x0 and y0. In particular, the slopes measured for the best-fit lines or plane will be equal to the displacements x0 and y0 if appropriate units are used for x, y, ωx, and ωy. If variables x and y are in units of pixels, then the discrete frequencies ωx, and ωy are multiples 2π/pixel, and the displacements x0 and y0 will be measured in pixels or fractions thereof. A measurement in conventional units such as nanometers can be found from the pixel size. For example, with pixels corresponding to 1 μm by 1 μm areas of the object, measurements to an accuracy of about 0.01 pixels indicate displacements x0 and y0 to an accuracy of about 10 nm.
Process 300 of
Another variation of process 300 determines the phase θ(ωx,ωy) from the product of one transformed function F1(ωx,ωy) or F2(ωx,ωy) and the complex conjugate of the other transformed function F*2(ωx,ωy) or F*1(ωx,ωy). The phase θ(ωx,ωy) determined from the product is the same as the phase θ(ωx,ωy) determined from the ratio because division by a complex value is equivalent to the combination of multiplication by the complex conjugate of the value and division by the magnitude of the value and the omitted division by the magnitude, i.e., by a real value, has no effect on the phase.
Step 520 determines the Fourier transform of the spatial correlation. It can be shown that the Fourier transform of the spatial correlation of two functions is equal to the product of the Fourier transform of the first function and the complex conjugate of the Fourier transform of the second function as shown in Equation 5. Accordingly, step 530 determines the phase of the transformed correlation function to determine the same phase θ(ωx,ωy) as found in step 330 of
The above descriptions of selected embodiments of the invention have concentrated on processes using Fourier Transforms. Fourier Transforms have the desirable property that shifts in the spatial domain result in phase delays in the frequency domain as indicated above in Equations 1 and 2. However, other transformations that transform a shifted function to a separable combination of the transform of the unshifted function and a factor depending on the shift x0 could be similarly used to measure the shift x0. Equations 6 illustrate an example of suitable behavior for a transform that permits separation of a function g(x0) from the transform of the shifted function for determination of shift x0. Examples of such transforms include z-transforms, Discrete Cosine Transforms (DCTs), and Wavelet transforms with certain base function.
Although the invention has been described with reference to particular embodiments, the description is only an example of the invention's application and should not be taken as a limitation. Various adaptations and combinations of features of the embodiments disclosed are within the scope of the invention as defined by the following claims.
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