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Foucault knife-edge test

The Foucault knife-edge test, developed by French physicist Léon Foucault in 1858, is an optical method for evaluating the surface accuracy of concave mirrors by analyzing shadow patterns, or shadowgrams, formed when a sharp knife edge interrupts the converging reflected light from a point source positioned at the mirror's center of curvature.^[1] This test reveals deviations from the ideal spherical or paraboloidal shape, such as spherical aberration or astigmatism, through the motion and distribution of shadows across the mirror's zones as the knife edge is moved.^[2] In the standard setup, a small light source is placed slightly offset from the optical axis at the mirror's radius of curvature—twice its focal length—and the observer views the mirror's exit pupil from behind the knife edge, which is positioned at the radius of curvature.^[3] For a perfect spherical mirror, the test produces a "null" result with uniform shadows that do not move relative to the knife edge at this position, confirming the surface's conformance to the expected curvature.^[3] Deviations cause shadows to advance or retreat across specific zones: for instance, in a paraboloidal mirror designed for telescopes, central zones appear brighter or darker compared to the edges due to varying local radii of curvature.^[1] The test's sensitivity stems from its ability to detect wavefront slope errors qualitatively, with shadow speed and direction indicating transverse and longitudinal aberrations; for example, spherical aberration manifests as circular shadow patterns, while coma produces elliptical or hyperbolic forms.^[2] Originally devised to improve astronomical optics, it has become a cornerstone for amateur telescope makers, offering simplicity and precision down to about 1/10th wave peak-to-valley accuracy without complex equipment.^[1] Quantitative extensions, such as measuring knife-edge positions in thousandths of an inch across zones, allow for numerical analysis of surface errors using mathematical models like Fourier series to invert shadow intensity data.^[4] Despite its advantages, the Foucault test has limitations, including reduced effectiveness for fast mirrors with focal ratios below f/4, asymmetrical errors like astigmatism, or when diffraction effects interfere with interpretation.^[1] It remains non-interferometric and more qualitative than modern methods like the Shack-Hartmann sensor, yet its low cost and ease of use continue to make it invaluable for precision mirror figuring in optics fabrication.^[2]

Introduction

Overview

The Foucault knife-edge test is a null test used to measure surface figure errors in concave mirrors, particularly those intended for telescopes, by employing a point light source and a knife-edge to visualize deviations in the reflected wavefront.^[5]^[1] Invented by French physicist Léon Foucault in 1858, it provides a qualitative assessment of mirror shape by observing shadows and light patterns that indicate aberrations such as astigmatism or spherical error.^[6]^[1] This method is especially valued by amateur telescope makers for figuring parabolic mirrors to high precision, achieving surface accuracies within fractions of a wavelength, such as λ/4 or better, which is essential for diffraction-limited performance in astronomical observations.^[7] Its effectiveness stems from the knife-edge's ability to sharply delineate zones of the mirror where the reflected rays converge or diverge from the ideal focus, allowing iterative polishing adjustments without complex instrumentation.^[5]^[8] The test's appeal lies in its simplicity and low cost, requiring only basic components like a pinhole light source for the point illumination, a razor blade as the knife-edge, and an adjustable stand to position the apparatus at the mirror's center of curvature.^[1]^[8] This accessibility has made it a cornerstone of hands-on optics since its development in the context of improving astronomical instruments.^[1]

Historical Development

The Foucault knife-edge test was invented by French physicist Léon Foucault in 1858 during his research on enhancing the performance of reflecting telescopes through precise evaluation of concave mirror surfaces.^[1] This method addressed limitations in earlier optical testing approaches, such as Isaac Newton's reliance on visual inspection of star images or pinpoints reflected by the mirror to assess figure accuracy, which lacked quantitative precision for detecting subtle aberrations like spherical error.^[9] Foucault first detailed the technique in his seminal paper, "Description des procédés employés pour reconnaître la configuration des surfaces optiques," presented to the Académie des Sciences, where he demonstrated its application in identifying deviations in mirror curvature by observing light blockage with a straight edge near the focus. In the early 20th century, the test evolved to support more systematic mirror figuring, notably through the introduction of zonal masks. French astronomer André Couder, chief optician at the Paris Observatory, developed the Couder mask in the 1920s, a patterned overlay that isolated specific annular zones on the mirror for targeted measurements, enabling finer corrections during parabolization.^[10] This advancement built on Foucault's foundational null test principle, where uniform darkening across zones indicates a perfect spherical or paraboloidal surface, and facilitated its use in professional observatories for high-precision optics. The test gained widespread adoption among amateur telescope makers (ATMs) in the mid-20th century, transforming it into a cornerstone of DIY telescope construction. Influential texts like Jean Texereau's How to Make a Telescope (originally published in French in 1951, with the first English edition in 1957 and a second edition in 1984) provided detailed guidance on implementing the test, including mask fabrication and interpretation, democratizing access to professional-level figuring techniques.^[11] Modern resources, such as Vladimir Sacek's comprehensive online compilation Telescope Optics (2006) and David Harbour's series of ATM articles and tutorials (2001–2008), further refined its application, emphasizing zonal analysis and error quantification for enthusiasts.^[1]^[12]

Principles

Basic Optical Principles

The Foucault knife-edge test relies on fundamental principles of geometric optics, particularly the law of reflection, which states that the angle of incidence equals the angle of reflection for rays striking a mirror surface. Under the paraxial approximation—valid for small angles relative to the optical axis—this law ensures that rays from a point source at the mirror's center of curvature reflect back along their incident paths in an ideal spherical mirror. The center of curvature is located at a distance R from the mirror vertex, where R = 2f and f is the focal length, positioning both the light source and observer (or knife-edge apparatus) at this point to capture the returning light.^[1] In a perfect spherical mirror, rays emanating from a point source at the center of curvature diverge, strike the mirror surface, and reflect back to converge precisely at the same point, forming a stigmatic image without aberrations.^[5] This reflection process generates a converging spherical wavefront after interacting with the mirror, with the wavefront's center of curvature coinciding with the center of curvature position at distance R from the mirror.^[13] The observer views this wavefront indirectly through the knife-edge, which is positioned near the focus to intercept the beam; by translating the knife-edge perpendicular to the optical axis, it blocks peripheral rays, producing observable shadows that reveal the light's convergence behavior.^[1] A key distinction arises between spherical and paraboloidal mirrors in this configuration. Spherical mirrors focus all zones of the surface to a single point at the center of curvature when illuminated from that point, resulting in uniform shadow progression across the aperture.^[5] In contrast, paraboloidal mirrors are designed to focus parallel rays (as from a distant source) to a single focal point but exhibit zonal shifts in focus when tested at the center of curvature, where inner and outer zones converge at slightly different positions due to the inherent geometry.^[1]

Aberration Detection Mechanism

Surface deviations on the mirror, such as bumps or depressions, induce longitudinal shifts in the zonal foci of the reflected rays, which in turn distort the overall shape of the converging wavefront. These irregularities alter the optical path length for rays originating from different annular zones of the mirror surface, causing the foci from affected zones to be displaced along the optical axis relative to those from an ideal surface.^[1] As the knife-edge is translated through the focal region, these longitudinal displacements become apparent because rays from defective zones converge either ahead of or behind the knife-edge position compared to rays from nominal zones. Consequently, the shadowgram displayed in the observer's view of the mirror exhibits characteristic light or dark bands, where zones with advanced foci appear brighter when the knife-edge is behind the focus and darker when ahead, and vice versa for retarded foci.^[2] This detection process is enhanced by a radial magnification effect in the shadowgram, enabling visual assessment of aberrations to an accuracy of about \lambda/10.^[1] The test primarily reveals spherical aberration through circular shadow boundaries that vary with defocus, but it also identifies astigmatism via asymmetric intensity distributions along principal axes, coma through elliptical or hyperbolic patterns (though less pronounced at the center of curvature), and turned-down edge defects as localized irregularities in the outer annular zones.^[5]^[2] A qualitative illustration of this mechanism is provided by a central depression in a paraboloidal mirror, which shortens the focal length of the inner zones relative to the outer ones, resulting in a "doughnut" shadow pattern characterized by a dark central region encircled by a brighter annular band when the knife-edge is positioned appropriately near the average focus.^[1]

Setup and Equipment

Required Components

The essential components for conducting the Foucault knife-edge test include a point light source, a knife-edge, a mirror support, viewing aids, and various accessories, each designed to facilitate precise optical evaluation of concave mirrors.^[14] The point light source serves as the illumination origin, simulating a point source at the mirror's center of curvature to reflect light back through the test setup. Typically, it consists of a pinhole with a diameter of 0.1–0.3 mm drilled in aluminum foil, illuminated by a bulb or high-brightness LED for stable, cool operation and to minimize thermal distortion. This configuration ensures a sharp, diffraction-limited spot essential for detecting surface irregularities on mirrors up to several meters in radius of curvature.^[14]^[15] The knife-edge is the core diagnostic tool, functioning to selectively block portions of the returning light rays from the mirror, revealing wavefront deviations as shadow patterns. It is usually a single-edged razor blade or an adjustable slit mounted on a carriage, capable of precise lateral movement perpendicular to the optical axis via a micrometer drive with resolution of approximately 0.001 inch (25 μm). This high precision allows for incremental adjustments to map zonal errors across the mirror surface.^[14]^[1] A sturdy mirror support is required to securely position the test mirror, typically with diameters ranging from 6 to 18 inches, facing the light source and knife-edge assembly. This vertical stand, often constructed from a tripod or adjustable platform with tip and tilt controls, maintains the mirror's alignment at the center of curvature while minimizing vibrations that could obscure observations.^[15]^[14] Viewing aids enhance the test's effectiveness by improving contrast and initial setup accuracy. A Ronchi grating, with line densities of 50–150 lines per inch, may be used optionally for preliminary alignment and coarse figuring checks, though the knife-edge remains the primary method; the entire setup is performed in darkroom conditions to maximize shadow visibility.^[14] Accessories include an adjustable platform for the light source and knife-edge, such as commercial units like the Glatter tester or custom-built versions with dial indicators for 0.001-inch motion, ensuring repeatable positioning along the optical axis. Zone masks, used to isolate specific annular regions of the mirror, are also essential but detailed in zonal testing procedures.^[16]^[15]

Mirror Positioning and Alignment

The initial setup for the Foucault knife-edge test requires precise positioning of the mirror at its center of curvature, determined by measuring the radius of curvature R. This is typically accomplished using a spherometer, which gauges the sagitta of the mirror's curve across its diameter to calculate R via the formula R = \frac{r^2}{2s} + \frac{s}{2}, where r is the mirror radius and s is the sagitta; alternatively, autocollimation with a flat mirror or the test setup itself can verify R by aligning the return beam to coincide with the incident path. The light source and knife-edge are then positioned at a distance R from the mirror vertex along the optical axis, ensuring the converging rays from the mirror focus back at this plane for a spherical surface.^[17]^[1]^[18] To minimize gravity-induced distortions, particularly in larger mirrors where sagging can introduce astigmatism or turned-down edges, the mirror is oriented vertically or slightly leaned back against a supportive cell, reducing flexure effects that could otherwise amplify apparent aberrations during testing. For initial rough alignment, a flat mirror may be temporarily introduced in the beam path to simulate a reference wavefront, allowing adjustment of the mirror's tilt and position until the reflected beam returns centered on the source without introducing extraneous shadows. This step ensures the optical axis aligns properly before proceeding to fine adjustments.^[19]^[1] Focusing the pinhole light source involves adjusting its position relative to a converging lens until the mirror's reflection produces a sharp, point-like image at the knife-edge plane, confirming that the source is effectively at the center of curvature and the beam is collimated for the return path. The knife-edge is then centered by laterally shifting it to bisect the returning beam, achieving a uniform null response—complete and even darkening across the mirror field—for a perfect spherical mirror, with no residual light gradients indicating misalignment.^[18]^[20] Common pitfalls in this alignment process include off-axis tilt of the mirror, which can mimic coma through asymmetrical shadow patterns, or improper centering that introduces cosine errors in zonal measurements, leading to false indications of surface irregularities. These are corrected through iterative adjustments: first using a laser pointer or auxiliary light for coarse centering of the return beam on the source, then fine-tuning with the pinhole and knife-edge under dim conditions to verify uniform illumination and null response across the mirror zones. Such careful iteration is essential to isolate true surface errors from setup artifacts.^[20]^[18]

Conducting the Test

Step-by-Step Procedure

The Foucault knife-edge test begins with illuminating a pinhole light source positioned at the center of curvature of the concave mirror under test, which is typically twice the mirror's focal length for amateur telescope making applications.^[1] The system is then aligned by adjusting the position of the tester until a uniform gray shadow, known as the null condition, covers the entire mirror surface when viewing through the knife-edge; this indicates the light rays are converging correctly at the knife-edge plane for a spherical reference surface.^[3] Next, the knife-edge is slowly advanced perpendicular to the optical axis from one side of the converging light beam to the other, allowing observation of the shadow transition across the mirror field; shadows appear darker in zones where the mirror surface deviates from the ideal figure, with the direction and speed of shadow movement revealing the nature of aberrations such as under- or over-correction.^[20] Observations are recorded qualitatively at multiple knife-edge positions corresponding to partial beam occlusions, such as 25%, 50%, and 75%, by noting the shadow patterns and any null zones where uniform gray appears, providing an initial assessment of the mirror's surface figure across the full aperture.^[3] To achieve parabolization from a spherical blank, the process is iterated by selectively polishing mirror zones based on the observed shadows—such as deepening the center if outer zones appear high—until the measured zonal null positions match the theoretical radius of curvature differences expected for an ideal paraboloid, confirming the correct profile.^[1] Zonal variations using masks can be briefly referenced for enhanced precision in targeted areas.^[20] The test must be conducted in a low-vibration environment, such as on isolated supports, to avoid false shadow signals from external disturbances like building motion.^[21]

Zonal Testing Methods

Zonal testing methods in the Foucault knife-edge test enable precise isolation of annular zones on a concave mirror to assess and correct figure errors during figuring. A key technique involves the use of a Couder mask, which consists of concentric rings inspired by Ronchi rulings, designed to expose one zone at a time by blocking light from adjacent areas.^[22] These masks typically divide the mirror into 10–20 zones from center to edge, with zone boundaries calculated to ensure equal optical path contributions for accurate focus measurements.^[22] The mask is placed directly on the mirror surface using support pins, allowing the tester to focus solely on the illuminated zone's shadowgram. For initial zone identification, tools such as the Everest pin stick or a Ronchi screen are employed to coarsely map zonal boundaries before fine-tuning with the knife-edge. The Everest pin stick, constructed from a wooden rod with pins inserted at calculated zone radii, is suspended across the mirror to mark zones with minimal diffraction interference, facilitating clear visualization of zone edges in the shadow pattern.^[10] A Ronchi screen, featuring evenly spaced parallel lines, can similarly aid in preliminary alignment and defect detection by producing striped interference patterns that highlight zonal irregularities.^[18] Once zones are identified, the observer transitions to the knife-edge for precise nulling. The zonal nulling procedure entails sequentially adjusting the knife-edge position to achieve a null shadowgram for each zone, where the entire zone appears uniformly illuminated or shadowed. This is accomplished by moving the knife-edge through the focal plane until the shadow from the targeted zone vanishes, recording the tester's displacement as the zonal focus position.^[1] These measured positions are then compared to the theoretical sagitta differences of an ideal paraboloid, which predict progressively longer radii of curvature toward the center, revealing any deviations that indicate over- or under-polished areas. Basic shadow patterns from individual zones appear as annular bands, with nulling confirming alignment to the expected paraboloidal profile.^[1] Modern aids enhance the efficiency of zonal testing through semi-automation and data management. Semi-automated testers, such as those developed by Mike Peck (often termed Robo-Foucault), use motorized stages to systematically scan zones and log knife-edge positions, reducing manual error in repetitive measurements.^[1] Software tools like FigureXP facilitate data logging and analysis by importing zonal readings to generate error maps and polishing corrections.^[23] For instance, in an f/4 mirror, inner zones exhibit longer focal lengths than outer ones in a paraboloid, necessitating deeper central polishing to align all zonal foci and achieve the required figure.^[1]

Analyzing Results

Shadowgram Interpretation

In the Foucault knife-edge test, shadowgram interpretation relies on observing the qualitative patterns of light and shadow across the mirror surface to assess its figure and detect gross errors. These patterns emerge as the knife edge intersects the converging light rays reflected from the mirror, revealing deviations from the ideal wavefront in a visually intuitive manner. The aberration detection mechanism magnifies these deviations, allowing qualitative assessment without numerical computation.^[1] For a perfect sphere positioned at its radius of curvature, the shadowgram exhibits uniform shadow advance with no distinct bands, resulting in a full null condition where the entire surface appears evenly gray at a single knife-edge position.^[24] In contrast, a well-figured paraboloid produces a characteristic "doughnut" or lozenge pattern, featuring a central dark spot surrounded by brighter edges, with a single null zone that shifts outward as the knife edge moves away from the focus.^[1] This smooth radial gradient in the shadowgram indicates the progressive deepening of the mirror's curve toward the center, confirming the parabolic profile.^[3] Common defects manifest as deviations from these ideal patterns. A turned-down edge appears as a bright outer rim with abrupt shadow termination, signaling excessive flattening at the periphery.^[1] Astigmatism produces elongated shadows that vary in orientation and intensity when the mirror is rotated, often showing non-uniform bands along perpendicular diameters.^[1] Over-correction or under-correction of spherical aberration results in multiple concentric bands, with brighter central zones for over-correction (resembling a hill) and darker ones for under-correction (indicating a depression).^[24] Visual cues in the shadowgram provide insights into error severity and type. The sharpness of bands correlates with the magnitude of surface errors, where crisper transitions denote larger deviations.^[1] Asymmetry in the pattern, such as uneven shadow distribution, often points to misalignment in the test setup or the presence of coma in the mirror figure.^[3] For example, a smooth, even gradient across zones signifies a good paraboloid, while wavy or irregular bands indicate polishing irregularities like micro-ripples or uneven figuring.^[1]

Quantitative Error Measurement

The quantitative analysis of the Foucault knife-edge test involves calculating surface errors from observed zonal shadow shifts, primarily through the measurement of longitudinal aberration (LA) and its conversion to transverse aberration for error assessment. For a fixed light source at the center of curvature, the longitudinal aberration for a zone at normalized radius ρ (where ρ = 0 at the center and ρ = 1 at the edge) is given by

LA = \frac{K D \rho^2}{8 F} = -\frac{K (\rho d)^2}{R},

where K is the conic constant (K = -1 for a paraboloid), D is the mirror diameter, d is the mirror radius (D/2), F is the f-ratio (focal length divided by diameter), and R is the radius of curvature at the vertex (R = 2 f for a paraboloid).^[1] This formula derives from the geometric optics of the conic surface, with the negative sign indicating that outer zones of a paraboloid focus beyond the paraxial focus.^[1] To quantify deviations from the ideal shape, the measured [LA](/page/L(a) values are compared to the theoretical LA for a perfect paraboloid using the residuals method. Residuals are computed by subtracting the ideal paraboloid LA from the measured LA at each zone, yielding the error in longitudinal displacement; these are then reduced relative to a reference zone (often the 70% zone) to isolate figure errors.^[1] The reduced longitudinal aberration (LR) is converted to relative transverse aberration (RTA) via

RTA = -\frac{\rho \, LR}{2 F},

expressed in linear units or scaled to Airy disc diameters for performance evaluation (where the Airy disc diameter is approximately 2.44 λ (2 F), with λ the wavelength, using the effective focal ratio of 2 F for the test setup).^[1] This RTA represents the lateral shift of rays from the ideal focus, providing a direct measure of zonal misalignment. Surface errors are derived from these residuals by relating LA to sagitta deviation δz ≈ -LA / 2 (for small errors in reflection), with wavefront error W = 2 δz. Errors are typically expressed in waves as peak-to-valley (P-V) deviation: P-V error = max |W| / λ. For diffraction-limited performance, the wavefront error should be less than 0.25 λ P-V, corresponding to a Strehl ratio near 0.80 and minimal degradation of the point spread function.^[25] Wavefront reconstruction uses the zonal RTA or slope data (β = RTA / (2 R)) to integrate deviations across the surface, plotting sagitta errors via numerical methods such as trapezoidal integration: ΔW ≈ (1/2) Σ (β_{i-1} + β_i) (x_i - x_{i-1}). This yields a full map of surface figure, guiding polishing corrections.^[2] As an illustrative example, for a 300 mm f/5 mirror with a 1 mm outer-zone sagitta error, the corresponding RTA at the outer zone reaches up to approximately 15 Airy disc diameters (using λ = 550 nm).^[1]

Applications and Comparisons

Practical Applications

The Foucault knife-edge test finds its primary application in the figuring of telescope primary mirrors, particularly for amateur astronomers crafting parabolic surfaces in Newtonian reflectors with diameters typically ranging from 8 to 16 inches.^[1] This method allows makers to iteratively polish the mirror, observing zonal deviations to achieve the required paraboloidal shape that focuses light without spherical aberration.^[1] In professional optical shops, the test serves as a reliable tool for quality control of concave surfaces during manufacturing, enabling rapid assessment of surface figure before final coating or assembly.^[1] Historically, Léon Foucault developed the test in 1858 to evaluate the precision of concave mirrors used in his experiments, including his experiments on the speed of light, where mirror accuracy was critical to the apparatus.^[1]^[26] Modern implementations have extended the test through automation, incorporating CCD cameras and software for digital capture and analysis of shadowgrams, reducing subjectivity and enabling precise zonal measurements.^[26] Notable examples include the SIXTEST software by Jim Burrows from the early 2000s, which processes Foucault data to compute mirror errors and evaluate performance, and robotic systems like the Robo Foucault Tester that automate knife-edge positioning and data collection.^[1]^[27] These advancements suit mirrors with focal ratios from f/3 to f/8. Recent developments as of 2024 include improved methods with double-shoot shadow grams and maskless testing for enhanced precision in digital analysis.^[26]^[28]^[29] The visual Foucault test achieves accuracy to approximately λ/8 peak-to-valley on the wavefront, sufficient for most amateur applications, while automated versions with CCD imaging can reach λ/20 or better by mitigating human error in interpretation.^[30]^[26] Beyond telescopes, the test is applied less commonly to evaluate aspheric lenses and molds in photonics manufacturing, where compensators adjust for non-spherical profiles to verify surface quality.^[31]^[32]

Comparison with Other Tests

The Foucault knife-edge test distinguishes itself from other optical testing methods primarily through its use of a sharp edge to interrupt converging light rays, enabling direct visualization of surface deviations in concave mirrors. In contrast, the Ronchi test employs a grating to produce band patterns, offering a quicker qualitative assessment but with reduced sensitivity to fine errors, typically resolving to about λ/2 compared to the Foucault test's capability for λ/10 or better.^[33]^[1] The Ronchi method shares the basic principle of light interruption with the Foucault test but lacks the knife-edge's precision, making it suitable for initial alignment rather than detailed figuring.^[34] The caustic test, which visualizes the focal curve using a wire or point source, provides an alternative for testing fast mirrors with f-ratios of f/2 to f/3, achieving accuracies around λ/20 by measuring deviations in both radial and transverse directions.^[2] Unlike the Foucault test, which focuses on longitudinal errors along the optical axis, the caustic method excels in detecting astigmatism and is less prone to subjective interpretation for inexperienced users, though it requires careful setup for slower mirrors.^[35]^[7] The Dall null test modifies the Foucault setup by incorporating a custom plano-convex lens to render a parabolic surface appear spherical, facilitating null testing without spherical aberration but necessitating precise alignment and high-quality auxiliary optics.^[36] This approach improves upon the standard Foucault test for parabolization verification yet introduces potential errors from lens imperfections, limiting its accessibility compared to the knife-edge method's simplicity.^[37]^[38] Interferometric tests, such as the Fizeau and Twyman-Green configurations, utilize phase-shifting interference patterns to measure wavefront errors with sub-wavelength precision, often reaching λ/100 accuracy, establishing them as the industrial standard for high-precision optics.^[39]^[40] These methods surpass the Foucault test in objectivity and quantitative output but demand expensive equipment and controlled environments, rendering them less practical for amateur telescope makers.^[41] The Foucault test's key advantages include its low cost, requiring no specialized optics beyond a light source and knife-edge, and high sensitivity for detecting zonal errors in concave surfaces, making it ideal for amateur applications.^[2]^[5] However, it is subjective in shadowgram interpretation, sensitive to dust and vibrations, measures slopes rather than absolute heights, and is unsuitable for convex or non-specular surfaces.^[42]^[1]

References

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The Foucault test, invented by Leon Foucault, uses a light source and a knife edge to check if a mirror surface is spherical by observing shadow patterns.Missing: explanation | Show results with:explanation
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This test is one of the oldest and most common tests for determining longitudinal and transverse aberrations. A knife edge is placed near the focus and passed ...
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Since 1858 the Foucault knife-edge test has been a simple and inexpensive method to determine the properties of a concave shaped mirror. As the.
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Foucault: This is the time honored amateur test using a knife-edge cutting into the returning light. A series of zones across the mirror face are measured ...
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A spherometer is used to measure the radius of curvature of a spherical surface. Most lenses have surfaces that are either spherical or close to it.
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Place you eye in the testing position, close behind the knife edge so you can look past it. You should see a fully illuminated mirror.
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[35]
[PDF] The Testing of Astronomical Telescope Optics
The Foucault test is a null test for a spherical mirror; this means that a perfect spheroid will darken evenly over its surface when seen under the knife-edge.
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Ross null test for conic mirrors - Optica Publishing Group
This testing method, called the Ross null test, requires a high-quality null lens and a standard Foucault test apparatus. ... Comparison of Ross and Dall Null ...
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[PDF] Testing Flat Surface Optical Components - The University of Arizona
For this purpose a good spherical mirror is used, with the flat acting also as a mirror, to obtain an apparatus similar to the one used for the knife-edge test.Missing: equipment | Show results with:equipment
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Optical Testing and Interferometry - ScienceDirect.com
Interferometers measure the wavefront deformations using the interference of light, by producing the interference of two wavefronts (Malacara-Hernández, 2007).
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Interferometry: What you need to know - Tower Optical Corporation
Sep 21, 2020 · They all displayed angles and shape distortions to much greater accuracy but depended upon a skilled test technician to properly interpret – and ...
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[PDF] An Improved Geometric Test for Optical Surfaces - UCL Discovery
Foucault test is the first scientific test method for telescope mirrors with high sensitivity (Wilson 1996) introduced by Léon Foucault in 1858 (Malacara 1978,.