Crownglass refractiveindex

where is σn0 affected by the environment parameters, such as pressure, temperature, and humidity. Considering the parameters above, σnair can be obtained by [31]

This section collects any data citations, data availability statements, or supplementary materials included in this article.

This symmetric scheme can reduce the influence of several systematic errors. The verification is presented in Section 4.

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A refractive index measurement method using Brewster’s Law and a focusing probe beam is proposed in this study. A P-polarized laser beam is focused on the surface vertex of the sample as a probe with a size of approximately 10 microns and is then reflected to an array detector. According to Brewster’s Law, a dark slit corresponding to the Brewster angle exists in the intensity distribution of the reflected light. Image processing is used to calculate the Brewster angle and the refractive index. In addition, a symmetric measurement scheme is proposed to reduce the error introduced by alignment errors. A prism and four spherical lens samples with different refractive indices or radii of curvature were tested with the proposed method. The results indicated that the accuracy can reach 10−4.

A light meter can help you find the correct exposure settings for your camera in any lighting situation. Your camera has a built-in light meter that evaluates the light reflected by your subject and the surrounding environment. However, this meter can be fooled by very bright or very dark scenes, resulting in overexposed or underexposed photos. A light meter can measure the light falling on your subject directly, without being affected by the background or the color of your subject. This way, you can get more accurate and consistent exposures.

Glass refractiveindex

First, the error estimation without the symmetric measurement scheme was conducted as proposed in Section 4.1. The measurement error σnair caused by that of the refractive index of the air σnair is calculated with Equation (8) as

This section demonstrates the abovementioned principle with the refractive index measurement system, as shown in Figure 7. A He-Ne laser with a wavelength of 632.8 nm was used as the light source. Expanded by the microscopic objective, the pinhole, and the collimating lens, the diameter of the collimated laser beam was approximately 10 mm. The extinction ratio of the polarizers was 500:1. The focal length and the diameter of the convergence lens were 175 mm and 25.4 mm, respectively. The CMOS (Daheng Imaging, MER-302-56U3C) was placed at d = 150 mm from the focal point of the convergence lens, with M × N = 2048 × 1536 resolution and pixel size p = 3.45 μm. The sample and the CMOS rotations were realized by a pair of co-axis stepping motor rotating tables (BOCIC, MRS-101 and MRS-103). The stepping angle of each of the tables was around 1.3 × 10−3 degrees.

According to Equation (5), the measurement error σn of the refractive index of the sample is mainly caused by that of air σn0, the angular measurement error of the incident angle at the center position σθS, and the angular measurement error of the angular offsets σθE.

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The measurement error σnS of the refractive index caused by the angular measurement error σθS of incident angle θS can be obtained by differentiating Equation (5) with respect to σθS as

Glass refractiveformula

Second, the angular offset θE between the chief ray corresponding to the horizontal center of the image and the Brewster-angle ray corresponding to the intensity minimum position is obtained by the image processing algorithm shown in Figure 5A. The first two steps draw the intensity distribution versus the column coordinate (representing θ) of each row, as shown in Figure 5B, and find the minimum intensity column coordinate in each row, marked as θEi, where i = 1, 2, … M. Generally, influenced by the angle γ, θEi varies with the row coordinate i. The next step is finding the angular offset θE. According to Equation (3), only when γ is zero is the incident angle α equal to θ. In other situations, α is greater than θ. If γ is farther from zero, α reaches the Brewster angle with a smaller θ. Thus, only in the row where γ is zero can α be equal to θ and θEi reach a maximum. Figure 5C shows that the maximum value of θEi, denoted as θEmax, can be adopted to calculate the angular offset θE as

The refractive index is one of the most important parameters of optical glasses and has a significant effect on optical properties. The measurement of optical glasses, especially for optical elements such as lenses, is urgently needed. However, several presented methods require the immersion of the sample in liquid and provide indirect measurements, while others require structural parameters as priori knowledge, which is complex and time-consuming. In this study, a Brewster-Law-based direct and simple measurement method for the refractive index of glasses with arbitrary shapes is proposed, and a laser beam is focused on the surface of the sample as a probe. The incident angle of the chief ray is close to the Brewster angle. The reflected light is collected by an array detector. The refractive index is calculated from the minimum intensity position obtained with image processing. Additionally, a symmetric measurement scheme is proposed to improve the accuracy. Using these methods, a prism and four spherical lens samples with different refractive indices or radii of curvature are tested and error analyses are carried out. Results indicate that the accuracy can reach 10−4.

According to the experimental system presented in Section 3.1 and the results in Section 3.2, the error budget for the measurement result of the lens is carried out as follows.

Refractiveindex of water

Finally, without the symmetric measurement scheme, the refractive index measurement error σn is estimated with Equation (19) as

Overall, the average of the data collected clockwise is greater than the reference at 10−3 order, while for the anticlockwise data, the average is less than the reference at a similar order. With and without using the symmetry measurement, the accuracy can reach 10−3 and 10−4, respectively. The second group of experiments indicated that for the samples with different materials, the results are relatively stable.

For the measurement of samples 2, 3, and 4, the reference value of the refractive index was also 1.5151. The average refractive indices of the averaged result of clockwise and anticlockwise data were 1.5146, 1.5145, and 1.5146, respectively. Moreover, the standard deviations were 7.5 × 10−5, 6.4 × 10−5, and 7.8 × 10−5. The averages were approximately equal to that of sample 1, and the standard deviations were in the same order of magnitude. For the data collected clockwise and anticlockwise, similar conclusions could be drawn.

According to the intensity distribution, an image processing method is used to find the minimum intensity position and the Brewster angle. Subsequently, the refractive index can be calculated. The detailed measurement of the Brewster angle and calculation of the refractive index are presented in Section 2.2.

The refractive index measurement clockwise, the refractive index measurement anticlockwise, and the average refractive index are abbreviated as RIC, RIAC, and RIA, respectively, in the table.

Refractiveindex of lens

If you want to use a light meter more effectively, there are certain tips and tricks to consider. For instance, use a tripod to keep your camera steady and avoid camera shake when using slow shutter speeds. You can also use an 18% gray card to meter your scene if you don't have a light meter or if you want to check your camera's meter accuracy. Additionally, exposure compensation can be used to fine-tune your exposure if you want to make your photos brighter or darker than the meter reading. Lastly, different metering modes can be used to suit different situations; matrix metering evaluates the entire scene and gives an average exposure, center-weighted metering gives more weight to the center of the frame and less to the edges, spot metering measures only a small area of the frame and ignores the rest, and partial metering measures a larger area than spot metering but still excludes the edges. By taking all of this into account, you can take full advantage of your camera's manual mode and achieve the desired creative results.

All of the above-mentioned are undetermined systematic errors, and thus σθS needs to be synthesized by the root square sum method. The angular measurement errors σθβ, σθx1, σθx2, σθy1, σθy2 caused by σβ, σx1, σx2, σy1, σy2 can be respectively expressed as

For the measurements of sample 5, the reference value of the refractive index was 1.7999 at 632.8 nm. For the data collected clockwise, the average was 1.8055 and the standard deviation was 1.0 × 10−4. For the data collected anticlockwise, the average was 1.7953 and the standard deviation was 5.1 × 10−5. For the averaged result of clockwise and anticlockwise data, the average was 1.8004 and the standard deviation was 7.1 × 10−5. With and without the symmetry measurement, the accuracy can reach around 5 × 10−3 and 5 × 10−4, respectively.

The synthesis error matches the experiment results, which is approximately 5 × 10−3 for both clockwise and counterclockwise data.

To use a light meter, you need to begin by setting your camera to manual mode and selecting the desired ISO and aperture settings. You can also set the shutter speed, but it is simpler to adjust it later based on the meter reading. Then, turn on the light meter and match the ISO and aperture settings with your camera. If you are using an incident meter, attach the diffuser to the sensor, and if you are using a spot meter, choose the spot size and angle that fits with your subject. After that, hold the light meter near your subject and point it towards your camera. If you are using an incident meter, make sure the diffuser covers the sensor completely. If you are using a spot meter, aim it at the most important part of your subject or the midtone of your scene. When you press the measure button, read the recommended shutter speed on the display and set your camera's shutter speed to match it. Take a test shot and check the histogram and LCD screen to determine if the exposure is correct. If not, adjust your shutter speed, aperture or ISO accordingly and repeat this process until you are pleased with the results.

Refractiveindex of air

where the pressure is nearly a normal atmosphere, σPa ≈ 0; σK = 6.4 °C, and σH = 11.6%. The value of tan(θE + θS) is equal to the reference refractive index.

The non-immersive method is another important part of the refractive index measurement of lenses. The structural parameters of the tested lens—including focal length, thickness, and radius of curvature (ROC)—need to be measured primarily, and the refractive index is calculated by the geometrical formula. Vani K. Chhaniwal et al. calculated the refractive index of a thin biconvex lens by using the thin-lens formula and the structural parameters were measured by a Michelson interferometer [22] and digital holographic interferometry [23]. The accuracy was able to reach 10−4. However, the thin-lens formula is only available for biconvex lens with long focal lengths. Based on fiber point-diffraction longitudinal interferometry, Lingfeng Chen et al. [24] proposed a non-immersive method that can be used for any spherical single lens and reach an accuracy of 2.2 × 10−4. However, the system is based on an interferometry system that is sensitive to the environment. Weiqian Zhao et al. [25] proposed a multi-parameter comprehensive measurement method for spherical lenses using laser differential confocal interference, by which the structural parameters and the refractive index can be measured at the same time. The accuracy for the refractive index measurement can reach 2.2 × 10−4. However, this system is complex and expensive.

The reason for the dark silt formation is presented below. The intensity distribution of the reflected light is determined by the distribution of the incident light and the reflectivity, while that of the collimated laser beam is generally Gaussian and the reflectivity can be calculated by the incident angle. For the focusing probe beam, the incident angles vary at different positions, which follows the model in Figure 3.

(A) Intensity curve in three typical rows in the measurement of sample 1; (B) Minimum intensity position curve in the measurement of sample 1.

The error of the result obtained by Equation (6) consists of the angular measurement error σθS and σθE. σθE is a random measurement error caused by the algorithm and does not change with or without the symmetric measurement. However, the error sources of σθS, including σβ, σx1, σx2, σy1, σy2, are all systematic errors that consist of positive or negative values. The error clockwise and anticlockwise are denoted as θS1 and θS2, respectively. For the quantitative evaluation of the errors, the angle approximation and equivalent infinitesimal can be used to simplify the equals as

If you want to take full control of your camera and capture well-exposed photos, you need to understand how to use a light meter. A light meter is a device that measures the intensity of light in a scene and helps you determine the optimal exposure settings for your camera. In this article, you will learn the basics of light metering, the different types of light meters, and how to use them to achieve the best results.

In this study, we propose a Brewster-Law-based direct and simple measurement method with a focusing probe beam for the refractive index of glasses with arbitrary shapes. A P-polarized laser beam is focused by a convergence lens on the surface of the sample as a focusing probe beam with a size of approximately 10 microns and then reflects to an array detector. The focusing probe beam is the incident light of the system, and the ray parallel to the optical axis of the convergence lens is defined as the chief ray. The incident angle of the chief ray is close to the Brewster angle. According to Brewster’s Law, a dark slit corresponding to the Brewster angle exists in the intensity distribution of the reflected light. Finally, image processing is used to calculate the Brewster angle and the refractive index by finding the minimum intensity position. The refractive index is measured by the reflection from an arbitrary surface of the sample; therefore, the structural parameters are not needed. Given that the probe requires only a tiny area for reflection, the method is available for samples with arbitrary shapes. Additionally, a symmetric measurement scheme is proposed to improve the accuracy. By using these methods, a prism and four spherical lens samples with different refractive indices or radii of curvature are tested and error analyses are carried out. Results indicate that the accuracy can reach 10−4.

(A) Flow chart for calculating the refractive index; (B) Minimum intensity position θEi in each row; (C) The maximum θEmax corresponding to the angular offset from the center θE.

Compared with the current non-immersion method, the proposed method does not require the structural parameters of the tested samples. Thus, the method can be used regardless of the shape of the sample, and the measurement process is clear and simple.

Figure 2A shows the layout of the optical measurement configuration of the system. The thin laser beam passes through the microscopic objective and collimating lens to generate a broad collimated laser beam, which is used as a light source. The broad beam is focused by a convergence lens to the focal point as a focusing probe, which is coincident to the surface vertex of the sample. The incident angle of the chief ray of the probe is close to the Brewster angle. Polarizers 1 and 2, through which the light passes, are both in P polarization state, guaranteeing that the probe is a P-polarized beam. After the probe is reflected by the sample, the reflected light propagates to the CMOS detector placed at a distance d away from the sample. The resolution and the pixel size of the image plane are denoted as M × N and p, respectively.

Refractiveindex of oil

The measurement error σnair of the refractive index caused by the error of the refractive index of air can be obtained by differentiating Equation (5) with respect to n0 as

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This paper is organized as follows. The system structure and the measurement principle are presented in Section 2. In Section 3, the refractive indices of samples with different shapes are tested. The error analyses are presented in Section 4. Finally, conclusions are summarized in Section 5.

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(A) Layout of the optical measurement configuration; (B) Intensity distribution of the reflected light; (C) Intensity curve of the reflected ray versus the incident angle.

Refractiveindex of diamond

Figure 8 shows the structure of the tested prism and spherical lens samples. Detailed information about the material, the reference value of the refractive index, and the structural parameters is listed in Table 1. The surface with ROC of R1 was used for reflection in the experiment for the lens. The Rayleigh length of the focusing probe beam was around 160 μm, and the maximum sag variation in the target surface within the laser reflection area was around 7.5 μm, which was less than the Rayleigh length, proving that the reflection area could be treated as a point. The reference refractive index of the samples was settled from the glass database. The material H-K9L and N-BK7 were glasses with the same properties but produced by different companies, so their refractive indices were the same.

From the first group of experiments, we can conclude that for the samples with different shapes in the experiment, the results were approximately equal. The data collected clockwise were greater than the reference at 10−3 order, while for the anticlockwise data, the average was less than the reference at a similar order. The accuracy of the average data was around 5.0 × 10−4 to 6.0 × 10−4.

Articles from Sensors (Basel, Switzerland) are provided here courtesy of Multidisciplinary Digital Publishing Institute (MDPI)

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Exposure is the amount of light that reaches your camera's sensor when you take a photo. It depends on three factors: aperture, shutter speed, and ISO. Aperture is the opening of your lens that controls how much light enters your camera. Shutter speed is the duration of time that your camera's shutter is open and allows light to hit your sensor. ISO is the sensitivity of your sensor to light. By adjusting these three settings, you can change the brightness and darkness of your photos.

σθS is caused by various error sources, including the tilt angle σβ, misalignment errors σx1 and σy1 of the surface vertex and the rotating center of the CMOS, and the misalignment errors σx2 and σy2 of the focal point and rotating center of the CMOS, as shown in Figure 10.

The refractive index measurement clockwise, the refractive index measurement anticlockwise, and the average refractive index are abbreviated as RIC, RIAC, and RIA, respectively, in the table.

Figure 1 shows the system layout of the proposed refractive index measurement system, which is composed of optical measurement and mechanical motion configurations divided by the black dotted line. The optical measurement configuration is organized for the refractive index measurement, comprising two polarizers and a laser, microscope, collimating lens, convergence lens, sample, and a complementary metal oxide semiconductor (CMOS) array detector. The mechanical motion configuration consists of two coaxial rotating tables, marked as Rotating Table 1 and Rotating Table 2. The green dotted line is the common rotational axis of these tables, which passes through the surface vertex of the sample. Rotating Tables 1 and 2 take control of the sample and the CMOS, respectively.

The Brewster method is a refractive index measurement method based on Brewster’s law [26,27,28], which can be expressed as the reflectivity of the P-polarized light approaching zero while it is incident in the Brewster angle, which is the inverse trigonometric value of the refractive index. In such a measurement system, a P-polarized parallel laser beam is incident on the sample and reflected to a photodiode to obtain the intensity. The minimum intensity position corresponding to the Brewster angle can be found by scanning the incident angle. The measurement accuracy of the refractive index depends on that of the angle [29,30]. The Brewster method enables simple and efficient measurement of the refractive index. However, the reflecting surface of the sample needs to be planar to provide a smooth reflective area with a size greater than the beam diameter. Thus, samples with only spherical or aspheric surfaces cannot be tested.

The results of the measurement of the samples made with H-K9L(N-BK7), including samples 1, 2, 3, and 4, are listed in Table 2.

Ten measurements were taken for each of the samples listed in Table 1, and each measurement took around five minutes because the mechanical rotation was not fully automatic. Figure 9 shows the data processing results of sample 1 as an example. Figure 9A is the intensity curve in three typical rows from the intensity distribution collected by the CMOS. The vertical axis is the grayscale value, and the horizontal axis is the column coordinate. The red, green, and blue curves correspond to the intensity curves in rows 600, 800, and 1000, respectively. In each curve, a minimum intensity position corresponding to θEi can be found. The column coordinates of the curves are different, which accords with the principle in Section 2.1. Figure 9B shows the row and column coordinates of the minimum intensity position. The vertical axis is the column coordinate, and the horizontal axis is the row coordinate. Different values of θEi make up the curve, and the maximum of the curve corresponds to θE. The results for the other samples are similar. The detailed results and analyses are demonstrated in Section 3.2.1 and Section 3.2.2, respectively.

For the measurements of sample 1, the reference value of the refractive index was 1.5151 at 632.8 nm. For the data collected clockwise, the average was 1.5187 and the standard deviation was 9.0 × 10−5. The average was approximately 3.6 × 10−3 greater than the reference, but the data had limited diversity. For the data collected anticlockwise, the average and the standard deviation were 1.5104 and 5.1 × 10−5, respectively. The average was 4.7 × 10−3 less than the reference. However, the diversity remained low. For the averaged result of clockwise and anticlockwise data, the average was 1.5146 and was only approximately 5.0 × 10−4 less than the reference. The standard deviation was 4.6 × 10−5.

Rotating the sample and the CMOS around the axis of the rotating tables can change the incident angle of the chief ray. The initial position of the sample and the CMOS is shown as a dotted line in Figure 2A. The rotation angle of the sample and the CMOS are marked as ω1 and ω2, respectively. Given that the incident angle is equal to the reflected angle, then ω2 = 180° − 2ω1. According to Snell’s Law, when the incident angle is close to the Brewster angle, the intensity distribution of the reflected light with a dark slit existing near the center can be illustrated as in Figure 2B. The center position of the distribution corresponds to the chief ray of the reflected light. Figure 2C shows the intensity curve versus the incident angle. The minimum position of the intensity curve corresponds to the Brewster angle.

There are two main types of light meters: incident and spot. Incident light meters measure the light falling on your subject from the source. They have a dome-shaped diffuser that covers the sensor and captures the light from all directions. You need to place the meter close to your subject and point it towards the camera. Spot light meters measure the light reflected by a specific area of your scene. They have a narrow angle of view and a target indicator that shows you what part of the scene you are metering. You need to point the meter at your subject from your camera's position.

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In the measurement of the refractive index of lenses, the liquid immersion method plays an important role. Smith [13] immersed a lens in a mixed liquid with varying refractive indices until it approximated that of the lens. Measuring the refractive index of the liquid can thus indirectly obtain that of the lens with an accuracy of 4.6 × 10−4. However, the mixed liquid used must be miscible, which is time-consuming for preparation. In addition, most of the miscible organic compounds are poisonous in nature. Other liquid immersion methods use non-miscible liquids. R. S. Kasana, et al. proposed a nondestructive technique using a Murty shearing interferometer [14]. The tested spherical lens is immersed in standard liquid with a certain refractive index inside a glass cell, from which the interferometric fringe is generated. The refractive index can be measured by analyzing the fringes with an accuracy of 10−4. Similarly, the refractive index of a lens can be measured by using computed tomography [15], Fabry–Perot interferometer [16], optical grating [17], acousto-optic grating [18], and Ronchi grating [19]. In these methods, the refractive index of the liquid does not need adjustments to fit that of the sample. However, the lens immersed shall be aligned to the optical axis, which is difficult in the liquid environment. Given that the refractive indices of the samples are obtained indirectly by measuring that of the liquid, the accuracy is limited by that of the liquid index measurement [20,21].

In Section 2.3, we propose a symmetric measurement scheme to improve the system’s accuracy. The results show the effectiveness of the method. Here, the error analyses of the symmetric measurement are given to verify the method theoretically.

This research was funded by the National Natural Science Foundation of China (NSFC) (51735002) and the Strategic Priority Research Program of the Chinese Academy of Sciences (XDA25020317).

In Figure 3, the xoy plane is the medium interface and the z axis is along the normal direction of the medium at the surface vertex. The red solid line is the incident light, while the green and blue dotted lines are the projection of the incident light on xoz and yoz plane, respectively. The incident angle is that between the incident light and the Z axis, which is marked as α. θ is the angle between the incident light and the xoz plane, and γ is the angle between the yoz plane. Vectors k1→ and k2→ are the normalized direction vectors parallel to the incident light and z axis, respectively, which can be expressed as

According to the experimental system, Table 5 shows the estimated error limits of σβ, σx1, σx2, σy1, and σy2. For the measurement of sample 5, θS is set at 1.0647 rad, and the turning radius R = 150 mm, equal to the distance between the CMOS and the rotating center. By the estimated error in Table 5 and Equations (10)–(16), the measurement error σnS can be calculated as

Then, the error estimation with the symmetric measurement scheme as proposed in Section 4.2 is given. σnair and σnE are the same as in Equations (22) and (24). However, for σnS, the influence of σβ, σy1, and σy2 can be reduced. σnS can be obtained by

Conceptualization, Y.H.; methodology, J.L.; software, J.L.; validation, J.L. and Y.H.; formal analysis, J.L.; data curation, J.L.; writing—original draft preparation, J.L.; writing—review and editing, Y.H. and Q.H.; project administration, Y.H. and Q.H.; funding acquisition, Y.H. and Q.H. All authors have read and agreed to the published version of the manuscript.

The refractive index is tested by noninterference measurement, given that the method is robust to noise and environmental vibrations.

Considering the effect of the above-mentioned errors on the measurement result, the synthetic measurement error of the refractive index σn is

For the measurement of the lens sample, the calculation for θEmax shall be no greater than two pixels. Thus, the measurement error σθE can be estimated as σθE ≈ 0.0025° according to Equation (4). σnE can be obtained with Equation (18) as

Based on Equations (21) and (22), the expressions of the error coefficients of σβ, σx1, σx2, σy1, σy2 for σθS1, σθS2, and σθS in Equations (10)–(14) can be simplified as listed in Table 4. With the symmetric measurement scheme, the errors from σβ, σy1, and σy2 can be reduced, while those from σx1 and σx2 remain the same, verifying the method’s feasibility.

We conducted two groups of experiments to verify the method and the system. In the first group, samples with the same refractive index but different shapes, i.e., samples 1, 2, 3, and 4, were tested to verify the validity for measuring the elements with arbitrary shapes. In the second group, samples with similar shapes (e.g., similar ROC of the surface for reflection) but different refractive indices, i.e., samples 2 and 5, were tested to estimate the accuracy and the consistency of the measurement of the different refractive indices.

According to the requirements of the system structure, the focal point of the convergence lens coincides with the surface vertex of the sample, and the common rotational axis of the two rotating tables passes through the surface vertex. These parameters are difficult to guarantee in real engineering. To reduce the alignment requirements of the system and guarantee high measurement accuracy, we introduce an additional measurement step, which is defined as the symmetric measurement scheme. The values of Brewster angle θB are obtained by rotating the sample and the CMOS clockwise and anticlockwise, as shown in Figure 6. The values are marked as θB1 and θB2, respectively. Finally, θB is determined as the average of the above two values as

The refractive index, defined as the ratio of the velocity of light in a vacuum and the material, is one of the most important physical parameters of optical glass. With its considerable influence on the working characteristics of optical systems, high-accuracy measurement of this parameter is required. Since the early 1900s, various methods have been proposed [1], including prism coupling [2], critical angle [3], interferometry [4,5], and ellipsometry [6]. Some of them can even determine the refractive index and the structure of the sample simultaneously [7,8,9,10]. These methods are now widely used and can reach high accuracy of up to 10−6, but they are only available for prisms and parallel plates. Samples with only spherical or aspheric surfaces, such as lenses, cannot be tested. However, the measurement of the refractive index of a lens is equally important because of its possible changes during the manufacturing procedure, which may considerably affect the optical properties [11,12].

For the focusing probe beam in Figure 1, the focal point of the convergence lens corresponds to the coordinate origin of the model and the optical axis of the incident light corresponds to the Z axis. The chief ray of the incident light lies on the yoz plane, and thus the angle γ is zero and θ is equal to the incident angle α, which is close to the Brewster angle. Given that the incident angles of the rays at other positions of the beam distribute around the chief ray similarly to a cone, the values of θ and γ distribute around the Brewster angle and zero, respectively. The distribution range is determined by the focal length and diameter of the beam. Given that the reflected light is collected by the CMOS, θ and γ correspond to the row and column coordinates, respectively. After the θ and γ of each CMOS pixel are determined, the incident angle α can be calculated with Equation (3). According to Snell’s Law, the result that the reflected intensity distribution versus the incident angle consists of a dark slit with a minimum close to zero can be obtained.

which also matches the experimental accuracy of approximately 5 × 10−4. Finally, the accuracy of the refractive index measurement method with the symmetric measurement scheme can reach 10−4.

The measurement error σnE of the refractive index caused by the angular measurement error σθE of incident angle θE can be obtained by differentiating Equation (5) with respect to σθE as

The Brewster angle is determined using two steps. First, the sample and the CMOS are rotated such that a distinct dark slit appears in the image. In this case, the angle θ of the chief ray of the reflected light, marked as θS and equal to the rotating angle of the sample ω1, is measured by the readings of the rotating tables, as shown in Figure 4.