Polarization Control with Optics - polarization of the light
Another type, a combined convex and concave lens called a convexo-concave lens is more commonly called a negative (diverging lens) meniscus lens. This lens, like the concavo-convex lens, has a concave side and a convex side, but the radius on the concave surface is less than the radius on the convex side.
The focal length of a lens f is the distance from a lens to the focal point F. Light rays (of a single frequency) traveling parallel to the optical axis of a convex or a concavo-convex lens will meet at the focal point which is on the same axis as the center of the lens.
Different focal lengths will change the field of view and the perspective of the object you are observing. It mostly depends on the distances between the object, lens, and viewing piece, but the index of refraction of the glass and other conditions do also affect the observations. With a camera lens, the sensor size, effective focal length, and pixels of resolution all factor into the final image as well. Longer focal length will often lead to greater magnification with a sharper image than digital zoom, while shorter focal length will lead to a wider field of view.
For systems with a wave distortion, the measured picture height distortion can be zero or close to zero even if a strong distortion is visible in the image. We can break down the line geometric distortion method into three different methods to measure these systems' distortion as specified in ISO 17850.
Distortion commonly occurs from aberrations near the edges of an image. Each type of distortion usually develops through different variables. Barrel distortion, for example, is often the result of a lens at full zoom, while pincushion distortion occurs most often from telephoto lenses. Waveform distortion results from a large angle camera in zoom mode, combining both barrel and pincushion distortion.
To find the focal length of a lens, measure the distances and plug the numbers into the focal length formula. Be sure all measurements use the same measurement system.
Imagedistortion inradiography
Example 2: The measured distance from a lens to the object is 10 centimeters and the distance from the lens to the image is 5 centimeters. The focal length equation shows:
A convex lens converges parallel rays to a focal point with a positive focal length. Because the light goes through the lens, positive image distances (and real images) are on the opposite side of the lens from the object. The image will be inverted (up-side down) relative to the actual image.
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The field of geometrical optics is very complicated, and it extends far beyond focal length. The principal plane of the lens, refractive index, wavelength, and many other formulas and properties all contribute greatly to the process of optical observation.
In general, rotationally symmetric optical systems function to form an image that is geometrically similar to the object. There are a few exceptions for some particular systems, such as fish-eye lenses, where geometric conditions are deliberately not maintained. Ideally, this function is accomplished according to the geometry of perspective projection. Deviations from the ideal image geometry are called distortion.
It is essential to test and analyze lens distortion to ensure high image quality. We recommend following ISO 17850 and using proper test charts to capture various images using different lens functions, e.g., zoom. We then suggest analyzing the results using evaluation software (e.g., iQ-Analyzer-X) to see where you can improve the camera system.
Convex and concave lenses come in different configurations. Plano-convex lenses are flat on one side and convex on the other while bi-convex (also called double-convex) lenses are convex on both sides. Plano-concave lenses are flat on one side and concave on the other side while bi-concave (or double-concave) lenses are concave on both sides.
where o refers to the distance from the object to the lens, i refers to the distance from the lens to the image and f is the focal length.
Pincushiondistortion in optics
Blaettler, Karen G. How To Calculate Focal Length Of A Lens last modified April 22, 2023. https://www.sciencing.com/calculate-focal-length-lens-7650552/
This method is applicable when the vertical line Ai is located closer to the vertical line at the center of the image than to Bi, use formula 2: $$Dhi=\frac{\left(Bi-Ai\right)}{2V}\times100%$$
Image distortion occurs when the straight lines of an image appear to be deformed or curved unnaturally. There are three types of lens distortion called barrel, pincushion, and waveform (also known as mustache) distortion. It is important to note that distortion occurs differently depending on the lens system and whether the lens can or cannot be removed from the camera.
Distortion in opticsformula
The local geometric distortion method is utilized when a single number for the distortion is not sufficient. In other words, we need a function for the distortion to correct the distortion in image processing. Keep in mind that when you need to address a specific image height, the local geometric distortion is more reliable.
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Barreldistortion
Blaettler, Karen G. "How To Calculate Focal Length Of A Lens" sciencing.com, https://www.sciencing.com/calculate-focal-length-lens-7650552/. 22 April 2023.
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Use this method when the horizontal line αi is located closer to the horizontal line through the center of the image than to βi, use formula 4: $$Dvi=\frac{\left(\beta i-\alpha i\right)}{2V}\times100%$$
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Example 1: The measured distance from a lens to the object is 20 centimeters and from the lens to the image is 5 centimeters. Completing the focal length formula yields:
Distortion in opticsexamples
If deriving a single number from the local geometric distortion, the maximum distortion measured for any of the image's geometric structures is the one that is reported.
Pincushiondistortion
Distortion in opticscalculator
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The relationship between these variables is also affected by the thickness of the lens. A thin lens relies more heavily on these variables, so it is less accurate to remove some of these variables for approximation
The TV distortion method is essentially a system that shows a steadily increasing distortion from the image center to the corners. The bending of a straight line in the original image is quantified at the image's top edge (see figures below). The ratio of the bending over the height of the image multiplied by 100 is the percentage of picture height distortion. This method is compliant with the process described in EBU Tech 3249 32493.
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When an object distance is very large, the u term becomes negligible because 1/u converges to approximately 0. For these objects that are very far away we can approximate:
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There are two basic types of lenses: convex and concave. Convex lenses are thicker in the middle than on the edges and cause light rays to converge to a point. Concave lenses are thicker on the edges than in the middle and cause light rays to diverge. These operate on very similar principles to a concave mirror and a convex mirror, but they permit light to pass through and get refracted instead of reflecting off. These mirrors are often used in combination with lenses for telescopes and cameras.
\(\frac{1}{20}+\frac{1}{5}=\frac{1}{f}\) \(\text{or}\; \frac{1}{20}+\frac{4}{20}=\frac{5}{20}\) \(\text{Reducing the sum gives }\frac{5}{20}=\frac{1}{4}\)
A combined concave and convex lens – known as a concavo-convex lens – is more commonly called the positive (converging lens) meniscus lens. This lens is convex on one side with a concave surface on the other side, and the radius of curvature on the concave side is greater than the radius of the convex side.
Specific lens systems (particularly small ones in mobile devices) will correct distortion at the maximum image height. These systems show the highest distortion level at lower distances from the optical center. The resulting type of distortion is often a mixture of barrel and pincushion distortion and is described with the term wave distortion.
Where: i is a suffix representing each picture width; αi, βi, and V shall be represented by the number of pixels in the output image.
Opticaldistortionmeaning
Before the 1590s, simple lenses dating back as far as the Romans and Vikings allowed limited magnification and simple eyeglasses. Zacharias Jansen and his father combined lenses from simple magnifying glasses to build microscopes and, from there, microscopes and telescopes changed the world with geometrical optics. Understanding the focal length of lenses was crucial to combining their powers.
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A concave lens diverges parallel rays away from a focal point, has a negative focal length and forms only virtual, smaller images. Negative image distances form virtual images on the same side of the lens as the object. The image will be oriented the same direction (right-side up) as the original image, just smaller.
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The total line distortion is calculated as: $$\left|D_{\mathrm{line}}i\right|=\sqrt{\mathrm{Dh}\mathrm{i}^2+\mathrm{Dv}\ \mathrm{i}^2}%$$
Where: i = a suffix representing each picture height; Ai, Bi, and V shall be represented by the number of pixels from the output image.
Image distortion is when the straight lines of an image appear to be deformed or curved unnaturally, creating different distortion types, including barrel, pincushion, and waveform. Distortion is often the result of the lens's geometrics and can significantly disrupt the image's quality.
Finding focal length uses the focal length formula and requires knowing the distance from the original object to the lens u and the distance from the lens to the image v. The lens formula says that the inverse of the distance from the object plus the distance to the image equals the inverse of the focal distance f. The equation, mathematically, is written:
ISO 903911 is the standard that defines methods to measure a lens that is separated from a camera. Sometimes, however, you cannot remove the lens from a camera (such as in a mobile phone), and thus the time-consuming methods described in ISO 9039 will not be adequate. As a result, ISO 178502 was introduced to define methods to measure distortion using a camera lens combination.
When measuring the local geometric distortion, we assume that the distortion close to the optical center is zero. Then you can calculate a regular grid based on the geometric positions of the nine structures (3x3) in the center of the image. This grid is expanded to the whole image and defines the nominal positions for each of the structures.
The oldest method that uses the camera-lens combination is the TV distortion method, created to analyze TV camera systems. This method requires a test chart with a regular grid of geometric structures such as those shown below.
Blaettler, Karen G. (2023, April 22). How To Calculate Focal Length Of A Lens. sciencing.com. Retrieved from https://www.sciencing.com/calculate-focal-length-lens-7650552/