Examples of aperture in the following topics:
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- The two major features of a lens are focal length and aperture.
- The focal length determines the magnification of the image, and the aperture controls the light intensity.
- The shutter is what opens and closes to allow light through the aperture.
- For a larger aperture, the f-number is generally small for a quick shutter speed.
- For a smaller aperture, the f-number is larger, allowing for a slower shutter speed.
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- (a) shows a light passing through a small circular aperture.
- This effect can be seen with light passing through small apertures or larger apertures.
- θ - angle the objects are separated by, in radian λ - wavelength of light D - aperture diameter. shows this concept visually.
- (a) This is a graph of intensity of the diffraction pattern for a circular aperture.
- (a) Monochromatic light passed through a small circular aperture produces this diffraction pattern.
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- For telescopes with circular apertures, the size of the smallest feature in an image that is diffraction limited is the size of the Airy disc, as shown in .
- As one decreases the size of the aperture in a lens, diffraction increases and the ring features from diffraction become more prominent.
- The denominator $nsin \theta$ is called the numerical aperture and can reach about 1.4 in modern optics, hence the Abbe limit is roughly d=λ/2.
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- The pupil of the human eye is its aperture.
- The iris is the diaphragm that serves as the aperture stop.
- Refraction in the cornea causes the effective aperture (the entrance pupil) to differ slightly from the physical pupil diameter.
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- Intensity pattern formed on a screen by diffraction from a square aperture.
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- The human eye is had an aperture, just like a camera.
- The pupil serves this function, and the iris is the aperture stop.
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- If a large aperture is used for the microscope, the electron's location can be well resolved (see Rayleigh criterion); but by the principle of conservation of momentum, the transverse momentum of the incoming photon and hence the new momentum of the electron resolves poorly.
- If a small aperture is used, the accuracy of both resolutions is the other way around.
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- For a star one generally can extrapolate the flux that one observes in the sky to the total flux, but the intensity from a galaxy or other extended source generally falls off gradually so one defines a magnitude within a certain aperture or down to a limiting intensity (surface brightness).
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- Diffraction effects are the deviations from rectilinear propagation that occurs when light encounters edges, screens and apertures.