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Entrance pupil information


The entrance pupil made by a single lens with an aperture (aperture stop) behind it. The entrance pupil is the image of the aperture stop viewed from the front of the optical system.
A camera lens adjusted for large and small aperture. The visible opening is the entrance pupil of the lens.
The apparent location of the anatomical pupil of a human eye (black circle) is the eye's entrance pupil location. The outside world appears to be seen from the point at the center of the entrance pupil. The anatomical pupil itself is slightly different from the entrance pupil because the image is magnified by the cornea.

In an optical system, the entrance pupil is the optical image of the physical aperture stop, as 'seen' through the front (the object side) of the lens system. The corresponding image of the aperture as seen through the back of the lens system is called the exit pupil. If there is no lens in front of the aperture (as in a pinhole camera), the entrance pupil's location and size are identical to those of the aperture. Optical elements in front of the aperture will produce a magnified or diminished image that is displaced from the location of the physical aperture. The entrance pupil is usually a virtual image: it lies behind the first optical surface of the system.

The entrance pupil is a useful concept for determining the size of the cone of rays that an optical system will accept. Once the size and the location of the entrance pupil of an optical system is determined, the maximum cone of rays that the system will accept from a given object plane is determined solely by the size of the entrance pupil and its distance from the object plane, without any need to consider ray refraction by the optics.[1]

In photography, the size of the entrance pupil (rather than the size of the physical aperture stop) is used to calibrate the opening and closing of the diaphragm aperture. The f-number ("relative aperture"), N, is defined by N = f / EN, where f is the focal length and EN is the diameter of the entrance pupil.[2] Increasing the focal length of a lens (i.e., zooming in) will usually cause the f-number to increase, and the entrance pupil location to move further back along the optical axis.

The center of the entrance pupil is the vertex of a camera's angle of view[3] and consequently its center of perspective, perspective point, view point, projection center[4] or no-parallax point.[5] This point is important in panoramic photography without digital image processing, because the camera must be rotated around the center of the entrance pupil to avoid parallax errors in the final, stitched panorama.[6][7] Panoramic photographers often incorrectly refer to the entrance pupil as a nodal point, which is a different concept. Depending on the lens design, the entrance pupil location on the optical axis may be behind, within or in front of the lens system; and even at infinite distance from the lens in the case of telecentric systems.

The entrance pupil of the human eye, which is not quite the same as the physical pupil, is typically about 4 mm in diameter. It can range from 2 mm (f/8.3) in a very brightly lit place to 8 mm (f/2.1) in the dark.[8]

Most optical systems are designed with a single aperture stop, and therefore have a single entrance pupil. In some cases, however, different elements serve as the aperture stop for objects at different distances.[1] In such cases, the system will have different entrance pupils for different object planes. Similarly, vignetting can cause different lateral locations at a given object plane to have different aperture stops, and therefore different entrance pupils.[1]

  1. ^ a b c Hecht, Eugene (2017). "5.3.2 Entrance and Exit Pupils". Optics (5th ed.). Pearson. ISBN 978-1-292-09693-3.
  2. ^ Jacobson, Ralph; et al. (1988). The Manual of Photography (8th ed.). Focal Press. ISBN 0-240-51268-5. p.49
  3. ^ Greivenkamp, John E. (2004). Field Guide to Geometrical Optics. SPIE Field Guides vol. FG01. Bellingham, Wash: SPIE. p. 27. ISBN 978-0-8194-5294-8. OCLC 53896720.
  4. ^ Lenhardt, Karl. "Optical Measurement Techniques with Telecentric Lenses" (PDF). Schneider Kreuznach. Archived from the original (PDF) on September 24, 2015. Retrieved Oct 14, 2014.
  5. ^ Littlefield, Rik (Feb 6, 2006). "Theory of the "No-Parallax" Point in Panorama Photography" (PDF). ver. 1.0. Retrieved Jan 14, 2007.
  6. ^ Kerr, Douglas A. (2005). "The Proper Pivot Point for Panoramic Photography" (PDF). The Pumpkin. Archived from the original (PDF) on Apr 7, 2008. Retrieved Jan 14, 2007.
  7. ^ van Walree, Paul. "Misconceptions in photographic optics". Archived from the original on April 19, 2015. Retrieved Jan 14, 2007. Item #6.
  8. ^ Hecht, Eugene (1987). Optics (2nd ed.). Addison Wesley. ISBN 0-201-11609-X.

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Entrance pupil

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In an optical system, the entrance pupil is the optical image of the physical aperture stop, as 'seen' through the front (the object side) of the lens...

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Pupil

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of the pupil as seen from outside the eye is the entrance pupil, which does not exactly correspond to the location and size of the physical pupil because...

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Aperture

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limits light propagated through the system. More specifically, the entrance pupil as the front side image of the aperture and focal length of an optical...

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Pupil magnification

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The pupil magnification of an optical system is the ratio of the diameter of the exit pupil to the diameter of the entrance pupil. The pupil magnification...

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Exit pupil

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vignetting. (The entrance pupil of the eye is the image of the anatomical pupil as seen through the cornea.) The location of the exit pupil thus determines...

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Eyepiece

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to this entrance pupil (i.e. with minimum aberrations for this distance). In a refracting astronomical telescope the entrance pupil is identical with...

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Human eye

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causes the effective aperture (the entrance pupil) to differ slightly from the physical pupil diameter. The entrance pupil is typically about 4 mm in diameter...

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Optical aberration

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subtended by the entrance pupil at this point, the magnitude of the aberration will be determined by the position and diameter of the entrance pupil. If the system...

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Camera lens

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from inside the camera is the lens's exit pupil. In this simple case, the aperture, entrance pupil, and exit pupil are all in the same place because the only...

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Etendue

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system's entrance pupil subtends as seen from the source. Equivalently, from the system point of view, the etendue equals the area of the entrance pupil times...

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Image formation

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scattered light that propagates toward the lens is collected by the entrance pupil of the imaging lens over the field of view. The Field of view of a lens...

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Telecentric lens

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optical lens (often an objective lens or a camera lens) that has its entrance or exit pupil, or both, at infinity. The size of images produced by a telecentric...

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Circle of confusion

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symmetrical lens, in which the entrance pupil and exit pupil are both of diameter A. More complex lens designs with a non-unity pupil magnification will need...

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Visual angle

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the center of the lens, and also represent the center of the eye's entrance pupil that is only a few millimeters in front of the lens. The three lines...

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Bokeh

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Coarse bokeh on a photo shot with an 85 mm lens and 70 mm entrance pupil diameter, which corresponds to f/1.2...

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Scientific method

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using an aperture to represent the entrance pupil of the eye, showed that the entire scene at the entrance pupil-focused on a single point of the rear...

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Numerical aperture

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f-number given by the ratio of the focal length f to the diameter of the entrance pupil D: N = f D . {\displaystyle N={\frac {f}{D}}.} This ratio is related...

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Troland

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effective pupil size. It is equal to retinal illuminance produced by a surface whose luminance is one nit when the apparent area of the entrance pupil of the...

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Refracting telescope

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eyepiece; D – Entrance pupil diameter; d – Virtual exit pupil diameter; L1 – Objective lens; L2 – Eyepiece lens e – Virtual exit pupil – Telescope equals...

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Macro photography

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so the entrance pupil diameter is comparable to that of conventional lenses (e.g., a 100 mm f/2.8 lens has a 100 mm/2.8 = 35.7 mm entrance-pupil diameter)...

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3D projection

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the entrance pupil (camera center), and d z {\displaystyle \mathbf {d} _{z}} is the distance, from the 3D point being projected, to the entrance pupil. Subsequent...

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Maksutov telescope

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symmetrical". The negative lens is usually full diameter and placed at the entrance pupil of the telescope (commonly called a "corrector plate" or "meniscus corrector...

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Optics

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is the focal length, and D {\displaystyle D} is the diameter of the entrance pupil. By convention, "f/#" is treated as a single symbol, and specific values...

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Moritz von Rohr

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also developed a method of computing depth of field from a camera's entrance pupil location and diameter, without reference to focal length and f-number...

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