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Pinhole camera

From Wikipedia, in a visual modern way
A home-made pinhole camera lens
A home-made pinhole camera lens

A pinhole camera is a simple camera without a lens but with a tiny aperture (the so-called pinhole)—effectively a light-proof box with a small hole in one side. Light from a scene passes through the aperture and projects an inverted image on the opposite side of the box, which is known as the camera obscura effect. The size of the images depends on the distance between the object and the pinhole.

History

Camera obscura

The camera obscura or pinhole image is a natural optical phenomenon. Early known descriptions are found in the Chinese Mozi writings (circa 500 BCE)[1] and the Aristotelian Problems (circa 300 BCE – 600 CE).[2]

A diagram depicting Ibn al-Haytham's observations of light's behaviour through a pinhole
A diagram depicting Ibn al-Haytham's observations of light's behaviour through a pinhole
Early pinhole camera. Light enters a dark box through a small hole and creates an inverted image on the wall opposite the hole.[3]
Early pinhole camera. Light enters a dark box through a small hole and creates an inverted image on the wall opposite the hole.[3]

Ibn al-Haytham (965–1039), an Arab physicist also known as Alhazen, described the camera obscura effect. Over the centuries others started to experiment with it, mainly in dark rooms with a small opening in shutters, mostly to study the nature of light and to safely watch solar eclipses.[4]

Giambattista Della Porta wrote in 1558 in his Magia Naturalis about using a concave mirror to project the image onto paper and to use this as a drawing aid.[5] However, at about the same time, the use of a lens instead of a pinhole was introduced. In the 17th century, the camera obscura with a lens became a popular drawing aid that was further developed into a mobile device, first in a little tent and later in a box. The photographic camera, as developed early in the 19th century, was basically an adaptation of the box-type camera obscura with a lens.

The term "pin-hole" in the context of optics was found in James Ferguson's 1764 book Lectures on select subjects in mechanics, hydrostatics, pneumatics, and optics.[6][7]

Early pinhole photography

The first known description of pinhole photography is found in the 1856 book The Stereoscope by Scottish inventor David Brewster, including the description of the idea as "a camera without lenses, and with only a pin-hole".

Sir William Crookes and William de Wiveleslie Abney were other early photographers to try the pinhole technique.[8]

Film and integral photography experiments

According to inventor William Kennedy Dickson, the first experiments directed at moving pictures by Thomas Edison and his researchers took place around 1887 and involved "microscopic pin-point photographs, placed on a cylindrical shell". The size of the cylinder corresponded with their phonograph cylinder as they wanted to combine the moving images with sound recordings. Problems arose in recording clear pictures "with phenomenal speed" and the "coarseness" of the photographic emulsion when the pictures were enlarged. The microscopic pin-point photographs were soon abandoned.[9] In 1893 the Kinetoscope was finally introduced with moving pictures on celluloid film strips. The camera that recorded the images, dubbed Kinetograph, was fitted with a lens.

Eugène Estanave experimented with integral photography, exhibiting a result in 1925 and publishing his findings in La Nature. After 1930 he chose to continue his experiments with pinholes replacing the lenticular screen.[10]

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Camera obscura

Camera obscura

A camera obscura is a darkened room with a small hole or lens at one side through which an image is projected onto a wall or table opposite the hole.

Mozi (book)

Mozi (book)

The Mozi, also called the Mojing or the Mohist canon, is an ancient Chinese text from the Warring States period (476–221 BC) that expounds the philosophy of Mohism. It propounds such Mohist ideas as impartiality, meritocratic governance, economic growth and aversion to ostentation, and is known for its plain and simple language.

Problems (Aristotle)

Problems (Aristotle)

Problems is an Aristotelian or possibly pseudo-Aristotelian collection of problems written in a question and answer format. The collection, gradually assembled by the peripatetic school, reached its final form anywhere between the third century BC and the 6th century AD. The work is divided by topic into 38 sections, and the whole contains almost 900 problems.

Ibn al-Haytham

Ibn al-Haytham

Ḥasan Ibn al-Haytham, Latinized as Alhazen, was a medieval mathematician, astronomer, and physicist of the Islamic Golden Age from present-day Iraq. Referred to as "the father of modern optics", he made significant contributions to the principles of optics and visual perception in particular. His most influential work is titled Kitāb al-Manāẓir, written during 1011–1021, which survived in a Latin edition. The works of Alhazen were frequently cited during the scientific revolution by Isaac Newton, Johannes Kepler, Christiaan Huygens, and Galileo Galilei.

Physics in the medieval Islamic world

Physics in the medieval Islamic world

The natural sciences saw various advancements during the Golden Age of Islam, adding a number of innovations to the Transmission of the Classics. During this period, Islamic theology was encouraging of thinkers to find knowledge. Thinkers from this period included Al-Farabi, Abu Bishr Matta, Ibn Sina, al-Hassan Ibn al-Haytham and Ibn Bajjah. These works and the important commentaries on them were the wellspring of science during the medieval period. They were translated into Arabic, the lingua franca of this period.

Solar eclipse

Solar eclipse

A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of the Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to the plane of the Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of the Sun is obscured. Unlike a lunar eclipse, which may be viewed from anywhere on the night side of Earth, a solar eclipse can only be viewed from a relatively small area of the world. As such, although total solar eclipses occur somewhere on Earth every 18 months on average, they recur at any given place only once every 360 to 410 years.

Magia Naturalis

Magia Naturalis

Magia Naturalis is a work of popular science by Giambattista della Porta first published in Naples in 1558. Its popularity ensured it was republished in five Latin editions within ten years, with translations into Italian (1560), French, (1565) Dutch (1566) and English (1658) printed.

Photography

Photography

Photography is the art, application, and practice of creating durable images by recording light, either electronically by means of an image sensor, or chemically by means of a light-sensitive material such as photographic film. It is employed in many fields of science, manufacturing, and business, as well as its more direct uses for art, film and video production, recreational purposes, hobby, and mass communication.

David Brewster

David Brewster

Sir David Brewster KH PRSE FRS FSA Scot FSSA MICE was a British scientist, inventor, author, and academic administrator. In science he is principally remembered for his experimental work in physical optics, mostly concerned with the study of the polarization of light and including the discovery of Brewster's angle. He studied the birefringence of crystals under compression and discovered photoelasticity, thereby creating the field of optical mineralogy. For this work, William Whewell dubbed him the "father of modern experimental optics" and "the Johannes Kepler of optics."

Thomas Edison

Thomas Edison

Thomas Alva Edison was an American inventor and businessman. He developed many devices in fields such as electric power generation, mass communication, sound recording, and motion pictures. These inventions, which include the phonograph, the motion picture camera, and early versions of the electric light bulb, have had a widespread impact on the modern industrialized world. He was one of the first inventors to apply the principles of organized science and teamwork to the process of invention, working with many researchers and employees. He established the first industrial research laboratory.

Phonograph

Phonograph

A phonograph, in its later forms also called a gramophone or since the 1940s called a record player, or more recently a turntable, is a device for the mechanical and analogue recording and reproduction of sound. The sound vibration waveforms are recorded as corresponding physical deviations of a spiral groove engraved, etched, incised, or impressed into the surface of a rotating cylinder or disc, called a "record". To recreate the sound, the surface is similarly rotated while a playback stylus traces the groove and is therefore vibrated by it, very faintly reproducing the recorded sound. In early acoustic phonographs, the stylus vibrated a diaphragm which produced sound waves which were coupled to the open air through a flaring horn, or directly to the listener's ears through stethoscope-type earphones.

Kinetoscope

Kinetoscope

The Kinetoscope is an early motion picture exhibition device, designed for films to be viewed by one person at a time through a peephole viewer window. The Kinetoscope was not a movie projector, but it introduced the basic approach that would become the standard for all cinematic projection before the advent of video: it created the illusion of movement by conveying a strip of perforated film bearing sequential images over a light source with a high-speed shutter. First described in conceptual terms by U.S. inventor Thomas Edison in 1888, it was largely developed by his employee William Kennedy Laurie Dickson between 1889 and 1892. Dickson and his team at the Edison lab in New Jersey also devised the Kinetograph, an innovative motion picture camera with rapid intermittent, or stop-and-go, film movement, to photograph movies for in-house experiments and, eventually, commercial Kinetoscope presentations.

Usage

The image of a pinhole camera may be projected onto a translucent screen for a real-time viewing (used for safe observation of solar eclipses) or to trace the image on paper. But it is more often used without a translucent screen for pinhole photography with photographic film or photographic paper placed on the surface opposite to the pinhole aperture.

A common use of pinhole photography is to capture the movement of the sun over a long period of time. This type of photography is called solarigraphy. Pinhole photography is used for artistic reasons, but also for educational purposes to let pupils learn about, and experiment with, the basics of photography.

Pinhole cameras with CCDs (charge-coupled devices) are sometimes used for surveillance because they are difficult to detect.

Related cameras, image forming devices, or developments from it include Franke's widefield pinhole camera, the pinspeck camera, and the pinhead mirror.

Modern manufacturing has enabled the production of high quality pinhole lenses[11] that can be applied to digital cameras; allowing photographers and videographers to achieve the camera obscura effect.

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Photographic film

Photographic film

Photographic film is a strip or sheet of transparent film base coated on one side with a gelatin emulsion containing microscopically small light-sensitive silver halide crystals. The sizes and other characteristics of the crystals determine the sensitivity, contrast, and resolution of the film.

Solarigraphy

Solarigraphy

Solarigraphy is a concept and a photographic practice based on the observation of the sun path in the sky and its effect on the landscape, captured by a specific procedure that combines pinhole photography and digital processing. Invented around 2000, solarigraphy uses photographic paper without chemical processing, a pinhole camera and a scanner to create images that catch the daily journey of the sun along the sky with very long exposure times, from several hours to several years. The longest known solarigraph was captured over the course of eight years. Solarigraphy is an extreme case of long-exposure photography, and the non-conventional use of photosensitive materials is what makes it different to other methods of sun paths capture such as the Yamazaki´s "heliographys"

Charge-coupled device

Charge-coupled device

A charge-coupled device (CCD) is an integrated circuit containing an array of linked, or coupled, capacitors. Under the control of an external circuit, each capacitor can transfer its electric charge to a neighboring capacitor. CCD sensors are a major technology used in digital imaging.

Surveillance

Surveillance

Surveillance is the monitoring of behavior, many activities, or information for the purpose of information gathering, influencing, managing or directing. This can include observation from a distance by means of electronic equipment, such as closed-circuit television (CCTV), or interception of electronically transmitted information like Internet traffic. It can also include simple technical methods, such as human intelligence gathering and postal interception.

Pinspeck camera

Pinspeck camera

A pinspeck camera is the optical reverse of a pinhole camera: a small (point-like) obstruction is placed in front of the film where the (pin) hole would be in a pinhole camera.

Pinhead mirror

Pinhead mirror

A pinhead mirror can be used to create a camera similar to a pinhole camera. Instead of passing through a tiny aperature, the light to form the image is reflected by a small disc-shaped mirror. One advantage is that a pinhead mirror can be swiveled to scan a scene or project a scene to different locations.

Characteristics of pinhole camera photography

  • As pinhole photographs have nearly infinite depth of field, everything appears in focus.
  • As there's no lens distortion, wide-angle images remain absolutely rectilinear.
  • Exposure times are usually long, resulting in motion blur around moving objects and the absence of objects that moved too fast.

Other special features can be built into pinhole cameras such as the ability to take double images by using multiple pinholes, or the ability to take pictures in cylindrical or spherical perspective by curving the film plane.

Construction

A home-made pinhole camera (on the left), wrapped in black plastic to prevent light leaks, and related developing supplies
A home-made pinhole camera (on the left), wrapped in black plastic to prevent light leaks, and related developing supplies

Pinhole cameras can be handmade by the photographer for a particular purpose. In its simplest form, the photographic pinhole camera can consist of a light-tight box with a pinhole in one end, and a piece of film or photographic paper wedged or taped into the other end. A flap of cardboard with a tape hinge can be used as a shutter. The pinhole may be punched or drilled using a sewing needle or small diameter bit through a piece of tinfoil or thin aluminum or brass sheet. This piece is then taped to the inside of the light-tight box behind a hole cut through the box. A cylindrical oatmeal container may be made into a pinhole camera.

The interior of an effective pinhole camera is black to avoid any reflection of the entering light onto the photographic material or viewing screen.[12]

Pinhole cameras can be constructed with a sliding film holder or back so the distance between the film and the pinhole can be adjusted. This allows the angle of view of the camera to be changed and also the effective f-stop ratio of the camera. Moving the film closer to the pinhole will result in a wide angle field of view and shorter exposure time. Moving the film farther away from the pinhole will result in a telephoto or narrow-angle view and longer exposure time.

Pinhole cameras can also be constructed by replacing the lens assembly in a conventional camera with a pinhole. In particular, compact 35 mm cameras whose lens and focusing assembly have been damaged can be reused as pinhole cameras—maintaining the use of the shutter and film winding mechanisms. As a result of the enormous increase in f-number, while maintaining the same exposure time, one must use a fast film in direct sunshine.

Pinholes (homemade or commercial) can be used in place of the lens on an SLR. Use with a digital SLR allows metering and composition by trial and error, and is effectively free, so is a popular way to try pinhole photography.[13]

Selection of pinhole size

Up to a certain point, the smaller the hole, the sharper the image, but the dimmer the projected image. Optimally, the size of the aperture should be 1/100 or less of the distance between it and the projected image.

Within limits, a small pinhole through a thin surface will result in a sharper image resolution because the projected circle of confusion at the image plane is practically the same size as the pinhole. An extremely small hole, however, can produce significant diffraction effects and a less clear image due to the wave properties of light.[14] Additionally, vignetting occurs as the diameter of the hole approaches the thickness of the material in which it is punched, because the sides of the hole obstruct the light entering at anything other than 90 degrees.

The best pinhole is perfectly round (since irregularities cause higher-order diffraction effects) and in an extremely thin piece of material. Industrially produced pinholes benefit from laser etching, but a hobbyist can still produce pinholes of sufficiently high quality for photographic work.

A method of calculating the optimal pinhole diameter was first published by Joseph Petzval in 1857. The smallest possible diameter of the image point and therefore the highest possible image resolution and the sharpest image are given when:[15]

(Where d is the pinhole diameter, f is the distance from pinhole to image plane or “focal length” and λ is the wavelength of light.)

The first to apply wave theory to the problem was Lord Rayleigh in 1891. But due to some incorrect and arbitrary deductions he arrived at:[16]

So his optimal pinhole was approximatively 1/3 bigger than Petzval’s.

The correct optimum can be found with Fraunhofer approximation of the diffraction pattern behind a circular aperture at:

This may be shortened to: (When d and f in millimetres and λ = 550 nm = 0.00055 mm, corresponding to yellow-green.)

For a pinhole-to-film distance of 1 inch or 25.4 mm, this works out to a pinhole of 0.185 mm (185 microns) in diameter. For f= 50 mm the optimal diameter is 0.259 mm.


The depth of field is basically infinite, but this does not mean that no optical blurring occurs. The infinite depth of field means that image blur depends not on object distance but on other factors, such as the distance from the aperture to the film plane, the aperture size, the wavelength(s) of the light source, and motion of the subject or canvas. Additionally, pinhole photography can not avoid the effects of haze.

An example of a 20-minute exposure taken with a pinhole cameraA photograph taken with a pinhole camera using an exposure time of 2s
An example of a 20-minute exposure taken with a pinhole camera
An example of a 20-minute exposure taken with a pinhole cameraA photograph taken with a pinhole camera using an exposure time of 2s
A photograph taken with a pinhole camera using an exposure time of 2s
A graph of the resolution limit of the pinhole camera as a function of focal length (image distance)
A graph of the resolution limit of the pinhole camera as a function of focal length (image distance)

In the 1970s, Young measured the resolution limit of the pinhole camera as a function of pinhole diameter[17] and later published a tutorial in The Physics Teacher.[18] Partly to enable a variety of diameters and focal lengths, he defined two normalized variables: resolution limit divided by the pinhole radius, and focal length divided by the quantity s2/λ, where s is the radius of the pinhole and λ is the wavelength of the light, typically about 550 nm. His results are plotted in the figure.

On the left-side of the graph, the pinhole is large, and geometric optics applies; the resolution limit is about 1.5 times the radius of the pinhole. (Spurious resolution is also seen in the geometric-optics limit.) On the right-side, the pinhole is small, and Fraunhofer diffraction applies; the resolution limit is given by the far-field diffraction formula shown in the graph and now increases as the pinhole is made smaller. In this formula, the radius of the pinhole is used instead of its diameter, that's why the constant is 0.61 instead of the more usual 1.22. In the region of near-field diffraction (or Fresnel diffraction), the pinhole focuses the light slightly, and the resolution limit is minimized when the focal length f (the distance between the pinhole and the film plane) is given by f = s2/λ. At this focal length, the pinhole focuses the light slightly, and the resolution limit is about 2/3 of the radius of the pinhole. The pinhole, in this case, is equivalent to a Fresnel zone plate with a single zone. The value s2/λ is in a sense the natural focal length of the pinhole.

The relation f = s2/λ yields an optimum pinhole diameter d = 2, so the experimental value differs slightly from the estimate of Petzval, above.

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Image resolution

Image resolution

Image resolution is the detail an image holds. The term applies to digital images, film images, and other types of images. "Higher resolution" means more image detail.

Circle of confusion

Circle of confusion

In optics, a circle of confusion (CoC) is an optical spot caused by a cone of light rays from a lens not coming to a perfect focus when imaging a point source. It is also known as disk of confusion, circle of indistinctness, blur circle, or blur spot.

Diffraction

Diffraction

Diffraction is defined as the interference or bending of waves around the corners of an obstacle or through an aperture into the region of geometrical shadow of the obstacle/aperture. The diffracting object or aperture effectively becomes a secondary source of the propagating wave. Italian scientist Francesco Maria Grimaldi coined the word diffraction and was the first to record accurate observations of the phenomenon in 1660.

Joseph Petzval

Joseph Petzval

Joseph Petzval was a mathematician, inventor, and physicist best known for his work in optics. He was born in the town of Szepesbéla in the Kingdom of Hungary.

John William Strutt, 3rd Baron Rayleigh

John William Strutt, 3rd Baron Rayleigh

John William Strutt, 3rd Baron Rayleigh, was a British mathematician and physicist who made extensive contributions to science. He spent all of his academic career at the University of Cambridge. Among many honours, he received the 1904 Nobel Prize in Physics "for his investigations of the densities of the most important gases and for his discovery of argon in connection with these studies." He served as president of the Royal Society from 1905 to 1908 and as chancellor of the University of Cambridge from 1908 to 1919.

Fraunhofer diffraction equation

Fraunhofer diffraction equation

In optics, the Fraunhofer diffraction equation is used to model the diffraction of waves when the diffraction pattern is viewed at a long distance from the diffracting object, and also when it is viewed at the focal plane of an imaging lens.

Depth of field

Depth of field

The depth of field (DOF) is the distance between the nearest and the furthest objects that are in acceptably sharp focus in an image captured with a camera.

Infinity

Infinity

Infinity is that which is boundless, endless, or larger than any natural number. It is often denoted by the infinity symbol .

Film plane

Film plane

A film plane is the surface of an image recording device such as a camera, upon which the lens creates the focused image. In cameras from different manufacturers, the film plane varies in distance from the lens. Thus each lens used has to be chosen carefully to assure that the image is focused on the exact place where the individual frame of film or digital sensor is positioned during exposure. It is sometimes marked on a camera body with the 'Φ' symbol where the vertical bar represents the exact location.

Haze

Haze

Haze is traditionally an atmospheric phenomenon in which dust, smoke, and other dry particulates suspended in air obscure visibility and the clarity of the sky. The World Meteorological Organization manual of codes includes a classification of particulates causing horizontal obscuration into categories of fog, ice fog, steam fog, mist, haze, smoke, volcanic ash, dust, sand, and snow. Sources for particles that cause haze include farming, traffic, industry, volcanic activity and wildfires. Seen from afar and depending on the direction of view with respect to the Sun, haze may appear brownish or bluish, while mist tends to be bluish grey instead. Whereas haze often is thought of as a phenomenon occurring in dry air, mist formation is a phenomenon in saturated, humid air. However, haze particles may act as condensation nuclei that leads to the subsequent vapor condensation and formation of mist droplets; such forms of haze are known as "wet haze".

Fraunhofer diffraction

Fraunhofer diffraction

In optics, the Fraunhofer diffraction equation is used to model the diffraction of waves when plane waves are incident on a diffracting object, and the diffraction pattern is viewed at a sufficiently long distance from the object, and also when it is viewed at the focal plane of an imaging lens. In contrast, the diffraction pattern created near the diffracting object and is given by the Fresnel diffraction equation.so, therefore

Fresnel diffraction

Fresnel diffraction

In optics, the Fresnel diffraction equation for near-field diffraction is an approximation of the Kirchhoff–Fresnel diffraction that can be applied to the propagation of waves in the near field. It is used to calculate the diffraction pattern created by waves passing through an aperture or around an object, when viewed from relatively close to the object. In contrast the diffraction pattern in the far field region is given by the Fraunhofer diffraction equation.

Calculating the f-number and required exposure

A fire hydrant photographed by a pinhole camera made from a shoe box, exposed on photographic paper to create the negative image (top). The positive image (bottom) was created digitally from the negative image. The length of the exposure was 40 seconds. There is noticeable flaring in the bottom-right corner of the image, likely due to extraneous light entering the camera box.
A fire hydrant photographed by a pinhole camera made from a shoe box, exposed on photographic paper to create the negative image (top). The positive image (bottom) was created digitally from the negative image. The length of the exposure was 40 seconds. There is noticeable flaring in the bottom-right corner of the image, likely due to extraneous light entering the camera box.

The f-number of the camera may be calculated by dividing the distance from the pinhole to the imaging plane (the focal length) by the diameter of the pinhole. For example, a camera with a 0.5 mm diameter pinhole, and a 50 mm focal length would have an f-number of 50/0.5, or 100 (f/100 in conventional notation).

Due to the large f-number of a pinhole camera, exposures will often encounter reciprocity failure.[19] Once exposure time has exceeded about 1 second for film or 30 seconds for paper, one must compensate for the breakdown in linear response of the film/paper to intensity of illumination by using longer exposures.

Exposures projected on to modern light-sensitive photographic film can typically range from five seconds up to as much as several hours, with smaller pinholes requiring longer exposures to produce the same size image. Because a pinhole camera requires a lengthy exposure, its shutter may be manually operated, as with a flap made of opaque material to cover and uncover the pinhole.

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Fire hydrant

Fire hydrant

A fire hydrant, fireplug, or firecock (archaic) is a connection point by which firefighters can tap into a water supply. It is a component of active fire protection. Underground fire hydrants have been used in Europe and Asia since at least the 18th century. Above-ground pillar-type hydrants are a 19th-century invention.

Focal length

Focal length

The focal length of an optical system is a measure of how strongly the system converges or diverges light; it is the inverse of the system's optical power. A positive focal length indicates that a system converges light, while a negative focal length indicates that the system diverges light. A system with a shorter focal length bends the rays more sharply, bringing them to a focus in a shorter distance or diverging them more quickly. For the special case of a thin lens in air, a positive focal length is the distance over which initially collimated (parallel) rays are brought to a focus, or alternatively a negative focal length indicates how far in front of the lens a point source must be located to form a collimated beam. For more general optical systems, the focal length has no intuitive meaning; it is simply the inverse of the system's optical power.

Reciprocity (photography)

Reciprocity (photography)

In photography, reciprocity is the inverse relationship between the intensity and duration of light that determines the reaction of light-sensitive material. Within a normal exposure range for film stock, for example, the reciprocity law states that the film response will be determined by the total exposure, defined as intensity × time. Therefore, the same response can result from reducing duration and increasing light intensity, and vice versa.

Shutter (photography)

Shutter (photography)

In photography, a shutter is a device that allows light to pass for a determined period, exposing photographic film or a photosensitive digital sensor to light in order to capture a permanent image of a scene. A shutter can also be used to allow pulses of light to pass outwards, as seen in a movie projector or a signal lamp. A shutter of variable speed is used to control exposure time of the film. The shutter is constructed so that it automatically closes after a certain required time interval. The speed of the shutter is controlled by a ring outside the camera, on which various timings are marked.

Coded apertures

A non-focusing coded-aperture optical system may be thought of as multiple pinhole cameras in conjunction. By adding pinholes, light throughput and thus sensitivity are increased. However, multiple images are formed, usually requiring computer deconvolution.

Modern day interest

A revival in popularity has become evident in recent years with the success of Kickstarter crowdfunding campaigns offering a range of pinhole photography products. Projects have included a camera crafted from wood[20] and the Pinhole Pro,[11] a lens designed for DSLR and MILC digital cameras.

Natural pinhole phenomenon

Replica images of a partial solar eclipse
Replica images of a partial solar eclipse

A pinhole camera effect can sometimes occur naturally. Small "pinholes" formed by the gaps between overlapping tree leaves will create replica images of the sun on flat surfaces. During an eclipse, this produces small crescents in the case of a partial eclipse, or hollow rings in the case of an annular eclipse.

Observation

Worldwide Pinhole Photography Day is observed on the last Sunday of April, every year.[21]

Photographers using the technique

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Billy Childish

Billy Childish

Billy Childish is an English painter, author, poet, photographer, film maker, singer and guitarist. Since the late 1970s, Childish has been prolific in creating music, writing and visual art. He has led and played in bands including the Pop Rivets, Thee Milkshakes, Thee Headcoats, and the Musicians of the British Empire, primarily working in the genres of garage rock, punk and surf and releasing more than 100 albums.

George Davison (photographer)

George Davison (photographer)

George Davison was an English photographer, a proponent of impressionistic photography, a co-founder of the Linked Ring Brotherhood of British artists and a managing director of Kodak UK. He was also a millionaire, thanks to an early investment in Eastman Kodak.

Barbara Ess

Barbara Ess

Barbara Ess was an American photographer. She often used a pinhole camera and was known for her No Wave musical and editorial work.

Wolf Howard

Wolf Howard

Wolf Howard is an English artist, poet and filmmaker living in Rochester, Kent and was a founder member of the Stuckists art group. He is also a drummer who has played in garage and punk bands, currently as a member of The Musicians of the British Empire (MBE's) with Billy Childish.

Steven Pippin

Steven Pippin

Steven Pippin is an English photographer and installation artist. Pippin works with converted or improvised photographic equipment and kinetic sculptures which are often based on physical models and are metaphors for social mechanisms.

Jesse Richards

Jesse Richards

Jesse Richards is a painter, filmmaker and photographer from New Haven, Connecticut and was affiliated with the international movement Stuckism. He has been described as "one of the most provocative names in American underground culture," and "the father of remodernist cinema."

Source: "Pinhole camera", Wikipedia, Wikimedia Foundation, (2023, March 3rd), https://en.wikipedia.org/wiki/Pinhole_camera.

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References
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  9. ^ History of the kinetograph, kinetoscope, & kinetophonograph [by] W. K. L. Dickson and Antonia Dickson. Literature of cinema. Arno Press. 1970. hdl:2027/mdp.39015002595158. ISBN 9780405016110.
  10. ^ Timby, Kim (31 July 2015). 3D and Animated Lenticular Photography. ISBN 9783110448061.
  11. ^ a b "Pinhole Pro Lens by Thingyfy". 2018.
  12. ^ "How to Make and Use a Pinhole Camera". Archived from the original on 2016-03-05.
  13. ^ "V3 - digital transformation news, analysis and insight". v3.co.uk. Retrieved 18 October 2018.
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  21. ^ "Worldwide Pinhole Photography Day". pinholeday.org.
Further reading
  • Eric Renner Pinhole Photography: From Historic Technique to Digital Application
External links

Media related to Pinhole cameras at Wikimedia Commons

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