In optics, particularly as it relates to film and photography, depth of field (DOF) is the distance between the nearest and farthest objects in a scene that appear acceptably sharp in an image. Although a lens can precisely focus at only one distance at a time, the decrease in sharpness is gradual on each side of the focused distance, so that within the DOF, the unsharpness is imperceptible under normal viewing conditions.
In some cases, it may be desirable to have the entire image sharp, and a large DOF is appropriate. In other cases, a small DOF may be more effective, emphasizing the subject while deemphasizing the foreground and background. In cinematography, a large DOF is often called deep focus, and a small DOF is often called shallow focus.
Precise focus is possible at only one distance; at that distance, a point object will produce a point image.^{[1]} At any other distance, a point object is defocused, and will produce a blur spot shaped like the aperture, which for the purpose of analysis is usually assumed to be circular. When this circular spot is sufficiently small, it is indistinguishable from a point, and appears to be in focus; it is rendered as “acceptably sharp”. The diameter of the circle increases with distance from the point of focus; the largest circle that is indistinguishable from a point is known as the acceptable circle of confusion, or informally, simply as the circle of confusion. The acceptable circle of confusion is influenced by visual acuity, viewing conditions, and the amount by which the image is enlarged (Ray 2000, 52–53). The increase of the circle diameter with defocus is gradual, so the limits of depth of field are not hard boundaries between sharp and unsharp.
For a 35 mm motion picture, the image area on the negative is roughly 22 mm by 16 mm (0.87 in by 0.63 in). The limit of tolerable error is usually set at 0.05 mm (0.002 in) diameter. For 16 mm film, where the image area is smaller, the tolerance is stricter, 0.025 mm (0.001 in). Standard depthoffield tables are constructed on this basis, although generally 35 mm productions set it at 0.025 mm (0.001 in). Note that the acceptable circle of confusion values for these formats are different because of the relative amount of magnification each format will need in order to be projected on a fullsized movie screen. (A table for 35 mm still photography would be somewhat different since more of the film is used for each image and the amount of enlargement is usually much less.)
Traditional (Scientific) depthoffield formulas and tables assume equal circles of confusion for near and far objects. Some authors, such as Merklinger (1992),^{[2]} have suggested that distant objects often need to be much sharper to be clearly recognizable, whereas closer objects, being larger on the film, do not need to be so sharp. The loss of detail in distant objects may be particularly noticeable with extreme enlargements. Achieving this additional sharpness in distant objects usually requires focusing beyond the hyperfocal distance, sometimes almost at infinity. For example, if photographing a cityscape with a traffic bollard in the foreground, this approach, termed the object field method by Merklinger, would recommend focusing very close to infinity, and stopping down to make the bollard sharp enough. With this approach, foreground objects cannot always be made perfectly sharp, but the loss of sharpness in near objects may be acceptable if recognizability of distant objects is paramount.
Other authors (Adams 1980, 51) have taken the opposite position, maintaining that slight unsharpness in foreground objects is usually more disturbing than slight unsharpness in distant parts of a scene.
Moritz von Rohr also used an object field method, but unlike Merklinger, he used the conventional criterion of a maximum circle of confusion diameter in the image plane, leading to unequal front and rear depths of field.
Several other factors, such as subject matter, movement, cameratosubject distance, lens focal length, selected lens fnumber, format size, and circle of confusion criteria also influence when a given defocus becomes noticeable. The combination of focal length, subject distance, and format size defines magnification at the film / sensor plane.
DOF is determined by subject magnification at the film / sensor plane and the selected lens aperture or fnumber. For a given fnumber, increasing the magnification, either by moving closer to the subject or using a lens of greater focal length, decreases the DOF; decreasing magnification increases DOF. For a given subject magnification, increasing the fnumber (decreasing the aperture diameter) increases the DOF; decreasing fnumber decreases DOF.
If the original image is enlarged to make the final image, the circle of confusion in the original image must be smaller than that in the final image by the ratio of enlargement. Cropping an image and enlarging to the same size final image as an uncropped image taken under the same conditions is equivalent to using a smaller format under the same conditions, so the cropped image has less DOF. (Stroebel 1976, 134, 136–37).
When focus is set to the hyperfocal distance, the DOF extends from half the hyperfocal distance to infinity, and the DOF is the largest possible for a given fnumber.
The comparative DOFs of two different format sizes depend on the conditions of the comparison. The DOF for the smaller format can be either more than or less than that for the larger format. In the discussion that follows, it is assumed that the final images from both formats are the same size, are viewed from the same distance, and are judged with the same circle of confusion criterion. (Derivations of the effects of format size are given under Derivation of the DOF formulas.)
“Same picture” for both formats
When the “same picture” is taken in two different format sizes from the same distance at the same fnumber with lenses that give the same angle of view, and the final images (e.g., in prints, or on a projection screen or electronic display) are the same size, DOF is, to a first approximation, inversely proportional to format size (Stroebel 1976, 139). Though commonly used when comparing formats, the approximation is valid only when the subject distance is large in comparison with the focal length of the larger format and small in comparison with the hyperfocal distance of the smaller format.
Moreover, the larger the format size, the longer a lens will need to be to capture the same framing as a smaller format. In motion pictures, for example, a frame with a 12 degree horizontal field of view will require a 50 mm lens on 16 mm film, a 100 mm lens on 35 mm film, and a 250 mm lens on 65 mm film. Conversely, using the same focal length lens with each of these formats will yield a progressively wider image as the film format gets larger: a 50 mm lens has a horizontal field of view of 12 degrees on 16 mm film, 23.6 degrees on 35 mm film, and 55.6 degrees on 65 mm film. Therefore, because the larger formats require longer lenses than the smaller ones, they will accordingly have a smaller depth of field. Compensations in exposure, framing, or subject distance need to be made in order to make one format look like it was filmed in another format.
Same focal length for both formats
Many smallformat digital SLR camera systems allow using many of the same lenses on both fullframe and “cropped format” cameras. If, for the same focal length setting, the subject distance is adjusted to provide the same field of view at the subject, at the same fnumber and finalimage size, the smaller format has greater DOF, as with the “same picture” comparison above. If pictures are taken from the same distance using the same fnumber, same focal length, and the final images are the same size, the smaller format has less DOF. If pictures taken from the same subject distance using the same focal length, are given the same enlargement, both final images will have the same DOF. The pictures from the two formats will differ because of the different angles of view. If the larger format is cropped to the captured area of the smaller format, the final images will have the same angle of view, have been given the same enlargement, and have the same DOF.
Same DOF for both formats
In many cases, the DOF is fixed by the requirements of the desired image. For a given DOF and field of view, the required fnumber is proportional to the format size. For example, if a 35 mm camera required f/11, a 4×5 camera would require f/45 to give the same DOF. For the same ISO speed, the exposure time on the 4×5 would be sixteen times as long; if the 35 camera required 1/250 second, the 4×5 camera would require 1/15 second. The longer exposure time with the larger camera might result in motion blur, especially with windy conditions, a moving subject, or an unsteady camera.
Adjusting the fnumber to the camera format is equivalent to maintaining the same absolute aperture diameter; when set to the same absolute aperture diameters, both formats have the same DOF.
Comparison of fast standard lenses in the four main formats when used for portraiture with appropriate circles of confusion to produce an uncropped image at 10x8 inches to be viewed at 25 cm show that the following settings with similar aperture diameters produce similar DoF:
For any of these, doubling the fnumber will approximately double the depth of field.
When the lens axis is perpendicular to the image plane, as is normally the case, the plane of focus (POF) is parallel to the image plane, and the DOF extends between parallel planes on either side of the POF. When the lens axis is not perpendicular to the image plane, the POF is no longer parallel to the image plane; the ability to rotate the POF is known as the Scheimpflug principle. Rotation of the POF is accomplished with camera movements (tilt, a rotation of the lens about a horizontal axis, or swing, a rotation about a vertical axis). Tilt and swing are available on most view cameras, and are also available with specific lenses on some small and mediumformat cameras.
When the POF is rotated, the near and far limits of DOF are no longer parallel; the DOF becomes wedgeshaped, with the apex of the wedge nearest the camera (Merklinger 1993, 31–32; Tillmanns 1997, 71). With tilt, the height of the DOF increases with distance from the camera; with swing, the width of the DOF increases with distance.
In some cases, rotating the POF can better fit the DOF to the scene, and achieve the required sharpness at a smaller fnumber. Alternatively, rotating the POF, in combination with a small fnumber, can minimize the part of an image that is within the DOF.
For a given subject framing and camera position, the DOF is controlled by the lens aperture diameter, which is usually specified as the fnumber, the ratio of lens focal length to aperture diameter. Reducing the aperture diameter (increasing the fnumber) increases the DOF because the circle of confusion is shrunk directly and indirectly by reducing the light hitting the outside of the lens which is focused to a different point than light hitting the inside of the lens due to spherical aberration caused by the construction of the lens;^{[3]} however, it also reduces the amount of light transmitted, and increases diffraction, placing a practical limit on the extent to which DOF can be increased by reducing the aperture diameter.
Motion pictures make only limited use of this control; to produce a consistent image quality from shot to shot, cinematographers usually choose a single aperture setting for interiors and another for exteriors, and adjust exposure through the use of camera filters or light levels. Aperture settings are adjusted more frequently in still photography, where variations in depth of field are used to produce a variety of special effects.
DOF with various apertures  


The advent of digital technology in photography has provided additional means of controlling the extent of image sharpness; some methods allow extended DOF that would be impossible with traditional techniques, and some allow the DOF to be determined after the image is made.
Focus stacking is a digital image processing technique which combines multiple images taken at different focus distances to give a resulting image with a greater depth of field than any of the individual source images. Available programs for multishot DOF enhancement include Adobe Photoshop, Syncroscopy AutoMontage, PhotoAcute Studio, Helicon Focus and CombineZ. Getting sufficient depth of field can be particularly challenging in macro photography. The images to the right illustrate the extended DOF that can be achieved by combining multiple images.
Wavefront coding is a method that convolves rays in such a way that it provides an image where fields are in focus simultaneously with all planes out of focus by a constant amount.
A plenoptic camera uses a microlens array to capture 4D light field information about a scene.
Colour apodization is a technique combining a modified lens design with image processing to achieve an increased depth of field. The lens is modified such that each colour channel has a different lens aperture. For example the red channel may be f/2.4, green may be f/2.4, whilst the blue channel may be f/5.6. Therefore the blue channel will have a greater depth of field than the other colours. The image processing identifies blurred regions in the red and green channels and in these regions copies the sharper edge data from the blue channel. The result is an image that combines the best features from the different fnumbers, (Kay 2011).
In 2013, Nokia implemented DOF control in some of its highend smartphones, called Refocus, which can change a picture's depth of field after the picture is taken. It works best when there are closeup and distant objects in the frame.^{[4]}
If the camera position and image framing (i.e., angle of view) have been chosen, the only means of controlling DOF is the lens aperture. Most DOF formulas imply that any arbitrary DOF can be achieved by using a sufficiently large fnumber. Because of diffraction, however, this isn't really true. Once a lens is stopped down to where most aberrations are well corrected, stopping down further will decrease sharpness in the plane of focus. At the DOF limits, however, further stopping down decreases the size of the defocus blur spot, and the overall sharpness may still increase. Eventually, the defocus blur spot becomes negligibly small, and further stopping down serves only to decrease sharpness even at DOF limits (Gibson 1975, 64). There is thus a tradeoff between sharpness in the POF and sharpness at the DOF limits. But the sharpness in the POF is always greater than that at the DOF limits; if the blur at the DOF limits is imperceptible, the blur in the POF is imperceptible as well.
For general photography, diffraction at DOF limits typically becomes significant only at fairly large fnumbers; because large fnumbers typically require long exposure times, motion blur may cause greater loss of sharpness than the loss from diffraction. The size of the diffraction blur spot depends on the effective fnumber , however, so diffraction is a greater issue in closeup photography, and the tradeoff between DOF and overall sharpness can become quite noticeable (Gibson 1975, 53; Lefkowitz 1979, 84).
Many lenses for small and mediumformat cameras include scales that indicate the DOF for a given focus distance and fnumber; the 35 mm lens in the image above is typical. That lens includes distance scales in feet and meters; when a marked distance is set opposite the large white index mark, the focus is set to that distance. The DOF scale below the distance scales includes markings on either side of the index that correspond to fnumbers. When the lens is set to a given fnumber, the DOF extends between the distances that align with the fnumber markings.
When the 35 mm lens above is set to f/11 and focused at approximately 1.3 m, the DOF (a “zone” of acceptable sharpness) extends from 1 m to 2 m. Conversely, the required focus and fnumber can be determined from the desired DOF limits by locating the near and far DOF limits on the lens distance scale and setting focus so that the index mark is centered between the near and far distance marks. The required fnumber is determined by finding the markings on the DOF scale that are closest to the near and far distance marks (Ray 1994, 315). For the 35 mm lens above, if it were desired for the DOF to extend from 1 m to 2 m, focus would be set so that index mark was centered between the marks for those distances, and the aperture would be set to f/11.
The focus so determined would be about 1.3 m, the approximate harmonic mean of the near and far distances.^{[5]} See the section Focus and fnumber from DOF limits for additional discussion.
If the marks for the near and far distances fall outside the marks for the largest fnumber on the DOF scale, the desired DOF cannot be obtained; for example, with the 35 mm lens above, it is not possible to have the DOF extend from 0.7 m to infinity. The DOF limits can be determined visually, by focusing on the farthest object to be within the DOF and noting the distance mark on the lens distance scale, and repeating the process for the nearest object to be within the DOF.
Some distance scales have markings for only a few distances; for example, the 35 mm lens above shows only 3 ft and 5 ft on its upper scale. Using other distances for DOF limits requires visual interpolation between marked distances. Since the distance scale is nonlinear, accurate interpolation can be difficult. In most cases, English and metric distance markings are not coincident, so using both scales to note focused distances can sometimes lessen the need for interpolation. Many autofocus lenses have smaller distance and DOF scales and fewer markings than do comparable manualfocus lenses, so that determining focus and fnumber from the scales on an autofocus lens may be more difficult than with a comparable manualfocus lens. In most cases, determining these settings using the lens DOF scales on an autofocus lens requires that the lens or camera body be set to manual focus.^{[6]}
On a view camera, the focus and fnumber can be obtained by measuring the focus spread and performing simple calculations. The procedure is described in more detail in the section Focus and fnumber from DOF limits. Some view cameras include DOF calculators that indicate focus and fnumber without the need for any calculations by the photographer (Tillmanns 1997, 67–68; Ray 2002, 230–31).
The hyperfocal distance is the nearest focus distance at which the DOF extends to infinity; focusing the camera at the hyperfocal distance results in the largest possible depth of field for a given fnumber (Ray 2000, 55). Focusing beyond the hyperfocal distance does not increase the far DOF (which already extends to infinity), but it does decrease the DOF in front of the subject, decreasing the total DOF. Some photographers consider this wasting DOF; however, see Object field methods above for a rationale for doing so. Focusing on the hyperfocal distance is a special case of zone focusing in which the far limit of DOF is at infinity.
If the lens includes a DOF scale, the hyperfocal distance can be set by aligning the infinity mark on the distance scale with the mark on the DOF scale corresponding to the fnumber to which the lens is set. For example, with the 35 mm lens shown above set to f/11, aligning the infinity mark with the ‘11’ to the left of the index mark on the DOF scale would set the focus to the hyperfocal distance.
Depth of field can be anywhere from a fraction of a millimeter to virtually infinite. In some cases, such as landscapes, it may be desirable to have the entire image sharp, and a large DOF is appropriate. In other cases, artistic considerations may dictate that only a part of the image be in focus, emphasizing the subject while deemphasizing the background, perhaps giving only a suggestion of the environment (Langford 1973, 81). For example, a common technique in melodramas and horror films is a closeup of a person's face, with someone just behind that person visible but out of focus. A portrait or closeup still photograph might use a small DOF to isolate the subject from a distracting background. The use of limited DOF to emphasize one part of an image is known as selective focus, differential focus or shallow focus.
Although a small DOF implies that other parts of the image will be unsharp, it does not, by itself, determine how unsharp those parts will be. The amount of background (or foreground) blur depends on the distance from the plane of focus, so if a background is close to the subject, it may be difficult to blur sufficiently even with a small DOF. In practice, the lens fnumber is usually adjusted until the background or foreground is acceptably blurred, often without direct concern for the DOF.
Sometimes, however, it is desirable to have the entire subject sharp while ensuring that the background is sufficiently unsharp. When the distance between subject and background is fixed, as is the case with many scenes, the DOF and the amount of background blur are not independent. Although it is not always possible to achieve both the desired subject sharpness and the desired background unsharpness, several techniques can be used to increase the separation of subject and background.
For a given scene and subject magnification, the background blur increases with lens focal length. If it is not important that background objects be unrecognizable, background deemphasis can be increased by using a lens of longer focal length and increasing the subject distance to maintain the same magnification. This technique requires that sufficient space in front of the subject be available; moreover, the perspective of the scene changes because of the different camera position, and this may or may not be acceptable.
The situation is not as simple if it is important that a background object, such as a sign, be unrecognizable. The magnification of background objects also increases with focal length, so with the technique just described, there is little change in the recognizability of background objects.^{[7]} However, a lens of longer focal length may still be of some help; because of the narrower angle of view, a slight change of camera position may suffice to eliminate the distracting object from the field of view.
Although tilt and swing are normally used to maximize the part of the image that is within the DOF, they also can be used, in combination with a small fnumber, to give selective focus to a plane that isn't perpendicular to the lens axis. With this technique, it is possible to have objects at greatly different distances from the camera in sharp focus and yet have a very shallow DOF. The effect can be interesting because it differs from what most viewers are accustomed to seeing.
The DOF beyond the subject is always greater than the DOF in front of the subject. When the subject is at the hyperfocal distance or beyond, the far DOF is infinite, so the ratio is 1:∞; as the subject distance decreases, near:far DOF ratio increases, approaching unity at high magnification. For large apertures at typical portrait distances, the ratio is still close to 1:1. The oftcited rule that 1/3 of the DOF is in front of the subject and 2/3 is beyond (a 1:2 ratio) is true only when the subject distance is 1/3 the hyperfocal distance.
As a lens is stopped down, the defocus blur at the DOF limits decreases but diffraction blur increases. The presence of these two opposing factors implies a point at which the combined blur spot is minimized (Gibson 1975, 64); at that point, the fnumber is optimal for image sharpness. If the final image is viewed under normal conditions (e.g., an 8″×10″ image viewed at 10″), it may suffice to determine the fnumber using criteria for minimum required sharpness, and there may be no practical benefit from further reducing the size of the blur spot. But this may not be true if the final image is viewed under more demanding conditions, e.g., a very large final image viewed at normal distance, or a portion of an image enlarged to normal size (Hansma 1996). Hansma also suggests that the finalimage size may not be known when a photograph is taken, and obtaining the maximum practicable sharpness allows the decision to make a large final image to be made at a later time.
Hansma (1996) and Peterson (1996) have discussed determining the combined effects of defocus and diffraction using a rootsquare combination of the individual blur spots. Hansma's approach determines the fnumber that will give the maximum possible sharpness; Peterson's approach determines the minimum fnumber that will give the desired sharpness in the final image, and yields a maximum focus spread for which the desired sharpness can be achieved.^{[8]} In combination, the two methods can be regarded as giving a maximum and minimum fnumber for a given situation, with the photographer free to choose any value within the range, as conditions (e.g., potential motion blur) permit. Gibson (1975), 64) gives a similar discussion, additionally considering blurring effects of camera lens aberrations, enlarging lens diffraction and aberrations, the negative emulsion, and the printing paper.^{[9]} Couzin (1982), 1098) gave a formula essentially the same as Hansma’s for optimal fnumber, but did not discuss its derivation.
Hopkins (1955), Stokseth (1969), and Williams and Becklund (1989) have discussed the combined effects using the modulation transfer function. Conrad's Depth of Field in Depth (PDF), and Jacobson's Photographic Lenses Tutorial discuss the use of Hopkins's method specifically in regard to DOF.
In semiconductor photolithography applications, depth of field is extremely important as integrated circuit layout features must be printed with high accuracy at extremely small size. The difficulty is that the wafer surface is not perfectly flat, but may vary by several micrometres. Even this small variation causes some distortion in the projected image, and results in unwanted variations in the resulting pattern. Thus photolithography engineers take extreme measures to maximize the optical depth of field of the photolithography equipment. To minimize this distortion further, semiconductor manufacturers may use chemical mechanical polishing to make the wafer surface even flatter before lithographic patterning.
A person may sometimes experience better vision in daylight than at night because of an increased depth of field due to constriction of the pupil (i.e., miosis).
The basis of these formulas is given in the section Derivation of the DOF formulae;^{[10]} refer to the diagram in that section for illustration of the quantities discussed below.
Let be the lens focal length, be the lens fnumber, and be the circle of confusion for a given image format. The hyperfocal distance is given by
Let be the distance at which the camera is focused (the “subject distance”). When is large in comparison with the lens focal length, the distance from the camera to the near limit of DOF and the distance from the camera to the far limit of DOF are
and
The depth of field is
Substituting for and rearranging, DOF can be expressed as
Thus, for a given image format, depth of field is determined by three factors: the focal length of the lens, the fnumber of the lens opening (the aperture), and the cameratosubject distance.
When the subject distance is the hyperfocal distance,
and
For , the far limit of DOF is at infinity and the DOF is infinite; of course, only objects at or beyond the near limit of DOF will be recorded with acceptable sharpness.
When the subject distance approaches the focal length, using the formulas given above can result in significant errors. For closeup work, the hyperfocal distance has little applicability, and it usually is more convenient to express DOF in terms of image magnification. Let be the magnification; when the subject distance is small in comparison with the hyperfocal distance,
so that for a given magnification, DOF is independent of focal length. Stated otherwise, for the same subject magnification, at the same fnumber, all focal lengths used on a given image format give approximately the same DOF. This statement is true only when the subject distance is small in comparison with the hyperfocal distance, however.
The discussion thus far has assumed a symmetrical lens for which the entrance and exit pupils coincide with the front and rear nodal planes, and for which the pupil magnification (the ratio of exit pupil diameter to that of the entrance pupil)^{[11]} is unity. Although this assumption usually is reasonable for largeformat lenses, it often is invalid for medium and smallformat lenses.
When , the DOF for an asymmetrical lens is
where is the pupil magnification. When the pupil magnification is unity, this equation reduces to that for a symmetrical lens.
Except for closeup and macro photography, the effect of lens asymmetry is minimal. At unity magnification, however, the errors from neglecting the pupil magnification can be significant. Consider a telephoto lens with and a retrofocus wideangle lens with , at . The asymmetricallens formula gives and , respectively. The symmetricallens formula gives in either case. The errors are −33% and 33%, respectively.
For given near and far DOF limits and , the required fnumber is smallest when focus is set to
the harmonic mean of the near and far distances. When the subject distance is large in comparison with the lens focal length, the required fnumber is
When the far limit of DOF is at infinity,
and
In practice, these settings usually are determined on the image side of the lens, using measurements on the bed or rail with a view camera, or using lens DOF scales on manualfocus lenses for small and mediumformat cameras. If and are the image distances that correspond to the near and far limits of DOF, the required fnumber is minimized when the image distance is
In practical terms, focus is set to halfway between the near and far image distances. The required fnumber is
The image distances are measured from the camera's image plane to the lens's image nodal plane, which is not always easy to locate. In most cases, focus and fnumber can be determined with sufficient accuracy using the approximate formulas above, which require only the difference between the near and far image distances; view camera users sometimes refer to the difference as the focus spread (Hansma 1996, 55). Most lens DOF scales are based on the same concept.
The focus spread is related to the depth of focus. Ray (2000, 56) gives two definitions of the latter. The first is the tolerance of the position of the image plane for which an object remains acceptably sharp; the second is that the limits of depth of focus are the imageside conjugates of the near and far limits of DOF. With the first definition, focus spread and depth of focus are usually close in value though conceptually different. With the second definition, focus spread and depth of focus are the same.
If a subject is at distance and the foreground or background is at distance , let the distance between the subject and the foreground or background be indicated by
The blur disk diameter of a detail at distance from the subject can be expressed as a function of the subject magnification , focal length , fnumber or alternatively the diameter of the entrance pupil (often called the aperture) according to
The minus sign applies to a foreground object, and the plus sign applies to a background object.
The blur increases with the distance from the subject; when , the detail is within the depth of field, and the blur is imperceptible. If the detail is only slightly outside the DOF, the blur may be only barely perceptible.
For a given subject magnification, fnumber, and distance from the subject of the foreground or background detail, the degree of detail blur varies with the lens focal length. For a background detail, the blur increases with focal length; for a foreground detail, the blur decreases with focal length. For a given scene, the positions of the subject, foreground, and background usually are fixed, and the distance between subject and the foreground or background remains constant regardless of the camera position; however, to maintain constant magnification, the subject distance must vary if the focal length is changed. For small distance between the foreground or background detail, the effect of focal length is small; for large distance, the effect can be significant. For a reasonably distant background detail, the blur disk diameter is
depending only on focal length.
The blur diameter of foreground details is very large if the details are close to the lens.
The magnification of the detail also varies with focal length; for a given detail, the ratio of the blur disk diameter to imaged size of the detail is independent of focal length, depending only on the detail size and its distance from the subject. This ratio can be useful when it is important that the background be recognizable (as usually is the case in evidence or surveillance photography), or unrecognizable (as might be the case for a pictorial photographer using selective focus to isolate the subject from a distracting background). As a general rule, an object is recognizable if the blur disk diameter is onetenth to onefifth the size of the object or smaller (Williams 1990, 205),^{[12]} and unrecognizable when the blur disk diameter is the object size or greater.
The effect of focal length on background blur is illustrated in van Walree's article on Depth of field.
The distance scales on most medium and smallformat lenses indicate distance from the camera’s image plane. Most DOF formulas, including those in this article, use the object distance from the lens’s front nodal plane, which often is not easy to locate. Moreover, for many zoom lenses and internalfocusing nonzoom lenses, the location of the front nodal plane, as well as focal length, changes with subject distance. When the subject distance is large in comparison with the lens focal length, the exact location of the front nodal plane is not critical; the distance is essentially the same whether measured from the front of the lens, the image plane, or the actual nodal plane. The same is not true for closeup photography; at unity magnification, a slight error in the location of the front nodal plane can result in a DOF error greater than the errors from any approximations in the DOF equations.
The asymmetrical lens formulas require knowledge of the pupil magnification, which usually is not specified for medium and smallformat lenses. The pupil magnification can be estimated by looking into the front and rear of the lens and measuring the diameters of the apparent apertures, and computing the ratio of rear diameter to front diameter (Shipman 1977, 144). However, for many zoom lenses and internalfocusing nonzoom lenses, the pupil magnification changes with subject distance, and several measurements may be required.
Most DOF formulas, including those discussed in this article, employ several simplifications:
The lens designer cannot restrict analysis to Gaussian optics and cannot ignore lens aberrations. However, the requirements of practical photography are less demanding than those of lens design, and despite the simplifications employed in development of most DOF formulas, these formulas have proven useful in determining camera settings that result in acceptably sharp pictures. It should be recognized that DOF limits are not hard boundaries between sharp and unsharp, and that there is little point in determining DOF limits to a precision of many significant figures.
A symmetrical lens is illustrated at right. The subject, at distance , is in focus at image distance . Point objects at distances and would be in focus at image distances and , respectively; at image distance , they are imaged as blur spots. The depth of field is controlled by the aperture stop diameter ; when the blur spot diameter is equal to the acceptable circle of confusion , the near and far limits of DOF are at and . From similar triangles,
and
It usually is more convenient to work with the lens fnumber than the aperture diameter; the fnumber is related to the lens focal length and the aperture diameter by
substitution into the previous equations gives
Rearranging to solve for and gives
and
The image distance is related to an object distance by the thin lens equation
applying this to and gives
and
solving for , , and in these three equations, substituting into the two previous equations, and rearranging gives the near and far limits of DOF:
and
Solving for the focus distance and setting the far limit of DOF to infinity gives
where is the hyperfocal distance. Setting the subject distance to the hyperfocal distance and solving for the near limit of DOF gives
For any practical value of , the focal length is negligible in comparison, so that
Substituting the approximate expression for hyperfocal distance into the formulas for the near and far limits of DOF gives
and
Combining, the depth of field is
Magnification can be expressed as
at the hyperfocal distance, the magnification then is
Substituting for and simplifying gives
It is sometimes convenient to express DOF in terms of magnification . Substituting
and
into the formula for DOF and rearranging gives
after Larmore (1965), 163).
Multiplying the numerator and denominator of the exact formula above by
gives
If the fnumber and circle of confusion are constant, decreasing the focal length increases the second term in the denominator, decreasing the denominator and increasing the value of the righthand side, so that a shorter focal length gives greater DOF.
The term in parentheses in the denominator is the hyperfocal magnification , so that
A subject distance is decreased, the subject magnification increases, and eventually becomes large in comparison with the hyperfocal magnification. Thus the effect of focal length is greatest near the hyperfocal distance, and decreases as subject distance is decreased. However, the near/far perspective will differ for different focal lengths, so the difference in DOF may not be readily apparent.
When , , and
so that for a given magnification, DOF is essentially independent of focal length. Stated otherwise, for the same subject magnification and the same fnumber, all focal lengths for a given image format give approximately the same DOF. This statement is true only when the subject distance is small in comparison with the hyperfocal distance, however.
When the subject distance is large in comparison with the lens focal length,
and
so that
For , the far limit of DOF is at infinity and the DOF is infinite; of course, only objects at or beyond the near limit of DOF will be recorded with acceptable sharpness.
When the subject distance approaches the lens focal length, the focal length no longer is negligible, and the approximate formulas above cannot be used without introducing significant error. At close distances, the hyperfocal distance has little applicability, and it usually is more convenient to express DOF in terms of magnification. The distance is small in comparison with the hyperfocal distance, so the simplified formula
can be used with good accuracy. For a given magnification, DOF is independent of focal length.
From the “exact” equations for near and far limits of DOF, the DOF in front of the subject is
and the DOF beyond the subject is
The near:far DOF ratio is
This ratio is always less than unity; at moderatetolarge subject distances, , and
When the subject is at the hyperfocal distance or beyond, the far DOF is infinite, and the near:far ratio is zero. It’s commonly stated that approximately 1/3 of the DOF is in front of the subject and approximately 2/3 is beyond; however, this is true only when .
At closer subject distances, it’s often more convenient to express the DOF ratio in terms of the magnification
substitution into the “exact” equation for DOF ratio gives
As magnification increases, the near:far ratio approaches a limiting value of unity.
When the subject distance is much less than hyperfocal, the total DOF is given to good approximation by
When additionally the magnification is small compared to unity, the value of in the numerator can be neglected, and the formula further simplifies to
The DOF ratio for two different formats is then
Essentially the same approach is described in Stroebel (1976), 136–39).
The results of the comparison depend on what is assumed. One approach is to assume that essentially the same picture is taken with each format and enlarged to produce the same size final image, so the subject distance remains the same, the focal length is adjusted to maintain the same angle of view, and to a first approximation, magnification is in direct proportion to some characteristic dimension of each format. If both pictures are enlarged to give the same size final images with the same sharpness criteria, the circle of confusion is also in direct proportion to the format size. Thus if is the characteristic dimension of the format,
With the same fnumber, the DOF ratio is then
so the DOF ratio is in inverse proportion to the format size. This ratio is approximate, and breaks down in the macro range of the larger format (the value of in the numerator is no longer negligible) or as distance approaches the hyperfocal distance for the smaller format (the DOF of the smaller format approaches infinity).
If the formats have approximately the same aspect ratios, the characteristic dimensions can be the format diagonals; if the aspect ratios differ considerably (e.g., 4×5 vs. 6×17), the dimensions must be chosen more carefully, and the DOF comparison may not even be meaningful.
If the DOF is to be the same for both formats the required fnumber is in direct proportion to the format size:
Adjusting the fnumber in proportion to format size is equivalent to using the same absolute aperture diameter for both formats, discussed in detail below in Use of absolute aperture diameter.
If the same lens focal length is used in both formats, magnifications can be maintained in the ratio of the format sizes by adjusting subject distances; the DOF ratio is the same as that given above, but the images differ because of the different perspectives and angles of view.
If the same DOF is required for each format, an analysis similar to that above shows that the required fnumber is in direct proportion to the format size.
Another approach is to use the same focal length with both formats at the same subject distance, so the magnification is the same, and with the same fnumber,
so the DOF ratio is in direct proportion to the format size. The perspective is the same for both formats, but because of the different angles of view, the pictures are not the same.
Cropping an image and enlarging to the same size final image as an uncropped image taken under the same conditions is equivalent to using a smaller format; the cropped image requires greater enlargement and consequently has a smaller circle of confusion. A cropped then enlarged image has less DOF than the uncropped image.
The aperture diameter is normally given in terms of the fnumber because all lenses set to the same fnumber give approximately the same image illuminance (Ray 2002, 130), simplifying exposure settings. In deriving the basic DOF equations, the substitution of for the absolute aperture diameter can be omitted, giving the DOF in terms of the absolute aperture diameter:
after Larmore (1965), 163). When the subject distance is small in comparison with the hyperfocal distance, the second term in the denominator can be neglected, leading to
With the same subject distance and angle of view for both formats, , and
so the DOFs are in inverse proportion to the absolute aperture diameters. When the diameters are the same, the two formats have the same DOF. Von Rohr (1906) made this same observation, saying “At this point it will be sufficient to note that all these formulae involve quantities relating exclusively to the entrancepupil and its position with respect to the objectpoint, whereas the focal length of the transforming system does not enter into them.” Lyon’s Depth of Field Outside the Box describes an approach very similar to that of von Rohr.
Using the same absolute aperture diameter for both formats with the “same picture” criterion is equivalent to adjusting the fnumber in proportion to the format sizes, discussed above under “Same picture” for both formats
The equations for the DOF limits can be combined to eliminate and solve for the subject distance. For given near and far DOF limits and , the subject distance is
the harmonic mean of the near and far distances. The equations for DOF limits also can be combined to eliminate and solve for the required fnumber, giving
When the subject distance is large in comparison with the lens focal length, this simplifies to
When the far limit of DOF is at infinity, the equations for and give indeterminate results. But if all terms in the numerator and denominator on the righthand side of the equation for are divided by , it is seen that when is at infinity,
Similarly, if all terms in the numerator and denominator on the righthand side of the equation for are divided by , it is seen that when is at infinity,
Most discussions of DOF concentrate on the object side of the lens, but the formulas are simpler and the measurements usually easier to make on the image side. If the basic imageside equations
and
are combined and solved for the image distance , the result is
the harmonic mean of the near and far image distances. The basic imageside equations can also be combined and solved for , giving
The image distances are measured from the camera's image plane to the lens's image nodal plane, which is not always easy to locate. The harmonic mean is always less than the arithmentic mean, but when the difference between the near and far image distances is reasonably small, the two means are close to equal, and focus can be set with sufficient accuracy using
This formula requires only the difference between the near and far image distances. View camera users often refer to this difference as the focus spread; it usually is measured on the bed or focusing rail. Focus is simply set to halfway between the near and far image distances.
Substituting into the equation for and rearranging gives
One variant of the thinlens equation is , where is the magnification; substituting this into the equation for gives
At moderatetolarge subject distances, is small compared to unity, and the fnumber can often be determined with sufficient accuracy using
For closeup photography, the magnification cannot be ignored, and the fnumber should be determined using the first approximate formula.
As with the approximate formula for , the approximate formulas for require only the focus spread rather than the absolute image distances.
When the far limit of DOF is at infinity, .
On manualfocus small and mediumformat lenses, the focus and fnumber usually are determined using the lens DOF scales, which often are based on the approximate equations above.
If the equation for the far limit of DOF is solved for , and the far distance replaced by an arbitrary distance , the blur disk diameter at that distance is
When the background is at the far limit of DOF, the blur disk diameter is equal to the circle of confusion , and the blur is just imperceptible. The diameter of the background blur disk increases with the distance to the background. A similar relationship holds for the foreground; the general expression for a defocused object at distance is
For a given scene, the distance between the subject and a foreground or background object is usually fixed; let that distance be represented by
then
or, in terms of subject distance,
with the minus sign used for foreground objects and the plus sign used for background objects. For a relatively distant background object,
In terms of subject magnification, the subject distance is
so that, for a given fnumber and subject magnification,
Differentiating with respect to gives
With the plus sign, the derivative is everywhere positive, so that for a background object, the blur disk size increases with focal length. With the minus sign, the derivative is everywhere negative, so that for a foreground object, the blur disk size decreases with focal length.
The magnification of the defocused object also varies with focal length; the magnification of the defocused object is
where is the image distance of the subject. For a defocused object with some characteristic dimension , the imaged size of that object is
The ratio of the blur disk size to the imaged size of that object then is
so for a given defocused object, the ratio of the blur disk diameter to object size is independent of focal length, and depends only on the object size and its distance from the subject.
This discussion thus far has assumed a symmetrical lens for which the entrance and exit pupils coincide with the object and image nodal planes, and for which the pupil magnification is unity. Although this assumption usually is reasonable for largeformat lenses, it often is invalid for medium and smallformat lenses.
For an asymmetrical lens, the DOF ahead of the subject distance and the DOF beyond the subject distance are given by^{[13]}
and
where is the pupil magnification.
Combining gives the total DOF:
When , the second term in the denominator becomes small in comparison with the first, and (Shipman 1977, 147)
When the pupil magnification is unity, the equations for asymmetrical lenses reduce to those given earlier for symmetrical lenses.
Except for closeup and macro photography, the effect of lens asymmetry is minimal. A slight rearrangement of the last equation gives
As magnification decreases, the term becomes smaller in comparison with the term, and eventually the effect of pupil magnification becomes negligible.
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