Hyperfocal distance

Accompanying figures

The following derivations refer to the accompanying figures. For clarity, half the aperture and circle of confusion are indicated.[3]

An object at distance H forms a sharp image at distance x  (blue line). Here, objects at infinity have images with a circle of confusion indicated by the brown ellipse where the upper red ray through the focal point intersects the blue line.

First using similar triangles hatched in green,

${\displaystyle {\begin{array}{crcl}&{\dfrac {x-f}{c/2}}&=&{\dfrac {f}{D/2}}\\\therefore &x-f&=&{\dfrac {cf}{D}}\\\therefore &x&=&f+{\dfrac {cf}{D}}\end{array}}}$

Then using similar triangles dotted in purple,

${\displaystyle {\begin{array}{crclcl}&{\dfrac {H}{D/2}}&=&{\dfrac {x}{c/2}}\\\therefore &H&=&{\dfrac {Dx}{c}}&=&{\dfrac {D}{c}}{\Big (}f+{\dfrac {cf}{D}}{\Big )}\\&&=&{\dfrac {Df}{c}}+f&=&{\dfrac {f^{2}}{Nc}}+f\end{array}}}$

as found above.

Objects at infinity form sharp images at the focal length f  (blue line). Here, an object at H forms an image with a circle of confusion indicated by the brown ellipse where the lower red ray converging to its sharp image intersects the blue line.

Using similar triangles shaded in yellow,

${\displaystyle {\begin{array}{crclcl}&{\dfrac {H}{D/2}}&=&{\dfrac {f}{c/2}}\\\therefore &H&=&{\dfrac {Df}{c}}&=&{\dfrac {f^{2}}{Nc}}\end{array}}}$

Thomas Sutton and George Dawson define focal range for what we now call hyperfocal distance:[2]

Focal Range. In every lens there is, corresponding to a given apertal ratio (that is, the ratio of the diameter of the stop to the focal length), a certain distance of a near object from it, between which and infinity all objects are in equally good focus. For instance, in a single view lens of 6 inch focus, with a 1/4 in. stop (apertal ratio one-twenty-fourth), all objects situated at distances lying between 20 feet from the lens and an infinite distance from it (a fixed star, for instance) are in equally good focus. Twenty feet is therefore called the “focal range” of the lens when this stop is used. The focal range is consequently the distance of the nearest object, which will be in good focus when the ground glass is adjusted for an extremely distant object. In the same lens, the focal range will depend upon the size of the diaphragm used, while in different lenses having the same apertal ratio the focal ranges will be greater as the focal length of the lens is increased. The terms 'apertal ratio' and 'focal range' have not come into general use, but it is very desirable that they should, in order to prevent ambiguity and circumlocution when treating of the properties of photographic lenses. 'Focal range' is a good term, because it expresses the range within which it is necessary to adjust the focus of the lens to objects at different distances from it – in other words, the range within which focusing becomes necessary.

Their focal range is about 1000 times their aperture diameter, so it makes sense as a hyperfocal distance with CoC value of f/1000, or image format diagonal times 1/1000 assuming the lens is a “normal” lens. What is not clear, however, is whether the focal range they cite was computed, or empirical.

Sir William de Wivelesley Abney says:[4]

The annexed formula will approximately give the nearest point p which will appear in focus when the distance is accurately focussed, supposing the admissible disc of confusion to be 0.025 cm:

${\displaystyle p=0.41\cdot f^{2}\cdot a}$

when

${\displaystyle f=}$ the focal length of the lens in cm

${\displaystyle a=}$ the ratio of the aperture to the focal length

That is, a is the reciprocal of what we now call the f-number, and the answer is evidently in meters. His 0.41 should obviously be 0.40. Based on his formulae, and on the notion that the aperture ratio should be kept fixed in comparisons across formats, Abney says:

It can be shown that an enlargement from a small negative is better than a picture of the same size taken direct as regards sharpness of detail. ... Care must be taken to distinguish between the advantages to be gained in enlargement by the use of a smaller lens, with the disadvantages that ensue from the deterioration in the relative values of light and shade.

John Traill Taylor recalls this word formula for a sort of hyperfocal distance:[5]

We have seen it laid down as an approximative rule by some writers on optics (Thomas Sutton, if we remember aright), that if the diameter of the stop be a fortieth part of the focus of the lens, the depth of focus will range between infinity and a distance equal to four times as many feet as there are inches in the focus of the lens.

This formula implies a stricter CoC criterion than we typically use today.

John Hodges discusses depth of field without formulas but with some of these relationships:[6]

There is a point, however, beyond which everything will be in pictorially good definition, but the longer the focus of the lens used, the further will the point beyond which everything is in sharp focus be removed from the camera. Mathematically speaking, the amount of depth possessed by a lens varies inversely as the square of its focus.

This "mathematically" observed relationship implies that he had a formula at hand, and a parameterization with the f-number or “intensity ratio” in it. To get an inverse-square relation to focal length, you have to assume that the CoC limit is fixed and the aperture diameter scales with the focal length, giving a constant f-number.

C. Welborne Piper may be the first to have published a clear distinction between Depth of Field in the modern sense and Depth of Definition in the focal plane, and implies that Depth of Focus and Depth of Distance are sometimes used for the former (in modern usage, Depth of Focus is usually reserved for the latter).[7] He uses the term Depth Constant for H, and measures it from the front principal focus (i. e., he counts one focal length less than the distance from the lens to get the simpler formula), and even introduces the modern term:

This is the maximum depth of field possible, and H + f may be styled the distance of maximum depth of field. If we measure this distance extra-focally it is equal to H, and is sometimes called the hyperfocal distance. The depth constant and the hyperfocal distance are quite distinct, though of the same value.

It is unclear what distinction he means. Adjacent to Table I in his appendix, he further notes:

If we focus on infinity, the constant is the focal distance of the nearest object in focus. If we focus on an extra-focal distance equal to the constant, we obtain a maximum depth of field from approximately half the constant distance up to infinity. The constant is then the hyper-focal distance.

At this point we do not have evidence of the term hyperfocal before Piper, nor the hyphenated hyper-focal which he also used, but he obviously did not claim to coin this descriptor himself.

Louis Derr may be the first to clearly specify the first definition,[8] which is considered to be the strictly correct one in modern times, and to derive the formula corresponding to it. Using ${\displaystyle p}$ for hyperfocal distance, ${\displaystyle D}$ for aperture diameter, ${\displaystyle d}$ for the diameter that a circle of confusion shall not exceed, and ${\displaystyle f}$ for focal length, he derives:

${\displaystyle p={\frac {(D+d)f}{d}}}$

As the aperture diameter, ${\displaystyle D}$ is the ratio of the focal length, ${\displaystyle f}$ to the numerical aperture, ${\displaystyle N}$; and the diameter of the circle of confusion, ${\displaystyle c=d}$, this gives the equation for the first definition above.

${\displaystyle p={\frac {({\tfrac {f}{N}}+c)f}{c}}={\frac {f^{2}}{Nc}}+f}$

George Lindsay Johnson uses the term Depth of Field for what Abney called Depth of Focus, and Depth of Focus in the modern sense (possibly for the first time),[9] as the allowable distance error in the focal plane. His definitions include hyperfocal distance:

Depth of Focus is a convenient, but not strictly accurate term, used to describe the amount of racking movement (forwards or backwards) which can be given to the screen without the image becoming sensibly blurred, i.e. without any blurring in the image exceeding 1/100 in., or in the case of negatives to be enlarged or scientific work, the 1/10 or 1/100 mm. Then the breadth of a point of light, which, of course, causes blurring on both sides, i.e. 1/50 in = 2e (or 1/100 in = e).

His drawing makes it clear that his e is the radius of the circle of confusion. He has clearly anticipated the need to tie it to format size or enlargement, but has not given a general scheme for choosing it.

Depth of Field is precisely the same as depth of focus, only in the former case the depth is measured by the movement of the plate, the object being fixed, while in the latter case the depth is measured by the distance through which the object can be moved without the circle of confusion exceeding 2e.

Thus if a lens which is focused for infinity still gives a sharp image for an object at 6 yards, its depth of field is from infinity to 6 yards, every object beyond 6 yards being in focus.

This distance (6 yards) is termed the hyperfocal distance of the lens, and any allowable confusion disc depends on the focal length of the lens and on the stop used.

If the limit of confusion of half of the disc (i.e. e) be taken as 1/100 in., then the hyperfocal distance

${\displaystyle H={\frac {Fd}{e}}}$,

d being the diameter of the stop, ...

Johnson's use of former and latter seem to be swapped; perhaps former was here meant to refer to the immediately preceding section title Depth of Focus, and latter to the current section title Depth of Field. Except for an obvious factor-of-2 error in using the ratio of stop diameter to CoC radius, this definition is the same as Abney's hyperfocal distance.

The term hyperfocal distance also appears in Cassell's Cyclopaedia of 1911, The Sinclair Handbook of Photography of 1913, and Bayley's The Complete Photographer of 1914.

Rudolf Kingslake is explicit about the two meanings:[1]

if the camera is focused on a distance s equal to 1000 times the diameter of the lens aperture, then the far depth ${\displaystyle D_{1}}$ becomes infinite. This critical object distance "h" is known as the Hyperfocal Distance. For a camera focused on this distance, ${\displaystyle D_{1}=\infty }$ and ${\displaystyle D_{2}=h/2}$, and we see that the range of distances acceptably in focus will run from just half the hyperfocal distance to infinity. The hyperfocal distance is, therefore, the most desirable distance on which to pre-set the focus of a fixed-focus camera. It is worth noting, too, that if a camera is focused on ${\displaystyle s=\infty }$, the closest acceptable object is at ${\displaystyle L_{2}=sh/(h+s)=h/(h/s+1)=h}$ (by equation 21). This is a second important meaning of the hyperfocal distance.

Kingslake uses the simplest formulae for DOF near and far distances, which has the effect of making the two different definitions of hyperfocal distance give identical values.