by Q.-Tuan Luong for the Large Format Page
f16 f22 f32 f45 f64 5% 30% 50% 20% 5%Would the project have been Smell the tidepools, the breakdown would have been probably quite different, but this still gives you an idea of what f-stops are commonly used.
If you don't want to read the explanations and wade in the math which follows, here are the important points explaned in more details in this article:
D(mm) F 1 16.6 2 22.6 3 32.2 4 32.6 5 32.9 6 45.2 7 45.4 8 45.6 9 45.8 10 64
If the circle of confusion is large, the image will look fuzzy. If the circle of confusion is small, then it will be indistinguishable to the eye from a point, and the image will look sharp. There is not a universal boundary between fuzzy and sharp. The blurring of an out of focus point occurs gradually. The calculations done in this document should be taken just as general guidelines. When you use a depth of field scale, you rely on the manufacturer's choice of a value for the acceptable circle of confusion. This value might not be the best for your use.
The brightness within the circle of confusion is constant. If we use the criterion that two points are resolved when their circle of confusion do not overlap (if the circles overlap, the two points are imaged in a continuous bright spot) then the resolution R is related to the diameter of the circle of confusion c by R = 1/c. This is the number of non-overlapping circles of confusion that can be fit in a unit length. If c is expressed in millimeters, then R represents the number of lines pairs per millimiters (lp/mm). One precision is necessary here. We have considered two bright points, separated by a dark space. This is the same situation as two bright lines separated by a dark line. Each element consists of a dark line and and bright line. The separation between each element is c. A source of confusion is that some authors consider a line pair (a dark line and a white line) to be two lines, so they would use R = 2/c. This corresponds to the number of pixels.
The smallest resolvable distance c0 is such that two dark lines separated by more than this distance (by a white line) are seen as two lines, while two dark lines separated by less than this distance would be seen as one line. It is generally agreed that at normal minimal viewing distance d0 (reading distance, around 25cm), the eye can resolve elements spaced at 0.2mm. A good choice for the diameter of the acceptable circle of confusion c on a print viewed at that distance is therefore 0.2mm. The resolution is R0 = 1/c0 = 5 lp/mm Some people feel that the eye can sense finer details.
The resolving power of the eye is approximatively inversely proportional to the viewing distance d. A common practice is that a print should be viewed from a distance approximately equal to the diagonal measurement of the print. The rationale is that the eye would then be at the center of projection if the image was taken with a normal lens (whose focal is equal to the diagonal measurement of the negative), resulting in a correct perspective. Personally I am not fond of this rule. After viewing the image as a whole, I always like to come closer to see the details. It is in order to preserve those details, even in extreme enlargements, that you use a large format camera in the first place !
The enlargement factor is the ratio of the linear dimension of a feature on the print by its corresponding feature on the negative. If the print and the negative don't have the same aspect ratio, it is not the ratio of the dimensions of the print and the negative.
Lets illustrate the formula c = c0/m * d/d0 by a few examples. We assume c0 = 0.2 (average eye resolution), and d/d0 = 1 (print viewed at the minimal distance). The formula becomes c = 0.2/m
To make a full-format 6x8 (150mm x 200mm) from a 35mm negative (24mm x 36mm), you match the two smaller dimensions, so the magnification is m = 150/24 = 6.25, and the acceptable circle of confusion on the negative is c= 0.2 * 1/6.25 = 0.032mm. This value appears to be used by most of the 35mm lens manufacturers on their depth of field scale. The diagonal of a 150mm x 200mm (6x8inch) print is 250mm (10inch), which corresponds to a normal minimal viewing distance.
To make a full-frame 8x10 (200mm x 250mm) from a 35mm negative (24mm x 36mm), you match the two larger dimensions, so the magnification is m = 250/36 = 7, and the acceptable circle of confusion on the negative is c = 0.2 * 1/7 = 0.028mm. This indicates the limitation of the depth of field scales commonly used: even a 8x10 looked closely won't appear critically sharp. To make the same print from a 4x5 (100mm x 125mm) negative, the magnification is 250/125 = 2, and the acceptable circle of confusion on the negative is 0.2 * 1/2 = 0.1mm. This value is often used for LF depth of field tables, but personally I don't find it adequate.
In summary, the acceptable circle of confusion on the negative depends on a number of factors, and it is better to determine the one which is best for you, rather than rely on the manufacturer's which is often not critical enough.
Calculations (see references) show that for small magnifications, the relation between the focus spread D and the diameter of the circle of confusion c is extremely simple, and gives you the admissible f-number:
N = D/(2c)where N is the f-stop number, regardless of the focal length or format used. Once you have determined what is an acceptable circle of confusion for you, this formula gives you the f-stop, proportional to the focus spread. As an example, here are the tabulated values that I would use, based on c=0.1 for 5x7. This gives a critically sharp 11x14 at minimum viewing distance, and has the advantage of being easy to remember. I've also included in the table the equivalent for 4x5 based on c=0.066, and 8x10 based on c=0.133 Distances are in mm.
focus spread admissible 4x5 5x7 8x10 fstop D (mm) N 1.4 2.2 2.8 11 2.1 3.2 4.2 16 3.0 4.5 6.0 22 4.2 6.4 8.4 32 6.0 9.0 12.0 45 8.5 12.8 17.0 64
The focus spread is sometimes refered to as depth of focus, the acceptable distance between imaging planes for a given circle of confusion and f-stop D = 2cN.
In the previous formula N is the effective f-number. For close-ups, you would replace the f-stop by the effective f-stop, and use instead the relation:
N = f/v * D/(2c) = 1/(1+M) * D/(2c)where f is the focal and v your total belows extension. M is the magnification. Since the ratio f/v is always smaller than 1, by using the previous formula, you always end up stopping down more than necessary. Note that at infinity, the ratio is exactly 1.
I think this approach is most useful for judging whether within the constraints dictated by the shutter speeds that you can use, you can get your subjects sufficiently in focus. For instance, you are trying to get a field of flowers in focus at the same time as a tree behind. You measure a focus spread of 10mm between the closest flower and the tree. In 5x7, you'd need to stop down at 45. Is the resulting shutter speed acceptable, given the small breeze ? If yes, you just go ahead and take the picture. If no, you might want to change the composition so that the closest flower would be a bit further.
As a general approach (ie independently from the constraints), the drawback of this approach is that it relies on the choice of an acceptable circle of confusion, which in turn depends on a number of factors, including the dimensions and display of the final print. Since you don't necessarily know what you'd like to do with your negative in the future, why don't you just use a very tight acceptable circle of confusion and stop down more ? The next two sections answer this from an optical point of view.
Strictly speaking, diffraction is a function of aperture size or the physical size of the hole and that is how it would be defined in a physics textbook. Which means that the larger area aperture in a 300mm lens at f/16 (as compared to a 50mm lens at f/16) should provide lower diffraction. However, diffraction patterns are angular patterns and as such are dependent on how far from the aperture you place the screen used to view it also. In photography, the aperture is at the optical center of the lens and the screen is (for infinity focus) one focal length away. The physical size of the diffraction blur is then the focal length divided by the apparent size of the aperture i.e., the definition of the f stop. Thus, in photography, diffraction is only a function of f stop and not a function of the focal length. In simpler terms, the larger aperture of the 300mm lens does offer lesser diffraction at the diaphragm (i.e., less bending around the diaphragm) but since the light now has a longer distance to travel (as compared to the 50mm lens), the smaller bending still results in a fair bit of blur at the viewing screen. N Dhananjay
The image of a point light source (such as a star) after diffraction appears not as a point, but as a central circular spot surrounded by a series of dark and bright rings. See references for details and formulas. Because a point source is imaged as a disk rather than a point, it will appear blured, and this limits the maximum resolution of the lens. The formula R = 1500/N explaned below, gives the maximum resolution of the lens as a function of the f-number N.
The central spot size due to diffraction, called the Airy disk, has a diameter of d = 2.44 x lambda x N. Note that this formula depends on the f-stop and not on the physical aperture of the lens. For a wavelength near the middle of the visible, lambda = 550 x 10 exp(-9) meters , d = 1.34 x 10 exp(-6) x N meters, or d = N / 750 if d is in mm. No lens can make a spot smaller than that value. 86% of the power is in the Airy disk, so it can be viewed as the image of the point. However unlike in the case of defocus, the brightness within the central diffraction spot is not constant, but it decreases from the center to its border, where it reaches 0, resulting in a dark ring. If we use the Rayleigh's criterion that two points are resolved when the dark ring of one coincides with the center of the Airy disk of the other, the corresponding resolution is R = 2/d.
fstop resolution limit N R (lp/mm) d (mm) 11 136 .014 16 93 .021 22 68 .029 32 46 .042 45 33 .059 64 23 .085These values correspond to the "diffraction limit" of resolution, the maximum resolution which could be achieved on perfect film by a perfect lens. Don't expect a real lens to deliver 136 lp/mm at f11.
As it can be seen from these values, stopping down the lens beyond a certain point degrades considerably the resolution. However, this is more of a concern to small camera users than to large format users who don't need a large enlargement ratio. At f22, the diffraction spot equals the acceptable circle of confusion for 35mm. At f64, it barely equals the acceptable circle of confusion for 4x5. There is still plenty of sharpness left, and these values indicate that you shouldn't be too worried about stopping down a lot if necessary. Some folks on the East Coast thought that that Ansel Adams f64 Group was lame and started a f180 Group.
An aggravation to note is that the fstop N is the effective aperture. Therefore, if you are working at 1:1, your f-number would be doubled (two f-stops), and the resulting resolution would be divided by two. Add to that the fact that you need to stop down a lot a close distances to get enough depth of field, and you see why there are not many folks doing macro work with LF
Although the more rigorous way to combine both effects is the use the MTF (see references), a good approximation is to use the root mean square error of the two diameters. The total circle of confusion is:
ct = sqrt( (D/(2N))^2 + (N/750)^2 )This quantity is mimimal when N = sqrt(375 D). For such a f-number, the diameter of the defocus circle of confusion is exactly equal to the diameter of the diffraction spot: D/(2N) = N/750.
This choice of f-stop is optimal, in the sense that it will yield the sharpess possible image at the depth of field limits. However, the larger your focus spread, the less sharp it will be. Sometimes you want to know whether it results in enough resolution for the enlargements you want to make. The resulting total circle of confusion has a diameter:
ct = sqrt(2)/750 N = N/530 = .0365 sqrt(D)If you have predetermined a value for the acceptable circle of confusion ct, this formula gives you the maximum focus spread and f-stop that you can use:
D = 750 ct^2 N = 530 ctLet suppose that you are assuming average eye resolution and minimal viewing distance, then ct = 2 * 0.2/m, where m is the enlargement factor. This gives you the following values:
m D(mm) N 2 30 106 3 13 70 4 7.5 53 5 4.8 42 6 3.3 35
The defocus and the diffraction result in two different light patterns, which in turn lead to two different definitions of resolution. Remember that in the defocus case, brightness in the circle is uniform, and two points are considered resolved when their circle of confusion do not overlap, resulting in a resolution R = 1/c, while in the diffraction case, brightness is more concentrated at the center. If one accepts the technical definition that two points are resolved using the Rayleigh's criterion, this would result in the resolution R = 2/d. For this reason, Bob Wheeler advocated combining the circle of confusion with the central half of the diffraction spot, ie using N/1500 instead of N/750, resulting in the optimum f-number: N = sqrt(750 D). In practice, this would mean using the next f-stop in the table below (ie for D=1.3mm, you'd use f32 instead of f22), which would imply stopping down even more.
However, Paul Hansma suggests that from a photographic point of view, the Rayleigh criterion is not really enough. The brightness between the two "resolved" objects is very close to the peak brightness, so we would not call them resolved if that is what we saw in a photo. To have a level of resolution comparable to that obtained with the circle of confusion, where there is no overlap, would call for having no overlap of the two diffraction spots. This would explain why N/750 fits his experimental results very well.
focus optimal resolution resolution maximum enlargment spread fstop at DOF limits for in-focus based on DOF limits D (mm) N ct(mm) R(lp/mm) d (mm) R(lp/mm) m .3 11 .021 95 .014 136 19 .7 16 .030 65 .021 93 13 1.3 22 .042 47 .029 68 9 2.7 32 .061 32 .042 46 6.4 5.4 45 .085 23 .059 33 4.6 11.0 64 .122 16 .085 23 3.2Here are tabulated values by whole millimeters focus spread. I give the f-stop is given in decimal values ("F"), followed by actual f-number ("N"). Now what does "decimal value" mean ? It is what you would read on a meter graduated in 1/10th of fstops, like many hand-held meters. For instance, "decimal" 22.33 means 22 and one third of a stop (0.33), "decimal" 22.5 means 22 and a half stop (0.5), whereas in f-numbers this would be respectively 25.4 and 26.9 which certainly speaks less to me. On my camera, I have stuck only the decimal values.
D(mm) F N 1 16.6 19.4 2 22.6 27.4 3 32.2 33.5 4 32.6 38.7 5 32.9 43.3 6 45.2 47.4 7 45.4 51.2 8 45.6 54.8 9 45.8 58.1 10 64 61.2The fstop given on these tables is optimal in the sense that it is the choice which yields the sharpest results at the DOF limits among all the other possible f-stops. Remark that this table implies that you have to stop down a lot ! This assumes that other considerations (wind, reciprocity...) do not prevent you from doing so, in which case you'd have to compromise. By compromising, I mean you would use an f-stop other than the optimal value. Then by applying the admissible f-stop above, you would see if that non optimal f-stop gives you a result which is acceptable, although you know now that it would not be the best possible. In general, calculations show that results pretty close to the optimal one are obtained within 1 fstop of the optimal value.
The previous calculations were done at zero magnification. As before, or close-ups, you would replace the f-stop by the effective f-stop.
Because of various optical aberrations, lenses are not perfect. However, stopping down enough corrects those aberrations pretty well in modern lenses, well enough that they can be considered diffraction limited at f22 and smaller apertures.
The final resolution r_final that you get on film depends not only on the aerial resolution of the lens r_lens but also on the resolution of the film r_film. However, when r_lens becomes critical, the effect of r_film becomes quite neglectible. In LF, since you have to stop down so much, this is almost always the case.
Several sources use the formula 1/r_final = 1/r_lens + 1/r_film to compute the final resolution. This formula is an approximation to the exact calculation consisting of the convolution of the response of the film and the response of the lens. This approximation is most valid when both the film and lens are being used near their resolution limits (spatial frequencies with very low contrast). This corresponds roughly to f-stops up to f16. Thus the formula is pretty good for 35mm and MF work. However, when the frequencies involved are nowhere near the film limits, the formula is a poor approximation which predits a worse 1/r_final than what you actual get. For f-stops of f32 and higher, what you get on film is in fact practically equal to the aerial resolution, and the formula shouldn't be used in that case.
Some people think that instead of using all that math, you should just rely on inspecting the ground glass. You would watch it through a lupe as you stop down, and see when the out of focus areas become sharp enough. For several years I have relied on this approach. I eventually found, when I switched to a higher power lupe for evaluating the transparency on the light box, that this yielded results less sharp than I wanted. The problem is that it is not that easy to make a good judgement of sharpness on the ground glass. The image is grainy, and when you stop down, it gets pretty dim, especially through a lupe in the corners of a wide-angle view.
Material on diffraction includes the Melles Griot catalog, and David Jacobson's lens tutorial. In the latter reference, defocus and diffraction are combined using the MTF. The resulting on-film resolution values were calculated by Bob Atkins. Using the formulas in this article, for c=0.035, at f32, D= 2 * 0.035 * 32 = 2.24, ct = .0365 * sqrt(2.24) = .054, which gives the resolution R = 2/.054 = 37 lp/mm, which is in the ballpark of Bob Atkins calculation of 43.5 lp/mm. Note that his data at f32 supports the observation that at high f-numbers, on-film resolution is pretty close to aerial resolution.
The idea of combining the effects of diffraction and defocus to find the optimal f-stop was introduced in the article View camera focussing in practice, page 1, page 2, page 3, page 4 (gif files, reproduced with the author's permission) by Paul Hansma in Phototechniques March/April 96. Most of the ideas developed in this page are from this article. Later, Bob Wheeler, in his Notes on view camera geometry, section 9.3, advocated combining the radius of the diffraction spot N/1500 with the circle of confusion, rather than the diameter N/750. His own data support this argument, which is theoretically sound. However Paul Hansma's experiments seem to have been conducted more carefully.
Struan Gray suggests this r.p.e.l-f usenet thread for a discussion of system resolution (ie combining lens resolution and film resolution).