Lens focal length
The focal length of a lens is normally represented in millimetres and is the basic description of a photographic lens. It is not at all the measurement of the actual length of the lens, but an estimate of the optical distance from where the light rays cover to form a clear image of a subject to the digital sensor or 35mm film at the focal plane in the camera. It is determined when the lens is focused at infinity.
It tells us the angle of the view, how much of the scene will be captured and the magnification. The longer that the focal length is, the more limited the angle of view will be, and the higher the magnification. Which also means that, the shorter the focal length, the wider the angle of view will be, and the lower the magnification.
Zoom lenses
A zoom lens has variable focal lengths. An advantage of a zoom lens is it’s versatility. They are ideal when taking photos of a variety of subjects and reduce the number of times you need to change the lens which can save time and limits the possibility of getting dust in the camera’s mirror box or on the sensor.
macro lenses
These lenses should be able to copy a life-size image of an object on the recording medium. They can offer a magnification factor of 1.0x or 1:1 at it’s closest focus setting. You can get very good enlargements of objects using a macro lens that only offers 0.5x maximum magnification.
- 0.2x: At the bottom of these lenses, some of them only give an image on the sensor that is a fifth of the size, when it is focused as close as possible
- 0.34x: Some lenses do better and produces an image that is one-third of the life-sized object shot at the minimum focus level
- 0.5x: these lenses offer half the size of the image
- 1.0x: produces a life-sized image on the sensor when it is focused as close as possible
- 5.0x: gives a bellows like magnification, giving images on the sensor that are up to five times the size
One feature of macro lenses is that they are “flat field” lenses. As general lenses suffer from field curvature, the point of focus would be a different distance towards the corners of the frame compared to the centre.
Wide angle lenses
A wide angle lens is where the focal length is a lot smaller than the focal length of a normal lens for a given film plane. It allows more of the scene to be included in the image. It is useful in architectural, interior, landscape photography. But, the photographer may not be able to move further from the scene to photograph it. The photographer can also wish to emphasise the difference in size or the distance between objects in the foreground and background. This exaggeration can be used to make the foreground objects more noticeable and impressive whilst capturing expansive backgrounds. They protect a larger image circle than the typical standard for a design lens of the same focal length which enables either large tilt and shift movements with a view camera or a wide field of view. In still photography, a normal lens for a specific format has a focal length that may be equal to the length of the diagonal of the image from or digital photosensor. In cinematography, the lens is normally double the size of the diagonal.
Normal lenses
Normal lenses reproduce a field of view that looks natural to the human observer under normal viewing conditions, as compared to lenses that have either longer or shorter focal lengths that produce an enlarged or developed field of view that distorts the perspective when viewed from a normal viewing distance. Lenses that have a shorter focal length are called wide angle lenses, whilst longer focal length lenses are called long-focus lenses. In still photography, a lens with a focal length that is equal to the size of the film or sensor format is considered to be a normal lens as its angle of view is similar to the angle that is subtended by a large print that is viewed at a typical viewing distance that is equal to the print diagonal. In cinematography, where the image is viewed at a bigger distance, a lens with a focal length of double the film or sensor diagonal is considered normal. The term can also be used as a synonym for a rectilinear lens.
Telephoto lenses
Telephoto lenses are a set type of long focus lenses in which the length of the lens is shorter than the focal length, which is achieved by including a lens group that is known as a telephoto group that makes the light path bigger to create a long focus lens in a smaller design. The angle of view and other effects of long focus lenses are the same specified focal length. Long focal length lenses are often referred to as telephoto lenses even though this is incorrect, a telephoto lens is incorporated in the telephoto group. They are sometimes broken into further subtypes. These are:
- Medium telephoto: lenses that cover between 30 degrees and 10 degrees of the field of view
- super telephoto: lenses that cover between 8 degrees through a 1 degree field of view
Lens structure
Lens structure is the design for use in still or cine cameras that is intended to construct a lens that gives the most acceptable performance of the subject that is being photographed within a range of restrictions that can include cost, weight, and materials. For a lot of other devices, such as telescopes, microscopes and theodolite where the visual image if noticed but often not recorded, the design can can be more straightforward than os the case in a camera where ever image is recorded on film or image sensor and can be subject to detailed inspection at a later stage. Photographic lenses also include those in enlargers and projectors.
Depth of field
The depth of field is also called the focus range or effective focus range. It is the distance between the nearest and furthest objects in scenes that appear very clearly in an image. They can exactly focus on only one distance at a time, but the decrease in sharpness is gradual on each side of the distance, so that within the depth of field, the unsharpness is unnoticeable under normal viewing conditions. It may be desirable to have an entirely sharp image, and a large depth of field is allowed. In other cases, a small depth of field may be more effective, emphasizing the subject whilst de-emphasizing the foreground and background. In cinematography, a large depth of field is called a deep focus, and a small depth of field is often called a shallow focus.
F-numbers
F-numbers are a combination of two terms. F/N is the concept that is used to indicate the size of the diaphragm opening, or the aperture, in a camera. Aperture openings can be measured as fractions of the focal length of a lens. The f, stand for focal length, in the aperture rating. Supposing that we had the definitive example of lenses, the 50mm, with an aperture of f/2.8, we can find out the diameter of the aperture opening like this:
If we open the aperture to maximum, it would be measured at:
The difference between the aperture of f/2.8 and the aperture of f/1.4 is a contrast of four times as much light. This is because the area of aperture opening is four times as big at f/1.4 as it is at f/2.8. A stop in photography nomenclature means that there is a difference of one exposure value, which is the double, or halving of the amount of light that is reaching the sensor. These are standard full stops that f-stops are rated in: 1, 1.4, 2, 2.8, 4, 5.6, 8, 11, 16, 22, 32, 45, 64. Here is an example of an f-number scale:
These settings all differ by one exposure value, or a full stop, and create a full f-stop scale. When we close down the 50mm f/1.4 lens from the maximum aperture of f/1.4 to an aperture of f/2.8, we are stopping down by two full stops. It has to be noted that a lot of cameras offer two additional f-stop scales beyond what is the standard full stop scale:
- A half-stop scale
- A third-stop scale
A lot of cameras default to a fractional scale rather than the full stop scale, this is why it is important to learn and memorize the full stop scale so that proper adjustments are made when changing the aperture setting on the camera.
There is an important relationship between the aperture and the shutter speed, as they are both rated in stops. Whilst the aperture is denoted in f-stops, the shutter speed changes are called stops or exposure values.
Diffraction limits
Diffraction is an effect that limits the resolution of photography. It happens because light starts to spread when passing through a small opening. It is normally insignificant, since smaller apertures often improve the sharpness by minimising lens aberrations. But, this method becomes counterproductive. Knowing this can help maximise the detail, and help avoid long exposures or high iso speeds that are unneeded. Light rays that are passing through a small aperture will begin to separate and obstruct with each other. This can become more important as the size of the aperture decreases relative to the wavelength of the light that is passing through, but it occurs to some extent for any aperture or intense light source. Since divergent rays now travel in different distances, some move out of the phase and begin to interfere with each other. This produces a diffraction pattern with top strengths where the amplitude of the light waves add, and less light where they subtract. If we were to measure the power of light reaching all of the positions on a line, these measurements would appear as bands.
For the ideal circular aperture, the 2-D diffraction pattern is called an airy disk, after it’s discoverer George Airy. The width of it is used to define the theoretical maximum resolution for an optical system. When the width of it’s central peak becomes largely relative to the pixel size in the camera, it will begin to have a visual impact on the image. Once they become any closer than half of their width, they are no longer resolvable.
Diffraction sets a basic resolution limit that is individualistic of the amount of megapixels, or the size of the film format. This depends on the f-number of the lens that is being used, and the wavelength of the light that is being seen. We can think of it as the smallest theoretical pixel of detail in photography. additionally, the beginning of diffraction is slow, prior to limiting the resolution, it can reduce the small-scale contrast by causing the airy disks to partially overlap. The size of the airy disk is practical in the context of the pixel size. As the result of the sensor’s anti-alising filter, the airy disk can have a diameter of 2-3 pixels before the diffraction limits the resolution. But, diffraction may have a visual impact prior to reaching the diameter. For example, a canon EOS 20D begins to show diffraction at f/11, whereas the canon Powershot G6 begins to show the effects at only f/5.6. Furthermore, the canon G6 does not need apertures that are as small as the 20D in order to achieve the same depth of field, due to a much smaller sensor size. Since the size of the disk can also depend on the wavelength of the light, each of the primary colours will reach its diffraction limit at a different aperture. When the lens aperture is at, for example, f/16 and the airy diameter is at 21.3m, it assumes that the light is in the middle of the visible spectrum.
A typical DSLR camera captures light with a wavelength of anywhere between from 450 to 680nm, so at best, the disk would have a diameter of 80%. Another complication is that sensors that utilize a bayer array can allocate twice the fraction of pixels to green as red or blue light, and then introduce these colours to produce the final full colour image. This can mean that as the diffraction limit is near, the first signs will be a loss of resolution in green and pixel-level luminosity. The blue light requires the smallest of apertures in order to reduce it’s resolution due to diffraction.
Only real world photography can show its visual impact. Even when the camera system is near or just past it’s diffraction limit, other factors such as focus accuracy, motion blur and imperfect lenses are more likely to be significant. Therefore, diffraction limits the total sharpness only when using a solid tripod, a mirror lock-up and a very high quality lens. Some diffraction can be good if you are willing to sacrifice sharpness at the focal plane in exchange for sharpness outside of the depth of field. On the other hand, very small aperture can be required to achieve long exposures, such as to induce a motion blur with flowing water. This means that diffraction is something to be aware of when choosing the exposure settings, similar to how we balance the other trade-off’s such as noise vs the shutter speed. This does not mean that larger apertures are better, although very small apertures create a soft image, most lenses are also soft when they are used wide open.
Camera systems have an optimal aperture that is in between the largest and smallest settings and with most lenses the optimal sharpness can be closer to the diffraction limit, but with some lenses this may occur prior to the diffraction limit. These calculations only show when the diffraction becomes significant, not the location of the optimum sharpness. This does not mean that the smaller pixels are worse, as both of the scenarios still have the same total resolution. But, the camera with smaller pixels will render the image with less artefacts. Smaller pixels can also give more creative flexibility, since they can yield a higher resolution when using a larger aperture in possible. Additionally when the other factors like noise and dynamic range are considered, the small vs large pixels debate becomes more complicated.