When a light ray hits the surface of a transparent medium at an angle, the ray is bent at the point of incidence as it crosses into the different medium. This change in the path of the light is known as refraction. A common example of
refraction
can be observed when a pencil is placed in a glass of water. The part of the pencil inside the water seems to be bent in relation to the part out of the water.
The extent and direction of
refraction
of light depends on the angle of incidence. A ray of light passing through a pane of glass will bend once, towards a line perpendicular to the plane of the glass at the point of incidence, and again as it emerges from the glass, this time being deflected away from the perpendicular . If both sides of the pane of glass are parallel, the angle of
refraction
will be the same at either side of the pane of glass, so that the ray will emerge parallel to the original ray but at a certain distance.
The extent of
refraction
also depends on the
optical density
of the medium. Different mediums cause different changes in direction - the extent of deflection of light in air, water or glass is different. Optical density effects the speed at which the light travels through the medium. The higher the optical density, the slower the light speed. In a vacuum, and at a good approximation in air, light travels at about 300,000 km per second, whereas in glass or water it travels more slowly - 200,000 km per second in glass and 225,000 km per second in water.
The
optical density
of transparent mediums is expressed by its Index of Refraction. The denser the medium is, the higher its
refractive index
will be. The lowest
refractive index
is 1, used for air or a vacuum, where light travels fastest. Glass has an approximate
refractive index
of 1.5 (depending on the type of glass) and water of 1.33 .
These principles are applied in lenses, which can converge or refract the light at a particular angle, depending on the curvature of the lens.
When the surface of incidence and the surface of emergence of a transparent medium such as glass are not parallel, a ray of light passing through the medium will emerge at an angle which is not identical to the angle of incidence .
The laws of
refraction
are employed when designing lenses for theatre luminaires. When a ray of light passes through a curved surface, it will bend away from the perpendicular at the point of exit . The curvature of the
lens
is calculated precisely in order to bend the rays of light in the desired direction, creating a focused and directional
beam
of light . The lenses of theatre luminaires use plane, convex, or concave surfaces in order to create different patterns of light beams.
The degree of deflection, and thus the "bending power" of a lens, depends on the following factors:
The angle of incidence of the light.
The curvature of the
lens
face. The more curved it is, the more it bends the light.
The index of
refraction
of the material from which the
lens
is made.
The
wavelength
of the light ray. Short waves (blue-violet) are deflected more than longer waves(red).
As the light emerges from the prism it bands way from the perpendicular to the surface, those enlarging the angle.
The prism refracts the different
wavelength
comprising
white light
at difrent angle, so that we see each color of the
spectrum
separately
Lenses of Theatrical Luminaires
All
lens
luminaires used in theatre have converging lenses. The larger the diameter of the lens, the more light it will collect, enhancing its optical efficiency. A
lens
is made of transparent material, usually glass or plastic, and is used to collect and focus light. There are two basic types of lenses: converging lenses and diverging lenses.
Converging lenses have convex surfaces and are thick at the center and thin at the edges. They collect the rays of light to a real focal point. When a
beam
of light hits a converging lens, it concentrates the light rays.
Diverging lenses have concave surfaces and are thin at the center and thick at the edges, causing the light to spread out.
When a light
beam
passes through converging lenses, the
lens
concentrates the rays of light.
When a light
beam
passes through a diverging lens, the
lens
spreads the rays of light.
When a parallel light
beam
passes through a converging lens, the rays will converge, meeting at a point called the focal point. The distance between the center of the
lens
and its focal point is called the focal length . Since light may be cast at a
lens
from either direction, the optical length can be measured from either side . The focal length is measured in inches or in centimeters. The focal length of a converging
lens
can be found by casting a parallel
beam
of light along the
optical axis
of the lens . Remember how to make a fire with spectacles or a magnifying glass when you went camping and forgot the matches?
The performance of lenses of theatrical luminaires is described by two parameters: focal length and
lens
diameter. The focal length is determined by the ability of the
lens
to concentrate the light, and the
lens
diameter determines the amount of light the
lens
will be able to collect. For example, a popular profile-spot
lens
is called 6x9. This means that the
lens
has a diameter of six inches and a focal length nine inches .
When a point
light source
is placed on the
optical axis
at the focal point of the
lens
, the emerging light
beam
will be parallel. When the source is moved towards the
lens
, the light will converge further. When the source is moved away from the
lens
, the light will spread out.
Owing to the difference in convergence of different light waves,chromatic
aberration
is caused which results in a ring of
rainbow
colors round the edge of the
beam
of light, particularly when sharply focused. This can be rectified by combining two different types of glass in the same lens. This type of high quality color corrected lenses is used in sophisticated lighting equipment such as scenic projectors and intelligent luminaires.
All
lens
luminaires used in theatre have converging lenses. The larger the diameter of the lens, the more light it will collect, making it more efficient . The most commonly used
lens
in theatrical luminaires is the PC (plano convex), which has one plane surface and one concave surface, calculated to converge
the light at the desired angle. As it is difficult to manufacture thick and heavy lenses, plano-convex lenses rarely exceed 240mm in diameter. Originally the lenses of PC luminaires were produced by hand polishing. In recent years, moulded lenses have become available. The plane side of these lenses, called pebble-convex or prism-convex lens, is often roughened with little bubbles in order to slightly blur the margins of the
beam
.
PC lenses with a large diameter and a prominent curvature, which could theoretically have been very efficient both in collecting the light and in bending it, are not used in the theatre. A large, thick glass
lens
is extremely heavy and would absorb a lot of heat which causes the glass to crack. For these reasons, the lenses of theatrical luminaire lenses are usually quite thin. When a more
efficient
lens
is required, with a shorter focal length and more efficient light collection, two solutions are employed:
1) compound lens
2) a fresnel lens.
A
compound lens
consists of two or more thin PC lenses, each contributing its bending power to the optical performance of the
lens
compound.
Fresnel lenses were originally invented for use in lighthouses in 1819 by the Frenchman August Fresnel.
Fresnel
designed a thin converging
lens
by stepping back the curvature on the concave side of a plano convex lens, in ringlike steps, thus eliminating the extra thick glass at the center of the lens.
Fresnel
ground each segment to optical precision and mounted them together in brass holders. In the early 1930 moulded fresnel
lens
were adopted in the theatre.