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39 Cards in this Set

  • Front
  • Back

Hue

The colour of light relating to it's wavelength

Luminousity

The perceived 'brightness' of a colour relating to the intensity of it's retinal stimulus

Saturation

Variation in depth of hue by mixing/diluting with white light

Limits of the visible spectrum

760nm to 390nm

Red in light spectrum

760-622

Green in light spectrum

577-492

Blue in light spectrum

492-455

Mirrors - centre of curvature

The centre of a sphere from which a mirror has been cut.

Mirrors - principal focus

The axial point where paraxial rays intersect or appear to intersect.

Mirrors - pole/vertex

The point at which the surface of the mirror intersects with the principal axis.

Mirrors - principal axis

The line joining the pole/vertex, principal focus and centre of curvature.

Mirrors - radius of curvature

The distance measured from the mirrors surface to the centre of curvature.

Mirrors - focal length

Measured from the mirror surface to the principal focus and is always 1/2 of the radius of curvature.

Velocity

Speed of travel in a given direction.

Wavelength

The distance between corresponding points on successive waves.

Frequency

The number of complete waves generated per second.

Amplitude

Maximum value of the wave.

The normal

A virtual line drawn perpendicular to the surface at the point of incidence.

Incident ray

The ray of light which strikes the reflecting/ refracting surface.

Reflected ray

The ray of light leaving the surface after being reflected.

Angle of incidence

The angle measured from the normal to the incident ray.

Angle of reflection

The angle measured from the normal to the reflected ray.

Angle of deviation

The angle between the original ray path at the surface and the ray leaving the surface.

Laws of reflection

1. The incident ray and the reflected ray lie in one plane which is perpendicular to the surface at the point of incidence.



2. The angle of reflection is equal to the angle of incidence.

Deviation formula mirrors

d = 180 - 2i

Nature of light formula

Velocity = frequency x wavelength

Angle of refraction

The angle measured from the normal to the refracted ray.

Laws of refraction

1. The ratio of the sine of the angle of incidence to the sine of the angle of refraction is a constant equal to the refractive index. Sin I ÷ sin i' = n



2. The incident ray and the refracted ray all lie in one plane which is perpendicular to the surface at the point of incidence.



n sin I = n' sin i'



i' = sin -1 (n sin I ÷ n')

Horizontal displacement in a parallel sided glass block

h = (t × tan i1) - (t x tan i1')

Lateral displacement in a parallel sided glass block

S = t sin ( i1' - i1') ÷ cos i1'

Critical angle formula

ic = sin -1 (n'÷n)

Regular (specular) reflection vs irregular (diffuse) reflection

Regular


Occurs at an optically plane surface


Occurs in a single definite direction


Laws of reflection apply


An observer would see a reflection of your source/object



Irregular


Occurs at non polished surfaces


Irregularities in the surface ace as separate plane reflectors


Reflections scattered in all directions


Allows an object to be seen from all directions

Optics prism definition

A transparent body bound by two inclined plane surfaces which intersect a straight line called the apex

Prisms Principal section definition

A 2D section through the prism perpendicular to the refracting faces.

Prisms refracting faces definition

The inclined polished faces of the prism which meet at the apex

Prisms apical angle definition

The angle contained in the principal section of the prism at the apex, between the two refracting faces and opposite to the base.

Vergence definition

Vergence (dioptres) at any position along a pencil of light is the reciprocal of the distance from that position (usually the surface of the lens) to a source (object) or focus (image)



Formula vergence = 1000 x n ÷ little L (distance in mm)

Definition wavefront

Wavefronts demonstrate the light radiating OUT from the source. It can be seen in a diagram that the wavefronts become flatter as they progress further from the source

Paraxial equations

n÷l = L


n' - n÷ r = F


n' ÷ l' = L'