The total deviation of a light ray refracted through a prism can be calculated, given the incidence angle . The same calculation allows for determination of the emergence angle .

fig4.gif
Deviation Diagram for a Prism

We have:
=+
A=+
=>A+=(+)+(+)
=>A+=+
=>=+-A (1)
sin()/sin()=n=>=arcsin{n*sin()}
=A-
=>=arcsin{n*sin(A-)} (2)
=arcsin{sin()/n}, because sin()/sin()=n again,
so (2)=>=arcsin{n*sin[A-arcsin(sin()/n)]} (3)
Now sin[A-arcsin(sin()/n)]=sin(A)*cos(arcsin(sin()/n))-cos(A)*sin()/n
So =arcsin{n*sin(A)*cos(arcsin(sin()/n))-cos(A)*sin()}
=arcsin{n*sin(A)*sqrt[1-(sin()/n)2]-cos(A)*sin()}
=>=arcsin{sin(A)*sqrt[n2-sin2()]-cos(A)*sin()} (4)

And finally:
(1)(4)=>

deviation.gif(5)

(5) gives the deviation angle , as a function of , n and A.

Here's a graph of the above equation, with A=60, nD=1.72803 (SF10 Crystal) and ranging from 45 to 80. Angles are measured in degrees on the graph. Note that the deviation has a minimum, close to 60. This fact can also be experimentally demonstrated using the angle readers of a spectroscope or numerically simulated (as in reference [2]).

deviationgraph.gif
Deviation Angle as a Function of Incidence Angle


The above calculation gives the deviation for an arbitrary angle . When the incidence angle and the emergence angle are the same, the prism is said to be in the position of minimum deviation, for a given wavelength. Because light gets dispersed into many wavelengths, this position can occur for a particular wavelength only. Below are the calculations that lead to the fundamental formula for prisms in the position of minimum deviation:

fig5.gif
Minimum Deviation Diagram for a Prism

For the position of minimum deviation, the ray travels perpendicular to the bisect of angle A, and incidence and emergence angles are equal. Then:
= and = (6)
Also: A=+, min=(-)+(-) (7)
(7)(6)=>A=2*, min=2*-2* or
=A/2 and min/2=-A/2 => =min/2+A/2 (8)
Now we know that n=sin()/sin() so from the last equation and (8) we get:

mindeviation.gif(9)

For nD=1.72803 and A=60, expression (9) gives min=59.54084145, which is exactly the minimum displayed on the graph above.

The actual proof that the angle min given by (9) is in fact the minimum of (5) is very complicated (it can be found in [3], page 81). It can be proved using calculus, that if is a root of the equation: d/d=0, with given by (5), then (A,n,)=2*arcin(n*sin(A/2))-A=min. A proof using Maple 9 commands, is provided courtesy of Robert Israel. After you execute the commands, try to understand why this is a perfectly valid proof.

> epsilon:=(A,n,alpha)->alpha+arcsin(sin(A)*sqrt(n^2-sin(alpha)^2)-cos(A)* sin(alpha))-A;
> S:= solve(diff(epsilon(A,n,alpha),alpha),alpha);
> S5:= simplify(S[5]) assuming n > 1, A > 0, A < Pi/2;#solutions are not ordered in Maple. May need to change S[5]->some other S[n] here.
> Q:=sqrt((1-cos(epsilon(A,n,S5)+A))/2) - n*sqrt((1-cos(A))/2);
> Q:= simplify(expand(Q)) assuming n>1,A > 0,A < Pi/2;
> simplify(combine(Q)) assuming A > 0,A < Pi/2,n > 1;

Because the light dispersion angle is very small, (on the order of 7) practically all the rays suffer minimum deviation. When a prism spectroscope is designed, its prism is placed in that position for usually the yellow part of the spectrum (sodium D lines). The Phasmatron spectroscope's prisms are placed in minimum deviation position for the green line of =5615.97363281A, its resonating wavelength.

References

  1. K.D. Alexopoulos, General Physics: Optics, 1st Edition, Athens 1966 (in Greek).
  2. M.A. Peterson's Simulation Displaying the Minimum Deviation for a Prism
  3. C.J. Smith, A Degree Physics Part III: Optics, Indian Edition 1985, Radha Publishing House.