Skip to main content

sign convention rules and image formation by a single curved surface

 

SIGN CONVENTION RULES FOR LENSES:

1) All distances are measured from the pole (or optic centre).

2) Distances measured along the direction of the incident light ray are taken as positive

3) Distances measured opposite to the direction of the incident light ray are taken as negative

4) The heights measured vertically above from the points on axis are taken as positive.

5) The heights measured vertically down from points on axis are taken as negative.

IMAGE FORMATION BY SINGLE CURVED SURFACE:


IMAGE FORMATION BY SINGLE CURVED SURFACE:

Consider a curved surface separating two media of refractive indices

n1 and n2 . A point object is placed on the principal axis at point

O. The ray, which travels along the principal axis passes through the pole

undeviated. The second ray, which forms an angle α with principal axis,

meets the interface (surface) at A. The angle of incidence is q1. The ray

bends and passes through the second medium along the line AI. The angle

of refraction is q2. The two refracted rays

meet at I and the image is formed there.

Let the angle made by the second

refracted ray with principal axis be g and

the angle between the normal and

principal axis be β.

PO is the object distance which we

denote as ‘u’

PI is image distance which we denote

as ‘v’

PC is radius of curvature which we denote as ‘R’

n1, n2 are refractive indices of two media.

 

In the triangle ACO, q1 = α + β

and in the triangle ACI, β= q2 + g => β g = q2

According to Snell’s law, we know

n1 sin q1 = n2 sin q2

substituting the values of q1 and q2, we get,

n1 sin(α+ β) = n2 sin(β- g) ................. (1)

If the rays move very close to the principal axis, the rays can be treated

as parallel and are called paraxial rays. Then the angles α,β and g become

very small. This approximation is called paraxial approximation.

sin (α+ β) = α+β and sin (β- g) = β- g     [since for very smaller angles sinq=q]

Substituting in equation (1)

n1 (α+ β) = n2 (β- g)

ð  n1α + n1 β = n2 β – n2 g ................(2)

since all angles are small, we can write

tan α = AN/NO = α            [since for very smaller angles tanq=q]

tan β = AN/NC = β

tan g = AN/NI = g

Substitute these in equation (2), we get,

n1  (AN/NO) + n1 (AN/NC) = n2 (AN/NC) – n2 (AN/NI) ............... (3)

As the rays move very close to the principal axis, the point N coincides

with pole of the interface (P). Therefore NI, NO, NC can be replaced by PI, PO and PC respectively.

After substituting these values in equation (3), we get,

n1/PO + n1/PC = n2/PC – n2/PI

n1/PO + n2/PI = (n2- n1) /PC ................(4)

Equation (4) shows the relation between refractive indices of two media, object distance, image distance and radius of curvature.

The above equation is true for the case we considered.

We can generalize equation (4) if we use the following sign convention.

For all purposes of applications of refraction at curved surfaces and through lenses following conventions are used. (recall sign convention rules for lenses)

Here PO is called the object distance (u)

PI is called the image distance (v)

PC is called radius of curvature (R)

According to sign convention mentioned above, we have

PO = -u ; PI = v ; PC = R

Substituting these values in equation (4) we get,

 

(n2/v) – (n1/u) = (n2-n1 ) /R ..........(5)

 

This formula can also be used for plane surfaces. In the case of a plane

surface, radius of curvature (R) approaches infinity. Hence 1/R becomes

zero. Substituting this in equation 5, we get formula for the plane surfaces

n2/v - n1/u = 0 => n2/v = n1/u


                thank you

Comments

Popular posts from this blog

Rules to draw ray diagrams & sign convention rules for spherical mirrors

  RULES TO DRAW RAY DIAGRAMS FOR SPHERICAL MIRRORS                                                                            Rule 1: The ray passing parallel to principal axis, after reflection passes through focus (or appears to be coming from focus in case of convex mirror) Rule 2: The ray passing through Focus (or appears to be passing through focus in case of convex mirror), after reflection becomes parallel to principal axis.                                                        Rule 3: The ray passing through principal axis comes back in the same path after reflection.      ...

prism and refractive index of prism

  PRISM:   A prism is a transparent medium separated from the surrounding medium by at least two plane surfaces which are inclined at a certain angle in such a way that, light incident on one of the plane surfaces emerges from the other plane surface. Consider a triangular glass prism. It contains  two triangular bases and three rectangular plane lateral surfaces. These lateral surfaces are inclined to each other. Let us consider that triangle PQR represents outline of the prism where it rests on its triangular base.       Let us assume that a light ray is incident on  the plane surface PQ of a prism at M as shown in figure. Draw a perpendicular to the surface at M. It becomes a normal to that surface. The angle between the incident ray and normal is called angle of incidence (i 1 ). The ray is refracted at M. It moves through prism and meets the other plane surface at N and finally comes out of the prism. The ray which comes out of the surfa...

Total internal reflection (T.I.R)

  TOTAL INTERNAL REFLECTION: We know that when light enters from denser medium to rarer medium it bends away to the normal.(i<r) What happens when angle of incidence goes on increasing?. Observe the diagram below. So as we increase angle of incidence the refracted ray continue to bend further away from normal and at one particular angle of incidence it grazes through the interface. This angle is known as critical angle. CRITICAL ANGLE: The angle of incidence for which refracted ray grazes through the interface when light is sent from denser to rarer medium is called critical angle. At critical angle,   i=c  and  r=90 0 Let C be the critical angle. Then r becomes 90 0 we get, µ1/µ2 = sin 90/ sin c (applying Snell’s law)   =>   µ 1 /µ 2 = 1/sin c . We get sin c = µ 2 / µ 1 .We know that µ 1 /µ 2 i.e., µ 12 is called refractive index of denser medium with respect to rarer medium sin c = 1/µ 12   What happens when angle of incidence is...