![Apparent Depth of a Liquid:
Rarer (a)
Denser (b)
O
O’
N
μb
hr
ha
i
r
r
i
sin i
bμa =
sin r
sin r
aμb =
sin i
or
hr
aμb =
ha
=
Real depth
Apparent depth
Apparent Depth of a Number of
Immiscible Liquids:
ha = ∑ hi / μi
i = 1
n
Apparent Shift:
Apparent shift = hr - ha = hr – (hr / μ)
= hr [ 1 - 1/μ]
TIPS:
1. If the observer is in rarer medium and the object is in denser medium then
ha < hr. (To a bird, the fish appears to be nearer than actual depth.)
2. If the observer is in denser medium and the object is in rarer medium then
ha > hr. (To a fish, the bird appears to be farther than actual height.)
μa](https://image.slidesharecdn.com/1rayoptics1-201006102804/85/ray-optics-class-12-ppt-slideshare-6-320.jpg)
ray optics class 12 ppt slideshare
- 1. RAY OPTICS - I 1. Refraction of Light 2. Laws of Refraction 3. Principle of Reversibility of Light 4. Refraction through a Parallel Slab 5. Refraction through a Compound Slab 6. Apparent Depth of a Liquid 7. Total Internal Reflection 8. Refraction at Spherical Surfaces - Introduction 9. Assumptions and Sign Conventions 10.Refraction at Convex and Concave Surfaces 11.Lens Maker’s Formula 12.First and Second Principal Focus 13.Thin Lens Equation (Gaussian Form) 14.Linear Magnification
- 2. Refraction of Light: Refraction is the phenomenon of change in the path of light as it travels from one medium to another (when the ray of light is incident obliquely). It can also be defined as the phenomenon of change in speed of light from one medium to another. Rarer Rarer Denser N N r i r i Laws of Refraction: I Law: The incident ray, the normal to the refracting surface at the point of incidence and the refracted ray all lie in the same plane. II Law: For a given pair of media and for light of a given wavelength, the ratio of the sine of the angle of incidence to the sine of the angle of refraction is a constant. (Snell’s Law) μ = sin i sin r (The constant μ is called refractive index of the medium, i is the angle of incidence and r is the angle of refraction.) μ
- 3. TIPS: 1. μ of optically rarer medium is lower and that of a denser medium is higher. 2. μ of denser medium w.r.t. rarer medium is more than 1 and that of rarer medium w.r.t. denser medium is less than 1. (μair = μvacuum = 1) 3. In refraction, the velocity and wavelength of light change. 4. In refraction, the frequency and phase of light do not change. 5. aμm = ca / cm and aμm = λa / λm Principle of Reversibility of Light: Rarer (a) N r i Denser (b) sin i aμb = sin r sin r bμa = sin i aμb x bμa = 1 or aμb = 1 / bμa If a ray of light, after suffering any number of reflections and/or refractions has its path reversed at any stage, it travels back to the source along the same path in the opposite direction. A natural consequence of the principle of reversibility is that the image and object positions can be interchanged. These positions are called conjugate positions. μ
- 4. Refraction through a Parallel Slab: Rarer (a) Rarer (a) Denser (b) N N r1 i1 i2 r2 M t δ y sin i1 aμb = sin r1 sin i2 bμa = sin r2 But aμb x bμa = 1 sin i1 sin r1 sin i2 sin r2 x = 1 It implies that i1 = r2 and i2 = r1 since i1 ≠ r1 and i2 ≠ r2. Lateral Shift: t sin δ y = cos r1 t sin(i1- r1) y = cos r1 or Special Case: If i1 is very small, then r1 is also very small. i.e. sin(i1 – r1) = i1 – r1 and cos r1 = 1 y = t (i1 – r1) or y = t i1(1 – 1 /aμb) μ
- 5. Refraction through a Compound Slab: Rarer (a) Rarer (a) Denser (b) N N μb r1 i1 r1 r2 r2 i1 Denser (c) μc N sin i1 aμb = sin r1 sin r1 bμc = sin r2 aμb x bμc x cμa = 1 sin r2 cμa = sin i1 aμb x bμc = aμcor bμc = aμc / aμbor μa μc > μb
- 6. Apparent Depth of a Liquid: Rarer (a) Denser (b) O O’ N μb hr ha i r r i sin i bμa = sin r sin r aμb = sin i or hr aμb = ha = Real depth Apparent depth Apparent Depth of a Number of Immiscible Liquids: ha = ∑ hi / μi i = 1 n Apparent Shift: Apparent shift = hr - ha = hr – (hr / μ) = hr [ 1 - 1/μ] TIPS: 1. If the observer is in rarer medium and the object is in denser medium then ha < hr. (To a bird, the fish appears to be nearer than actual depth.) 2. If the observer is in denser medium and the object is in rarer medium then ha > hr. (To a fish, the bird appears to be farther than actual height.) μa
- 7. Total Internal Reflection: Total Internal Reflection (TIR) is the phenomenon of complete reflection of light back into the same medium for angles of incidence greater than the critical angle of that medium. N N N N O r = 90° ic i > ic i Rarer (air) Denser (glass) μg μa Conditions for TIR: 1. The incident ray must be in optically denser medium. 2. The angle of incidence in the denser medium must be greater than the critical angle for the pair of media in contact.
- 8. Relation between Critical Angle and Refractive Index: Critical angle is the angle of incidence in the denser medium for which the angle of refraction in the rarer medium is 90°. sin i gμa = sin r sin ic = sin 90° = sin ic or 1 aμg = gμa 1 aμg = sin ic or 1 sin ic = aμg λg sin ic = λa Also Red colour has maximum value of critical angle and Violet colour has minimum value of critical angle since, 1 sin ic = aμg = 1 a + (b/ λ2) Applications of T I R: 1. Mirage formation 2. Looming 3. Totally reflecting Prisms 4. Optical Fibres 5. Sparkling of Diamonds
- 9. Spherical Refracting Surfaces: A spherical refracting surface is a part of a sphere of refracting material. A refracting surface which is convex towards the rarer medium is called convex refracting surface. A refracting surface which is concave towards the rarer medium is called concave refracting surface. •• C CP P R R A B AB APCB – Principal Axis C – Centre of Curvature P – Pole R – Radius of Curvature •• Denser MediumDenser Medium Rarer MediumRarer Medium
- 10. Assumptions: 1. Object is the point object lying on the principal axis. 2. The incident and the refracted rays make small angles with the principal axis. 3. The aperture (diameter of the curved surface) is small. New Cartesian Sign Conventions: 1. The incident ray is taken from left to right. 2. All the distances are measured from the pole of the refracting surface. 3. The distances measured along the direction of the incident ray are taken positive and against the incident ray are taken negative. 4. The vertical distances measured from principal axis in the upward direction are taken positive and in the downward direction are taken negative.
- 11. Refraction at Convex Surface: (From Rarer Medium to Denser Medium - Real Image) •CP RO • Denser MediumRarer Medium • • IM μ2μ1 α βγ i r i = α + γ γ = r + β or r = γ - β A tan α = MA MO tan β = MA MI tan γ = MA MC or α = MA MO or β = MA MI or γ = MA MC According to Snell’s law, μ2sin i sin r μ1 = or i r μ1 = μ2 or μ1 i = μ2 r Substituting for i, r, α, β and γ, replacing M by P and rearranging, μ1 PO μ2 PI μ2 - μ1 PC + = Applying sign conventions with values, PO = - u, PI = + v and PC = + R vu μ1 - u μ2 v μ2 - μ1 R + = N
- 12. Refraction at Convex Surface: (From Rarer Medium to Denser Medium - Virtual Image) μ1 - u μ2 v μ2 - μ1 R + = Refraction at Concave Surface: (From Rarer Medium to Denser Medium - Virtual Image) μ1 - u μ2 v μ2 - μ1 R + = • CP R • Denser MediumRarer Medium • • I M μ2μ1 αβ γ i r A v uO N O • C PR • Denser MediumRarer Medium • I M μ2μ1 α β γ r A v u • i N
- 13. Refraction at Convex Surface: (From Denser Medium to Rarer Medium - Real Image) •C P RO • Denser Medium Rarer Medium • • IM μ2 μ1 α βγ r A vu N iμ2 - u μ1 v μ1 - μ2 R + = Refraction at Convex Surface: (From Denser Medium to Rarer Medium - Virtual Image) μ2 - u μ1 v μ1 - μ2 R + = Refraction at Concave Surface: (From Denser Medium to Rarer Medium - Virtual Image) μ2 - u μ1 v μ1 - μ2 R + =
- 14. Note: 1. Expression for ‘object in rarer medium’ is same for whether it is real or virtual image or convex or concave surface. 2. Expression for ‘object in denser medium’ is same for whether it is real or virtual image or convex or concave surface. 3. However the values of u, v, R, etc. must be taken with proper sign conventions while solving the numerical problems. 4. The refractive indices μ1 and μ2 get interchanged in the expressions. μ1 - u μ2 v μ2 - μ1 R + = μ2 - u μ1 v μ1 - μ2 R + =
- 15. Lens Maker’s Formula: R1 P1 • O • μ2 μ1 i A vu N1 R2 C1 • • I1 N2 L C N P2 • C2 • I • μ1 For refraction at LP1N, μ1 CO μ2 CI1 μ2 - μ1 CC1 + = (as if the image is formed in the denser medium) For refraction at LP2N, (as if the object is in the denser medium and the image is formed in the rarer medium) μ2 -CI1 μ1 CI -(μ1 - μ2) CC2 + = Combining the refractions at both the surfaces, μ1 CO (μ2 - μ1)( CC1 + = 1μ1 CI CC2 + ) 1 Substituting the values with sign conventions, 1 - u (μ2 - μ1) R1 + = 11 v R2 - ) 1 ( μ1
- 16. Since μ2 / μ1 = μ 1 - u μ2 R1 + = 11 v R2 - ) 1 ( μ1 - 1)( or 1 - u (μ – 1) R1 + = 11 v R2 - ) 1 ( When the object is kept at infinity, the image is formed at the principal focus. i.e. u = - ∞, v = + f. So, (μ – 1) R1 = 11 f R2 - ) 1 ( This equation is called ‘Lens Maker’s Formula’. Also, from the above equations we get, 1 - u f + = 11 v
- 17. First Principal Focus: First Principal Focus is the point on the principal axis of the lens at which if an object is placed, the image would be formed at infinity. F1 f1 F2 f2 Second Principal Focus: Second Principal Focus is the point on the principal axis of the lens at which the image is formed when the object is kept at infinity. F2 f2 F1 f1
- 18. Thin Lens Formula (Gaussian Form of Lens Equation): For Convex Lens: f • R u C A B A’ B’ M Triangles ABC and A’B’C are similar. A’B’ AB = CB’ CB Triangles MCF2 and A’B’F2 are similar. A’B’ MC = B’F2 CF2 v A’B’ AB = B’F2 CF2 or • 2F2 • F2 • F1 • 2F1 CB’ CB = B’F2 CF2 CB’ CB = CB’ - CF2 CF2 According to new Cartesian sign conventions, CB = - u, CB’ = + v and CF2 = + f. 1 v f - = 11 u
- 19. Linear Magnification: Linear magnification produced by a lens is defined as the ratio of the size of the image to the size of the object. m = I O A’B’ AB = CB’ CB + I - O = + v - u According to new Cartesian sign conventions, A’B’ = + I, AB = - O, CB’ = + v and CB = - u. m I O = v u =or Magnification in terms of v and f: m = f - v f Magnification in terms of v and f: m = f f - u Power of a Lens: Power of a lens is its ability to bend a ray of light falling on it and is reciprocal of its focal length. When f is in metre, power is measured in Dioptre (D). P = 1 f End of Ray Optics - I