Physics > Refraction of Light > 3.0 Apparent shift of an object
Refraction of Light
1.0 Introduction
2.0 Laws of refraction
3.0 Apparent shift of an object
4.0 Thin lenses
4.1 Sign convention
4.2 Some important terms
4.3 Ray tracing
4.4 Image formed by covex lens
4.5 Image formed by concave lens
5.0 Lens makers formula & Other Functions of lens.
5.1 Thin Lens Formula
5.2 Magnification and Power of lens
5.3 Combination of lenses
5.4 Displacement method to find focal length.
5.5 Silvering of lens
6.0 Total internal reflection
7.0 Refraction through prism
8.0 Scattering of light
9.0 Optical instruments
9.1 Spectrometer
9.2 Simple microscope
9.3 Compound microscope
9.4 Astronomical telescope (Refracting type)
9.5 Terrestrial telescope
9.6 Galileo's terrestrial telescope
9.7 Reflecting type telescope
3.1 Shift due to a glass slab
4.2 Some important terms
4.3 Ray tracing
4.4 Image formed by covex lens
4.5 Image formed by concave lens
5.2 Magnification and Power of lens
5.3 Combination of lenses
5.4 Displacement method to find focal length.
5.5 Silvering of lens
9.2 Simple microscope
9.3 Compound microscope
9.4 Astronomical telescope (Refracting type)
9.5 Terrestrial telescope
9.6 Galileo's terrestrial telescope
9.7 Reflecting type telescope
There are two types of shift due to a glass slab.
1. Normal shift
2. Lateral shift
3.1.1 Normal shift
$OA = x$
${I_1}A = \mu x$ (Apparent image due to refraction from the 1st surface)
$$\begin{equation} \begin{aligned} {I_1}B = {I_1}A + AB \\ {I_1}B = \mu x + t \\\end{aligned} \end{equation} $$
$IB = \frac{{{I_1}B}}{\mu }$ (Apparent image due to reflection from the 2nd surface).
$$\begin{equation} \begin{aligned} IB = \left( {\frac{{\mu x + t}}{\mu }} \right) \\ IB = \left( {x + \frac{t}{\mu }} \right) \\\end{aligned} \end{equation} $$
Shift $(OI)$ is given by,
$$\begin{equation} \begin{aligned} OI = (OA + AB) - (BI) \\ OI = (x + t) - \left( {x + \frac{t}{\mu }} \right) \\ OI = t\left[ {1 - \frac{t}{\mu }} \right] \\\end{aligned} \end{equation} $$
3.1.2 Lateral shift
When the medium is same on both sides of a glass slab, then the deviation of the emergent ray is zero. That is the emergent ray is parallel to the incident ray but it does suffer lateral shift or lateral displacement with respect to the incident ray as shown in the figure.
Mathermatically lateral shift is given by, $$d = \left( {1 - \frac{1}{\mu }} \right)ti$$
Derivation of lateral shift
$$AB\cos r = AC$$ or $$AB = \frac{t}{{\cos r}}$$
$$d = AB\sin (i - r)$$ So, $$\begin{equation} \begin{aligned} d = \frac{t}{{\cos r}}\left[ {\sin i\cos r - \cos i\sin r} \right] \\ d = t\left[ {\sin i - \cos i\tan r} \right]\quad ...(i) \\\end{aligned} \end{equation} $$
From Snell's law,
$$\frac{{\sin i}}{{\sin r}} = \mu $$ or $$\sin r = \frac{{\sin i}}{\mu }$$
Therefore, $$\tan r = \frac{{\sin r}}{{\cos r}} = \frac{{\sin r}}{{\sqrt {1 - {{\sin }^2}r} }}$$
$$\tan r = \frac{{\frac{{\sin i}}{\mu }}}{{\sqrt {1 - {{\left( {\frac{{\sin i}}{\mu }} \right)}^2}} }} = \frac{{\sin i}}{{\sqrt {{\mu ^2} - {{\sin }^2}i} }}\quad ...(i)$$
From equation $(i)$ and $(ii)$ we get,
$$d = t\left[ {\sin i - \frac{{\sin i\cos i}}{{\sqrt {{\mu ^2} - {{\sin }^2}i} }}} \right]$$
$$d = \left[ {1 - \frac{{\cos i}}{{\sqrt {{\mu ^2} - {{\sin }^2}i} }}} \right]t\sin i$$
Note:
For $i \to 0$,
$$d = \mathop {\lim }\limits_{i \to 0} \left[ {1 - \frac{{\cos i}}{{\sqrt {{\mu ^2} - {{\sin }^2}i} }}} \right]t\sin i$$
$$d = \left[ {1 - \frac{1}{\mu }} \right]ti$$