The magnification \( m \) of a mirror is calculated using the formula: \[ m = - \frac{v}{u} \] In this formula:
\( v \) represents the image distance,
\( u \) represents the object distance.
For a real and enlarged image, the image distance \( v \) is positive, and the object distance \( u \) is negative. The condition that the image precisely touches the pencil implies that the sum of the image and object distances equals the focal length. Consequently: \[ v + u = f \] Additionally, the relationship between the focal length \( f \), object distance \( u \), and image distance \( v \) for a mirror is defined by the mirror equation: \[ \frac{1}{f} = \frac{1}{v} + \frac{1}{u} \] These two equations can be used to determine the magnification produced by the mirror.
Two charges \( +q \) and \( -q \) are placed at points \( A \) and \( B \) respectively which are at a distance \( 2L \) apart. \( C \) is the midpoint of \( AB \). The work done in moving a charge \( +Q \) along the semicircle CSD (\( W_1 \)) and along the line CBD (\( W_2 \)) are 
Find work done in bringing charge q = 3nC from infinity to point A as shown in the figure : 