In this article we are going to learn about the formula for spherical mirror ,sign convention for concave mirror, sign convention for convex mirror and also the sign convention for spherical lenses.
A spherical refracting surface is the part of a sphere separating two transparent media .There are two types of spherical refracting surfaces.
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The spherical refracting surfaces have such components:
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What is sign convention?
It is a selection of physical significance of signs for a particular quantity.
For sign convention we need to follow some assumptions/write the rules for sign convention:
The refraction through the spherical surface follows the following assumptions
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r=2f
1/v+1/u=1/f
Where v is the image distance, u is the object distance f is the focal length of the lens.
This is also the formula for conjugate foci.
m=-v/u
m is the linear magnification of the lens.
Linear magnification can also be the ratio of the height of the image to the height of the object.
m=I/O
=length or height of the image / length or height of the object
mA=length of the image along the principal axis / length of the object along the principal axis
The spherical mirror longitudinal magnification is equal to the square of the linear magnification.
mA=m2
µ1 = refractive index of medium 1
µ2 = refractive index of medium 2
R = radius of curvature of a spherical surface.
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xy=f2
Where, x = u – f ; y = v – f
Where = refractive index of the material of the lens with respect to the surrounding medium.
r1= radius of curvature of the medium 1 ;
r2 = radius of curvature of the medium 2.
Power can be expressed as:
P=1/f
Here, f is focal length (meters) and D is the unit of power which is measured in dioptre.
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NCERT Physics Notes:
Focal length of a concave mirror is taken as the negative and the focal length of a convex mirror is taken as positive.
The pair of points is such that when an object is placed at one focal point on one side the image will be formed at the other focal point on the other side . These two focal points are called conjugate foci.
The point on the principal axis of the lens through which the rays of light emerge out without deviation after refraction is known as the optical centre of the lens.
If the thickness of a lens is much less than the radius of curvature of two surfaces then that lens is known as a thin lens.
Focal length is the distance between the optical centre and the principal focus of a lens.
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