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**Consider Refraction at Spherical Surfaces:**

Starting point for the development of lens equations Vast majority of quality lenses that are used today have segments containing spherical shapes. The aim is to use refraction at surfaces to simultaneously image a large number of object points which may emit at different wavelengths. Point V (Vertex) (object distance) (image distance) i - Angle of incidence t - Angle of refraction r - Angle of reflection The ray SA emitted from point S will strike the surface at A, refract towards the normal, resulting in the ray AP in the second medium (n2) and strike the point P.

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All rays emerging from point S and striking the surface at the same angle i will be refracted and converge at the same point P. Let’s return to Fermat’s Principal Using the Law of cosines:

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**Note: Si, So, R are all positive variables here**

Note: Si, So, R are all positive variables here. Now, we can let d(OPL)/d = 0 to determine the path of least time. Then the derivative becomes We can express this result in terms of the original variables lo and li:

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However, if the point A on the surface changes, then the new ray will not intercept the optical axis at point P. Assume new small vaules of the radial angle so that cos 1, lo so, and li si. Again, subscripts o and i refer to object and image locations, respectively. This is known as the first-order theory, and involves a paraxial approximation. The field of Gaussian Optics utilizes this approach. Note that we could have also started with Snell’s law: n1sin 1= n2sin2 and used sin .

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**Using spherical (convex) surfaces for imaging and focusing**

Object focus i) Spherical waves from the object focus refracted into plane waves. Suppose that a point at fo is imaged at a point very far away (i.e., si = ). so fo = object focal length ii) Plane waves refracted into spherical waves. Suppose now that plane waves (parallel rays) are incident from a point emitting light from a point very far away (i.e., so = ).

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**Diverging rays revealing a virtual image point using concave spherical surfaces.**

fi < 0 si < 0 Signs of variables are important. Virtual image point Parallel rays impinging on a concave surface. The refracted rays diverge and appear to emanate from the virtual focal point Fi. The image is therefore virtual since rays are diverging from it.

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**A virtual object point resulting from converging rays**

A virtual object point resulting from converging rays. Rays converging from the left strike the concave surface and are refracted such that they are parallel to the optical axis. An object is virtual when the rays converge toward it. so < 0 here.

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The combination of various surfaces of thin lenses will determine the signs of the corresponding spherical radii.

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S (a) (b) (c) As the object distance so is gradually reduced, the conjugate image point P gradually changes from real to virtual. The point P’ indicates the position of the virtual image point that would be observed if we were standing in the glass medium looking towards S.

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**We will use virtual image points to locate conjugate image points.**

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**In the paraxial approximation:**

The 2nd surface “sees” rays coming towards it from the P’ (virtual image point) which becomes the 2nd object point for the 2nd surface. Therefore Thus, at the 2nd surface: (B) Add Equations (A) & (B)

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**Let d 0 (this is the thin lens approximation) and nm 1:**

and is known as the thin-lens equation, or the Lens maker’s formula, in which so1 = so and si2 = si, V1 V2, and d 0. Also note that For a thin lens (c) fi = fo = f and Convex f > 0 Concave f < 0 Also, known as the Gaussian lens formula

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**Location of focal lengths for converging and diverging lenses**

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**If a lens is immersed in a medium**

with Object f 2f Real image 2f f Convex thin lens Simplest example showing symmetry in which so = 2f si = 2f f Object Virtual image 2 3 1 si so Concave, f < 0, image is upright and virtual, |si| < |f|

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**Note that a ray passing through the center is drawn as a straight line.**

Ideal behavior of 2 sets of parallel rays; all sets of parallel rays are focused on one focal plane.

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For case (b) below

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**Tracing a few key rays through a positive and negative lens**

Consider the Newtonian form of the lens equations. S2 yo S1 From the geometry of similar triangles:

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Newtonian Form: xo > 0 if the object is to the left of Fo. xi > 0 if the image is to the right of Fi. The result is that the object and image must be on the opposite sides of their respective focal points. Define Transverse (or Lateral) Magnification:

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**Image forming behavior of a thin positive lens.**

f 2f 2f f

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**MT > 0 Erect image and MT < 0 Inverted image**

MT > 0 Erect image and MT < 0 Inverted image. All real images for a thin lens will be inverted. f 2f Simplest example 2f-2f conjugate imaging gives Define Longitudinal Magnification, ML This implies that a positive dxo corresponds to a negative dxi and vice versa. In other words, a finger pointing toward the lens is imaged pointing away from it as shown on the next slide.

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**The number-2 ray entering the lens parallel to the central axis limits the image height.**

Image orientation for a thin lens: The transverse magnification (MT) is different from the longitudinal magnification (ML).

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(a) The effect of placing a second lens L2 within the focal length of a positive lens L1. (b) when L2 is positive, its presence adds convergence to the bundle of rays. (c) When L2 is negative, it adds divergence to the bundle of rays.

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**Two thin lenses separated by a distance smaller than either focal length.**

Note that d < si1, so that the object for Lens 2 (L2) is virtual. Note the additional convergence caused by L2 so that the final image is closer to the object. The addition of ray 4 enables the final image to be located graphically.

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**Note that d > si1, so that the object for Lens 2 (L2) is real.**

Fig Two thin lenses separated by a distance greater than the sum of their focal lengths. Because the intermediate image is real, you could start with point Pi’ and treat it as if it were a real object point for L2. Therefore, a ray from Pi’ through Fo2 would arrive at P1.

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**For the compound lens system, so1 is the object distance and si2 is the image distance.**

The total transverse magnification (MT) is given by

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For this two lens system, let’s determine the front focal length (ffl) f1 and the back focal length (bfl) f2. Let si2 then this gives so2 f2. so2 = d – si1 = f2 si1 = d – f2 but From the previous slide, we calculated si2. Therefore, if so1 we get, fef = “effective focal length”

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Suppose that we have in general a system of N lenses whose thicknesses are small and each lens is placed in contact with its neighbor. ………N Then, in the thin lens approximation: Fig A positive and negative thin lens combination for a system having a large spacing between the lenses. Parallel rays impinging on the first lens enable the position of the bfl.

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Example A Example B Example A: Two identical converging (convex) lenses have f1 = f2 = +15 cm and separated by d = 6 cm. so1 = 10 cm. Find the position and magnification of the final image. si1 = -30 cm at (O’) which is virtual and erect Then so2 = |si1| + d = 30 cm + 6 cm = 36 cm si2 = i’ = +26 cm at I’ Thus, the image is real and inverted.

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**The magnification is given by**

Thus, an object of height yo1 = 1 cm has an image height of yi2 = -2.17cm Example B: f1= +12 cm, f2 = -32 cm, d = 22 cm An object is placed 18 cm to the left of the first lens (so1 = 18 cm). Find the location and magnification of the final image. si1 = +36 cm in back of the second lens, and thus creates a virtual object for the second lens. so2 = -|36 cm – 22 cm| = -14 cm Image is real and Inverted si2 = i’ = +25 cm; The magnification is given by Thus, if yo1 = 1 cm this gives yi2 = cm

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PHY 102: Lecture 10 10.1 Index of Refraction 10.2 Total Internal Reflection 10.3 Prism and Rainbows 10.4 Lenses 10.5 Formation of Images 10.6 Lens Equations.

PHY 102: Lecture 10 10.1 Index of Refraction 10.2 Total Internal Reflection 10.3 Prism and Rainbows 10.4 Lenses 10.5 Formation of Images 10.6 Lens Equations.

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