Reflection and Refraction of Light

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Reflection and Refraction of Light Physics 102 28 March 2002 Lecture 6 28 Mar 2002 Physics 102 Lecture 6 1

Light waves and light rays Last time we showed: Time varying B fields E fields B fields to create a selfsustaining, propagating electromagnetic wave EM waves are transverse, and travel at the speed of light in fact, light is a form of electromagnetic radiation We can think of light as a wave or as a particle. When the wavelength is much smaller than the optics, we use rays next week we consider wave aspects and later, particle aspects. 28 Mar 2002 Physics 102 Lecture 6 2

Reflection of light When light reflects from a surface: angle of incidence = angle of reflection θ inc θ ref The image formed in a plane mirror is upright, the same size as the object, and at the same distance behind the mirror as the object is in front. The image is a virtual image, as the light rays don t pass through it. 28 Mar 2002 Physics 102 Lecture 6 3

What is wrong with this? Manet s The Bar at the Folies Bergeres 28 Mar 2002 Physics 102 Lecture 6 4

Does Venus see herself in the mirror? Venus and Cupid by A. No, she sees us Diego Velasquez B. Yes, she sees herself C. Can t tell with the above picture. 28 Mar 2002 Physics 102 Lecture 6 5

Spherical mirrors This past week you found that the image and object distances are related to the focal length by: 1 d o + 1 d i 1 = f with magnification: m For Concave Mirrors: 1 2 3 d = d i o d o d i Position Type Magnification Object at 1 Real Inverted & Smaller Object at 2 Real Inverted & Larger Object at 3 Virtual Upright & Larger (makeup mirror) 28 Mar 2002 Physics 102 Lecture 6 6

You are in WAWAs to buy health food. You can t find any and so scan the store by looking in the security mirror. The mirror and image are: A. Concave and Real B. Concave and Virtual C. Convex and Real D. Flat and Virtual E. Convex and Virtual 28 Mar 2002 Physics 102 Lecture 6 7

For a convex mirror, the image is always virtual, upright, and smaller. Object Image How should we think of the diverging rays? 28 Mar 2002 Physics 102 Lecture 6 8

Index of refraction and Snell s Law Light travels slower in a material than in a vacuum but the frequency of light remains the same. The velocity ratio is the index of refraction : n=c/v. Generally, n>1, but n is often very close to 1 (for air, n=1.0003). When light travels from one medium to another part is reflected and part is refracted with direction given by Snell s Law: n1 sin θ1 = n2 sin θ2 (NB: light bends towards normal in denser medium) 28 Mar 2002 Physics 102 Lecture 6 9

A. a greater depth than it really is. B. the same depth. C. a smaller depth than it really is. 28 Mar 2002 Physics 102 Lecture 6 10

28 Mar 2002 Physics 102 Lecture 6 11

Total internal reflection Going from a more optically dense medium (e.g., water) to a less dense medium (e.g., air), the refraction angle is 90 at the critical angle of incidence. The critical angle is n sinθ = n sinθ 1 c 2 2 sinθ c = n c n 2 1 = 1 / 1. 333 θ = 48. 7 0 For incident angles greater than the critical angle, total internal reflection takes place. 28 Mar 2002 Physics 102 Lecture 6 12

Brewster s Angle Light can be polarized on reflection from a surface Light is partially polarized parallel to the surface (e.g., horizontally when reflecting off a lake) The polarization is 100% when the incident angle is the Brewster angle tanθ B = n n 2 1 1.56 = 1 θ = B 57 0 n = 1 1 n = 156. 2 θ B 28 Mar 2002 Physics 102 Lecture 6 13

Brewster s Angle Demo: Geometry 28 Mar 2002 Physics 102 Lecture 6 14

Prisms and the dispersion of light The index of refraction typically depends slightly on λ (normally higher for shorter wavelength light). Recall: going into an optically denser medium, light is refracted towards the normal. Shorter wavelengths (violet, blue) are thus refracted more than longer wavelengths (red, orange). Picture copyright 1994 by Encyclopedia Britannica Prism Rainbow 28 Mar 2002 Physics 102 Lecture 6 15

Lenses Light incident on a lens is refracted at entry and exit. Converging lenses focus parallel rays through a real focal point. Diverging lenses focus rays through a virtual focus point. converging lens (f is positive) diverging lens (f is negative) 28 Mar 2002 Physics 102 Lecture 6 16

Image formation with lenses Just as for mirrors, RAY TRACE with three magic lines to locate the image. Thin lens equation: 1 1 1 + = do di f Signs: f positive for a converging lens, negative for diverging one d o is positive for a real object, negative for a virtual one d i is positive for a real image, negative for a virtual one m d = d i o Note: blue line is through center of lens, not center of curvature! Note: d i is positive when on the right (unlike for mirrors). 28 Mar 2002 Physics 102 Lecture 6 17

The lens in an overhead projector forms an image P of a point P on an overhead transparency. If the screen is moved closer to the projector, the lens must be: A. moved up B. left where it is C. moved down to keep the image in focus. 28 Mar 2002 Physics 102 Lecture 6 18

A lens is used to image an object onto a screen. If the right half of the lens is covered, A. the left half of the image disappears. B. the right half of the image disappears. C. the entire image disappears. D. the image becomes fuzzy. E. the image becomes faint. 28 Mar 2002 Physics 102 Lecture 6 19

The magnifying glass The closest an object can be and still be focused by the eye is the near point at roughly 25 cm. Closer objects appear larger (angular size ~h/d radians), so they have maximum apparent size at the near point. If the eye is held near a converging lens, and an object is brought within the focal distance (~10 cm), a large virtual image is formed. Virtual image retina The virtual image from the first optic is the object for the eye s lens 28 Mar 2002 Physics 102 Lecture 6 20

The microscope Systems of lenses can be combined. Tiny object 28 Mar 2002 Physics 102 Lecture 6 21

Two converging lenses, or mirrors, can be used to form a telescope. Telescopes First lens (aperture) is large. It collects lots of light from an object and concentrates it into a smaller area, making the object appear brighter. 28 Mar 2002 Physics 102 Lecture 6 22

PUZZLER Theresa took a spring break sailing cruise in the sunny Caribbean. Her group spent the night on an isolated beach but unfortunately left Theresa there sleeping while they returned to the ship. When she awoke, she grabbed her glasses to scan the horizon for her friends. Not finding them, she decided to start a fire to send smoke signals. Could she use her glasses to start the fire? 28 Mar 2002 Physics 102 Lecture 6 23