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Electromagnetic Waves Physics 202 Professor Lee Carkner Lecture 21 PAL #20 EM Radiation Acceleration of lightsail craft F = ma = prA a = prA/m pr = 2I/c I = Ps/4pr2 = (3.9X1026)/(4p(1.5X1011)2) = 1379 W pr = (2)(1379)/(3X108) = 9.2X10-6 N/m2 a = (9.2X10-6)(2.25X108)/5000 = 0.41 m/s2 Time to get to moon d = ½at2 t = (2d/a)½ = [(2)(3.8X108)/(0.41)] ½ t = 43054 sec ~ 12 hours Problems Sunlight only pushes in one direction How do you stop or go back? Gravity and inherited motion also important Consider a dust grain near a star. If the grain is perfectly balanced between light pressure out and gravity in, what happens to the grain if the mass doubles (but the size stays the same)? A) Goes in B) Goes out C) Stays put Consider a dust grain near a star. If the grain is perfectly balanced between light pressure out and gravity in, what happens to the grain if the mass doubles and the surface area doubles? A) Goes in B) Goes out C) Stays put Consider a dust grain near a star. If the grain is perfectly balanced between light pressure out and gravity in, what happens to the grain if the distance from the star doubles? A) Goes in B) Goes out C) Stays put Polarization   The plane containing the E vectors is called the plane of oscillation   Most light sources are unpolarized  Any given wave has a random plane of oscillation Polaroid   Polaroid is a sheet of material that will only pass through the components of the E vectors in a certain direction   If you put a horizontal Polaroid sheet on top of a vertical Polaroid sheet no light gets through Polarization and Intensity  The sum of all of the y components should be equal to the sum of all of the z components  I = ½ I0 This is true only when the incident light is completed unpolarized What about polarized light hitting Polaroid? Incident Polarized Light  For polarized light incident on a sheet of Polaroid, the resultant intensity depends on the angle q between the original direction of polarization and the sheet  E = E0 cos q  I = I0 cos2 q   For unpolarized light that pass through two polarizing sheets, q is the angle between the two sheets Multiple Sheets Sheet Angles Means of Polarization  This alignment permits only the components in that direction to pass  The dust grains are partially aligned by the galactic magnetic field and so the light is partially polarized Light can also be polarized by reflection Reflection and Refraction When light passes from one medium to another (e.g. from air to water) it will generally experience both reflection and refraction  Refraction is the bending of the portion of the light that does penetrate the surface Geometry   Angles  Angle of incidence (q1): the angle between the incident ray and the normal  Angle of reflection (q1’):  Angle of refraction (q2): the angle of the refracted ray and the normal Laws  Law of Reflection   Law of Refraction  n2 sin q2 = n1 sin q1  Where n1 and n2 are the indices of refraction of the mediums involved Index of Refraction Every material has an index of refraction that determines its optical properties   n is always greater than or equal to 1 Large n means more bending General Cases  n2 = n1   q2 = q1  e.g. air to air  n2 > n1   q2 < q1  e.g. air to glass  n2 < n1   q2 > q1  e.g. glass to air Total Internal Reflection  Consider the case where q2 = 90 degrees   For angles greater than 90 there is no refraction and the light is completely reflected  n1 sin qc = n2 sin 90 qc = sin-1 (n2/n1)  This is the case of total internal reflection, where no light escapes the first medium Chromatic Dispersion   In general, n is larger for shorter wavelengths   Incident white light is spread out into its constituent colors  Chromatic dispersion with raindrops causes rainbows Chromatic Dispersion Polarization By Reflection  Light reflected off of a surface is generally polarized   When unpolarized light hits a horizontal surface the reflected light is partially polarized in the horizontal direction and the refracted light is partially polarized in the vertical direction Brewster Angle  At qB the reflected and refracted rays are perpendicular to each other, so qB + qr = 90  qB = tan-1 (n2/n1) If we start out in air n1 = 1 so: qB = tan-1 n  Next Time Read: 34.1-34.6 Homework: Ch 33, P: 37, Ch 34, P: 7, 9, 10, 11, 12, 13, 15