All right, so let's move on to number four. Four is a polarizer question and it says, an ideal polarizer with its transmission axis rotated to 30 degrees relative to the vertical is placed in a beam of unpolarized light of intensity ten watts per square meter, after passing through the polarizer, what is the intensity of the beam? So, unpolarized light is like sunlight, and now we're going to send that sunlight through a polarizer. So remember we were drawing our polarizers like circles, with an arrow to indicate the transmission axis, and it says that it is 30 degrees relative to the vertical. They want to know how much is coming through the other side. So, if this is the intensity of the sunlight coming in, we want to know I on the other side of this polarizer. So how should I approach this problem? Somebody give me a thought. Eudora I see you hiding back there, what should I do for this problem? >> (student speaking) You can use malus's law. >> Okay, we can maybe use malus's law. All right, what is malus's law? Let's talk about malus's law for a second. Malus law says the intensity coming out is I naught cosine squared of theta. Okay, and when we talked about this in class we drew the following picture. We said, oh here's our sunlight, there is some intensity of the sunlight coming in, I'm gonna put my first polarizer up and that means there is I naught coming through that polarizer and I'm gonna draw the second polarizer at an angle-theta, and if I want to know how much is coming through, then Malus's law holds. I equals I naught cosine squared theta. Okay, this is the one that we did in class, but that looks a little different than this, doesn't it Eudoria? Because here we only have one polarizer whereas in malus's law, we drew it with two polarizers. So what's the purpose of that first polarizer in this picture? What's the purpose of this polarizer? >> (student speaking) To direct, or let through, one direction of like -- Exactly, to only let through vertical polarization, okay. That's not what this arrow is indicating so let's draw with a dashed line, this is the continuation of the beam, right? It keeps going through and if I think about the polarization that came through after this first polarizer, it's vertical, that's what that arrow represents. Okay, and that's what we called I naught, and now when you go through the second polarizer -- how much goes through the second polarizer, it is I naught times cosine squared of theta. But, how much of I sun gets through the first polarizer to I naught? Do you remember what we did in class? There's some factor that I need to include here. Is it all of I sun that came through, or is it some fraction of I sun that came through? Well, I sun is unpolarized. Okay, it has a polarization like this, going up and down, but it also has a polarization like this, going into and out of the board. This guy only picks out one of those. It picks out the vertical, it eliminates the horizontal, so what factor should I put here? >> (student speaking) one half. 1/2, it's gonna pick out half of the light, right? Since this is vertical, that's half of the light, the other one horizontal gets extinguished at that first polarizer. Alright, so that looks pretty close to this except our polarizer is not vertical anymore, right? It's off at this angle 30 degrees, and so the question is does that matter at all? If I hold up a polarizer and I look at the Sun, which you should never do of course, because it's a little bright, even if you cut it down with a polarizer it's still very bright, but let's say you do that, let's say you look up at the Sun with your polarizer -- with your polarized sunglasses, and now you turn your head sideways. Does the Sun get any dimmer? No, it doesn't, because it is unpolarized. Okay, it doesn't have any particular polarization, it has a combination of vertical and horizontal and you can combine those to make everything in between. So this is in fact exactly the same as this. Okay, because if I rotated my Sun by 30 degrees, it's gonna look exactly the same as this problem over here. So what's the intensity? It's Isun over 2. And they told us what Isun was, it was 10 watts per square meter, so we are just going to divide that by 2 and we get 5 watts per square meter.
Table of contents
- 0. Math Review31m
- 1. Intro to Physics Units1h 24m
- 2. 1D Motion / Kinematics3h 56m
- Vectors, Scalars, & Displacement13m
- Average Velocity32m
- Intro to Acceleration7m
- Position-Time Graphs & Velocity26m
- Conceptual Problems with Position-Time Graphs22m
- Velocity-Time Graphs & Acceleration5m
- Calculating Displacement from Velocity-Time Graphs15m
- Conceptual Problems with Velocity-Time Graphs10m
- Calculating Change in Velocity from Acceleration-Time Graphs10m
- Graphing Position, Velocity, and Acceleration Graphs11m
- Kinematics Equations37m
- Vertical Motion and Free Fall19m
- Catch/Overtake Problems23m
- 3. Vectors2h 43m
- Review of Vectors vs. Scalars1m
- Introduction to Vectors7m
- Adding Vectors Graphically22m
- Vector Composition & Decomposition11m
- Adding Vectors by Components13m
- Trig Review24m
- Unit Vectors15m
- Introduction to Dot Product (Scalar Product)12m
- Calculating Dot Product Using Components12m
- Intro to Cross Product (Vector Product)23m
- Calculating Cross Product Using Components17m
- 4. 2D Kinematics1h 42m
- 5. Projectile Motion3h 6m
- 6. Intro to Forces (Dynamics)3h 22m
- 7. Friction, Inclines, Systems2h 44m
- 8. Centripetal Forces & Gravitation7h 26m
- Uniform Circular Motion7m
- Period and Frequency in Uniform Circular Motion20m
- Centripetal Forces15m
- Vertical Centripetal Forces10m
- Flat Curves9m
- Banked Curves10m
- Newton's Law of Gravity30m
- Gravitational Forces in 2D25m
- Acceleration Due to Gravity13m
- Satellite Motion: Intro5m
- Satellite Motion: Speed & Period35m
- Geosynchronous Orbits15m
- Overview of Kepler's Laws5m
- Kepler's First Law11m
- Kepler's Third Law16m
- Kepler's Third Law for Elliptical Orbits15m
- Gravitational Potential Energy21m
- Gravitational Potential Energy for Systems of Masses17m
- Escape Velocity21m
- Energy of Circular Orbits23m
- Energy of Elliptical Orbits36m
- Black Holes16m
- Gravitational Force Inside the Earth13m
- Mass Distribution with Calculus45m
- 9. Work & Energy1h 59m
- 10. Conservation of Energy2h 54m
- Intro to Energy Types3m
- Gravitational Potential Energy10m
- Intro to Conservation of Energy32m
- Energy with Non-Conservative Forces20m
- Springs & Elastic Potential Energy19m
- Solving Projectile Motion Using Energy13m
- Motion Along Curved Paths4m
- Rollercoaster Problems13m
- Pendulum Problems13m
- Energy in Connected Objects (Systems)24m
- Force & Potential Energy18m
- 11. Momentum & Impulse3h 40m
- Intro to Momentum11m
- Intro to Impulse14m
- Impulse with Variable Forces12m
- Intro to Conservation of Momentum17m
- Push-Away Problems19m
- Types of Collisions4m
- Completely Inelastic Collisions28m
- Adding Mass to a Moving System8m
- Collisions & Motion (Momentum & Energy)26m
- Ballistic Pendulum14m
- Collisions with Springs13m
- Elastic Collisions24m
- How to Identify the Type of Collision9m
- Intro to Center of Mass15m
- 12. Rotational Kinematics2h 59m
- 13. Rotational Inertia & Energy7h 4m
- More Conservation of Energy Problems54m
- Conservation of Energy in Rolling Motion45m
- Parallel Axis Theorem13m
- Intro to Moment of Inertia28m
- Moment of Inertia via Integration18m
- Moment of Inertia of Systems23m
- Moment of Inertia & Mass Distribution10m
- Intro to Rotational Kinetic Energy16m
- Energy of Rolling Motion18m
- Types of Motion & Energy24m
- Conservation of Energy with Rotation35m
- Torque with Kinematic Equations56m
- Rotational Dynamics with Two Motions50m
- Rotational Dynamics of Rolling Motion27m
- 14. Torque & Rotational Dynamics2h 5m
- 15. Rotational Equilibrium3h 39m
- 16. Angular Momentum3h 6m
- Opening/Closing Arms on Rotating Stool18m
- Conservation of Angular Momentum46m
- Angular Momentum & Newton's Second Law10m
- Intro to Angular Collisions15m
- Jumping Into/Out of Moving Disc23m
- Spinning on String of Variable Length20m
- Angular Collisions with Linear Motion8m
- Intro to Angular Momentum15m
- Angular Momentum of a Point Mass21m
- Angular Momentum of Objects in Linear Motion7m
- 17. Periodic Motion2h 9m
- 18. Waves & Sound3h 40m
- Intro to Waves11m
- Velocity of Transverse Waves21m
- Velocity of Longitudinal Waves11m
- Wave Functions31m
- Phase Constant14m
- Average Power of Waves on Strings10m
- Wave Intensity19m
- Sound Intensity13m
- Wave Interference8m
- Superposition of Wave Functions3m
- Standing Waves30m
- Standing Wave Functions14m
- Standing Sound Waves12m
- Beats8m
- The Doppler Effect7m
- 19. Fluid Mechanics2h 27m
- 20. Heat and Temperature3h 7m
- Temperature16m
- Linear Thermal Expansion14m
- Volume Thermal Expansion14m
- Moles and Avogadro's Number14m
- Specific Heat & Temperature Changes12m
- Latent Heat & Phase Changes16m
- Intro to Calorimetry21m
- Calorimetry with Temperature and Phase Changes15m
- Advanced Calorimetry: Equilibrium Temperature with Phase Changes9m
- Phase Diagrams, Triple Points and Critical Points6m
- Heat Transfer44m
- 21. Kinetic Theory of Ideal Gases1h 50m
- 22. The First Law of Thermodynamics1h 26m
- 23. The Second Law of Thermodynamics3h 11m
- 24. Electric Force & Field; Gauss' Law3h 42m
- 25. Electric Potential1h 51m
- 26. Capacitors & Dielectrics2h 2m
- 27. Resistors & DC Circuits3h 8m
- 28. Magnetic Fields and Forces2h 23m
- 29. Sources of Magnetic Field2h 30m
- Magnetic Field Produced by Moving Charges10m
- Magnetic Field Produced by Straight Currents27m
- Magnetic Force Between Parallel Currents12m
- Magnetic Force Between Two Moving Charges9m
- Magnetic Field Produced by Loops andSolenoids42m
- Toroidal Solenoids aka Toroids12m
- Biot-Savart Law (Calculus)18m
- Ampere's Law (Calculus)17m
- 30. Induction and Inductance3h 37m
- 31. Alternating Current2h 37m
- Alternating Voltages and Currents18m
- RMS Current and Voltage9m
- Phasors20m
- Resistors in AC Circuits9m
- Phasors for Resistors7m
- Capacitors in AC Circuits16m
- Phasors for Capacitors8m
- Inductors in AC Circuits13m
- Phasors for Inductors7m
- Impedance in AC Circuits18m
- Series LRC Circuits11m
- Resonance in Series LRC Circuits10m
- Power in AC Circuits5m
- 32. Electromagnetic Waves2h 14m
- 33. Geometric Optics2h 57m
- 34. Wave Optics1h 15m
- 35. Special Relativity2h 10m
32. Electromagnetic Waves
Polarization & Polarization Filters
Video duration:
6mPlay a video:
Related Videos
Related Practice