Feb 16, 2011

1. Feb 16, 2011 Finish Polarization The Radiation Spectrum HW & Questions

2. LCD Displays

3. Bees can see polarized light  polarization of blue sky enables them to navigate Humans: Haidinger’s Brush Vikings: Iceland Spar?

4. Many invertebrates can see polarization, e.g. the Octopus Not to navigate (they don’t go far) Perhaps they can see transparent jellyfish better? unpolarized polarized

5. Polarization and Stress Tests In a transparent object, each wavelength of light is polarized by a different angle. Passing unpolarized light through a polarizer, then the object, then another polarizer results in a colorful pattern which changes as one of the polarizers is turned.

8. CD cover seen in polarized light from monitor

9. 3D movies Polarization is also used in the entertainment industry to produce and show 3-D movies. Three-dimensional movies are actually two movies being shown at the same time through two projectors. The two movies are filmed from two slightly different camera locations. Each individual movie is then projected from different sides of the audience onto a metal screen. The movies are projected through a polarizing filter. The polarizing filter used for the projector on the left may have its polarization axis aligned horizontally while the polarizing filter used for the projector on the right would have its polarization axis aligned vertically. Consequently, there are two slightly different movies being projected onto a screen. Each movie is cast by light which is polarized with an orientation perpendicular to the other movie. The audience then wears glasses which have two Polaroid filters. Each filter has a different polarization axis - one is horizontal and the other is vertical. The result of this arrangement of projectors and filters is that the left eye sees the movie which is projected from the right projector while the right eye sees the movie which is projected from the left projector. This gives the viewer a perception of depth.

10. Stokes Parameters:

11. Linear Polarized:

12. Linear Polarized:

13. Linear Polarized (45 deg):

14. Linear Polarized (- 45 degrees):

15. Left-hand Circular:

16. Right-hand Circular:

17. Unpolarized:

18. The Radiation Spectrum Rybicki & Lightman, Section 2.3 Consider Transverse E-field What is the spectrum? Energy / time as a function of frequency Note: Radians / sec Define the Fourier Transform of

19. Eqn. 1 The inverse is Eqn. 2 Take complex conjugate of Eqn. (1):

20. So…. and

21. But since We have So eqn. (b) eqn. (a) Also Now From Eqn. (a), (b) So…

22. Parseval’s Theorem for Fourier Transforms: Proof:

24. Poynting Theorem: Energy /time/area Integrate over pulse: So…

25. Electromagnetic Potentials Rybicki & Lightman, Chapter 3

26. Electromagnetic Potentials Instead of worrying about E and B, we can use the scalar and vector potentials Simpler: 1 scalar and 1 vector quantity instead of 2 vector quantities. Relativistic treatment is simpler.

27. (1) So Therefore, there exists a φ such that (2) or

28. Equations (1) & (2) already satisfy 2 of Maxwell’s Equations – what about the others? becomes For reasons which will become clear in a minute, we re-write this last equation as (3)

29. The 4th Maxwell equation becomes Since we get (4)

30. GUAGE TRANSFORMATIONS (1)-(4) do not determine A and φ uniquely: one can add the gradient of an arbitrary scalar ψ to A and leave B unchanged Likewise E will be unchanged if you add These are called GUAGE TRANSFORMATIONS

31. For the LORENTZ GUAGE we take so that (3) and (4) simplify to (5) (6)

32. RETARDED POTENTIALS It turns out that the solutions to (5) and (6) can be expressed as integrals over sources of charge, provided you properly take into account the fact that changes in the E and B fields can move no faster than the speed of light.

33. RETARDED POTENTIALS At point r =(x,y,z), integrate over charges at positions r’ (7) (8) where [ρ] evaluate ρ at retarded time: Similar for [j]