Diffraction II PREFLIGHT

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The following three questions refer to the material you were to read in preparation for the lesson. Questions one and three require you to write a three or four sentence response. Number two is a multiple choice question. Click in the appropriate circle.

You may change your mind as often as you wish. When you are satisfied with your responses, click the SUBMIT button at the bottom of this page. Don't submit more than once. (If you absolutely HAVE to resubmit it, put a note on the end to that effect.)




1. Double Slit Diffraction

Copyright © 1996, 1997 Serge G. Vtorov

In this applet, we are given a "fancier" version of the previous quiz applet, with the added variable of color, or wavelength of light. Using the graph on the right hand side, set the distance so that some even number of bumps or fringes appears (no half bumps.) Record the wavelength and the distance between the slits and the distance to the screen. Now, change the wavelength to some other color, and note how many fringes appear. Adjust the distance between the slits so that the SAME whole number of fringes (no fractions) appears as you started with. Record the new wavelength and new distance between the slits. By dividing (Wave_1 - Wave_2) / (d_1 - d_2), we should be able to figure out the dependence of slit separation and wavelength. Does this agree with the book?




2.


Rayleigh, who is given the credit for explaining why the sky is blue, also suggested that because diffraction blurs any point source, we can't tell if there's two stars or one star unless we can find a "dip" in the intensity between the two stars. So if we use the "single slit" difraction pattern for each star, the dip disappears when the stars are theta < 1.22 lambda/aperture apart, where lambda is the wavelength of light and aperture is the size of the circular lens/mirror/pinhole we are using to take pictures with. It turns out that Rayleigh was wrong, in the sense that modern computers CAN tell that there are two stars there, even when they are closer than that. Which of the following IS NOT an explanation for this?

A circular aperture is "blurrier" than some other shape, like a square.

A computer can fit thousands of possible combinations to the shape, and find the 2-star combination that fits best (Forward modelling).

A computer can invert the data using Fast Fourier Transform to "undo" diffraction (Reverse modelling).

Computers can be more precise than human vision.


3. Single Slit Diffraction

In Problem 1, I asked how the relationship between separation of the double slits and wavelength changed the number or spacing of the diffraction pattern. You can do the same thing with this physlet, though there is a more limited range of fringes available, so pick something in the middle, say 7 fringes and find the relationship between wavelength and slit width. How is this answer different/same as that in problem 1?





honors extra

The youngest person ever to receive a Nobel prize, got it for his work in crystallography. He figured out a way to take pictures of the atoms in a crystal, which may have been the first pictures of atoms. Who was he? And how old was he? Since an atom is on the order of 0.1 nm wide, what wavelength of light would be needed to take a picture of an atom? Remembering the Quiz about the oil immersion microscope, how the greater the magnification the darker the image, how did he get enough light to see an atom?





Below is a space for your thoughts, including general comments about today's assignment (what seemed impossible, what reading didn't make sense, what we should spend class time on, what was "cool", etc.):




You may change your mind as often as you wish. When you are satisfied with your responses, click the SUBMIT button.

I received no help from anyone on this assignment.