1 00:00:00,090 --> 00:00:02,490 The following content is provided under a Creative 2 00:00:02,490 --> 00:00:04,059 Commons license. 3 00:00:04,059 --> 00:00:06,330 Your support will help MIT OpenCourseWare 4 00:00:06,330 --> 00:00:10,690 continue to offer high quality educational resources for free. 5 00:00:10,690 --> 00:00:13,320 To make a donation or view additional materials 6 00:00:13,320 --> 00:00:17,270 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:17,270 --> 00:00:20,805 at ocw@mit.edu. 8 00:00:20,805 --> 00:00:24,660 SHAOUL EZEKIEL: Now we're ready to look at Fresnel diffraction. 9 00:00:24,660 --> 00:00:27,120 We're going to look at Fresnel diffraction associated 10 00:00:27,120 --> 00:00:30,150 with a single slit. 11 00:00:30,150 --> 00:00:34,530 And then later, we'll look at Fresnel diffraction associated 12 00:00:34,530 --> 00:00:37,030 with circular apertures. 13 00:00:37,030 --> 00:00:41,840 The setup for observing Fresnel diffraction is here, 14 00:00:41,840 --> 00:00:46,200 is the laser, is the beam from the laser again reflected 15 00:00:46,200 --> 00:00:48,870 by this mirror. 16 00:00:48,870 --> 00:00:52,590 And then we reflect the beam again by this mirror 17 00:00:52,590 --> 00:00:55,140 into this lens. 18 00:00:55,140 --> 00:00:59,130 Now this is a short focal length lens that focuses the light 19 00:00:59,130 --> 00:01:05,330 and passes it through a pinhole over here, which we center it 20 00:01:05,330 --> 00:01:07,950 at the focus spot. 21 00:01:07,950 --> 00:01:10,540 The light coming out from the pinhole 22 00:01:10,540 --> 00:01:14,100 then is shown on the card here and then goes 23 00:01:14,100 --> 00:01:17,820 and falls onto the screen. 24 00:01:17,820 --> 00:01:19,900 So this is the setup. 25 00:01:19,900 --> 00:01:25,360 Now I'm going to bring in the slit. 26 00:01:25,360 --> 00:01:31,590 So I'm going to put this slit in front of the laser beam 27 00:01:31,590 --> 00:01:33,290 without disturbing anything, I hope. 28 00:01:36,920 --> 00:01:41,380 So here is the single slit. 29 00:01:41,380 --> 00:01:43,770 Now I'm going to adjust the spacing 30 00:01:43,770 --> 00:01:49,837 to be very small, so that we start out with the Fraunhofer 31 00:01:49,837 --> 00:01:50,670 diffraction pattern. 32 00:01:50,670 --> 00:01:51,510 Now here it is. 33 00:01:51,510 --> 00:01:55,170 You can see on the screen, we see the Fraunhofer diffraction 34 00:01:55,170 --> 00:02:00,140 pattern because the slit width is small enough, 35 00:02:00,140 --> 00:02:01,980 so that we're in the Fraunhofer region. 36 00:02:05,430 --> 00:02:09,830 Now what I'm going to do is I'm going 37 00:02:09,830 --> 00:02:13,950 to start to widen the slit, so to bring in the Fresnel 38 00:02:13,950 --> 00:02:14,950 diffraction pattern. 39 00:02:14,950 --> 00:02:16,890 So here I am. 40 00:02:16,890 --> 00:02:18,390 I start widening. 41 00:02:18,390 --> 00:02:20,550 And you can see now you have to watch 42 00:02:20,550 --> 00:02:22,450 what happens to the fringes. 43 00:02:22,450 --> 00:02:24,420 Now things are going to get pretty bright. 44 00:02:24,420 --> 00:02:28,230 And so what I'm going to do, I'm going 45 00:02:28,230 --> 00:02:32,580 to introduce another screen that is not so sensitive, so 46 00:02:32,580 --> 00:02:36,030 that we can observe the bright Fresnel pattern on that one. 47 00:02:36,030 --> 00:02:37,780 Here we are. 48 00:02:37,780 --> 00:02:40,680 And you can see, I get a dark line in the middle. 49 00:02:40,680 --> 00:02:43,820 Now we get two. 50 00:02:43,820 --> 00:02:55,250 And others, you can see how the fringes behave in this case. 51 00:02:55,250 --> 00:02:57,720 I want to see what the fringes near the edges 52 00:02:57,720 --> 00:03:00,930 look like and in the center. 53 00:03:07,050 --> 00:03:13,400 Now I know that the effect is not observable 54 00:03:13,400 --> 00:03:15,870 very well under these conditions. 55 00:03:15,870 --> 00:03:21,920 So what I'm going to do is to turn down the room lights 56 00:03:21,920 --> 00:03:26,690 and see if we can improve the visibility of the Fresnel 57 00:03:26,690 --> 00:03:29,900 diffraction pattern. 58 00:03:29,900 --> 00:03:32,990 Now with the room lights dimmed, we're 59 00:03:32,990 --> 00:03:36,440 going to start again with the Fraunhofer diffraction pattern 60 00:03:36,440 --> 00:03:38,010 on the sensitive screen. 61 00:03:38,010 --> 00:03:41,240 So again, you can see that, at present, we 62 00:03:41,240 --> 00:03:45,080 have Fraunhofer diffraction. 63 00:03:45,080 --> 00:03:49,810 And I hope it's a little clearer than with the room lights on. 64 00:03:49,810 --> 00:03:50,310 OK? 65 00:03:50,310 --> 00:03:51,950 So I'm going to start here. 66 00:03:51,950 --> 00:03:56,330 And then as I increase the slit width, 67 00:03:56,330 --> 00:04:00,680 we're going to have a transition to Fresnel diffraction. 68 00:04:00,680 --> 00:04:04,080 But as we know, the brightness is going to get pretty large. 69 00:04:04,080 --> 00:04:09,830 So I will then bring in the other screen here, 70 00:04:09,830 --> 00:04:12,650 so that we're not going to saturate 71 00:04:12,650 --> 00:04:15,500 the camera too much when we observe Fresnel diffraction. 72 00:04:15,500 --> 00:04:16,250 So here we go. 73 00:04:16,250 --> 00:04:17,690 This is Fraunhofer. 74 00:04:17,690 --> 00:04:22,860 Then I will now go make the transition to Fresnel. 75 00:04:22,860 --> 00:04:27,200 And it's very, very interesting how 76 00:04:27,200 --> 00:04:32,420 the light going through the slit solves Maxwell's equations. 77 00:04:32,420 --> 00:04:35,270 And here we are. 78 00:04:35,270 --> 00:04:39,090 We got that dark line in the middle. 79 00:04:39,090 --> 00:04:45,060 And then we have to go back again and have 80 00:04:45,060 --> 00:04:51,920 the two lines, then the three. 81 00:04:51,920 --> 00:04:55,000 Now it's very important to notice 82 00:04:55,000 --> 00:05:01,150 that the contrast is not 100% like it is in the Fraunhofer 83 00:05:01,150 --> 00:05:02,830 diffraction. 84 00:05:02,830 --> 00:05:05,530 And those of you who will do the calculation 85 00:05:05,530 --> 00:05:09,220 will, of course, understand what I'm referring to. 86 00:05:09,220 --> 00:05:11,860 The spacing, you notice that the spacing between the fringes 87 00:05:11,860 --> 00:05:14,410 gets tighter and tighter as you approach 88 00:05:14,410 --> 00:05:20,050 the center or the center between the two slits. 89 00:05:20,050 --> 00:05:24,850 In fact, the fringe spacing gets so fine with large slit 90 00:05:24,850 --> 00:05:30,370 separation that you can't even resolve them by eye. 91 00:05:30,370 --> 00:05:33,770 So there's lot of information in that diffraction pattern. 92 00:05:33,770 --> 00:05:38,100 And I hope that you've adjusted your monitors, 93 00:05:38,100 --> 00:05:42,490 so that you can see these patterns. 94 00:05:42,490 --> 00:05:49,470 So here we are all the way to Fraunhofer. 95 00:05:49,470 --> 00:05:52,110 And there's a little transition, which 96 00:05:52,110 --> 00:06:00,630 is not that easy to calculate, and then go into Fresnel. 97 00:06:04,291 --> 00:06:05,220 Here we are. 98 00:06:05,220 --> 00:06:08,700 Make it larger and larger. 99 00:06:08,700 --> 00:06:14,650 You can even see the fringes in the center. 100 00:06:14,650 --> 00:06:17,280 Now that we've seen Fresnel diffraction associated 101 00:06:17,280 --> 00:06:20,970 with a single slit, now we're ready to look 102 00:06:20,970 --> 00:06:23,970 at Fresnel diffraction associated 103 00:06:23,970 --> 00:06:26,500 with circular apertures.