1 00:00:00,090 --> 00:00:02,490 The following content is provided under a Creative 2 00:00:02,490 --> 00:00:04,030 Commons license. 3 00:00:04,030 --> 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 --> 00:00:17,260 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:17,260 --> 00:00:18,220 at ocw.mit.edu. 8 00:00:21,176 --> 00:00:22,690 SHAOUL EZEKIEL: Now we're all set 9 00:00:22,690 --> 00:00:26,530 to look at the Fraunhofer diffraction pattern associated 10 00:00:26,530 --> 00:00:29,830 with the two-dimensional multi slits. 11 00:00:29,830 --> 00:00:33,500 The setup, again just to remind you, same as before-- 12 00:00:33,500 --> 00:00:34,990 here's the laser. 13 00:00:34,990 --> 00:00:39,000 Here's the beam from the laser reflected by this mirror 14 00:00:39,000 --> 00:00:42,190 and reflected by this mirror into a lens. 15 00:00:42,190 --> 00:00:45,640 Now, the lens here is used to expand the beam so that we 16 00:00:45,640 --> 00:00:51,580 can illuminate quite a chunk of a two-dimensional multiple 17 00:00:51,580 --> 00:00:52,990 slits. 18 00:00:52,990 --> 00:00:59,780 And then the diffracted light then goes on onto the screen. 19 00:00:59,780 --> 00:01:04,180 Now let's look at the two-dimensional multiple slits. 20 00:01:04,180 --> 00:01:06,700 What we have for you-- 21 00:01:06,700 --> 00:01:10,660 we have two Ronchi rulings. 22 00:01:10,660 --> 00:01:13,888 Each one has so many lines per inch. 23 00:01:13,888 --> 00:01:15,430 I'm not going to tell you because I'm 24 00:01:15,430 --> 00:01:18,890 going to leave that, again, as an exercise. 25 00:01:18,890 --> 00:01:22,870 So we have two identical Ronchi rulings that are crossed. 26 00:01:22,870 --> 00:01:25,970 The first one is fixed, which is over here. 27 00:01:25,970 --> 00:01:29,230 And the second one is attached to a rotation 28 00:01:29,230 --> 00:01:31,960 stage behind the first. 29 00:01:31,960 --> 00:01:35,320 So we can rotate the second Ronchi ruling, 30 00:01:35,320 --> 00:01:38,830 and then we can see what it does to the diffraction pattern. 31 00:01:38,830 --> 00:01:42,430 So now let's look at the screen. 32 00:01:42,430 --> 00:01:46,570 And then as we-- 33 00:01:46,570 --> 00:01:48,820 and as you can see on the screen now, 34 00:01:48,820 --> 00:01:53,110 you see the two-dimensional diffraction pattern 35 00:01:53,110 --> 00:01:56,320 of multiple slits. 36 00:01:56,320 --> 00:02:00,610 You can see that they look different than the single slit. 37 00:02:00,610 --> 00:02:02,280 We have a lot more dots. 38 00:02:02,280 --> 00:02:04,030 And again, as I say, I'm going to leave it 39 00:02:04,030 --> 00:02:06,790 as an exercise for you to figure them all out. 40 00:02:06,790 --> 00:02:08,590 Again, I'd like to draw attention 41 00:02:08,590 --> 00:02:13,850 to the dots around here, to all these cross terms 42 00:02:13,850 --> 00:02:16,190 in this pattern. 43 00:02:16,190 --> 00:02:22,420 So this pattern, then, is associated with the rulings 44 00:02:22,420 --> 00:02:24,160 crossed or orthogonal. 45 00:02:24,160 --> 00:02:26,350 Now what I'm going to do, I'm going 46 00:02:26,350 --> 00:02:33,880 to rotate the Ronchi ruling or the multiple slits 47 00:02:33,880 --> 00:02:35,400 in the back of the fixed one. 48 00:02:35,400 --> 00:02:35,900 See? 49 00:02:35,900 --> 00:02:38,240 So again you can see that the pattern rotates. 50 00:02:38,240 --> 00:02:42,130 Now, if we get rid of the insert and then look 51 00:02:42,130 --> 00:02:45,340 at the entire pattern, now you can 52 00:02:45,340 --> 00:02:54,400 see what happens as I rotate the Ronchi ruling in the back. 53 00:02:54,400 --> 00:02:55,200 Here we are. 54 00:02:55,200 --> 00:02:57,180 I could rotate the other way. 55 00:02:57,180 --> 00:03:00,660 And I hope you can see all the weak spots, which are 56 00:03:00,660 --> 00:03:03,900 the cross terms in the pattern. 57 00:03:03,900 --> 00:03:08,430 Now, in order for you to calculate the line spacings 58 00:03:08,430 --> 00:03:11,610 in the Ronchi rulings, I will give you 59 00:03:11,610 --> 00:03:14,220 the information you need. 60 00:03:14,220 --> 00:03:20,220 We have a plane wave that impinges on the Ronchi ruling. 61 00:03:20,220 --> 00:03:24,660 And the diameter of it is about a little over a centimeter. 62 00:03:24,660 --> 00:03:28,350 The screen is about 100 centimeters away 63 00:03:28,350 --> 00:03:31,560 from the Ronchi rulings. 64 00:03:31,560 --> 00:03:35,820 And the wavelength of the light, as before, is 6328. 65 00:03:35,820 --> 00:03:37,850 And with all this information, you 66 00:03:37,850 --> 00:03:42,480 should be able to calculate the number of lines 67 00:03:42,480 --> 00:03:45,750 per inch or millimeter of the Ronchi ruling. 68 00:03:45,750 --> 00:03:47,715 But you need still one more information, 69 00:03:47,715 --> 00:03:51,300 and that is the scale on the screen. 70 00:03:51,300 --> 00:03:52,920 And I'm not going to put a scale on. 71 00:03:52,920 --> 00:03:55,830 But I will tell you that the separation 72 00:03:55,830 --> 00:04:01,470 between these dots here, these pair of dots, 73 00:04:01,470 --> 00:04:04,450 is about 6 millimeters. 74 00:04:04,450 --> 00:04:06,750 So now, you have all the information 75 00:04:06,750 --> 00:04:11,970 you need to calculate the spacing between the lines 76 00:04:11,970 --> 00:04:14,400 in the Ronchi ruling. 77 00:04:14,400 --> 00:04:18,450 Now, just before we quit, if we can pull away-- 78 00:04:18,450 --> 00:04:22,800 the camera pull away-- and show you the extent of the pattern, 79 00:04:22,800 --> 00:04:26,310 now you can see the pattern extends quite a bit. 80 00:04:26,310 --> 00:04:34,010 And now we can come in again and back to where we were before. 81 00:04:37,300 --> 00:04:39,760 This completes our demonstrations 82 00:04:39,760 --> 00:04:43,560 of two-dimensional Fraunhofer diffraction pattern. 83 00:04:43,560 --> 00:04:47,790 Next, what we have for you is Fresnel diffraction. 84 00:04:47,790 --> 00:04:50,170 So when we come back, we'll have the setup 85 00:04:50,170 --> 00:04:53,140 rearranged so we can look at some Fresnel diffraction 86 00:04:53,140 --> 00:04:54,690 patterns.