1 00:00:14,140 --> 00:00:11,230 [Music] 2 00:00:16,580 --> 00:00:14,150 magnetic reconnection is the process of 3 00:00:17,810 --> 00:00:16,590 disconnecting or connecting the magnetic 4 00:00:19,880 --> 00:00:17,820 fields to each other 5 00:00:22,099 --> 00:00:19,890 directing energy into the earth on the 6 00:00:24,019 --> 00:00:22,109 day side and then letting it go on the 7 00:00:26,870 --> 00:00:24,029 night side and the interplay between 8 00:00:29,960 --> 00:00:26,880 those two is what produces all la space 9 00:00:32,089 --> 00:00:29,970 weather around the earth that has big 10 00:00:34,610 --> 00:00:32,099 effects can damage our spacecraft can 11 00:00:36,560 --> 00:00:34,620 hurt astronauts can upset the flow of 12 00:00:38,780 --> 00:00:36,570 electron or G and our electric grid on 13 00:00:41,330 --> 00:00:38,790 the surface of the earth MMS is a 14 00:00:44,030 --> 00:00:41,340 mission with four spacecraft that are 15 00:00:46,389 --> 00:00:44,040 traveling in formation in an orbit that 16 00:00:49,880 --> 00:00:46,399 takes them out into two special places 17 00:00:53,479 --> 00:00:49,890 near the earth one upstream toward the 18 00:00:54,950 --> 00:00:53,489 Sun on downstream away from the Sun both 19 00:00:57,709 --> 00:00:54,960 of those places have magnetic 20 00:01:01,069 --> 00:00:57,719 reconnection we have never before NMS 21 00:01:02,990 --> 00:01:01,079 had the ability to essentially run the 22 00:01:05,960 --> 00:01:03,000 camera fast enough to catch it as it 23 00:01:08,810 --> 00:01:05,970 goes by to make mini measurements per 24 00:01:10,850 --> 00:01:08,820 second the science payload for her mass 25 00:01:14,480 --> 00:01:10,860 is all mounted on a single deck plate 26 00:01:16,460 --> 00:01:14,490 but it consists of some 25 boxes per 27 00:01:18,920 --> 00:01:16,470 spacecraft divided into three general 28 00:01:20,539 --> 00:01:18,930 groups of instruments that's those for 29 00:01:23,420 --> 00:01:20,549 measuring fields electric and magnetic 30 00:01:25,520 --> 00:01:23,430 those for measuring plasmas in a third 31 00:01:27,560 --> 00:01:25,530 for measuring energetic particles the 32 00:01:29,030 --> 00:01:27,570 magnetic field sensors are out on arms 33 00:01:31,160 --> 00:01:29,040 that extend away from the spacecraft 34 00:01:33,530 --> 00:01:31,170 they're fixed but the spacecraft is 35 00:01:36,260 --> 00:01:33,540 spinning slowly about once every 20 36 00:01:36,890 --> 00:01:36,270 seconds the electric field is quite a 37 00:01:39,950 --> 00:01:36,900 bit different 38 00:01:41,899 --> 00:01:39,960 it consists of four wires that extend 39 00:01:44,600 --> 00:01:41,909 out away from the spacecraft with a ball 40 00:01:47,420 --> 00:01:44,610 on the end of each of them that actually 41 00:01:48,740 --> 00:01:47,430 contacts the plasma all four of those 42 00:01:51,200 --> 00:01:48,750 are spinning around with the spacecraft 43 00:01:53,510 --> 00:01:51,210 at this twenty second period and then 44 00:01:55,580 --> 00:01:53,520 there's a third axis that extends their 45 00:01:56,870 --> 00:01:55,590 booms that extend along the spin axis of 46 00:01:58,789 --> 00:01:56,880 the spacecraft both upward and downward 47 00:02:00,560 --> 00:01:58,799 with a probe at the ends you've got 48 00:02:03,319 --> 00:02:00,570 three components of the electric field 49 00:02:05,719 --> 00:02:03,329 they can measure everything from up to 50 00:02:07,670 --> 00:02:05,729 small Wiggles and vibrations of the 51 00:02:08,740 --> 00:02:07,680 electric field another sensor called the 52 00:02:12,220 --> 00:02:08,750 searchcoil magnet 53 00:02:15,100 --> 00:02:12,230 that is just a loop of wire connected to 54 00:02:16,600 --> 00:02:15,110 a suitable amplifier and is designed to 55 00:02:18,490 --> 00:02:16,610 measure the fluctuations at higher 56 00:02:21,940 --> 00:02:18,500 frequencies then you could get with the 57 00:02:25,420 --> 00:02:21,950 DC magnetometers for the plasmas there 58 00:02:26,830 --> 00:02:25,430 are eight boxes two boxes at each of the 59 00:02:28,990 --> 00:02:26,840 four points of the compass on the 60 00:02:29,710 --> 00:02:29,000 spacecraft those are equally spaced all 61 00:02:33,180 --> 00:02:29,720 the way around the spacecraft 62 00:02:35,320 --> 00:02:33,190 essentially that is a real key 63 00:02:38,020 --> 00:02:35,330 ingredient for being able to see the 64 00:02:40,360 --> 00:02:38,030 entire sky instantaneously without 65 00:02:42,850 --> 00:02:40,370 waiting for the spacecraft to spin then 66 00:02:44,949 --> 00:02:42,860 there's also a hot plasma composition 67 00:02:47,310 --> 00:02:44,959 analyzer one per spacecraft it has a 68 00:02:50,500 --> 00:02:47,320 sensor head that looks all around in a 69 00:02:52,600 --> 00:02:50,510 360-degree annulus sticks out the side 70 00:02:55,240 --> 00:02:52,610 of the spacecraft and sweeps out the 71 00:02:57,520 --> 00:02:55,250 whole sky twice per spin it measures the 72 00:02:59,430 --> 00:02:57,530 chemical species of the particles the 73 00:03:01,780 --> 00:02:59,440 third set are the energetic particles 74 00:03:03,130 --> 00:03:01,790 analyzers and they are measuring much 75 00:03:05,530 --> 00:03:03,140 more energetic particles that are 76 00:03:07,930 --> 00:03:05,540 accelerated by the reconnection process 77 00:03:09,670 --> 00:03:07,940 ultimately the thing we will be doing is 78 00:03:11,860 --> 00:03:09,680 comparing our observations with 79 00:03:14,199 --> 00:03:11,870 simulations of the entire magnetosphere 80 00:03:16,780 --> 00:03:14,209 as it is influenced by the solar wind 81 00:03:19,150 --> 00:03:16,790 coming in down to the details of what 82 00:03:20,949 --> 00:03:19,160 reconnection is occurring people who do 83 00:03:23,170 --> 00:03:20,959 those simulations that try to apply them 84 00:03:26,620 --> 00:03:23,180 to all other kinds of places like in the 85 00:03:30,970 --> 00:03:26,630 solar atmosphere at other Astrophysical 86 00:03:32,170 --> 00:03:30,980 stars and other objects and they are 87 00:03:34,270 --> 00:03:32,180 very interested in whether those 88 00:03:36,160 --> 00:03:34,280 simulations are accurate and reflect 89 00:03:37,630 --> 00:03:36,170 reality well this is going to be the 90 00:03:40,120 --> 00:03:37,640 first time we actually bump them up 91 00:03:42,310 --> 00:03:40,130 against hard data on what's going on in 92 00:03:43,780 --> 00:03:42,320 their eye I'm almost certain I'm very 93 00:03:45,819 --> 00:03:43,790 certain they're going to learn something 94 00:03:47,040 --> 00:03:45,829 from that and the simulations will get 95 00:03:49,110 --> 00:03:47,050 better 96 00:03:51,060 --> 00:03:49,120 we're doing a measure thing at rates 97 00:03:53,610 --> 00:03:51,070 that have never been done before and in 98 00:03:56,880 --> 00:03:53,620 places that have been hard to reach or 99 00:04:01,110 --> 00:03:56,890 even see because they go by too fast to