1 00:00:00,010 --> 00:00:04,030 [building music] 2 00:00:04,050 --> 00:00:08,070 [building music] 3 00:00:08,090 --> 00:00:12,080 [drumbeats] >>KATRINA: The Magnetospheric Multiscale Mission. 4 00:00:12,100 --> 00:00:16,110 Designed to study the fundamental physics phenomenon called "magnetic 5 00:00:16,130 --> 00:00:20,140 reconnection," it's a complex conglomeration of advanced instruments 6 00:00:20,160 --> 00:00:24,200 developed by NASA and France, Austria, Sweden, Germany, Japan 7 00:00:24,220 --> 00:00:28,270 and several American universities and research institutes. [swoosh] 8 00:00:28,290 --> 00:00:32,290 And right here at NASA's Goddard Space Flight Center, we're proud to contribute with 9 00:00:32,310 --> 00:00:36,390 a whole suite of instruments called the Fast Plasma Investigation. 10 00:00:36,410 --> 00:00:40,400 [drums, music] 11 00:00:40,420 --> 00:00:44,430 >>CRAIG: Magnetic reconnection is a phenomenon where magnetic fields come together and essentially merge, releasing 12 00:00:44,450 --> 00:00:48,480 energy. It occurs in stellar environments, our own Sun, 13 00:00:48,500 --> 00:00:52,500 it occurs in planetary environments like around the Earth, and it occurs 14 00:00:52,520 --> 00:00:56,530 in the interplanetary space. For another thing, we're trying to learn how to 15 00:00:56,550 --> 00:01:00,580 harness nuclear fusion as an energy source 16 00:01:00,600 --> 00:01:04,610 and one of the roadblocks is our lack of understanding of magnetic reconnection. 17 00:01:04,630 --> 00:01:08,650 >>KATRINA: So why have we chosen Earth's magnetosphere to study this process 18 00:01:08,670 --> 00:01:12,690 of magnetic reconnection? >>CRAIG: The magnetosphere is a convenient location 19 00:01:12,710 --> 00:01:16,750 to study it. And we need to understand magnetic reconnection in the Earth's 20 00:01:16,770 --> 00:01:20,770 magnetosphere because it has a profound influence on space weather. >>KATRINA: And 21 00:01:20,790 --> 00:01:24,830 space weather near Earth is caused by storms on the Sun that can affect our satellites 22 00:01:24,850 --> 00:01:28,840 and communications, right? >>CRAIG: Yes, you could put it that way. >>KATRINA: How long do we have 23 00:01:28,860 --> 00:01:32,870 to make these measurements? >>CRAIG: Only a very short period of time. The region where the 24 00:01:32,890 --> 00:01:36,890 magnetic reconnection is occurring sweeps over the spacecraft in only about 25 00:01:36,910 --> 00:01:40,930 a tenth of a second, so we have to get our measurements made in that short time. 26 00:01:40,950 --> 00:01:45,000 [drumming] 27 00:01:45,020 --> 00:01:49,030 >>KATRINA: So I'm told that magnetic reconnection happens really quickly, 28 00:01:49,050 --> 00:01:53,070 from the perspective of the spacecraft anyway as they fly through the region. How does the 29 00:01:53,090 --> 00:01:57,080 Fast Plasma Investigation suite of instruments help us to measure this? 30 00:01:57,100 --> 00:02:01,110 >>ULRIK: So on each satellite we have four spectrometers, 31 00:02:01,130 --> 00:02:05,160 dual ion spectrometers and dual electron 32 00:02:05,180 --> 00:02:09,170 spectrometers, and as the satellite goes around, we can very quickly all the way 33 00:02:09,190 --> 00:02:13,200 around the satellite capture the events. >>KATRINA: So the dual electron spectrometer 34 00:02:13,220 --> 00:02:17,250 is developed here at Goddard. What exactly does that measure? >>ULRIK: They're measuring the energy, 35 00:02:17,270 --> 00:02:21,270 the direction, and the abundance of the electrons, how many electrons there are there. 36 00:02:21,290 --> 00:02:25,320 >>KATRINA: Could you show me a little bit about how it works? >>ULRIK: The instrument has this box at the end, 37 00:02:25,340 --> 00:02:29,360 here which is our electronics box, where we have all the power supplies and the controls 38 00:02:29,380 --> 00:02:33,420 for the instrument. [instrument moving] And you can see the 39 00:02:33,440 --> 00:02:37,430 aperture opening here of one of the sensor heads, and that enables, that opening goes 40 00:02:37,450 --> 00:02:41,480 180 degrees around. >>KATRINA: So you have four of these instruments 41 00:02:41,500 --> 00:02:45,500 on each of the four satellites, so you have 16 in total of 42 00:02:45,520 --> 00:02:49,530 the electron spectrometers. That's a lot of instruments! Has Goddard ever done 43 00:02:49,550 --> 00:02:53,570 something like this before where it's had to build and test so many 44 00:02:53,590 --> 00:02:57,600 instruments at once? >>ULRIK: To the best of my knowledge, this is the 45 00:02:57,620 --> 00:03:01,660 largest multiple build that has been done at Goddard. 46 00:03:01,680 --> 00:03:05,670 [door opening] >>KATRINA: Well the hard work is about to pay off! 47 00:03:05,690 --> 00:03:09,700 The four MMS spacecraft are set to launch in March of 2015. 48 00:03:09,720 --> 00:03:13,720 Thanks to the incredible talents and collaborations of scientists and 49 00:03:13,740 --> 00:03:17,740 engineers, here at Goddard and across the globe, we're finally on our way to solving this 50 00:03:17,760 --> 00:03:21,780 physics mystery, and uncovering the dynamics of magnetic reconnection. 51 00:03:21,800 --> 00:03:25,800 [boom] [drum drum drum drum] [exciting music] 52 00:03:25,820 --> 00:03:29,830 [exciting music fades out] 53 00:03:29,850 --> 00:03:33,850 54 00:03:33,870 --> 00:03:35,195