WEBVTT FILE 1 00:00:00.080 --> 00:00:04.250 Music 2 00:00:04.270 --> 00:00:08.250 Music 3 00:00:08.270 --> 00:00:12.270 Music 4 00:00:12.290 --> 00:00:16.309 Music 5 00:00:16.329 --> 00:00:20.389 The course of geomagnetic activity disturbances caused by 6 00:00:20.410 --> 00:00:24.390 flares on the sun, by big blogs of plasma coming out from the 7 00:00:24.410 --> 00:00:28.400 sun towards the Earth. The Earth's magnetic field is battered and shaken. 8 00:00:28.420 --> 00:00:32.400 Some of that energy is captured in the earth's magnetic field and through a 9 00:00:32.420 --> 00:00:36.420 variety of processes that energy, energizes particles in the 10 00:00:36.440 --> 00:00:40.599 Earth's radiation belts, up to energies that are hazardous to 11 00:00:40.620 --> 00:00:44.620 spacecraft and astronauts. The Radiation Belt Storm Probes 12 00:00:44.640 --> 00:00:48.800 mission, is NASA's mission to study the Earth's Van Allen Radiation 13 00:00:48.820 --> 00:00:52.830 Belts. Two invisible regions of highly charged 14 00:00:52.850 --> 00:00:56.850 particles in space that surround the Earth. Each of the two 15 00:00:56.870 --> 00:01:00.860 RBSP spacecraft carries five instrument suites and a 16 00:01:00.880 --> 00:01:04.860 total of eight instruments, the two spacecraft are identical. 17 00:01:04.879 --> 00:01:08.880 The region of space that we're talking about where the Radiation Belt Storm 18 00:01:08.900 --> 00:01:12.890 Probe spacecraft will go, is one that's occupied by communication 19 00:01:12.910 --> 00:01:16.899 spacecraft, by weather spacecraft, by all sorts of spacecraft that you use 20 00:01:16.920 --> 00:01:20.930 on a daily basis. 21 00:01:20.950 --> 00:01:24.940 There are two Van Allen Radiation Belts. The one closer to Earth about, 22 00:01:24.960 --> 00:01:28.949 1.000 miles up. above the Earth's equator contains highly 23 00:01:28.970 --> 00:01:32.960 charged protons that are trapped there for years and years. 24 00:01:32.980 --> 00:01:37.000 The further out radiation belt, the outer radiation belt, 25 00:01:37.020 --> 00:01:41.190 at about a twelfth of a distance to the moon, contains a mixture of energetic 26 00:01:41.210 --> 00:01:45.240 electrons and energetic ions. Both of them are hazardous but hazardous in 27 00:01:45.260 --> 00:01:49.280 different ways and at different times. They're always changing waxing 28 00:01:49.300 --> 00:01:53.479 waning, increasing and decreasing in strength, we don't understand 29 00:01:53.500 --> 00:01:57.490 why. The goals of the Radiation Belt Storm 30 00:01:57.510 --> 00:02:01.500 Probes mission are to determine where the charged particles in the Earth's 31 00:02:01.520 --> 00:02:05.520 radiation belts come from, how they get energized, and how they're 32 00:02:05.540 --> 00:02:09.610 lost into space. The first use for the data 33 00:02:09.630 --> 00:02:13.620 from the mission will be by scientists who attempt to understand the physical processes 34 00:02:13.640 --> 00:02:17.709 that are occurring in the radiation belts. They'll use those data to develop 35 00:02:17.730 --> 00:02:21.730 models for space weather in the Earth's environment, the hazardous features that 36 00:02:21.750 --> 00:02:25.770 surround us. However the data can also be used by engineers 37 00:02:25.790 --> 00:02:29.790 to better design spacecraft. For example if you know how much radiation 38 00:02:29.810 --> 00:02:33.820 is out there, you know how thick to shield your spacecraft with walls 39 00:02:33.840 --> 00:02:37.850 of metal. The Earth's radiation belts pose a hazard to 40 00:02:37.870 --> 00:02:41.880 astronauts, a hazard because radiation, prolonged exposure to radiation 41 00:02:41.900 --> 00:02:45.930 can cause cancer. What we want to do is understand 42 00:02:45.950 --> 00:02:49.940 just how much radiation is out there, and just where it is and we can 43 00:02:49.960 --> 00:02:53.950 warn astronauts when to be inside and outside their spacecraft. 44 00:02:53.970 --> 00:02:57.960 The RBSP spacecraft are focused on the dynamic 45 00:02:57.980 --> 00:03:02.049 radiation belts in the Earth's inner magnetosphere, they're the only 46 00:03:02.070 --> 00:03:06.060 spacecraft that focus on those. Consequently they're a critical component 47 00:03:06.080 --> 00:03:10.100 in the series of phenomenon that link the Sun to the Earth. 48 00:03:10.120 --> 00:03:14.130 music 49 00:03:14.150 --> 00:03:18.130 beep 50 00:03:18.150 --> 00:03:22.180 beep 51 00:03:22.200 --> 00:03:26.269