1 00:00:00,000 --> 00:00:03,000 Thanks, Jennifer. 2 00:00:03,000 --> 00:00:09,000 Aurora tell us in a dramatic way that something invisible is happening above our heads in space to light up our skies. 3 00:00:09,000 --> 00:00:14,000 We can use sophisticated Earth-orbiting satellites to learn more about the causes of the aurora. 4 00:00:14,000 --> 00:00:19,000 The Imager for Magnetosphere-to-Aurora Global Exploration, or IMAGE, 5 00:00:19,000 --> 00:00:24,000 is a NASA satellite that lets us see the invisible activity that swirls around the Earth 6 00:00:24,000 --> 00:00:26,000 and eventually causes aurora to appear. 7 00:00:26,000 --> 00:00:30,000 When a solar storm collides with Earth, one of the first signs of the disturbance 8 00:00:30,000 --> 00:00:33,000 is a collection of particles called the ring current. 9 00:00:33,000 --> 00:00:38,000 It's an invisible river of charged particles extending over 30,000 kilometers from Earth. 10 00:00:38,000 --> 00:00:42,000 Much of the matter in this current actually comes from the Earth's upper atmosphere 11 00:00:42,000 --> 00:00:46,000 in gigantic plumes and fountains of gas from the polar regions. 12 00:00:46,000 --> 00:00:49,000 But we still don't know how the particles get their energy. 13 00:00:49,000 --> 00:00:53,000 Another part of the upper atmosphere, seen by IMAGE for the first time, 14 00:00:53,000 --> 00:00:56,000 is what scientists call the plasmasphere. 15 00:00:56,000 --> 00:00:59,000 It extends out into space at least 10,000 kilometers. 16 00:00:59,000 --> 00:01:02,000 You should think of it as the outer limits to the ionosphere. 17 00:01:02,000 --> 00:01:06,000 During severe storms, parts of the plasmasphere are stripped off, 18 00:01:06,000 --> 00:01:11,000 but then reform as new gas flows out of the Earth's upper reaches. 19 00:01:11,000 --> 00:01:18,000 And, of course, IMAGE also provides scientists with movie-like, high-resolution views of the aurora seen from space. 20 00:01:18,000 --> 00:01:22,000 Over the South Pole, the satellite dips down to 1,000 kilometers 21 00:01:22,000 --> 00:01:26,000 to show us never-before-seen details in auroral structure. 22 00:01:26,000 --> 00:01:30,000 The aurora in the South Pole is called Aurora Australis. 23 00:01:30,000 --> 00:01:34,000 Over the North Pole, we see a more distant view and a bigger picture. 24 00:01:34,000 --> 00:01:38,000 We can relate this big picture with views of the ring current and plasmasphere 25 00:01:38,000 --> 00:01:42,000 to track the evolution of an aurora from cradle to grave. 26 00:01:42,000 --> 00:01:45,000 The reason why we're so keen to understand the aurora 27 00:01:45,000 --> 00:01:48,000 is that the aurora are kind of like a final examination. 28 00:01:48,000 --> 00:01:50,000 If we can really understand how they work, 29 00:01:50,000 --> 00:01:54,000 that means we also understand all the other things about Earth's environment as well. 30 00:01:54,000 --> 00:01:58,000 We have billions of dollars of satellite technology in space, 31 00:01:58,000 --> 00:02:00,000 astronauts living and working in space, 32 00:02:00,000 --> 00:02:04,000 and on the ground, many kinds of systems that are affected by solar storms. 33 00:02:04,000 --> 00:02:09,000 An electrical blackout in Canada back in 1989 cost billions of dollars. 34 00:02:09,000 --> 00:02:13,000 We have lost over $2 billion of expensive communication and research satellites 35 00:02:13,000 --> 00:02:15,000 in the last 10 years alone. 36 00:02:15,000 --> 00:02:19,000 Solar storms have tremendous potential to cause damage to us. 37 00:02:19,000 --> 00:02:22,000 Only by understanding aurora and the events that lead up to them 38 00:02:22,000 --> 00:02:28,000 can we improve our ability to predict how to avoid the harmful effects of space weather storms. 39 00:02:28,000 --> 00:02:32,000 The real challenge is to get enough early warning that a storm is approaching. 40 00:02:32,000 --> 00:02:36,000 That's why it's also important to look at the sun for clues to the next storm. 41 00:02:36,000 --> 00:02:37,000 Thanks, Sten. 42 00:02:37,000 --> 00:02:41,000 Okay, guys, now it's your turn to apply data analysis and measurement skills 43 00:02:41,000 --> 00:02:43,000 with this really cool activity. 44 00:02:43,000 --> 00:02:45,000 Sten, they are gorgeous, aren't they? 45 00:02:45,000 --> 00:02:47,000 Aren't they amazing?