1 00:00:09,070 --> 00:00:06,030 Sound Effect 2 00:00:09,090 --> 00:00:13,140 Music, Narrator: In 2006 NASA launched the Solar 3 00:00:13,160 --> 00:00:17,170 TErrestrial RElations Observatory, or STEREO, spacecraft. 4 00:00:17,190 --> 00:00:21,210 Over the last 4 years, the two spacecraft have slowly made their way along Earth's 5 00:00:21,230 --> 00:00:25,240 orbit, with STEREO A advancing ahead, and STEREO B falling 6 00:00:25,260 --> 00:00:29,270 behind. As they've separated, our view of the sun 7 00:00:29,290 --> 00:00:33,360 has increased. Other satellites near Earth, 8 00:00:33,380 --> 00:00:37,510 such as SOHO, and now SDO, continue to watch the sun from Earth's 9 00:00:37,530 --> 00:00:41,560 perspective, while the STEREO spacecraft see increasingly different views. 10 00:00:41,580 --> 00:00:45,600 Now STEREO A and B are almost exactly opposite each other 11 00:00:45,620 --> 00:00:49,700 and for the first time in human history, we have a view of the entire sun 12 00:00:49,720 --> 00:00:53,740 Music 13 00:00:53,760 --> 00:00:57,850 The sun has a huge 14 00:00:57,870 --> 00:01:01,930 influence on everyday life, and with our increased reliance on technology, this 15 00:01:01,950 --> 00:01:05,950 influence just keeps getting stronger. Coronal mass 16 00:01:05,970 --> 00:01:09,990 ejections and solar flares are the hurricanes of space weather and they have the power to 17 00:01:10,010 --> 00:01:14,070 disrupt our navigation systems, communications and even electrical grids, 18 00:01:14,090 --> 00:01:18,090 so it's vital we know when they are coming. Just as protecting our homes 19 00:01:18,110 --> 00:01:22,140 requires the best possible weather forecast, protecting these systems requires 20 00:01:22,160 --> 00:01:26,230 the best possible space weather forecast. Sunspots and 21 00:01:26,250 --> 00:01:30,290 other active regions on the sun can help predict a new round of such space weather, but 22 00:01:30,310 --> 00:01:34,340 before STEREO we were able to see only one side of the sun at a time; 23 00:01:34,360 --> 00:01:38,380 we couldn't tell what was starting to form on the far side. Since the sun 24 00:01:38,400 --> 00:01:42,440 takes about 27 days to rotate once, solar activity had plenty of time 25 00:01:42,460 --> 00:01:46,500 to build unnoticed. Scientists first began 26 00:01:46,520 --> 00:01:50,520 to get a sense of the far side with SOHO's Michelson Doppler Imager which worked almost 27 00:01:50,540 --> 00:01:54,560 like an ultrasound to give a view of the sun's back based on observations of the ripples on 28 00:01:54,580 --> 00:01:58,640 its front. Now STERE can make direct observations and 29 00:01:58,660 --> 00:02:02,660 eliminate any uncertainty about activity on the far side of the sun. 30 00:02:02,680 --> 00:02:06,680 This unprecedented view will last for at least another 8 years as the 31 00:02:06,710 --> 00:02:10,720 spacecraft slowly continue their journey. They will cross behind the sun, 32 00:02:10,740 --> 00:02:14,770 and then once again continue to opposite sides of the sun, this time with their position 33 00:02:14,790 --> 00:02:18,810 reversed. During that time, astronomers will be able to see 34 00:02:18,830 --> 00:02:22,890 magnetic active regions wherever they form on the sun, so we will know about regions on the far 35 00:02:22,910 --> 00:02:26,940 side well before any Earth-based observatory can see them. 36 00:02:26,960 --> 00:02:30,980 The full view of the sun from STEREO and SDO 37 00:02:31,000 --> 00:02:35,030 coupled with the other spacecraft in NASA's Heliophysics fleet, will help scientists 38 00:02:35,050 --> 00:02:39,080 understand our dynamic star and give us more time to prepare for the next big 39 00:02:39,100 --> 00:02:43,140 storm. Static 40 00:02:43,160 --> 00:02:47,160 static