1 00:00:00,600 --> 00:00:02,202 PUNCH is an acronym. 2 00:00:02,202 --> 00:00:03,837 It stands for Polarimeter 3 00:00:03,837 --> 00:00:06,840 to Unify the Corona and Heliosphere. 4 00:00:07,073 --> 00:00:09,476 The corona is the outer atmosphere of the Sun. 5 00:00:09,476 --> 00:00:13,046 It's the part that is no longer gravitationally bound to the Sun, 6 00:00:13,113 --> 00:00:18,018 and it has so much energy that it flows outwards, filling our solar system 7 00:00:18,084 --> 00:00:21,488 and pushes against the interstellar medium making a bubble — 8 00:00:21,588 --> 00:00:23,390 and that is the heliosphere. 9 00:00:23,390 --> 00:00:26,192 And this system of how the corona turns 10 00:00:26,192 --> 00:00:29,195 into the heliosphere is what PUNCH is trying to study. 11 00:00:29,462 --> 00:00:35,535 So PUNCH is fundamentally four cameras that work together to make composite 12 00:00:35,668 --> 00:00:37,103 movies. 13 00:00:37,103 --> 00:00:40,940 We have a Narrow Field Imager that views the space close to the Sun, 14 00:00:41,174 --> 00:00:43,676 and then we have three separate Wide Field Imagers, 15 00:00:43,676 --> 00:00:46,679 each of which has a large, squarish field of view 16 00:00:46,746 --> 00:00:50,417 that looks way off to the side up to 45 degrees away from the Sun. 17 00:00:50,750 --> 00:00:54,654 That allows us to do something that no other mission has been able to do, 18 00:00:54,654 --> 00:00:59,125 which is routinely track coronal mass ejections, space storms, 19 00:00:59,392 --> 00:01:02,395 all the way across the solar system as they approach the Earth. 20 00:01:02,829 --> 00:01:06,466 By better understanding these storms and better understanding 21 00:01:06,466 --> 00:01:08,668 how they propagate on their way to the Earth, 22 00:01:08,668 --> 00:01:13,073 we'll be able to inform our partners on how to better forecast 23 00:01:13,073 --> 00:01:14,507 these events in the future. 24 00:01:14,507 --> 00:01:17,777 And that's really important for protecting our astronauts, 25 00:01:18,078 --> 00:01:20,914 our satellites, and our power grids. 26 00:01:20,914 --> 00:01:24,517 Once we launch and start producing images you'll be able to look at PUNCH 27 00:01:24,517 --> 00:01:28,321 data directly and see the kind of science we're engaged in. 28 00:01:28,421 --> 00:01:31,991 You'll be able to see things that are present in the sky right now 29 00:01:32,225 --> 00:01:35,628 and you just — you're not aware of them because they're washed out by the 30 00:01:35,862 --> 00:01:38,264 the brightness of the sky itself. 31 00:01:38,264 --> 00:01:41,468 We are poised to do tremendous science with PUNCH, 32 00:01:41,468 --> 00:01:45,905 because it provides this global context of what is happening in the corona 33 00:01:45,905 --> 00:01:49,008 and what is happening throughout the inner solar system, 34 00:01:49,008 --> 00:01:52,078 so that we can connect the details to the bigger picture. 35 00:01:52,345 --> 00:01:56,716 You might say that PUNCH is the next chapter in the study of heliophysics 36 00:01:56,716 --> 00:02:01,187 as we bring imaging and cross-scale understanding out, 37 00:02:01,387 --> 00:02:06,392 so that we can develop a coherent understanding of the entire system 38 00:02:06,392 --> 00:02:10,930 that starts at the corona and extends out to envelop the planets themselves.