1 00:00:10,677 --> 00:00:12,345 PUNCH stands for 2 00:00:12,345 --> 00:00:16,266 Polarimeter Unify the Corona and Heliosphere. 3 00:00:16,599 --> 00:00:19,602 The corona is the outer atmosphere of the sun. 4 00:00:19,811 --> 00:00:22,772 It's the part of the sun that you get to see during a total 5 00:00:22,772 --> 00:00:26,234 solar eclipse, where the moon blocks out the main body of the sun. 6 00:00:26,943 --> 00:00:30,655 PUNCH makes artificial eclipses all the time, so that we can see that 7 00:00:30,655 --> 00:00:35,035 corona as it turns into the solar wind and fills our solar system 8 00:00:35,035 --> 00:00:38,038 with material. 9 00:00:42,500 --> 00:00:45,628 The solar wind is important to study because it's the way 10 00:00:45,628 --> 00:00:49,758 that the sun sends out material out into our solar system. 11 00:00:49,758 --> 00:00:51,342 It's constantly bombarding 12 00:00:51,342 --> 00:00:55,138 all of the planets, including Earth and Earth's magnetic field. 13 00:00:55,388 --> 00:00:58,933 And it's very important to understand, because of space weather, 14 00:00:58,933 --> 00:01:02,854 the big solar storms that have to propagate through the solar wind, 15 00:01:03,063 --> 00:01:05,899 and they impact our astronauts 16 00:01:05,899 --> 00:01:09,611 and Earth's magnetic field and cause effects like the aurora 17 00:01:16,951 --> 00:01:18,661 Parker Solar Probe is so 18 00:01:18,661 --> 00:01:22,624 cool because it's flying through the outer parts of the corona right 19 00:01:22,624 --> 00:01:26,211 now, measuring that material that's coming off of the sun. 20 00:01:26,461 --> 00:01:29,380 Meanwhile, PUNCH is going to take global images, 21 00:01:29,380 --> 00:01:34,385 seeing how that corona turns into the solar wind and fills our solar system. 22 00:01:34,552 --> 00:01:38,264 So we'll be able to connect the details that Parker Solar Probe sees 23 00:01:38,431 --> 00:01:41,559 with the big picture, the global picture of what's happening 24 00:01:41,559 --> 00:01:44,562 everywhere. 25 00:01:49,192 --> 00:01:50,693 PUNCH is comprised 26 00:01:50,693 --> 00:01:54,948 of four small satellites, their suitcase sized satellites. 27 00:01:55,115 --> 00:02:00,662 Each one has an instrument that together looks at the global picture. 28 00:02:00,662 --> 00:02:03,873 So we have one instrument, the Narrow Field Imager. 29 00:02:03,873 --> 00:02:07,627 It looks pretty close to the sun and really gets that the solar corona, 30 00:02:07,627 --> 00:02:09,170 the atmosphere of the sun. 31 00:02:09,170 --> 00:02:11,756 And then we have three wide field imagers 32 00:02:11,756 --> 00:02:15,051 that because of their orbit, they look in different places of the sky. 33 00:02:15,051 --> 00:02:18,596 And together we piece together the whole global image 34 00:02:18,888 --> 00:02:22,559 of the material coming off of the sun, filling our solar system. 35 00:02:29,107 --> 00:02:32,318 PUNCH is orbiting in a place that we call low Earth orbit. 36 00:02:32,318 --> 00:02:33,153 That means it's 37 00:02:33,153 --> 00:02:37,282 sort of the closest to Earth it can be, while still being in outer space. 38 00:02:37,282 --> 00:02:39,159 And above Earth's atmosphere. 39 00:02:39,159 --> 00:02:42,162 That would, block the light. 40 00:02:48,543 --> 00:02:49,335 The PUNCH ride share 41 00:02:49,335 --> 00:02:53,089 SPHEREx is incredibly exciting for two reasons. 42 00:02:53,089 --> 00:02:56,259 One is practical, and because it is an efficient way 43 00:02:56,259 --> 00:02:59,137 to get up into space and to use the taxpayers money. 44 00:02:59,137 --> 00:03:03,183 The second reason is that both PUNCH and SPHEREx are exploring 45 00:03:03,183 --> 00:03:07,437 the big picture. SPHEREx is exploring the big picture of the cosmos, and PUNCH 46 00:03:07,437 --> 00:03:10,815 is exploring the big picture of the sun and how it fills our solar 47 00:03:10,815 --> 00:03:13,818 system. 48 00:03:18,406 --> 00:03:19,574 PUNCH links 49 00:03:19,574 --> 00:03:23,369 to the Heliophysics System Observatory, which is all of these missions 50 00:03:23,369 --> 00:03:26,831 that we have in heliophysics connecting the sun 51 00:03:26,831 --> 00:03:30,376 and how that material fills the solar system and impacts 52 00:03:30,627 --> 00:03:33,922 Earth and Earth's environment and fills the whole solar system. 53 00:03:34,589 --> 00:03:38,551 So punch provides the global picture that all of those other missions, 54 00:03:38,927 --> 00:03:41,763 we can combine with all of those other missions 55 00:03:41,763 --> 00:03:46,184 to really understand this full connected system between the sun and the Earth. 56 00:03:53,524 --> 00:03:56,236 The sun is in a period of heightened activity. 57 00:03:56,236 --> 00:03:57,612 That means there are more of these 58 00:03:57,612 --> 00:04:00,949 solar storms, these magnetic explosions on the sun, 59 00:04:01,407 --> 00:04:06,371 these magnetic explosions, come outwards and they can impact our satellites. 60 00:04:06,371 --> 00:04:07,622 They can hurt our astronauts. 61 00:04:07,622 --> 00:04:09,958 So they're really important to understand. 62 00:04:09,958 --> 00:04:13,503 PUNCH s going to watch those in three dimensions 63 00:04:13,503 --> 00:04:17,006 and will be able to tell if they're coming towards the earth or going away 64 00:04:17,006 --> 00:04:20,134 from the Earth, or in some other direction in the solar system. 65 00:04:20,426 --> 00:04:24,222 Meanwhile, Parker Solar Probe is sampling some of those solar storms 66 00:04:24,222 --> 00:04:29,060 right after they're formed, right at the beginning in tremendous detail. 67 00:04:29,227 --> 00:04:33,147 And together with PUNCH, we can really understand how they evolve 68 00:04:33,147 --> 00:04:36,150 through the inner solar system. 69 00:04:41,572 --> 00:04:42,824 What I'm so excited 70 00:04:42,824 --> 00:04:45,910 for about PUNCH is that PUNCH sees 71 00:04:45,910 --> 00:04:48,997 not just the global scale and the big solar storms. 72 00:04:48,997 --> 00:04:52,917 It also sees the daily little storms that happen all of the time. 73 00:04:53,334 --> 00:04:55,211 The sun is never quiet. 74 00:04:55,211 --> 00:05:00,049 It is constantly putting out bursts of of magnetic field and material. 75 00:05:00,300 --> 00:05:03,428 And those bursts of magnetic field, the material impact 76 00:05:03,428 --> 00:05:07,348 the Earth and can drive, space weather events like 77 00:05:07,598 --> 00:05:11,477 impacting our radiation belts, impacting our satellites. 78 00:05:11,686 --> 00:05:15,231 And PUNCH is going to see the big storms and the smaller storms 79 00:05:21,988 --> 00:05:24,991 One cool upcoming mission is called EZIE.. 80 00:05:25,074 --> 00:05:28,578 EZIE is going to connect the magnetic field of the Earth. 81 00:05:28,786 --> 00:05:32,165 And, during these solar storms, when they impact the Earth, 82 00:05:32,415 --> 00:05:35,877 the connection between the Earth's magnetic field and Earth's ionosphere, 83 00:05:35,877 --> 00:05:39,297 the currents that flow through ionosphere is what EZIE is going to measure. 84 00:05:39,922 --> 00:05:44,218 Now, PUNCH’s noise is the high altitude aurora, 85 00:05:44,218 --> 00:05:46,137 the northern lights and the southern lights 86 00:05:46,137 --> 00:05:49,766 that occurred during these magnetic reconfigurations 87 00:05:49,766 --> 00:05:52,018 and current systems that happen during the solar storm. 88 00:05:52,018 --> 00:05:56,439 So our noise is going to be related to what EZIE is measuring directly. 89 00:05:56,439 --> 00:05:59,525 And we can really work together with them to solve these problems 90 00:05:59,525 --> 00:06:02,528 in heliophysics. 91 00:06:07,033 --> 00:06:09,369 Our viewers can learn more about PUNCH at [nasa.gov/punch] NASA 92 00:06:09,369 --> 00:06:10,995 Dot gov slash punch.