WEBVTT FILE 1 00:00:00.000 --> 00:00:03.940 If you’re looking to catch the April 8 total solar eclipse, 2 00:00:03.940 --> 00:00:06.650 you’ll want to be somewhere with clear skies. 3 00:00:06.650 --> 00:00:11.710 For some scientists, that means heading above the clouds. 4 00:00:11.710 --> 00:00:14.950 5 00:00:14.950 --> 00:00:17.200 During the 2024 solar eclipse, 6 00:00:17.200 --> 00:00:21.870 the WB-57 airplanes will be flying at an altitude of about 50,000 feet, 7 00:00:21.870 --> 00:00:27.620 chasing the eclipse shadow over the coast of Mexico near Mazatlan. 8 00:00:27.620 --> 00:00:31.760 Three science teams will be using two WB-57 jet planes 9 00:00:31.760 --> 00:00:34.370 to study different aspects of the eclipse. 10 00:00:34.370 --> 00:00:38.550 Firstly, these two teams with instruments in the nose and wings 11 00:00:38.550 --> 00:00:44.220 will be looking at the Sun’s outer atmosphere known as the corona. 12 00:00:44.220 --> 00:00:48.730 Scientists often study the corona using spacecraft with coronagraphs. 13 00:00:48.730 --> 00:00:52.390 These are occulting disks that help block out the bright Sun. 14 00:00:52.390 --> 00:00:56.040 But they also cover up the inner part of the corona. 15 00:00:56.040 --> 00:00:57.570 During a total solar eclipse, 16 00:00:57.570 --> 00:01:03.610 the Moon perfectly blocks the Sun’s bright disk, allowing the entire corona to appear. 17 00:01:03.610 --> 00:01:07.910 A total eclipse gives us the best view of the corona we can get. 18 00:01:07.910 --> 00:01:10.880 And it’s even better when viewed from above. 19 00:01:10.880 --> 00:01:16.320 The most exciting part of using the WB-57 is to get over the clouds. 20 00:01:16.320 --> 00:01:21.960 And to get to a layer of the atmosphere where it's so much less dense. 21 00:01:21.960 --> 00:01:25.240 This means you can access wavelengths of light 22 00:01:25.240 --> 00:01:27.530 that you normally wouldn't be able to access on the ground. 23 00:01:27.530 --> 00:01:30.300 The team led by the University of Hawaii 24 00:01:30.300 --> 00:01:34.280 will measure different wavelengths of light using spectrometers and cameras. 25 00:01:34.280 --> 00:01:39.560 Their instruments will give insight into the corona’s chemical composition and temperature. 26 00:01:39.560 --> 00:01:45.360 We want to figure out what kind of processes are operating in the Sun, 27 00:01:45.360 --> 00:01:47.640 just above its surface or at the surface. 28 00:01:47.640 --> 00:01:51.070 For the team led by the Southwest Research Institute, 29 00:01:51.070 --> 00:01:53.890 this will be their second time chasing an eclipse, 30 00:01:53.890 --> 00:01:57.740 so they’re using an improved camera setup. 31 00:01:57.740 --> 00:02:02.110 In 2024, we're flying an evolution of the experiment, we flew in 2017. 32 00:02:02.110 --> 00:02:06.120 Back then we flew two cameras in two different wavelength ranges. 33 00:02:06.120 --> 00:02:11.230 For this experiment, we're flying four cameras that can measure in seven different wavelength ranges. 34 00:02:11.230 --> 00:02:14.580 And that gives us more information about the kinds of structures that we're going to see. 35 00:02:14.580 --> 00:02:18.750 The corona could hold clues to what creates solar wind, 36 00:02:18.750 --> 00:01:58.830 the stream of charged particles coming from the Sun that can cause auroras, 37 00:01:58.830 --> 00:02:27.520 but also potential threats to our satellites and astronauts. 38 00:02:27.520 --> 00:02:30.830 The Sun can also affect technology closer to home 39 00:02:30.830 --> 00:02:34.340 and the eclipse allows scientists to analyze those changes. 40 00:02:34.340 --> 00:02:37.330 Beneath the plane, the team led by Virginia Tech 41 00:02:37.330 --> 00:02:40.020 will mount an instrument called an ionosonde 42 00:02:40.020 --> 00:02:45.910 to study how the Moon’s shadow will affect Earth’s upper atmosphere known as the ionosphere. 43 00:02:45.910 --> 00:02:49.420 This is an electrically charged region of the upper atmosphere 44 00:02:49.420 --> 00:02:52.000 where GPS signals and radio waves travel. 45 00:02:52.000 --> 00:02:55.810 So during the eclipse, when the Moon casts a dark shadow on Earth, 46 00:02:55.810 --> 00:03:00.020 scientists will see how that lack of solar radiation changes the ionosphere.  47 00:03:00.020 --> 00:03:07.760 Sometimes GPS systems can be adversely impacted because of certain perturbations or variations in the ionosphere. 48 00:03:07.760 --> 00:03:14.180 So, using this experiment, we can characterize and understand how changes in the solar radiation 49 00:03:14.180 --> 00:03:18.470 can impact some of these technologies that we rely on in our daily lives. 50 00:03:18.470 --> 00:03:25.320 Being in the air not only gives the teams a better vantage point, but it gives them a longer eclipse too. 51 00:03:25.320 --> 00:03:28.600 One of the main advantages of flying the instrument on the plane 52 00:03:28.600 --> 00:03:32.960 is that you will be able to track the totality over an extended interval of time. 53 00:03:32.960 --> 00:03:37.880 The jets will launch from NASA’s Johnson Space Center in Houston, Texas, 54 00:03:37.880 --> 00:03:40.570 and travel 460 miles per hour 55 00:03:40.570 --> 00:03:45.500 allowing them to briefly chase the Moon’s shadow as it sweeps across Mexico and Texas. 56 00:03:45.500 --> 00:03:51.500 This means the instruments will observe the eclipse 25% longer than from the ground, 57 00:03:51.500 --> 00:03:54.880 giving these teams a unique chance to do science. 58 00:03:54.880 --> 00:03:58.500 We might not actually even know what we're going to see. 59 00:03:58.500 --> 00:04:00.460 And that's part of the excitement 60 00:04:00.460 --> 00:04:02.470 is opening brand new discovery space 61 00:04:02.470 --> 00:04:06.000 and learning new things about the Sun. 62 00:04:06.000 --> 00:04:19.483