WEBVTT FILE 1 00:00:00.433 --> 00:00:04.037 How do these features in the solar corona, this atmosphere of the Sun, 2 00:00:04.204 --> 00:00:05.772 how do those change? 3 00:00:05.772 --> 00:00:09.809 Sometimes they escape from the Sun. Sometimes they go back towards the Sun. 4 00:00:10.243 --> 00:00:13.246 And that region is hard to really study. 5 00:00:13.480 --> 00:00:16.850 And we're going to get this little glimpse from Earth. 6 00:00:16.850 --> 00:00:18.551 My name is Laura Peticolas, 7 00:00:18.551 --> 00:00:22.822 and I am the principal investigator for the Eclipse Megamovie 2024 project. 8 00:00:23.323 --> 00:00:28.094 So, what's really unique about the eclipse, especially one like the one coming up, 9 00:00:28.361 --> 00:00:32.665 is that it's covering a very large path on land. 10 00:00:32.932 --> 00:00:34.701 And that means a lot of observers 11 00:00:34.701 --> 00:00:38.004 can be viewing it over an extended period of time. 12 00:00:38.438 --> 00:00:43.810 In this case, we are able to take images along that entire path in ways 13 00:00:43.810 --> 00:00:48.815 that you can't just do from one location on Earth or one location in space. 14 00:00:49.015 --> 00:00:51.184 And that gives us this really unique dataset. 15 00:00:52.018 --> 00:00:55.989 In 2017, we made a movie of all the images. 16 00:00:55.989 --> 00:01:00.760 This time, we know how to make the movie more dynamic 17 00:01:00.894 --> 00:01:04.631 and we're going to have more exposures, meaning that we'll be able 18 00:01:04.631 --> 00:01:08.001 to see more of the features in the solar corona than we were before. 19 00:01:08.368 --> 00:01:13.239 And, although it's maybe not what one might think in terms of a movie, 20 00:01:13.239 --> 00:01:17.277 in terms of people and a plot, but for us solar physicists, 21 00:01:17.510 --> 00:01:19.145 it is very exciting to see 22 00:01:19.145 --> 00:01:22.415 even the smallest changes in the corona at the timescale we're going to get.