WEBVTT FILE 1 00:00:05.270 --> 00:00:07.480 What will be the best outcome of the GOLD mission? 2 00:00:07.500 --> 00:00:10.750 The best outcome for the GOLD mission will be a comprehensive understanding 3 00:00:10.770 --> 00:00:12.920 of the thermosphere and ionosphere 4 00:00:12.940 --> 00:00:17.340 and how it responds to geomagnetic storms, plasma bubbles, 5 00:00:17.360 --> 00:00:19.770 and forcing from below like waves and tides 6 00:00:19.790 --> 00:00:22.560 and that’s what we really hope to get out of this. 7 00:00:22.580 --> 00:00:24.700 What can GOLD bring to the science community? 8 00:00:24.720 --> 00:00:29.380 GOLD is an unprecedented opportunity to look at the full disk of the Americas 9 00:00:29.400 --> 00:00:34.050 that we can look at the temperature and composition of the thermosphere and ionosphere 10 00:00:34.070 --> 00:00:37.150 and this will really help us study things like geomagnetic storms, 11 00:00:37.170 --> 00:00:42.660 plasma bubbles and the waves and tides that propagate from up from below. 12 00:00:42.680 --> 00:00:44.920 Why should we learn about the ionosphere and thermosphere? 13 00:00:44.940 --> 00:00:47.830 The ionosphere and thermosphere are part our near-space environment 14 00:00:47.850 --> 00:00:51.820 and this is the region where communication and navigation signals have to transit 15 00:00:51.840 --> 00:00:56.300 and when they do they can be impacted by different kinds of variability that happens there. 16 00:00:56.320 --> 00:00:58.870 And when there is variability you can get errors 17 00:00:58.890 --> 00:01:03.770 and so the idea is to be able to forecast this variability and mitigate those errors. 18 00:01:03.790 --> 00:01:05.910 What does GOLD do that has never been done before? 19 00:01:05.930 --> 00:01:08.150 What GOLD does that’s never been done before 20 00:01:08.170 --> 00:01:14.050 is take high resolution images of the full disk at a really high time frequency 21 00:01:14.070 --> 00:01:14.890 - every 30 minutes. 22 00:01:14.910 --> 00:01:19.400 So we’re going to be able to see the dramatic changes that happen on daily to hourly scales 23 00:01:19.420 --> 00:01:21.929 and that’s something we’ve never been able to do before.