1 00:00:03,990 --> 00:00:01,829 sa stands for stratospheric aerosol and 2 00:00:05,550 --> 00:00:04,000 gas experiment it's the third generation 3 00:00:11,990 --> 00:00:05,560 so we call it sage iii 4 00:00:15,589 --> 00:00:12,000 [Music] 5 00:00:18,150 --> 00:00:15,599 what it does is it looks at ozone 6 00:00:20,150 --> 00:00:18,160 water vapor aerosols in the atmosphere 7 00:00:22,390 --> 00:00:20,160 using a solar occultation technique so 8 00:00:24,550 --> 00:00:22,400 it locked onto the sun or the moon and 9 00:00:25,910 --> 00:00:24,560 it tracks that as it does as it rises 10 00:00:27,750 --> 00:00:25,920 through the atmosphere or sets through 11 00:00:30,230 --> 00:00:27,760 the atmosphere of the planet so that we 12 00:00:32,470 --> 00:00:30,240 can get vertical profiles of those gases 13 00:00:34,150 --> 00:00:32,480 more specifically it's ozone that we're 14 00:00:36,630 --> 00:00:34,160 really tracking 15 00:00:38,950 --> 00:00:36,640 we hope to see recovering ozone 16 00:00:40,630 --> 00:00:38,960 throughout the entire stratosphere so 17 00:00:42,389 --> 00:00:40,640 and you know ozone's very important it 18 00:00:44,389 --> 00:00:42,399 protects us from the uv radiation 19 00:00:47,190 --> 00:00:44,399 without that protection we would have 20 00:00:49,270 --> 00:00:47,200 lowered crop yields you know our plants 21 00:00:50,950 --> 00:00:49,280 really don't like uv radiation and we 22 00:00:53,510 --> 00:00:50,960 would have problems too we would have 23 00:00:55,590 --> 00:00:53,520 more skin cancers and cataracts so we 24 00:00:57,670 --> 00:00:55,600 really need that ozone layer in the 25 00:00:59,590 --> 00:00:57,680 stratosphere to protect us i've been 26 00:01:01,830 --> 00:00:59,600 working on this for 20 years now and 27 00:01:03,349 --> 00:01:01,840 it's it's it's going to be amazing to 28 00:01:06,310 --> 00:01:03,359 watch it up there and you know get up