WEBVTT FILE 1 00:00:00.000 --> 00:00:01.310 2 00:00:01.330 --> 00:00:03.300 Every one of the instruments on here 3 00:00:03.320 --> 00:00:06.320 has had to be spec'd to work 4 00:00:06.340 --> 00:00:08.540 at phenomenal levels. 5 00:00:08.560 --> 00:00:11.210 So we're going to be flying in the background atmosphere. 6 00:00:11.230 --> 00:00:13.450 That usually means there's very little 7 00:00:13.470 --> 00:00:15.450 of whatever you're trying to measure. 8 00:00:15.470 --> 00:00:16.980 For something like CO2 9 00:00:17.000 --> 00:00:18.450 we need such high sensitivity - 10 00:00:18.470 --> 00:00:20.630 there's lots of CO2 there, 11 00:00:20.650 --> 00:00:23.690 so every tiny change in it makes a difference. 12 00:00:23.710 --> 00:00:25.220 For something like ozone, 13 00:00:25.240 --> 00:00:27.470 we're going to be looking at very small numbers 14 00:00:27.490 --> 00:00:29.000 in the background atmosphere. 15 00:00:29.020 --> 00:00:32.000 For something like NOx, NO and NO2, 16 00:00:32.020 --> 00:00:34.810 the numbers are the lowest, even today, 17 00:00:34.830 --> 00:00:36.810 the lowest that instrument has ever measured 18 00:00:36.830 --> 00:00:38.490 was earlier on in the flight today. 19 00:00:38.510 --> 00:00:41.470 So the instrument is a cavity enhanced system, 20 00:00:41.490 --> 00:00:43.370 so we take light from the laser 21 00:00:43.390 --> 00:00:45.570 and put it through a sampling cell. 22 00:00:45.590 --> 00:00:48.850 And then we look and see how much light disappears 23 00:00:48.870 --> 00:00:50.590 when we have a certain amount 24 00:00:50.610 --> 00:00:53.380 of any of the four gases that we measure. 25 00:00:53.400 --> 00:00:55.250 For a given amount of CO2 26 00:00:55.270 --> 00:00:56.720 that's in the atmosphere, 27 00:00:56.740 --> 00:00:58.380 a certain amount will be absorbed 28 00:00:58.400 --> 00:00:59.620 of the laser light 29 00:00:59.640 --> 00:01:01.130 and then we can tell from that 30 00:01:01.150 --> 00:01:02.990 how much CO2 there is. 31 00:01:03.010 --> 00:01:05.630 We do a lot of profiles over TCCON sites, 32 00:01:05.650 --> 00:01:08.440 which are sites that look up at the sun 33 00:01:08.460 --> 00:01:11.780 and give us a total column of CO2 and methane 34 00:01:11.800 --> 00:01:14.540 between that site and the sun. 35 00:01:14.560 --> 00:01:18.040 But we also fly underneath some of the satellites. 36 00:01:18.060 --> 00:01:20.320 So today we've been doing an underpass 37 00:01:20.340 --> 00:01:22.580 under the OCO-2 satellite, 38 00:01:22.600 --> 00:01:25.460 where they measure CO2 columns. 39 00:01:25.480 --> 00:01:27.630 So we'll be sending all of the CO2 profiles 40 00:01:27.650 --> 00:01:28.900 that we measure 41 00:01:28.920 --> 00:01:31.170 to the OCO2 team 42 00:01:31.190 --> 00:01:33.880 to help with the validation of their instrument. 43 00:01:33.900 --> 00:01:35.930 A project like ATom 44 00:01:35.950 --> 00:01:38.580 is ideally suited for that, 45 00:01:38.600 --> 00:01:40.830 so it just takes a little extra coordination 46 00:01:40.850 --> 00:01:43.110 to try and get the most out of that. 47 00:01:43.130 --> 00:01:44.340 Looking at the real time data 48 00:01:44.360 --> 00:01:46.030 does give us ideas about 49 00:01:46.050 --> 00:01:47.780 what we should be interested in 50 00:01:47.800 --> 00:01:49.480 when it comes to looking at the data. 51 00:01:49.500 --> 00:01:51.680 Because there is a huge amount of data 52 00:01:51.700 --> 00:01:54.350 that's going to be produced from ATom, 53 00:01:54.370 --> 00:01:56.310 so I think there'll be a lot 54 00:01:56.330 --> 00:01:58.370 of the wider science community 55 00:01:58.390 --> 00:02:00.210 who end up using this data set, 56 00:02:00.230 --> 00:02:02.230 and I can see it being invaluable 57 00:02:02.250 --> 00:02:05.230 to all the modeling community. 58 00:02:05.250 --> 00:02:06.440 From what I've heard from them, 59 00:02:06.460 --> 00:02:08.870 they are very excited about the whole project. 60 00:02:08.890 --> 00:02:15.716