1 00:00:00,067 --> 00:00:01,835 So our primary mission here is 2 00:00:01,835 --> 00:00:03,270 satellite validation. 3 00:00:03,270 --> 00:00:06,506 So we just launched this next generation system and in order 4 00:00:06,506 --> 00:00:11,912 to validate its performance independently we've got our 5 00:00:11,912 --> 00:00:16,583 aircraft sensor with well calibrated instruments and we 6 00:00:16,583 --> 00:00:19,753 use that to give us high confidence--we're flying very 7 00:00:19,753 --> 00:00:23,557 high in the atmosphere--and it gives us very good comparisons to what 8 00:00:23,557 --> 00:00:25,259 the satellite is seeing. 9 00:00:25,259 --> 00:00:31,231 Today we're doing a mission, uh....wheels up...from Warner Robins 10 00:00:31,231 --> 00:00:34,568 Georgia...Air Force Base at seventeen hundred... 11 00:00:34,568 --> 00:00:37,838 ...we do have another long wave trough beginning to approach the 12 00:00:37,838 --> 00:00:41,909 West Coast later in the period by day 7, indicating that the 13 00:00:41,909 --> 00:00:43,343 wave train is back. 14 00:00:43,343 --> 00:00:47,114 So, the "go, no-go" decision is 100% dependent, of course, from 15 00:00:47,114 --> 00:00:48,048 day to day on each mission. 16 00:00:48,048 --> 00:00:52,252 Today, the reason we decided on a "go" is because we're in 17 00:00:52,252 --> 00:00:55,555 Huntsville and we have a very long loiter time over this 18 00:00:55,555 --> 00:00:56,223 location. 19 00:00:56,223 --> 00:00:59,660 And we have an "LMA" and a pretty intense instrument 20 00:00:59,660 --> 00:01:00,294 network here. 21 00:01:00,294 --> 00:01:04,731 Even though the case itself is not great--we're not expecting a 22 00:01:04,731 --> 00:01:08,001 ton of lightning with these systems-- we can still get some 23 00:01:08,001 --> 00:01:09,503 really good data out of it. 24 00:01:09,503 --> 00:01:11,972 So it looks like the mission's a go. 25 00:01:12,005 --> 00:01:13,407 Any instrument teams have any...questions? 26 00:01:13,407 --> 00:01:17,010 (music) 27 00:01:17,044 --> 00:01:23,617 We've coordinated ABI, special scans, 30 second imagery, uh, 17 28 00:01:23,617 --> 00:01:26,820 Zulu to 2230 Zulu today. 29 00:01:26,853 --> 00:01:31,792 We're getting a little bit of what's called potential energy--we call it 30 00:01:31,792 --> 00:01:34,328 convective potential energy, and it's helping fire up these 31 00:01:34,361 --> 00:01:35,028 storms. 32 00:01:35,062 --> 00:01:37,731 And so this is what the models were kind of picking up on 33 00:01:37,764 --> 00:01:38,665 earlier. 34 00:01:38,699 --> 00:01:39,967 We call it convective initiation. 35 00:01:40,000 --> 00:01:43,170 That's what today's mission is really geared toward. 36 00:01:43,170 --> 00:01:50,277 Yeah, yeah, so I got the satellite, the visible, and then 37 00:01:50,277 --> 00:01:52,012 I got CPL... 38 00:01:52,646 --> 00:01:55,315 The GLM--the Geostationary Lightning Mapper--is an optical 39 00:01:55,349 --> 00:02:01,888 instrument and we have virtually no other optical measurement to 40 00:02:01,922 --> 00:02:05,325 corroborate what the GLM is seeing except for an instrument 41 00:02:05,359 --> 00:02:07,527 that we've developed for the airplane. 42 00:02:07,561 --> 00:02:10,364 So we're looking down on cloud top at lightning. 43 00:02:10,397 --> 00:02:12,799 Some things that we've shown is that if you're able to 44 00:02:12,833 --> 00:02:15,769 incorporate lightning into a forecasting environment we can 45 00:02:15,802 --> 00:02:19,106 do things like increase lead time before severe weather hits, 46 00:02:19,139 --> 00:02:21,908 decrease false alarm rates we're able to forecast severe weather 47 00:02:21,942 --> 00:02:25,045 a lot better, which of course means time and, maybe more 48 00:02:25,078 --> 00:02:26,847 importantly, saving lives. 49 00:02:26,880 --> 00:02:29,016 So we don't know where the lightning originated. 50 00:02:29,049 --> 00:02:32,686 So the GLM gives us where the flashes are beginning, where 51 00:02:32,686 --> 00:02:35,355 they're propagating, and then with the ground based you can 52 00:02:35,389 --> 00:02:37,157 tell where they went to ground, 53 00:02:37,190 --> 00:02:40,861 so if you're, say, at an airport, baggage handling, 54 00:02:40,894 --> 00:02:44,431 fueling, you're outdoors, you may not realize you have a 55 00:02:44,464 --> 00:02:48,535 non-zero risk above you of the lightning propagating overhead 56 00:02:48,568 --> 00:02:52,039 or coming from some distance away, and so the GLM can help us 57 00:02:52,072 --> 00:02:55,275 depict that and improve your situational awareness. 58 00:02:55,308 --> 00:02:59,513 (off mic voices) 59 00:02:59,513 --> 00:03:02,015 The data coming from this system is just phenomenal. 60 00:03:02,015 --> 00:03:08,321 We're seeing data at three times the data rate, double the 61 00:03:08,355 --> 00:03:13,293 resolution typically, and it's just meteorologically, we're 62 00:03:13,627 --> 00:03:17,497 seeing features that we have never, necessarily, noticed 63 00:03:17,531 --> 00:03:20,667 before from the longer lag data from the previous satellite 64 00:03:20,700 --> 00:03:22,002 systems. 65 00:03:25,005 --> 00:03:28,008 The advantage of having a high altitude aircraft is that we can 66 00:03:28,041 --> 00:03:34,648 make, as best we can, a measurement that mimics what the 67 00:03:34,681 --> 00:03:36,349 satellite is seeing. 68 00:03:36,383 --> 00:03:41,154 (music) 69 00:03:41,188 --> 00:03:42,522 We're at seventy thousand feet, your typical 70 00:03:42,556 --> 00:03:46,426 airliner is down around thirty-five thousand feet. 71 00:03:46,460 --> 00:03:50,197 If we sit here on the ground and we see an airliner way up high 72 00:03:50,230 --> 00:03:54,401 making a contrail, we look down from the U2 almost from the same 73 00:03:54,434 --> 00:03:57,370 distance and see that airliner well below us making contrails 74 00:03:57,404 --> 00:03:59,539 So we're twice as high as an airliner. 75 00:03:59,573 --> 00:04:27,334 (music) 76 00:04:27,334 --> 00:04:30,270 So what this is going to enable people to do is see 77 00:04:30,303 --> 00:04:33,840 mesoscale features that we really didn't have a good handle 78 00:04:33,874 --> 00:04:34,708 on. 79 00:04:34,741 --> 00:04:39,713 And that's why having the aircraft in place, it allows us 80 00:04:39,746 --> 00:04:45,352 to get deeper insights into this phenomenology that's kind of new 81 00:04:45,385 --> 00:04:47,687 to us because we've never been able to stare at the Earth with 82 00:04:47,721 --> 00:04:48,788 this kind of resolution. 83 00:04:48,822 --> 00:04:55,028 (jet engine) 84 00:04:55,061 --> 00:04:56,696 Pogo clear! 85 00:04:56,730 --> 00:05:13,380 (music) 86 00:05:13,413 --> 00:05:16,816 Flying really high in the stratosphere, at twenty 87 00:05:16,850 --> 00:05:21,821 kilometers--what that enables us to do is overfly a target of 88 00:05:21,855 --> 00:05:25,525 interest and match the view geometry of the satellite and 89 00:05:25,559 --> 00:05:29,563 that gives us very high confidence that we're collecting 90 00:05:29,596 --> 00:05:31,998 what the satellite is seeing. 91 00:05:32,032 --> 00:05:47,013 (music)