1 00:00:00,010 --> 00:00:04,140 2 00:00:04,160 --> 00:00:08,200 Astronomers use radio telescopes to study distant stars and galaxies. 3 00:00:08,220 --> 00:00:12,210 They use a band of microwave frequencies reserved for scientists 4 00:00:12,230 --> 00:00:16,290 studying the heavens and the earth. 5 00:00:16,310 --> 00:00:20,320 By international treaty there are no transmissions allowed in this band, so I can't set up a television transmitter, 6 00:00:20,340 --> 00:00:24,360 say, and operate here. It's dedicated, set aside, 7 00:00:24,380 --> 00:00:28,370 for what we call "passive use," or in this case the microwave radiometer 8 00:00:28,390 --> 00:00:32,480 listening to the natural signals from the Earth. 9 00:00:32,500 --> 00:00:36,480 NASA is using this band to study the water content of soil for its 10 00:00:36,500 --> 00:00:40,520 Earth-observing SMAP mission, which stands for "Soil Moisture Active Passive." 11 00:00:40,540 --> 00:00:44,530 The "active passive" part really refers to the instrument, 12 00:00:44,550 --> 00:00:48,540 so the active portion is a microwave radar, 13 00:00:48,560 --> 00:00:52,540 and the passive portion is a microwave radiometer that we built here at Goddard Space Flight Center. 14 00:00:52,560 --> 00:00:56,610 15 00:00:56,630 --> 00:01:00,610 Every molecule naturally gives off or absrobs microwave energy 16 00:01:00,630 --> 00:01:04,610 to maintain a balance with its surroundings. The amount given off 17 00:01:04,630 --> 00:01:08,620 by the soil depend on its temperature and its water content. The molecules in the soil 18 00:01:08,640 --> 00:01:12,630 with the water, they're bouncing around off of each other and emitting microwaves. 19 00:01:12,650 --> 00:01:16,640 The dry soil lets out a lot of these microwaves and the wetter soil lets out 20 00:01:16,660 --> 00:01:20,640 fewer of these microwaves. The challenge is that the neighboring bands 21 00:01:20,660 --> 00:01:24,640 have radars and communications systems 22 00:01:24,660 --> 00:01:28,650 and those transmissions can unintentionally leak into our spectrum. 23 00:01:28,670 --> 00:01:32,650 So we had to develop dedicated technology for SMAP 24 00:01:32,670 --> 00:01:36,670 to try to separate out the 25 00:01:36,690 --> 00:01:40,670 natural signals from the earth and the human-made signals 26 00:01:40,690 --> 00:01:44,690 that we don't want. The signals that we want 27 00:01:44,710 --> 00:01:48,730 the SMAP radiometer to listen to, they vary slowly in time. 28 00:01:48,750 --> 00:01:52,740 they are very broadband. And in fact what they are is, 29 00:01:52,760 --> 00:01:56,780 it sounds like - if you were to hook up a radio receiver and listen to it 30 00:01:56,800 --> 00:02:00,980 yourself, it would sound like noise, it would sound like static. 31 00:02:01,000 --> 00:02:04,990 So we look for signals that don't look like static and that's what we want to throw away 32 00:02:05,010 --> 00:02:09,180 and keep the static for ourselves. 33 00:02:09,200 --> 00:02:13,200 So the team here at Goddard developed specialized hardare and software. 34 00:02:13,220 --> 00:02:17,230 It separates out the signals that the radiometer receives in time and frequency 35 00:02:17,250 --> 00:02:21,230 and for every spot on the ground, 36 00:02:21,250 --> 00:02:25,240 looks for outliers and if it sees those, it just removes them from the measurement. 37 00:02:25,260 --> 00:02:29,240 Throws away the bad, keeps the good, and produces the data 38 00:02:29,260 --> 00:02:33,250 to give us good measurements of soil moisture here today 39 00:02:33,270 --> 00:02:37,250 to allow us to improve weather forecasting, drought and flood predictions, 40 00:02:37,270 --> 00:02:41,300 and forecast crop yields better. 41 00:02:41,320 --> 00:02:53,687