1 00:00:00,200 --> 00:00:04,360 [ music ] VO: The ATLAS instrument 2 00:00:04,380 --> 00:00:08,540 on the ICESat-2 satellite measures elevation by timing the 3 00:00:08,560 --> 00:00:12,690 flight of laser light pulses that leave the satellite, bounce off 4 00:00:12,710 --> 00:00:16,750 the surface and return to ATLAS. The speed of light is very 5 00:00:16,770 --> 00:00:20,820 fast, and so a regular stopwatch would give us too wide a range 6 00:00:20,840 --> 00:00:24,890 of time, a big margin of error. The timing has to be ultra- 7 00:00:24,910 --> 00:00:32,050 precise, less than one billionth of a second, in order the measure the height of the 8 00:00:32,070 --> 00:00:36,250 surface within just a few centimeters. Phil: I'm Phil Luers. I'm deputy instrument 9 00:00:36,270 --> 00:00:40,320 systems engineer on the ICESat-2 mission. Calculating the elevation of the ice 10 00:00:40,340 --> 00:00:44,370 is all about time of flight. It's time of flight of the photon from the laser 11 00:00:44,390 --> 00:00:48,400 down to the surface of the ice and back. So what 12 00:00:48,420 --> 00:00:52,470 we are doing is creating time tags of the 13 00:00:52,490 --> 00:00:56,590 transmit, when the laser fires, and time tags of the receipt of the photon. 14 00:00:56,610 --> 00:01:00,700 So it's all starts with the transmitter. When the laser fires, 15 00:01:00,720 --> 00:01:04,860 it puts out billions and billions of photons, and we pick off a little bit of that and we send it to a 16 00:01:04,880 --> 00:01:09,030 detector, and we produce a start pulse, and that is the start of our timing system. 17 00:01:09,050 --> 00:01:13,180 The spacecraft sends us a position and attitude message every second 18 00:01:13,200 --> 00:01:17,390 that tells us where we are in the orbit. From that we calculate where we 19 00:01:17,410 --> 00:01:21,390 think the spots are on the ground. We have a rough database of the whole 20 00:01:21,410 --> 00:01:25,410 Earth with elevation as it travels up and down mountains and down into valleys and over 21 00:01:25,430 --> 00:01:29,430 ice sheets. For each spot, we calculate where we think the surface is 22 00:01:29,450 --> 00:01:33,500 and we open up a range window. For every photon that's received in 23 00:01:33,520 --> 00:01:37,680 that range window, we produce a time tag. 24 00:01:37,700 --> 00:01:41,720 Now the Sun produces a lot of green photons too, 25 00:01:41,740 --> 00:01:45,750 many more than our laser does. So our laser produces billions and 26 00:01:45,770 --> 00:01:49,880 billions of photons with every shot. If you add the noise in there, you won't 27 00:01:49,900 --> 00:01:54,010 be able to tell the Sun's photons from the laser photons. 28 00:01:54,030 --> 00:01:58,200 So if you just took one shot, the one laser photon would be lost in the 29 00:01:58,220 --> 00:02:04,180 noise, but if you take took two hundred shots, now finally you have enough surface signal 30 00:02:04,200 --> 00:02:08,200 coming up out of the noise that flight software on board can pick out "this is noise, 31 00:02:08,220 --> 00:02:12,290 and this is the signal from the surface." Once we downlink the photon time tags from 32 00:02:12,310 --> 00:02:16,400 the receiver and the transmitter and we have the range windows, we put those all together 33 00:02:16,420 --> 00:02:20,430 you have the transmit time tags, you have the time until the range window 34 00:02:20,450 --> 00:02:24,470 opened, you have the received time tags in the range window. You 35 00:02:24,490 --> 00:02:28,520 calculate all that put together gives you the time of flight of a photon, 36 00:02:28,540 --> 00:02:32,580 which ultimately gives you the distance between the spacecraft and the ground. 37 00:02:32,600 --> 00:02:36,620 So if you know where the spacecraft is, and you know the time of flight, you know the distance 38 00:02:36,640 --> 00:02:40,660 to the ground, now you have the elevation of the ice. 39 00:02:40,680 --> 00:02:44,710 VO: Technology that can measure elevation adds a third dimension 40 00:02:44,730 --> 00:02:48,770 to how we map our Earth, and allows us to study change 41 00:02:48,790 --> 00:02:52,940 across the poles and beyond. 42 00:02:52,960 --> 00:02:56,950 [ music, beeping ] 43 00:02:56,970 --> 00:03:01,000 [ beeping ] 44 00:03:01,020 --> 00:03:04,665