WEBVTT FILE 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