1 00:00:01,280 --> 00:00:02,310 - [Amanda] Hi, everyone. 2 00:00:02,310 --> 00:00:03,670 My name is Amanda Armstrong, 3 00:00:03,670 --> 00:00:05,440 and I will be your instructor for this course, 4 00:00:05,440 --> 00:00:07,490 remote sensing foundations. 5 00:00:07,490 --> 00:00:10,260 In this first lecture, we will be moving pretty quickly 6 00:00:10,260 --> 00:00:12,240 from particle physics to Google Earth Engine, 7 00:00:12,240 --> 00:00:15,340 as we dive into the exciting world of remote sensing. 8 00:00:15,340 --> 00:00:16,990 Upon completion of this module, 9 00:00:16,990 --> 00:00:20,880 my hope is that you will be able to define remote sensing, 10 00:00:20,880 --> 00:00:23,710 define how and where remote sensing is used in industry, 11 00:00:23,710 --> 00:00:26,370 science and commercial applications, 12 00:00:26,370 --> 00:00:28,120 name and define the components 13 00:00:28,120 --> 00:00:30,420 of the electromagnetic spectrum, 14 00:00:30,420 --> 00:00:33,050 understand how energy and matter interact 15 00:00:33,050 --> 00:00:35,070 with surface terrain, 16 00:00:35,070 --> 00:00:36,260 understand and distinguish 17 00:00:36,260 --> 00:00:38,310 between active and passive sensors 18 00:00:38,310 --> 00:00:40,530 and what they are used to measure. 19 00:00:40,530 --> 00:00:43,540 And finally, let's get your Google Earth Engine 20 00:00:43,540 --> 00:00:44,543 account set up. 21 00:00:45,910 --> 00:00:46,833 Let's get started. 22 00:00:49,980 --> 00:00:51,850 So what is remote sensing? 23 00:00:51,850 --> 00:00:53,560 Perhaps the most simplified definition 24 00:00:53,560 --> 00:00:55,140 would be the collection of information 25 00:00:55,140 --> 00:00:58,060 about an object without making physical contact with it. 26 00:00:58,060 --> 00:00:59,880 However, for the purposes of this course 27 00:00:59,880 --> 00:01:00,950 I'd like to add some words 28 00:01:00,950 --> 00:01:02,860 onto the front end of that definition. 29 00:01:02,860 --> 00:01:05,480 So I think of it more as the science of identifying, 30 00:01:05,480 --> 00:01:07,480 observing, collecting, and measuring objects 31 00:01:07,480 --> 00:01:10,620 without coming into direct contact with them. 32 00:01:10,620 --> 00:01:12,770 Did you know that a remote sensing is accomplished 33 00:01:12,770 --> 00:01:14,830 by humans and animals with the aid of our eyes 34 00:01:14,830 --> 00:01:17,913 and other senses, like smell and hearing, every day. 35 00:01:19,220 --> 00:01:21,370 And another important point that I wanna make, 36 00:01:21,370 --> 00:01:23,840 is that satellites don't actually take pictures 37 00:01:23,840 --> 00:01:26,250 of our planet, but what they do is they record 38 00:01:26,250 --> 00:01:28,440 the electromagnetic energy that's reflected 39 00:01:28,440 --> 00:01:30,853 or admitted from objects on earth. 40 00:01:33,290 --> 00:01:37,230 So which industries and careers utilize remote sensing? 41 00:01:37,230 --> 00:01:39,640 I won't read this slide to you, but as you can see, 42 00:01:39,640 --> 00:01:42,660 remote sensing analysis is used in many sectors, 43 00:01:42,660 --> 00:01:46,320 and where it is used is growing every year. 44 00:01:46,320 --> 00:01:49,210 From commercial to nonprofit, to science, 45 00:01:49,210 --> 00:01:50,763 to engineering and medicine. 46 00:01:51,920 --> 00:01:55,090 There are a whole host of different career options 47 00:01:55,090 --> 00:01:58,853 for those that have a background in remote sensing analysis. 48 00:02:01,010 --> 00:02:03,520 Okay, so let's delve a little bit deeper 49 00:02:03,520 --> 00:02:05,740 into some of the science 50 00:02:05,740 --> 00:02:08,740 behind what we are measuring in remote sensing. 51 00:02:08,740 --> 00:02:11,190 I remember when I took my first remote sensing course 52 00:02:11,190 --> 00:02:12,160 in graduate school, 53 00:02:12,160 --> 00:02:13,820 we spent the first month or so of class 54 00:02:13,820 --> 00:02:15,280 brushing up on physics, 55 00:02:15,280 --> 00:02:16,180 which might not sound 56 00:02:16,180 --> 00:02:18,080 related to the study of measuring objects 57 00:02:18,080 --> 00:02:20,580 without coming into direct contact with them. 58 00:02:20,580 --> 00:02:22,830 But in order to understand what we are measuring 59 00:02:22,830 --> 00:02:25,150 when a satellite measures the surface of the earth, 60 00:02:25,150 --> 00:02:26,960 we need to go back to some of the basics 61 00:02:26,960 --> 00:02:29,560 of particle physics and our understanding of energy. 62 00:02:30,490 --> 00:02:33,530 A quark is one of the fundamental particles in physics. 63 00:02:33,530 --> 00:02:34,970 Fundamental means that the particle 64 00:02:34,970 --> 00:02:36,380 does not have a substructure. 65 00:02:36,380 --> 00:02:38,080 So it cannot be split. 66 00:02:38,080 --> 00:02:40,760 Quarks are the fundamental building blocks 67 00:02:40,760 --> 00:02:43,170 of all particles that we know of. 68 00:02:43,170 --> 00:02:46,710 They join to form subatomic structures 69 00:02:46,710 --> 00:02:48,570 such as protons and neutrons 70 00:02:48,570 --> 00:02:51,900 which are components of the nuclei of atoms. 71 00:02:51,900 --> 00:02:55,200 Quarks are known to be one of the fundamental particles 72 00:02:55,200 --> 00:02:56,033 that interact 73 00:02:56,033 --> 00:02:58,400 through all four fundamental forces of physics. 74 00:02:58,400 --> 00:03:00,940 Gravitation, electromagnetism, 75 00:03:00,940 --> 00:03:03,610 and the strong and weak interactions. 76 00:03:03,610 --> 00:03:05,210 Though the measurement of their properties 77 00:03:05,210 --> 00:03:08,430 of mass spin and parity is mostly theoretical, 78 00:03:08,430 --> 00:03:11,740 interactions of quarks is believed to be the foundation 79 00:03:11,740 --> 00:03:13,690 of our knowledge of energy. 80 00:03:13,690 --> 00:03:15,830 Which as I will show you is essential 81 00:03:15,830 --> 00:03:18,580 to understanding the interpreting of satellite imagery. 82 00:03:19,930 --> 00:03:24,040 Okay, so energy is the basis for remote sensing, but how? 83 00:03:24,040 --> 00:03:26,350 Well we know that we can measure the movement 84 00:03:26,350 --> 00:03:30,510 of particles in space, which have a sinusoidal shape. 85 00:03:30,510 --> 00:03:33,320 We can measure their wavelength 86 00:03:34,270 --> 00:03:37,763 which is the distance from one wave crust to another, 87 00:03:39,090 --> 00:03:42,940 and is usually measured in units, like meters or nanometers. 88 00:03:42,940 --> 00:03:44,460 We can also measure their frequency 89 00:03:44,460 --> 00:03:45,730 or the number of crusts 90 00:03:45,730 --> 00:03:49,080 passing a fixed point in a given period of time, 91 00:03:49,080 --> 00:03:52,750 which often measured in hertz units. 92 00:03:52,750 --> 00:03:54,990 And finally, we can also measure their amplitude, 93 00:03:54,990 --> 00:03:56,590 which is the height of each peak 94 00:03:57,440 --> 00:03:59,970 and measured in energy levels. 95 00:03:59,970 --> 00:04:01,950 The greater the amplitude of a wave, 96 00:04:01,950 --> 00:04:04,073 the more energy it is carrying. 97 00:04:06,610 --> 00:04:08,340 When we look at all three together, 98 00:04:08,340 --> 00:04:10,760 we can see how wavelength and frequency range 99 00:04:10,760 --> 00:04:12,950 from low to high energy states. 100 00:04:12,950 --> 00:04:15,450 This is called the electromagnetic spectrum. 101 00:04:15,450 --> 00:04:18,940 The entire distribution of electromagnetic radiation, 102 00:04:18,940 --> 00:04:21,380 according to frequency or wavelength, 103 00:04:21,380 --> 00:04:24,040 although all electromagnetic waves 104 00:04:24,040 --> 00:04:26,290 travel at the speed of light in a vacuum, 105 00:04:26,290 --> 00:04:29,520 they do so at a wide range of frequencies, 106 00:04:29,520 --> 00:04:31,963 wavelengths and photon energies. 107 00:04:34,620 --> 00:04:37,150 This figure shows some of the most common sources 108 00:04:37,150 --> 00:04:39,170 of electromagnetic energy. 109 00:04:39,170 --> 00:04:42,020 As you can see, we come into contact with a whole suite 110 00:04:42,020 --> 00:04:43,840 of electromagnetic energy emitters, 111 00:04:43,840 --> 00:04:47,380 that emit at varying frequencies and wavelengths every day, 112 00:04:47,380 --> 00:04:49,560 from x-rays to cell phones. 113 00:04:49,560 --> 00:04:53,433 But the most important by far is the sun. 114 00:04:54,940 --> 00:04:56,360 All of the energy from the sun 115 00:04:56,360 --> 00:04:59,150 that reaches the earth arrives as solar radiation, 116 00:04:59,150 --> 00:05:01,740 part of a large collection of energy 117 00:05:01,740 --> 00:05:04,830 called the electromagnetic radiation spectrum. 118 00:05:04,830 --> 00:05:08,280 Solar radiation includes visible light, ultraviolet light, 119 00:05:08,280 --> 00:05:11,450 infrared, radio waves, x-rays and gamma rays. 120 00:05:11,450 --> 00:05:14,363 Radiation is one way to transfer heat and light. 121 00:05:16,320 --> 00:05:18,190 A very simplified view of remote sensing 122 00:05:18,190 --> 00:05:19,500 would be to say that remote sensing 123 00:05:19,500 --> 00:05:22,000 is measuring the reflection of the sun's radiation 124 00:05:22,000 --> 00:05:25,180 as it comes into contact with different surfaces on earth. 125 00:05:25,180 --> 00:05:27,370 However, it is not quite that simple, 126 00:05:27,370 --> 00:05:29,750 because some of the energy that reaches earth 127 00:05:29,750 --> 00:05:32,870 is absorbed and some is reflected back. 128 00:05:32,870 --> 00:05:34,664 The reflected radiation is also absorbed 129 00:05:34,664 --> 00:05:37,490 or scattered on its way back to the sensor. 130 00:05:37,490 --> 00:05:39,240 Spend a minute studying this graphic, 131 00:05:39,240 --> 00:05:40,580 which shows the percentages 132 00:05:40,580 --> 00:05:42,510 of incident and reflected energy, 133 00:05:42,510 --> 00:05:43,970 and you'll begin to understand 134 00:05:43,970 --> 00:05:46,350 why it is necessary to have a grasp of physics 135 00:05:46,350 --> 00:05:48,623 in order to interpret satellite imagery. 136 00:05:52,740 --> 00:05:55,530 It is also important to note that not all of the radiation 137 00:05:55,530 --> 00:05:57,280 reaches the earth surface directly. 138 00:06:01,160 --> 00:06:03,520 In addition, energy from the sun is composed 139 00:06:03,520 --> 00:06:05,123 of many kinds of radiation. 140 00:06:06,000 --> 00:06:07,470 Both in the visible range 141 00:06:07,470 --> 00:06:10,713 and also outside the range of human vision. 142 00:06:12,700 --> 00:06:14,620 This energy is absorbed or scattered 143 00:06:14,620 --> 00:06:17,260 through the atmosphere before it reaches earth. 144 00:06:17,260 --> 00:06:20,750 The sun's energy can therefore be transmitted 145 00:06:20,750 --> 00:06:22,470 which is to pass through the material 146 00:06:22,470 --> 00:06:25,300 or the atmosphere, absorbed, 147 00:06:25,300 --> 00:06:28,440 which is absorbed and converted into other forms of energy, 148 00:06:28,440 --> 00:06:31,540 scattered or deflected in many directions, 149 00:06:31,540 --> 00:06:36,540 reflected which is returned at a given angle or emitted, 150 00:06:37,210 --> 00:06:41,113 which usually is what occurs over longer wavelengths. 151 00:06:45,520 --> 00:06:47,490 By understanding how radiation from the sun 152 00:06:47,490 --> 00:06:50,440 interacts with the atmosphere, then with the earth surfaces, 153 00:06:50,440 --> 00:06:53,480 as well as how it is reflected from the surfaces 154 00:06:53,480 --> 00:06:54,810 back to space. 155 00:06:54,810 --> 00:06:56,940 We can begin to understand the nature of the energy 156 00:06:56,940 --> 00:06:59,140 that is measured by satellite. 157 00:06:59,140 --> 00:07:01,540 Each surface because of its makeup 158 00:07:01,540 --> 00:07:05,100 and texture has what is called a spectral signature. 159 00:07:05,100 --> 00:07:07,770 A spectral signature is a unique distribution 160 00:07:07,770 --> 00:07:10,703 of reflected emitted and absorbed radiation of an object. 161 00:07:12,580 --> 00:07:15,570 Here is a graph that shows the percent reflectance 162 00:07:15,570 --> 00:07:18,410 of some common features on the earth surface. 163 00:07:18,410 --> 00:07:22,310 As you can see, snow and ice are highly reflective 164 00:07:22,310 --> 00:07:23,563 as well as clouds, 165 00:07:24,400 --> 00:07:27,230 whereas clear water and turbid water 166 00:07:27,230 --> 00:07:29,613 have a very low percent reflectance. 167 00:07:33,960 --> 00:07:35,830 You can also imagine that different satellites 168 00:07:35,830 --> 00:07:38,130 are constructed to measure differing ranges 169 00:07:38,130 --> 00:07:39,600 of spectral reflectance, 170 00:07:39,600 --> 00:07:41,110 with high accuracy and precision, 171 00:07:41,110 --> 00:07:44,070 depending on what the satellite is designed to measure. 172 00:07:44,070 --> 00:07:46,100 Here are two quick examples of how scientists 173 00:07:46,100 --> 00:07:49,390 use spectral signatures to understand the earth surfaces. 174 00:07:49,390 --> 00:07:51,810 On the left is a graph showing percent reflectance 175 00:07:51,810 --> 00:07:54,510 of surface features by a Landsat satellite. 176 00:07:54,510 --> 00:07:57,630 The ranges of wavelength are grouped into bands or channels, 177 00:07:57,630 --> 00:07:59,480 with one being visible blue light, 178 00:07:59,480 --> 00:08:03,200 two being green, three red and four near-infrared. 179 00:08:03,200 --> 00:08:06,100 As you can see, vegetation has a high reflection 180 00:08:06,100 --> 00:08:08,990 in the near-infrared channel, band four, 181 00:08:08,990 --> 00:08:10,100 and a low reflection 182 00:08:10,100 --> 00:08:12,890 in the visible red channel, band three. 183 00:08:12,890 --> 00:08:16,060 Water mostly reflects in the visible light range. 184 00:08:16,060 --> 00:08:19,133 So it will look dark in the near-infrared, 185 00:08:20,560 --> 00:08:23,820 vegetation reflects more than soil in the near-infrared 186 00:08:23,820 --> 00:08:25,133 and less than soil in red. 187 00:08:26,380 --> 00:08:30,430 On the right, a study by As-syakur in 2012, 188 00:08:30,430 --> 00:08:31,930 compared spectral signatures 189 00:08:31,930 --> 00:08:34,240 converted to digital number across different bands 190 00:08:34,240 --> 00:08:36,423 or channels using one satellite. 191 00:08:37,310 --> 00:08:41,090 They compared signatures and used them to map, 192 00:08:41,090 --> 00:08:44,953 built up and bear land in an urban area in Bali. 193 00:08:48,620 --> 00:08:51,050 So now that we are gaining a better understanding 194 00:08:51,050 --> 00:08:53,160 of what satellites are actually measuring, 195 00:08:53,160 --> 00:08:55,000 let's talk about how they do it. 196 00:08:55,000 --> 00:08:57,660 There are two main mechanisms for measuring, 197 00:08:57,660 --> 00:08:59,093 active and passive. 198 00:09:01,160 --> 00:09:03,573 Passive sensors rely on natural energy. 199 00:09:05,210 --> 00:09:08,360 So they record energy that is naturally reflected 200 00:09:08,360 --> 00:09:10,403 or admitted from the Earth's surface. 201 00:09:11,580 --> 00:09:14,310 The most common source of radiation is reflected sunlight, 202 00:09:14,310 --> 00:09:16,720 but the downside is that they can only detect energy 203 00:09:16,720 --> 00:09:18,960 when the naturally occurring energy is available. 204 00:09:18,960 --> 00:09:21,090 Or in other words, during the day. 205 00:09:21,090 --> 00:09:23,310 The most popular passive remote sensing 206 00:09:24,160 --> 00:09:26,830 examples of devices are various types 207 00:09:26,830 --> 00:09:28,843 of radiometers and spectrometers. 208 00:09:30,485 --> 00:09:31,650 Some of the instrument names 209 00:09:31,650 --> 00:09:34,240 clearly identify what they measure. 210 00:09:34,240 --> 00:09:39,060 So a spectrometer distinguishes and analyzes spectral bands, 211 00:09:39,060 --> 00:09:40,720 a radiometer on the other hand determines 212 00:09:40,720 --> 00:09:43,160 the power of radiation emitted by the object, 213 00:09:43,160 --> 00:09:45,400 in particular band ranges. 214 00:09:45,400 --> 00:09:48,850 A spectro radiometer finds out the power of radiation 215 00:09:48,850 --> 00:09:50,313 in several band ranges. 216 00:09:51,200 --> 00:09:53,140 Hyperspectral radiometers operate 217 00:09:53,140 --> 00:09:55,840 with the most accurate type of passive sensor 218 00:09:55,840 --> 00:09:57,710 that is used in remote sensing. 219 00:09:57,710 --> 00:09:59,340 Due to extremely high resolution, 220 00:09:59,340 --> 00:10:01,040 it differentiates hundreds 221 00:10:01,040 --> 00:10:03,760 of ultimately narrow spectral bands 222 00:10:03,760 --> 00:10:07,160 within the visible near-infrared and microwave regions. 223 00:10:07,160 --> 00:10:08,940 There is also the imaging radiator, 224 00:10:08,940 --> 00:10:11,963 which scans the object or surface to reproduce the image. 225 00:10:13,657 --> 00:10:15,020 And a sounder which senses 226 00:10:15,020 --> 00:10:17,360 the atmosphere conditions vertically. 227 00:10:17,360 --> 00:10:19,300 Finally, there is also an accelerometer 228 00:10:19,300 --> 00:10:23,390 which detects changes in speed per unit time. 229 00:10:23,390 --> 00:10:26,913 These are all examples of passive remote sensing devices. 230 00:10:28,280 --> 00:10:30,370 However, for the purposes of this course, 231 00:10:30,370 --> 00:10:32,763 and probably one of the most popular ones, 232 00:10:34,100 --> 00:10:37,763 an example of a passive sensor is Landsat. 233 00:10:39,390 --> 00:10:41,940 Landsat definitely stands out as the most 234 00:10:41,940 --> 00:10:44,250 long lasting earth absorbing mission. 235 00:10:44,250 --> 00:10:48,510 It's monitored our planet and recorded the obtained data, 236 00:10:48,510 --> 00:10:50,860 which has enabled us to analyze 237 00:10:50,860 --> 00:10:53,903 the way the planet has changed within a 40 year time span. 238 00:10:55,620 --> 00:10:57,910 One of the mission's great pluses 239 00:10:57,910 --> 00:11:00,970 is that the information is accessible to the public 240 00:11:02,150 --> 00:11:05,230 and with interpretations that are applied regularly 241 00:11:05,230 --> 00:11:09,670 in geology mapping, ecology, forestry, and agriculture, 242 00:11:09,670 --> 00:11:12,620 also in Marine sciences, meteorology, 243 00:11:12,620 --> 00:11:15,040 and other applications as well. 244 00:11:15,040 --> 00:11:18,590 You will most likely be using a lot of Landsat imagery 245 00:11:18,590 --> 00:11:20,423 at times during this course. 246 00:11:22,470 --> 00:11:25,860 Active sensors are the other main category of sensor type. 247 00:11:25,860 --> 00:11:27,760 Each active sensor in remote sensing 248 00:11:27,760 --> 00:11:29,710 directs its signal to the object 249 00:11:29,710 --> 00:11:32,633 and then checks the response or the received quantity. 250 00:11:34,520 --> 00:11:35,670 Active sensors are known 251 00:11:35,670 --> 00:11:38,630 for using artificial forms of energy. 252 00:11:38,630 --> 00:11:40,730 Active remote sensing techniques 253 00:11:40,730 --> 00:11:42,850 differ by what they transmit. 254 00:11:42,850 --> 00:11:44,550 They either transmit lighter waves 255 00:11:44,550 --> 00:11:46,300 and by what they determine, 256 00:11:46,300 --> 00:11:50,070 which can be distance, height or atmospheric conditions. 257 00:11:50,070 --> 00:11:52,530 A few examples include radar. 258 00:11:52,530 --> 00:11:57,020 Radar is a sensor assisting with radio signals. 259 00:11:57,020 --> 00:12:01,540 Its specific feature is the antenna emitting impulses. 260 00:12:01,540 --> 00:12:03,990 When the energy flow and radar active remote sensing 261 00:12:03,990 --> 00:12:04,860 meets an obstacle, 262 00:12:04,860 --> 00:12:08,240 it scatters back to the sensor to some degree. 263 00:12:08,240 --> 00:12:10,640 Based on its amount and traveling time, 264 00:12:10,640 --> 00:12:13,593 it is possible to estimate how far away the target is. 265 00:12:14,460 --> 00:12:17,820 Lidar is another example of an active remote sensor. 266 00:12:17,820 --> 00:12:20,740 Lidar stands for light detection and ranging. 267 00:12:20,740 --> 00:12:23,380 Lidar determines distance with light. 268 00:12:23,380 --> 00:12:24,870 Lidar active remote sensing 269 00:12:24,870 --> 00:12:26,890 implies transmitting light impulses 270 00:12:26,890 --> 00:12:29,630 and checking the quantity retrieved. 271 00:12:29,630 --> 00:12:31,130 The target location and distance 272 00:12:31,130 --> 00:12:33,030 are understood by multiplying the time 273 00:12:33,030 --> 00:12:34,130 by the speed of light. 274 00:12:35,000 --> 00:12:38,650 There is also the laser altimeters, which measure elevation 275 00:12:38,650 --> 00:12:41,340 with lidar and ranging instruments, 276 00:12:41,340 --> 00:12:42,690 which estimate the range 277 00:12:42,690 --> 00:12:45,240 either with one or two identical devices 278 00:12:45,240 --> 00:12:48,373 on different platforms, sending signals to each other. 279 00:12:51,040 --> 00:12:55,040 Apart from a wide variety of implementation, 280 00:12:55,040 --> 00:12:56,500 active remote sensors 281 00:12:56,500 --> 00:13:00,450 basically have no restrictions as to research conditions. 282 00:13:00,450 --> 00:13:03,290 Active types of remote sensing systems, 283 00:13:03,290 --> 00:13:05,590 fully function at any time of day 284 00:13:05,590 --> 00:13:07,590 as they don't require sunlight, 285 00:13:07,590 --> 00:13:09,260 and they're relatively independent 286 00:13:09,260 --> 00:13:11,690 of atmospheric conditions. 287 00:13:11,690 --> 00:13:13,830 Various types of remote sensing technology 288 00:13:13,830 --> 00:13:17,000 find implementations both in scientific branches 289 00:13:17,000 --> 00:13:19,403 and far more practical industries as well. 290 00:13:20,920 --> 00:13:21,930 Some other examples 291 00:13:21,930 --> 00:13:24,220 include the Shuttle Radar Topography Mission, 292 00:13:24,220 --> 00:13:26,880 which is also known as SRTM, 293 00:13:26,880 --> 00:13:29,283 which collected all the Earth's elevation data. 294 00:13:30,560 --> 00:13:34,680 Also lidar active remote sensing in the sky 295 00:13:34,680 --> 00:13:36,840 assisted in the elaboration 296 00:13:36,840 --> 00:13:39,233 of digital models of our planet surfaces. 297 00:13:40,370 --> 00:13:42,870 Data acquired with remote sensing instruments 298 00:13:42,870 --> 00:13:47,010 serve agriculturists and foresters alike as well. 299 00:13:47,010 --> 00:13:49,190 They are critical and hard to reach places, 300 00:13:49,190 --> 00:13:51,463 and in Marine sciences and rescue missions. 301 00:13:52,380 --> 00:13:53,470 Finally sounders, 302 00:13:53,470 --> 00:13:55,040 which is another type of active sensor, 303 00:13:55,040 --> 00:13:57,720 assist in developing weather forecasts 304 00:13:57,720 --> 00:13:59,420 with vertical profiles of humidity, 305 00:13:59,420 --> 00:14:02,460 precipitation temperature and the absence 306 00:14:02,460 --> 00:14:03,913 or presence of clouds. 307 00:14:06,850 --> 00:14:08,760 Okay, now we have defined remote sensing 308 00:14:08,760 --> 00:14:11,470 and talked about what it measures and how. 309 00:14:11,470 --> 00:14:13,310 The last thing we're going to do in this first week 310 00:14:13,310 --> 00:14:15,340 is talk a little bit about how we will be working 311 00:14:15,340 --> 00:14:17,690 with satellite imagery this semester. 312 00:14:17,690 --> 00:14:21,490 In this course we will use Google Earth Engine platform. 313 00:14:21,490 --> 00:14:24,500 Google Earth Engine is an online environment platform 314 00:14:24,500 --> 00:14:26,300 updated with data daily. 315 00:14:26,300 --> 00:14:28,763 It's towards petabytes of satellite imagery. 316 00:14:31,580 --> 00:14:34,810 It's a great platform for image analysis, 317 00:14:34,810 --> 00:14:39,810 because it puts many millions of gigabytes of information 318 00:14:40,750 --> 00:14:42,750 right at your fingertips. 319 00:14:42,750 --> 00:14:44,390 It's used as an environment 320 00:14:44,390 --> 00:14:47,290 to collaboratively share data and algorithms 321 00:14:47,290 --> 00:14:52,290 and visualizations and you can share them using simple URLs. 322 00:14:55,440 --> 00:14:57,500 Google Earth Engine also offers the ability 323 00:14:57,500 --> 00:14:59,880 to perform analysis on large scale data sets, 324 00:14:59,880 --> 00:15:03,020 including to detect measure, identify, characterize, 325 00:15:03,020 --> 00:15:06,313 and interpret geospatial data sets. 326 00:15:08,260 --> 00:15:10,080 The majority of the dataset analysis 327 00:15:10,080 --> 00:15:12,130 is roster format oriented, 328 00:15:12,130 --> 00:15:13,880 which we'll go over more next week. 329 00:15:14,910 --> 00:15:18,110 And finally, one thing to note is that Google Earth Engine 330 00:15:18,110 --> 00:15:19,770 has a very vast data catalog. 331 00:15:19,770 --> 00:15:22,080 We'll learn how to work 332 00:15:22,080 --> 00:15:23,990 and search within this data catalog 333 00:15:23,990 --> 00:15:25,730 and how to utilize the different data sets 334 00:15:25,730 --> 00:15:27,060 that are found within it. 335 00:15:27,060 --> 00:15:29,670 The data catalog includes the complete archive 336 00:15:29,670 --> 00:15:32,260 of pre-processed georeferenced scenes, 337 00:15:32,260 --> 00:15:36,680 which include all of the Landsat missions, MODIS, 338 00:15:36,680 --> 00:15:40,680 terrain, land cover, atmospheric, climate and weather data, 339 00:15:40,680 --> 00:15:44,833 as well as demographic and epidemiological data as well. 340 00:15:48,840 --> 00:15:50,380 Lastly, here are the instructions 341 00:15:50,380 --> 00:15:52,900 to activate your Google Earth Engine account. 342 00:15:52,900 --> 00:15:54,860 Please follow them carefully to join 343 00:15:54,860 --> 00:15:56,610 our University of Vermont 344 00:15:56,610 --> 00:15:59,883 Geospatial Technologies and Spatial Analysis Group. 345 00:16:00,890 --> 00:16:03,490 And also please reach out if you have any questions. 346 00:16:04,650 --> 00:16:06,183 Take care until next week.