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These are the user uploaded subtitles that are being translated: 1 00:00:05,220 --> 00:00:10,170 In this lecture, we will talk about a probabilistic state estimation technique 2 00:00:10,170 --> 00:00:14,102 using a sampling-based distribution representation known as 3 00:00:14,102 --> 00:00:15,500 the Particle Filter. 4 00:00:16,890 --> 00:00:21,490 Instead of a fully defined function, the Particle Filter represents 5 00:00:21,490 --> 00:00:26,310 a distribution with a set of samples, referred to as particles. 6 00:00:28,320 --> 00:00:30,510 These particles represent the distribution. 7 00:00:31,520 --> 00:00:36,270 The statistics of the samples match the statistics of the distribution, 8 00:00:36,270 --> 00:00:38,790 such as the mean or standard deviation. 9 00:00:38,790 --> 00:00:42,040 However, they can be more complicated metrics as well. 10 00:00:43,290 --> 00:00:46,970 In this way, there are no parameters as were seen in the mean and 11 00:00:46,970 --> 00:00:49,620 covariances of the Gaussian models. 12 00:00:49,620 --> 00:00:51,730 Instead, a full population is tracked. 13 00:00:52,880 --> 00:00:56,720 In essence, the particle filter population represents a mixture 14 00:00:56,720 --> 00:01:00,680 of Gaussian distributions that we have seen in the first week. 15 00:01:01,680 --> 00:01:04,130 Here, the variance will go to 0. 16 00:01:04,130 --> 00:01:05,320 With 0 variance, 17 00:01:05,320 --> 00:01:08,380 the Gaussian distributions become Dirac Delta functions. 18 00:01:10,080 --> 00:01:14,100 Initially, a set of particles represent the underlying belief state. 19 00:01:15,240 --> 00:01:19,550 Each particle is a pair of the pose and the weight of that pose. 20 00:01:19,550 --> 00:01:25,070 This is similar to representing a probability function 21 00:01:25,070 --> 00:01:29,380 where the weight is the probability of that pose in the underlying distribution. 22 00:01:30,820 --> 00:01:34,630 Here, darker colors represent higher weights, and 23 00:01:34,630 --> 00:01:36,969 lighter colors represent lower weights. 24 00:01:38,280 --> 00:01:39,610 Just like the Kalman filter, 25 00:01:40,810 --> 00:01:43,500 a motion model will move the underlying distribution. 26 00:01:44,680 --> 00:01:49,130 Here, the particles move based on odometry measurements taken from the robot. 27 00:01:51,060 --> 00:01:56,570 A companion uncertainty model captures the noise underlying the motion model. 28 00:01:56,570 --> 00:01:59,430 For instance, this could be wheel slip or friction changes. 29 00:02:00,490 --> 00:02:04,220 In the particle filter, where we do not track the motion model 30 00:02:04,220 --> 00:02:09,350 in explicit parameters, we add sampled noise from the motion noise model. 31 00:02:09,350 --> 00:02:10,378 In this case, 32 00:02:10,378 --> 00:02:16,394 we use a Gaussian distribution to model noise with 0 mean and non-0 covariance. 33 00:02:16,394 --> 00:02:20,050 Noise is uniquely added to each particle. 34 00:02:20,050 --> 00:02:23,426 So separate samples are made for each particle. 35 00:02:23,426 --> 00:02:25,132 After the noise is added, 36 00:02:25,132 --> 00:02:30,100 the dispersion of the particles captures the uncertainty due to movement. 37 00:02:31,830 --> 00:02:35,990 Like the Kalman filter, we can use a separate set of observations 38 00:02:35,990 --> 00:02:38,970 to constrain our noise and update our belief distribution. 39 00:02:40,310 --> 00:02:43,230 Here we will leverage the LIDAR correlation 40 00:02:43,230 --> 00:02:45,850 from previous lectures on map registration. 41 00:02:47,410 --> 00:02:51,730 We will update the weights of the particles to reflect the correlation score 42 00:02:51,730 --> 00:02:56,540 from the map registration by utilizing the current weights as a prior belief. 43 00:02:58,430 --> 00:03:03,790 The new set of particles captures the distribution after odometry and 44 00:03:03,790 --> 00:03:05,810 sensor measurements. 45 00:03:05,810 --> 00:03:11,386 However, this may not be the optimal set to represent the distribution. 46 00:03:11,386 --> 00:03:15,649 Here, you can see that only a few particles have significant weights. 47 00:03:16,700 --> 00:03:19,090 Most of the particles are lightly colored and 48 00:03:19,090 --> 00:03:21,920 do not give much information about the distribution. 49 00:03:24,340 --> 00:03:27,420 To make the set of particles more accurately represent 50 00:03:27,420 --> 00:03:31,950 the belief state distribution, we check the number of effective particles. 51 00:03:33,200 --> 00:03:37,230 The number of effective particles acts as a criterion for 52 00:03:37,230 --> 00:03:39,260 when to resample particles. 53 00:03:40,720 --> 00:03:45,300 This resampling process provides a probabilistically motivated way 54 00:03:45,300 --> 00:03:47,960 to prune out lower weighted particles. 55 00:03:49,950 --> 00:03:51,130 With the set of large and 56 00:03:51,130 --> 00:03:56,280 small weights, using the cumulative probability function can aid in sampling. 57 00:03:57,350 --> 00:04:00,840 With normalized weights, the sum of the weights is 1, and 58 00:04:00,840 --> 00:04:04,810 can be represented as a monotonically increasing cumulative function. 59 00:04:06,260 --> 00:04:09,511 We sample a number ,uniformly, between 0 and 60 00:04:09,511 --> 00:04:14,400 1 of the cumulative range and find which weight includes that number. 61 00:04:17,190 --> 00:04:20,760 The particles with the indices found in the resampling approach 62 00:04:20,760 --> 00:04:24,780 become the new set of particles to be fed into the next odometry update. 63 00:04:25,960 --> 00:04:27,880 Particles may be duplicated, but 64 00:04:27,880 --> 00:04:31,650 the odometry noise will differentiate these particles. 65 00:04:31,650 --> 00:04:36,363 This approach provides a good way to approach a multi-nodal belief state 66 00:04:36,363 --> 00:04:40,324 distribution and non-linear effects of your motion model.5916

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