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B659: Principles of Intelligent Robot Motion Spring 2013 Kris Hauser

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Presentation on theme: "B659: Principles of Intelligent Robot Motion Spring 2013 Kris Hauser"— Presentation transcript:

1 B659: Principles of Intelligent Robot Motion Spring 2013 Kris Hauser
3D Sensing and Mapping B659: Principles of Intelligent Robot Motion Spring 2013 Kris Hauser

2 Agenda A high-level overview of visual sensors and perception algorithms Core concepts Camera / projective geometry Point clouds Occupancy grids Iterative closest points algorithm

3 Proprioceptive: sense one’s own body
Motor encoders (absolute or relative) Contact switches (joint limits) Inertial: sense accelerations of a link Accelerometers Gyroscopes Inertial Measurement Units (IMUs) Visual: sense 3D scene with reflected light RGB: cameras (monocular, stereo) Depth: lasers, radar, time-of-flight, stereo+projection Infrared, etc Tactile: sense forces Contact switches Force sensors Pressure sensors Other Motor current feedback: sense effort GPS Sonar

4 Sensing vs Perception Sensing: acquisition of signals from hardware
Perception: processing of “raw” signals into “meaningful” representations Example: Reading pixels from a camera is sensing. Declaring “it’s a rounded shape with skin color”, “it’s a face”, or “it’s a smiling face” are different levels of perception. Especially at lower levels of perception like signal processing, the line is blurry, and the often the processed results can be essentially considered “sensed”. Digits

5 3D Perception Topics Sensors: visible-light cameras, depth sensors, laser sensors (Some) perception tasks: Stereo reconstruction Object recognition 3D mapping Object pose recognition Key issues: How to represent and optimize camera transforms? How to fit models in the presence of noise? How to represent large 3D models?

6 Visual Sensors Visible-light cameras: cheap, low power, high resolution, high frame rates Data: 2D field of RGB pixels Stereo cameras Depth field sensors Two major types: infrared pattern projection (Kinect, ASUS, PrimeSense) and time-of-flight Data: 2D field of depth values (SwissRanger) Sweeping laser sensors Data: 1D field of depth values Hokuyo, SICK, Velodyne Can be mounted on a tilt/spin mount to get 3D field of view Bumblebee stereo camera ASUS Xtion depth sensor Hokuyo laser sensor

7 Sensors vary in strengths / weaknesses
Velodyne (DARPA grand challenge) 1.3 million readings/s $75k price tag

8 Image formation Light bounces off an object, passes through a lens and lands on a CCD pixel on the image plane Depth of focus Illumination and aperture Color: accomplished through use of filters, e.g. Bayer filter Each channel’s in-between pixels are interpolated

9 Idealized projective geometry
Let: Zim: distance from image plane to focal point along the depth axis (X,Y,Z): point in 3D space relative to focal point, Z > 0 Then, image space point is: Xc = Zim X / Z Yc = Zim Y / Z …Which get scaled and offset to get pixel coordinates x Image plane (X,Z) (Xc,Zim) Focal point z

10 Issues with real sensors
Motion blur Distortion caused by lenses Non-square pixels Exposure Noise Film grain Salt-and-pepper noise Shot noise Motion blur Distortion Exposure

11 Calibration Determine camera’s intrinsic parameters
Focal length Field of view Pixel dimensions Radial distortion That determine the mapping from image pixels to an idealized pinhole camera Rectification

12 Stereo vision processing
Dense reconstruction Given two rectified images, find binocular disparity at each pixel Take a small image patch around each pixel in the left image, search for the best horizontal shifted copy in the right image What size patch? What search size? What matching criterion? Works best for highly textured scenes

13 Point Clouds Unordered list of 3D points P={p1,…,pn}
Each point optionally annotated by: Color (RGB) Sensor reading ID# (why?) Estimated surface normal (nx,ny,nz) No information about objects, occlusions, topology Point Cloud Library (PCL)

14 3D Mapping Each frame of a depth sensor gives a narrow snapshot of the world geometry from a given position 3D mapping is the process of stitching multiple views into a global model

15 Three scenarios: Consider two raw point clouds P1 and P2 from cameras with transformations T1 and T2. Goal: build point cloud P in frame T1 (assume identity) Case 1: relative transformations known Simple union P = P1  (T2-1  P2) Case 2: small transformation Pose registration problem Vast majority of points correspond between scenes Case 3: large transformation Significant fraction of points do not correspond, lighting differences, more occlusions Pose registration must be more robust to outliers

16 Case 2: Small transformations
Visual odometry: estimate relative motion of subsequent frames using optical flow Define feature points in P1 (e.g., corner detector) Estimate a transformation of an image patch around feature that best matches P2 (defines optical flow field) Transformation: translation, rotation, scale Fit T2 to match these feature transforms

17 Case 3: Large transformations
Iterative closest point algorithm Input: initial guess for T2 Repeat until convergence: Find nearest neighbor pairings between P1 and T2P2 Select those pairs that fall below some distance threshold (outlier rejection) Assign an error metric and optimize T2 to minimize this metric

18 Case 3: Large transformations
Iterative closest point algorithm Input: initial guess for T2 Repeat until convergence: Find nearest neighbor pairings between P1 and T2P2 Select those pairs that fail to satisfy some distance criteria (outlier rejection) Assign an error metric and optimize T2 to minimize this metric What metric? What criteria? How to minimize?

19 What metrics for matching?
Position Surface normal Color Nearest neighbor methods Fast data structures, e.g. K-D trees For large scans usually want a constant sized subsample Projection-based methods Render scene from perspective of T1 to determine a match Very fast (used in Kinect Fusion algorithm) Only uses position information

20 What criteria for outlier rejection?
Distance too large (e.g., top X%) Inconsistencies with neighboring pairs On boundary of scan

21 How to optimize? Want to find rotation R, translation t of T2 to minimize some error function Sum of squared point-to-point differences 𝐸 𝑅,𝑡 = 𝑖=1 𝑛 𝑝 𝑖 −(𝑅 𝑞 𝑖 +𝑡) 2 Closed-form solution (SVD) Very fast per step Sum of squared point-to-plane differences 𝐸 𝑅,𝑡 = 𝑖=1 𝑛 𝑛 𝑖 𝑇 𝑝 𝑖 − 𝑛 𝑖 𝑇 (𝑅 𝑞 𝑖 +𝑡) 2 Must use numerical methods Deal with rotation variable Tends to lead ICP to converge with fewer iterations

22 Other applications of ICP
Fitting 3D triangulated models to point clouds for object recognition / pose estimation

23 Stitching multiple scans
In its most basic form, multi-view 3D mapping is simply a repetition of the two-camera case But two major issues: Drift and “closing the loop” Point clouds become massive after many scans This time

24 Point cloud growth problem
With N points, at F frames/sec, and T seconds of run time, NFT points are gathered Kinect: N=307200, F=30, T=60 => 552,960,000 points With RGB in 4 bytes, XYZ in 12 bytes => 8 GB / min Solutions: Forget earlier scans (short term memory) Build persistent, “collapsed” representation of environment geometry Polygon meshes Occupancy grids Key issue: how to estimate with low # of points and update later?

25 Occupancy grids Store a grid G with a fixed minimum resolution
Mark which cells (voxels) are occupied by a point Representation size is independent of T Two options for updating on a new scan Compute ICP to align current scan to prior scan, then add points to G Modify ICP to work directly with the representation G

26 Probabilistic Occupancy Grids with Ray Casting
Scans are noisy, so simply adding points is likely to overestimate occupied cells Ray casting approaches: Each cell has a probability of being free/occupied/unseen Each scan defines a line segment that passes through free space and ends in an occupied cell (or near one) Walk along the segment, increasing P(free(c)) of each encountered cell c, and finally increase P(occupied(c)) for the terminal cell c

27 Probabilistic Occupancy Grids with Ray Casting
Scans are noisy, so simply adding points is likely to overestimate occupied cells Ray casting approaches: Each cell has a probability of being free/occupied/unseen Each scan defines a line segment that passes through free space and ends in an occupied cell (or near one) Walk along the segment, increasing P(free(c)) of each encountered cell c, and finally increase P(occupied(c)) for the terminal cell c

28 Compact geometry representations within a cell
On-line averaging On-line least squares estimation of fitting plane

29 Handling large 3D grids Problem: tabular 3D grid storage increases with O(N3) 10243 is 1Gb Solutions Store hash table only of occupied cells Octree data structure OctoMap Library (

30 Dynamic Environments Real environments have people, animals, objects that move around Two options: Map static parts by assuming dynamic objects will average out as noise over time (probabilistic occupancy grids) Segment (and possibly model) dynamic objects

31 Related topics Sensor fusion Object segmentation and recognition
Simultaneous Localization and Mapping (SLAM) Next-best-view planning

32 Next time Kalman filtering Welch and Bishop (2001) Principles Ch. 8
Zeeshan


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