Topic 4 - SLAM

Introduction:

SLAM (Simultaneous Localization and Mapping) is the computational problem of constructing or updating a map of an unknown environment while simultaneously keeping track of an agent's location within it.

IMPORTANT: Before proceeding further, start to download two docker images, one for each SLAM system that will be used: image for A-LOAM and image for ORB-SLAM3. Moreover, download the following .bag files: arm_put_car.bag and kitti00_200.bag.

LOAM

LOAM is a standard 3D laser localization method introduced in LOAM: Lidar Odometry and Mapping in Real-time. In short, LOAM takes point clouds as input. Based on them, it estimates the odometry by scan registration with feature matching approach and maps the environment. It is also possible to include IMU measurements in the process. It is focused on minimizing drift in odometry estimation and the classic LOAM version does not involve a loop closure mechanism.

HINT: The loop closure mechanism identifies revisited locations. Upon recognizing a return to a previously visited site, it corrects any accumulated errors in the estimated trajectory and map. This correction enhances the overall map accuracy and localization precision.

The original code is not available anymore since the authors made it private, creating kaarta company. We will instead use A-LOAM - Advanced implementation of LOAM. It uses Eigen and Ceres Solver to simplify and create a clean code structure, which makes it a perfect learning material for SLAM beginners.

Very general steps of LOAM operation:

  1. The system detects edge and planar features in each scan based on local curvature and determines the exact moment of measurement for each point.
  2. Each scan is first matched to the previous one to roughly estimate the transformation (odometry) and 'straighten out' the point cloud.
  3. After 'straightening out', the scan is matched to the map (collection of all previous points) to further improve the quality of the alignment.

TODO:

Docker container setup

A-LOAM implementation makes use of some dependencies e.g., CERES and PCL, so for convenience, the docker image with all installed dependencies was prepared (image for A-LOAM). You can check the Dockerfile here.

  1. Load the downloaded docker image:
docker load < arm_image03.tar.gz
  1. Run the docker container with mp_loam_run_gpu_nvidia.sh script if you have nvidia GPU or mp_loam_run_cpu.sh script otherwise:
bash mp_loam_run_gpu_nvidia.sh
bash mp_loam_run_cpu.sh
  1. You can attach to a running container in another terminal with:
docker exec -it MP_LOAM bash

IMPORTANT: Remember to give container access to the display for each terminal session you open with the command: xhost +local:root.

A-LOAM setup

  1. Download A-LOAM repository:
cd /catkin_ws/src
git clone https://github.com/HKUST-Aerial-Robotics/A-LOAM.git
  1. Build the catkin workspace along with A-LOAM code and source the environment variables:
cd /catkin_ws
catkin_make
source devel/setup.bash

Run A-LOAM:

We will test the A-LOAM system with the use of publically available KITTI Odometry dataset. It consists of 22 sequences, for 11 of which there are ground truth trajectories that can be used for the evaluation of the SLAM system. The data is not saved as .bag files, so to process it in ROS one can use kitti_helper.launch from the aloam_velodyne package. The whole dataset weights a lot and there is no point in using all of it during the classes, so the .bag file (kitti00_200.bag) with the first 200 scans of 00 sequence was prepared.

  1. Run A-LOAM ROS node along with the visualisation in rviz:
roslaunch aloam_velodyne aloam_velodyne_HDL_64.launch
  1. Replay the lidar data from downloaded .bag file:
rosbag play kitti00_200.bag

HINT: You can copy data to the container with the docker cp command: docker cp [FILE_TO_COPY] [CONTAINER_NAME]:[DIRECTORY_IN_THE_CONTAINER].

Expected result:

In rviz you can see:

HINT: To see the ground truth trajectory click the square next to GT group in rviz:

Considering the clear implementation, you can conveniently analyze the code. Notice the order of point cloud processing in the following files: laserMapping.cpp, laserOdometry.cpp, scanRegistration.cpp.

ORB-SLAM3

ORB-SLAM3 is the first real-time SLAM library able to perform Visual, Visual-Inertial and Multi-Map SLAM with monocular, stereo and RGB-D cameras, using pin-hole and fisheye lens models. It is based on detecting the ORB features on an image, matching the features by the descriptors and final optimization. It is a third version of an ORB-SLAM system. A very brief changelog of versions:

ORB-SLAM3 system consist of three threads:

The threads work asynchronously, which leads to obtaining slightly different results upon different runs.

Steps of tracking (1-3) and mapping (4-6) processes:

  1. Detection and description of ORB features in the image.
  2. Matching features from the current and previous frame based on descriptors.
  3. Calculation of transformation.
  4. Verification if the frame is a key one (needed for improving the system accuracy).
  5. Finding additional matches to the recently seen features from the map.
  6. Transformation correction.

TODO:

We will test the stereovision (obtaining 3D information from two cameras placed apart) version of the system on our own data (arm_put_car.bag) recorded from the car which circled the Piotrowo campus. The whole route was about 1.3 km long. The data sequence consists of images from two cameras(~20 Hz), DGPS data (~10 Hz) and AHRS data (~200 Hz). DGPS data provided localization information with an accuracy of about several centimeters, which is enough for our purpose to evaluate the localization accuracy of the system.

Docker container setup

ORB-SLAM3 has a couple of dependencies (Pangolin, OpenCV, Eigen3) and a few inconveniences in order to build it for ROS, so to save your time the docker image with ORB-SLAM3 and its dependencies installed was prepared (image for ORB-SLAM3). You can check the Dockerfile here.

  1. Load the downloaded docker image:
docker load < arm_image04.tar.gz
  1. Run the docker container with mp_orb3_run_gpu_nvidia.sh script if you have nvidia GPU or mp_orb3_run_cpu.sh script otherwise:
bash mp_orb3_run_gpu_nvidia.sh
bash mp_orb3_run_cpu.sh
  1. You can attach to a running container in another terminal with:
docker exec -it MP_ORB3 bash

Stereo vision camera calibration:

To run the stereovision version of the ORB-SLAM3 on our data we have to provide the parameters of the used camera configuration. The initially prepared configuration file PP.yaml can be found in the /ORB-SLAM3/Examples/Stereo directory. Current values are correct for a different camera configuration, so the task is to correct the values. You have to modify the following parameters:

To obtain all of the necessary stereovision system parameters, it has to be calibrated. In this example, it was already done with the use of kalibr toolbox. Here is the description of how it was done. The output of the calibration process was the following (you can also find it in /ORB_SLAM3/scripts/stereoCalibrationResult.txt):

cam0:
  cam_overlaps: [1]
  camera_model: pinhole
  distortion_coeffs: [-0.23248459123344795, 0.08191912671589296, 7.839314739418238e-05, 4.2075874672940684e-05]
  distortion_model: radtan
  intrinsics: [589.7363083173951, 590.0729541236071, 369.91183932674056, 298.34374442536097]
  resolution: [720, 540]
  rostopic: /pylon_stereo_node/left/image_raw
cam1:
  T_cn_cnm1:
  - [0.9997283077554007, 0.02320592542857902, 0.0021899081072863703, -0.32185797263546406]
  - [-0.0232254786906617, 0.9996863295720175, 0.00937121157638949, 0.0074867236444067856]
  - [-0.001971753560855992, -0.00941952715496201, 0.9999536912757833, -0.002949869596374046]
  - [0.0, 0.0, 0.0, 1.0]
  cam_overlaps: [0]
  camera_model: pinhole
  distortion_coeffs: [-0.2303444874136257, 0.07876654742388302, 9.186197190170094e-05,
    -0.0005160611286370294]
  distortion_model: radtan
  intrinsics: [589.5069022640636, 589.958834706832, 379.29038618376575, 283.91319737264314]
  resolution: [720, 540]
  rostopic: /pylon_stereo_node/right/image_raw

HINT: The explanation of the output above can be found here and here. kalibr notation of camera intrinsics [fu fv pu pv] is equivalent to [fx fy cx cy].

Some of the parameters can be taken directly from the kalibr calibration output. To obtain the bf value, R, and P matrices, we have to use stereoRectify function from OpenCV, which calculates the transformations (R, P) necessary to get and use the canonical camera configuration (re-project image planes onto a common plane parallel to the line between optical centers of images) for depth estimation. You can use the prepared script template /ORB-SLAM3/scripts/stereoCalibration.py and fill the values of K (camera intrinsic matrix), d (distortion coefficients vector), R (rotation matrix) and T (translation vector). You should also adjust the image size in stereoRectify()function call from (0, 0) to (720, 540). To get the output of stereoRectify() run:

python /ORB_SLAM3/scripts/stereoCalibration.py

HINT: Notice if the transformation (R, T) is meant to transform the coordination system of left camera to the coordinate system of right camera or the other way around.

Camera intrinsic matrix:

RGB image of a cubic frame

Homogeneous transformation matrix (T_cn_cnm1 is in this form):

https://automaticaddison.com/wp-content/uploads/2020/08/1-homogeneous-n-1-nJPG.jpg

Run ORB-SLAM3:

  1. Run roscore:
roscore
  1. Run ORB-SLAM3 ROS node along with the visualization (insert the correct topic names for the left and right camera topics - rosbag info [.bag file]):
cd /ORB_SLAM3/
rosrun ORB_SLAM3 Stereo /ORB_SLAM3/Vocabulary/ORBvoc.txt Examples/Stereo/PP.yaml true [topicLeft] [topicRight]
  1. Replay the lidar data from the downloaded .bag file:
rosbag play -r 0.25 --pause arm_put_car.bag

HINT: --pause means that the data will be played after pressing the spacebar. Since the ORB-SLAM3 is quite computationally demanding, we slow down the publish rate with the -r flag (0.25 - 4 times slower).

  1. After the replay of all data, shut down the ORB-SLAM3 node with ctrl + c. The output trajectory will be saved to FrameTrajectory_TUM_Format.txt. Move it to the scripts directory:
mv /ORB_SLAM3/FrameTrajectory_TUM_Format.txt /ORB_SLAM3/scripts/orbslam3.txt

Trajectory evaluation:

To evaluate the output trajectory we will compare it with the DGPS data as a ground truth. DGPS data is already processed to the correct format (TUM trajectory format with poses in UTM coordinate system). You can download it from here. We will use the evaluation script from the ORB-SLAM3 repository: avaluate_ate.py. Run the evaluation with:

cd /ORB_SLAM3/scripts
python evaluate_ate.py dgps.txt orbslam3.txt --verbose --plot trajs.png

Example output:

compared_pose_pairs 1460 pairs
absolute_translational_error.rmse 21.493264 m
absolute_translational_error.mean 20.317460 m
absolute_translational_error.median 22.098146 m
absolute_translational_error.std 7.011507 m
absolute_translational_error.min 9.798730 m
absolute_translational_error.max 35.219433 m

The script computes the best overlap of the two given trajectories and calculates the absolute translational error. The system is not deterministic so the results can vary a little between runs. The output trajectories can be displayed with:

eog trajs.png

Example trajectories: