Optimal Point Cloud Alignment
This package implements optimal point cloud alignment of two given point clouds. It relies on the following libraries which can be found on my github as well: jsCore cudaPcl dpMMlowVar bbTrans. The approach and the algorithm is described in more detail on our project page and the paper. The algorithms are described in more detail in the supplement. See below for install instructions.
If you use it please cite:
Julian Straub, Trevor Campbell, Jonathan P. How, John W. Fisher III. "Efficient Globally Optimal Point Cloud Alignment using Bayesian Nonparametric Mixtures".
This code is dependent on Eigen3, Boost, CUDA, OpenCV and PCL. It has been tested on Ubuntu 14.04 with
- Eigen3 (3.0.5)
- Boost (1.54)
- CUDA (6.5)
- OpenCV (2.4)
- PCL (1.7)
This package uses the pods build system. Used widely at CSAIL MIT the build system makes it easy to break up software projects into small packages that can be checked out and compiled automatically (see below).
Install Eigen3, Boost, OpenCV, and PCL (install instructions are at http://pointclouds.org/downloads/linux.html)
sudo apt-get install libeigen3-dev libboost-dev libopencv-dev libpcl-1.7-all-dev
Install the appropriate CUDA version matching with your nvidia drivers. On our machines we use
libcuda1-340 cuda-6-5 cuda-toolkit-6-5
Clone this repository and compile the code:
git clone email@example.com:jstraub/dpOptTrans.git; cd dpOptTrans make checkout; make configure; make -j6; make install;
Note that this will checkout several other necessary repositories. To update all repositories run
make update; make configure; make -j6; make install;
To run the BB algorithm on two point clouds run a command like this:
cd build/bin/; ./dpOptTransPly -l 60 -t 0.001 -a ../../data/bunny_rnd/bun_zipper.ply -b ../../data/bunny_rnd/bun_zipper_angle_90_translation_0.3.ply -o test
This will generate a outputfile test.csv which contains the optimal rotation as a quaternion, the optimal translation, the lower bounds for rotation as well as translation and the number of clusters used for the alignment in surface normal as well as Euclidean space. So for the command above you should get an output file containing the following:
q_w q_x q_y q_z t_x t_y t_z lb_S3 lb_R3 KvmfA KvmfB KgmmA KgmmB K 0.707106 0.381209 -0.0583649 0.592684 0.254969 -0.144869 -0.0632762 0.114808 184.636 8 8 35 35 1
To get additional visualization for the result try running the python script:
cd python; python alignBuddha.py
The methods in python/helpers.py show how to form the arguments of all provided executables.
./dpOptTransPly -h Allowed options: -h [ --help ] produce help message -l [ --lambdaDeg ] arg lambda in degree for DPvMF-means -t [ --lambdaT ] arg lambda in meters for DPMeans -a [ --in_a ] arg path to first input file -b [ --in_b ] arg path to second input file -o [ --out ] arg path to output file -s [ --scale ] arg scale for point-cloud -e [ --egi ] make the vMF MM pis uniform - like a EGI -d [ --display ] display results -v [ --verbose ] be verbose