official source code of paper 'PatchmatchNet: Learned Multi-View Patchmatch Stereo'
- 13.12.2021: New unified format for training and evaluation datasets, support for arbitrary image sizes and multi-camera setups, and new names for script parameters.
- 27.09.2021: The code now allows for Torchscript export and includes a pre-trained TorchScript module.
PatchmatchNet is a novel cascade formulation of learning-based Patchmatch which aims at decreasing memory consumption and computation time for high-resolution multi-view stereo. If you find this project useful for your research, please cite:
@misc{wang2020patchmatchnet,
title={PatchmatchNet: Learned Multi-View Patchmatch Stereo},
author={Fangjinhua Wang and Silvano Galliani and Christoph Vogel and Pablo Speciale and Marc Pollefeys},
journal={CVPR},
year={2021}
}
- python 3.8
- CUDA >= 10.1
pip install -r requirements.txt
- Download our pre-processed dataset: DTU's evaluation set, Tanks & Temples and ETH3D benchmark. Each dataset is already organized as follows:
root_directory
├──scan1 (scene_name1)
├──scan2 (scene_name2)
├── images
│ ├── 00000000.jpg
│ ├── 00000001.jpg
│ └── ...
├── cams
│ ├── 00000000_cam.txt
│ ├── 00000001_cam.txt
│ └── ...
└── pair.txt
Note:
- The subfolders for Tanks & Temples and ETH3D will not be named
scanN
but the lists included under./lists/eth3d
and./lists/tanks
will have the correct naming conventions. - If the folders for images and cameras, and the pair file don't follow the standard naming conventions you can modify
the settings of
MVSDataset
indatasets/mvs.py
to specify the customimage_folder
,cam_folder
, andpair_path
- The
MVSDataset
is configured by default for JPEG images. If you're using a different format (e.g., PNG) you can change theimage_extension
parameter ofMVSDataset
accordingly.
Camera file cam.txt
stores the camera parameters, which includes extrinsic, intrinsic, minimum depth and maximum depth:
extrinsic
E00 E01 E02 E03
E10 E11 E12 E13
E20 E21 E22 E23
E30 E31 E32 E33
intrinsic
K00 K01 K02
K10 K11 K12
K20 K21 K22
DEPTH_MIN DEPTH_MAX
pair.txt
stores the view selection result. For each reference image, N (10 or more) best source views are stored in the file:
TOTAL_IMAGE_NUM
IMAGE_ID0 # index of reference image 0
10 ID0 SCORE0 ID1 SCORE1 ... # 10 best source images for reference image 0
IMAGE_ID1 # index of reference image 1
10 ID0 SCORE0 ID1 SCORE1 ... # 10 best source images for reference image 1
...
- In
eval.sh
, setDTU_TESTING
,ETH3D_TESTING
orTANK_TESTING
as the root directory of corresponding dataset and uncomment the evaluation command for corresponding dataset (default is to evaluate on DTU's evaluation set). If you want to change the output location (default is same as input one), modify the--output_folder
parameter. For Tanks the--scan_list
can be intermediate or advanced and for ETH3D it can be test or train. CKPT_FILE
is the checkpoint file (our pretrained model is./checkpoints/params_000007.ckpt
), change it if you want to use your own model. If you want to use the model from the TorchScript module instead, you can specify the checkpoint file as./checkpoints/module_000007.pt
and set the option--input_type module
.- Test on GPU by running
sh eval.sh
. The code includes depth map estimation and depth fusion. The outputs are the point clouds inply
format. - For quantitative evaluation on DTU dataset, download SampleSet and
Points. Unzip them and place
Points
folder inSampleSet/MVS Data/
. The structure looks like:
SampleSet
├──MVS Data
└──Points
In evaluations/dtu/BaseEvalMain_web.m
, set dataPath
as path to SampleSet/MVS Data/
, plyPath
as directory that
stores the reconstructed point clouds and resultsPath
as directory to store the evaluation results. Then run
evaluations/dtu/BaseEvalMain_web.m
in matlab.
The results look like:
Acc. (mm) | Comp. (mm) | Overall (mm) |
---|---|---|
0.427 | 0.277 | 0.352 |
- For detailed quantitative results on Tanks & Temples and ETH3D, please check the leaderboards (Tanks & Temples, ETH3D)
- For evaluation, we support preparing the custom dataset from COLMAP's results. The script
colmap_input.py
(modified based on the script from MVSNet) converts COLMAP's sparse reconstruction results into the same format as the datasets that we provide. After reconstruction, COLMAP will generate a folderCOLMAP/dense/
, which containsCOLMAP/dense/images/
andCOLMAP/dense/sparse
. Then you need to run like this:
python colmap_input.py --input_folder COLMAP/dense/
- The default output location is the same as the input one. If you want to change that, set the
--output_folder
parameter. - The default behavior of the converter will find all possible related images for each source image. If you want to constrain
the max number of related images set the
--num_src_images
parameter. - In
eval.sh
, setCUSTOM_TESTING
as the root directory of the dataset, set--output_folder
as the directory to store the reconstructed point clouds (default is same as input directory), set--image_max_dim
to an appropriate size (this is determined by the available GPU memory and the desired processing speed) or use the native size by removing the parameter, and uncomment the evaluation command. Test on GPU by runningsh eval.sh
.
Download pre-processed DTU's training set. The dataset is already organized as follows:
root_directory
├── Cameras_1
│ ├── train
│ │ ├── 00000000_cam.txt
│ │ ├── 00000000_cam.txt
│ │ └── ...
│ └── pair.txt
├── Depths_raw
│ ├── scan1
│ │ ├── depth_map_0000.pfm
│ │ ├── depth_visual_0000.png
│ │ ├── depth_map_0001.pfm
│ │ ├── depth_visual_0001.png
│ │ └── ...
│ ├── scan2
│ └── ...
└── Rectified
├── scan1_train
│ ├── rect_001_0_r5000.png
│ ├── rect_001_1_r5000.png
│ ├── ...
│ ├── rect_001_6_r5000.png
│ ├── rect_002_0_r5000.png
│ ├── rect_002_1_r5000.png
│ ├── ...
│ ├── rect_002_6_r5000.png
│ └── ...
├── scan2_train
└── ...
To use this dataset directly look into the Legacy Training section below. For the current version of training the
dataset needs to be converted to a format compatible with MVSDataset
in ./datasets/mvs.py
using the script
convert_dtu_dataset.py
as follows:
python convert_dtu_dataset.py --input_folder <original_dataset> --output_folder <converted_dataset> --scan_list ./lists/dtu/all.txt
The converted dataset will now be in a format similar to the evaluation datasets:
root_directory
├── scan1 (scene_name1)
├── scan2 (scene_name2)
│ ├── cams (camera parameters)
│ │ ├── 00000000_cam.txt
│ │ ├── 00000001_cam.txt
│ │ └── ...
│ ├── depth_gt (ground truth depth maps)
│ │ ├── 00000000.pfm
│ │ ├── 00000001.pfm
│ │ └── ...
│ ├── images (images at 7 light indexes)
│ │ ├── 0 (light index 0)
│ │ │ ├── 00000000.jpg
│ │ │ ├── 00000001.jpg
│ │ │ └── ...
│ │ ├── 1 (light index 1)
│ │ └── ...
│ ├── masks (depth map masks)
│ │ ├── 00000000.png
│ │ ├── 00000001.png
│ │ └── ...
│ └── pair.txt
└── ...
- In
train.sh
, setMVS_TRAINING
as the root directory of the converted dataset; set--output_path
as the directory to store the checkpoints. - Train the model by running
sh train.sh
. - The output consists of one checkpoint (model parameters) and one TorchScript module per epoch named as
params_<epoch_id>.ckpt
andmodule_<epoch_id>.pt
respectively.
To train directly on the original DTU dataset the legacy training
script train_dtu.py
(using the legacy MVSDataset
from datasets/dtu_yao.py
) needs to be called from the train.sh
script.
- In
train.sh
, setMVS_TRAINING
as the root directory of the original dataset; set--logdir
as the directory to store the checkpoints. - Uncomment the appropriate section for legacy training and comment out the other entry.
- Train the model by running
sh train.sh
.
--patchmatch_iteration
represents the number of iterations of Patchmatch on multi-stages (e.g., the default number 1,2,2
means 1 iteration on stage 1, 2 iterations on stage 2 and 2 iterations on stage 3). --propagate_neighbors
represents the
number of neighbors for adaptive propagation (e.g., the default number 0,8,16
means no propagation for Patchmatch on
stage 1, using 8 neighbors for propagation on stage 2 and using 16 neighbors for propagation on stage 3). As explained in
our paper, we do not include adaptive propagation for the last iteration of Patchmatch on stage 1 due to the requirement
of photometric consistency filtering. So in our default case (also for our pretrained model), we set the number of propagation
neighbors on stage 1 as 0
since the number of iteration on stage 1 is 1
. If you want to train the model with more
iterations on stage 1, change the corresponding number in --propagate_neighbors
to include adaptive propagation for
Patchmatch expect for the last iteration.
This project is done in collaboration with "Microsoft Mixed Reality & AI Zurich Lab".
Thanks to Yao Yao for open-sourcing his excellent work MVSNet. Thanks to Xiaoyang Guo for open-sourcing his PyTorch implementation of MVSNet MVSNet-pytorch.