Git Product home page Git Product logo

autoreg-pde-diffusion's Introduction

Benchmarking Autoregressive Conditional Diffusion Models for Turbulent Flow Simulation

This repository contains the source code for the paper Benchmarking Autoregressive Conditional Diffusion Models for Turbulent Flow Simulation by Georg Kohl, Liwei Chen, and Nils Thuerey. Our work benchmarks neural operators for the prediction of turbulent flow fields from an initial condition across a range of architectures:

  1. Autoregressive conditional diffusion models (ACDMs): This method relies on the DDPM approach, a class of generative models based on a parameterized Markov chain. They can be trained to learn the conditional distribution of a target variable given a conditioning. In our case, the target variable is the flow field at the next time step, and the conditioning is the flow field at the current time step, i.e., the simulation trajectory is created via autoregressive unrolling of the model. We showed that ACDMs can accurately and probabilistically predict turbulent flow fields, and that the resulting trajectories align with the statistics of the underlying physics. Furthermore, ACDMs can generalize to flow parameters beyond the training regime, and exhibit high temporal rollout stability, without compromising the quality of generated samples.

  2. U-Net Variants: We consider a range of different training variants of the backbone U-Net used in ACDM. It can be trained as a classic next-step predictor, with unrolled training to improve the stability, or with additional training noise. Furthermore, we also implement PDE-Refiner based on this U-Net.

  3. ResNets and Fourier Neural Operators: Our source code also integrates Dilated ResNets and Fourier Neural Operators, as established flow prediction architectures.

  4. Latent-Space Transformers: Finally, we provide different implementation variants of latent-space transformers. These architectures contain an autoencoder to embed the flow states in a smaller latent space. A secondary transformer model computes updated latent spaces forward in time, that can be decoded to create flow trajectories. We train the combined architecture end-to-end.

All architectures are evaluated on three carefully designed data sets of varying difficulty:

  1. Incompressible Wake Flow (Inc): This relatively simple data set contains 91 incompressible wake flow trajectories simulated with PhiFlow at Reynolds numbers 100-1000. Each sequence contains 1300 temporal snapshots of pressure and velocity.

predictions_full_inc_var_vort.mp4

  1. Transonic Cylinder Flow (Tra): This data set contains 41 sequences of a two-dimensional transonic cylinder flow simulated with the fluid solver SU2. Each sequence has a different Mach number between 0.5 and 0.9 at Reynolds number 10000, making the flows in the transonic regime highly chaotic. All trajcetories feature 1000 temporal snapshots of pressure, density, and velocity.

predictions_full_tra_long_pres.mp4

  1. Isotropic Turbulence (Iso): This highly complex, underdetermined data set consists of 1000 two-dimensional sequences sliced from three-dimensional, isotropic turbulence simulations. The flows were computed with DNS and the raw data is provided by the Johns Hopkins Turbulence Database. Each sequence contains 1000 temporal snapshots of pressure and velocity, including the velocity z-component.

predictions_full_iso_vort.mp4

Further information about this work can be also found at our project website. Feel free to contact us if you have questions or suggestions regarding our work or the source code provided here.


Simple ACDM Demonstration

Open In Colab

Using the button above, you can run a simple example notebook in Google Colab that demonstrates ACDM (a Google account is required). Instead, it is also possible to locally run the provided acdm-demo.ipynb file, by following the installation instructions in the next section and running the notebook inside the created conda environment afterwards.

Installation

In the following, Linux is assumed as the OS but the installation on Windows should be similar.

We recommend to install the required python packages (see requirements.yml) via a conda environment (e.g. using miniconda), but it may be possible to directly install them with pip (e.g. via venv for a separate environment) as well.

conda env create -f requirements.yml
conda activate ACDM

In the following, all commands should be run from the root directory of this source code.

Directory Structure and Basic Usage

The directory src/turbpred contains the general code base of this project. The src/lsim directory contains the LSiM metric that is used for evaluations. The data directory contains data generation scripts, and downloaded or generated data sets should end up there as well. The models directory contains pretrained model checkpoints once they are downloaded (see below). The runs directory contains model checkpoints as well as further log files when training models from scratch. The results directory contains the results from the sampling, evaluation, and plotting scripts. Sampled model predictions are written to this directory as compressed numpy arrays. These arrays are read by the plotting scripts, which in turn write the resulting plots to the results directory as well.

The scripts in src contain the main training, sampling, and plotting functionality. Each script contains various configuration options and architecture selections at the beginning of the file. All files should be run directly with Python according to the following pattern:

python src/training_*.py
python src/sample_models_*.py
python src/plot_*.py

Downloading our Data and Models

Our data sets can be downloaded via any web browser, ftp, or rsync here: http://doi.org/10.14459/2024mp1734798 (rsync password: m1734798.001). Use this command to directly download all data sets at the training and evaluation resolution of $128 \times 64$ (about 146 GB):

rsync -P rsync://[email protected]/m1734798.001/128_* ./data

Once the download is complete, the data set archives can be extracted with:

unzip -o -d data "data/128_*.zip"

To separately download the individiual data subsets, replace the 128_* path in the rsync and unzip commands above with one of the following archive names:

Archive Name Size Description
128_inc.zip 13.8 GB Data set $\texttt{Inc}$ of incompressible wake flows with Reynolds numbers $100 - 1000$ at training resolution $128 \times 64$
128_tra.zip 12.1 GB Data set $\texttt{Tra}$ of compressible cylinder flows with Mach numbers $0.5 - 0.9$ at training resolution $128 \times 64$
128_iso.zip 119.8 GB Data set $\texttt{Iso}$ with isotropic turbulence data from the JHTDB at training resolution $128 \times 64$
256_inc.zip 44.3 GB High-resolution version of $\texttt{Inc}$ at the simulation resolution $256 \times 128$
256_tra.zip 42.0 GB High-resolution version of $\texttt{Tra}$ at resolution $256 \times 128$
128_tra_small.zip 301 MB Small subset from $\texttt{Tra}$ consisting of a single flow trajectory with Mach number $0.7$ at resolution $128 \times 64$
checkpoints.zip 1.9 GB Pretrained model checkpoints for each investigated architecture and data set
checkpoints_acdm_tra.zip 75 MB Small subset of the checkpoints file consisting of the ACDM architecture on the $\texttt{Tra}$ data set
(checksums.sha512) (1.0 KB) (Checksum file only used to check archive validity)

Pretrained model weights for each data set and investigated architecture can be downloaded and extraced in the same way as described for the data above (rsync password: m1734798.001):

rsync -P rsync://[email protected]/m1734798.001/checkpoints.zip ./models
unzip -o -d models "models/checkpoints.zip"

The model checkpoints can be directly sampled on the downloaded data sets with the src/sample_models_*.py scripts.

If problems with the .zip archives occur, it is recommended to check them for corruption. This can be achieved by comparing the SHA512 hash of downloaded files with the corresponding content of the provided checksum file. The checksums for the downloaded archives can be downloaded and checked via (rsync password: m1734798.001):

rsync -P rsync://[email protected]/m1734798.001/checksums.sha512 ./data
cd data
sha512sum -c --ignore-missing checksums.sha512

If the hashes do not match, restart the download or try a different download method.


Model Training from Scratch

Once the data sets are downloaded or generated, model architectures can be trained from scratch using the src/training_*.py scripts. The resulting model checkpoints are identical to the downloaded models described above. The training scripts contain different various configuration options and an architecture selection at the beginning of the file.

Training Monitoring with Tensorboard

During training, various values, statistics and plots are logged to Tensorboard, allowing for monitoring the training progress. To start Tensorboard, use the following command:

tensorboard --logdir=runs --port=6006

and open http://localhost:6006/ in your browser to inspect the logged data.


Data Generation from Scratch and Data Processing

Generation with PhiFlow: Incompressible Wake Flow (Inc)

Click to expand detailed PhiFlow generation instructions

Vorticity Plot Inc

To generate data with the fluid solver PhiFlow, perform the following steps:

  1. Download the PhiFlow source code and follow the installation instructions. We use the PyTorch backend, that should work out of the box with a correction installation of PhiFlow. Our scripts assume the usage of version 2.0.3 at commit abc82af2! Substantially newer versions might not work.
  2. Ensure that the packages numpy, matplotlib, and imageio are installed in the python environment used for PhiFlow.
  3. Add our data generation scripts that handle the solver setup and data export to the PhiFlow installation by copying all files from the data/generation_scripts/PhiFlow directory to the demos directory in your PhiFlow directory.
  4. The copied files contain the PhiFlow scene for the Inc training and test data set (.py files), that can be run in the same way as the other example PhiFlow scene files in the demos directory. The corresponding batch generation scripts (.sh files) simply run the scene multiple times with different parameters to build the full data set.
  5. Adjust paths and settings in the python generation file if necessary, and run it or alternatively the batch script to generate the data.
  6. Copy or move the generated data set directory to the data directory of this source code for training. Make sure to follow the data set structure described below.

Generation with SU2: Transonic Cylinder Flow (Tra)

Click to expand detailed SU2 generation instructions

Pressure Plot Tra

To generate data with the fluid solver SU2, perform the following steps:

  1. Follow the general SU2 installation instructions with the Python Modules. We ran the generation on SU2 version 7.3.1 (Blackbird)! Substantially newer versions might not work. Make sure that you have access to an MPI implementation on your system as well, since our generation script runs SU2 via the mpiexec command. Try running the provided SU2 test cases to ensure the installation was successful.
  2. Ensure that the packages numpy, matplotlib, and scipy are installed in the python environment used for SU2.
  3. Add our data generation scripts that handle the solver setup and data export to the SU2 installation by copying all files from the data/generation_scripts/SU2 directory to a new directory in the root of your SU2 installation (for example called SU2_raw). These include the main generation script data_generation.py, the python helper file convert_data.py to convert the data to compressed numpy arrays, as well as the mesh file grid_quad_2d.su2 for all simulations. Furthermore, the SU2 configuration files for the three consecutive simulations (1. steady simulation as initialization: steady.cfg, 2. unsteady warmup: unsteady_2d_initial.cfg, 3. actual simulation for data generation: unsteady_2d_lowDissipation.cfg) run by the python script are included.
  4. Adjust paths and settings in the python generation file if necessary, and run it with the following command to generate the data (from the root directory of the SU2 installation):
python SU2_raw/data_generation.py [Thread count] [Reynolds number] [List of Mach numbers] [List of corresponding simulation folder IDs] [Restart iteration]

For example, to create three simulations at Mach numbers 0.6, 0.7, and 0.8 with Reynolds number 10000 using 112 threads, run the following command:

python SU2_raw/data_generation.py 112 10000 0.60,0.70,0.80 0,1,2 -1
  1. Copy or move the generated data set directory to the data directory of this source code for training.
  2. Post-process the data set directory structure with the src/convert_SU2_structure.py script (adjust script settings if necessary), that also extracts some information from the auxiliary simulation files. Make sure that the converted data directory follows the data set structure described below.

Download from the Johns Hopkins Turbulence Database: Isotropic Turbulence (Iso)

Click to expand detailed JHTDB download instructions

Vorticity Plot Iso

To extract sequences from the Johns Hopkins Turbulence Database, the required steps are:

  1. Install the pyJHTDB package for local usage, and make sure numpy is available.
  2. Request an authorization token to ensure access to the full data base, and add it to the script data/generation_scripts/JHTDB/get_JHTDB.py
  3. Adjust the paths and settings in the script file if necessary, and run the script to download and convert the corresponding regions of the DNS data. The script data/generation_scripts/JHTDB/get_JHTDB_scheduler.py can be run instead as well. It reconnects to the data base automatically in case the connection is unstable or is otherwise interrupted, and resumes the download.
  4. Copy or move the downloaded data set directory to the data directory of this source code for training if necessary. Make sure to follow the data set structure described below.

Data Set Structure

Ensure that the data set folder structure resulting from the data generation is the following to ensure the data set can be loaded correctly: data/[datasetName]/sim_[simNr]/[field]_[timestep].npz. Here datasetName is any string, but has to be adjusted accordingly when creating data set objects. The simulation folder numbers should be integers with a fixed width of six digits and increase continuously. Similarly, the timestep numbering should consist of integers with a fixed width of six digits and increase continuously. Start and end points for both can be configured when creating Dataset objects. Fields should be strings that describe the physical quantity, such as pressure, density, or velocity. Velocity components are typically stored in a single array, apart from the Iso case where the velocity z-component is stored separately as velocityZ. For example, a density snapshot at timestep zero from the Tra data set is referenced as data/128_tra/sim_000000/density_000000.npz.

General Data Post-Processing

src/copy_data_lowres.py can be used to downsample the generation resolution of 256x128 to the training and evaluation resolution of 128x64 for the simulated data sets. It processes all .npz data files, while creating copies of all supplementary files in the input directory. Computing mean and standard deviation statistics for the data normalization to a standard normal distribution is performed via src/compute_data_mean_std.py.


Experiments on Extremely Long Rollouts

On the Inc and Tra data sets dicussed above, we observed that it is possible to train models that are unconditionally stable and do not diverge, even after 200 000 rollout steps. Key criteria for training models with such stability are outlined here.


Citation

If you use the source code, models, or data sets provided here, please consider citing our work:

@article{kohl2023_acdm,
  author = {Georg Kohl and Li{-}Wei Chen and Nils Thuerey},
  title = {Benchmarking Autoregressive Conditional Diffusion Models for Turbulent Flow Simulation},
  journal = {arXiv},
  year = {2023},
  eprint = {2309.01745},
  primaryclass = {cs},
  publisher = {arXiv},
  url = {https://doi.org/10.48550/arXiv.2309.01745},
  doi = {10.48550/arXiv.2309.01745},
  archiveprefix = {arxiv}
}

Acknowledgements

This work was supported by the ERC Consolidator Grant SpaTe (CoG-2019-863850).

autoreg-pde-diffusion's People

Contributors

georgkohl avatar thunil avatar visriv avatar

Recommend Projects

  • React photo React

    A declarative, efficient, and flexible JavaScript library for building user interfaces.

  • Vue.js photo Vue.js

    ๐Ÿ–– Vue.js is a progressive, incrementally-adoptable JavaScript framework for building UI on the web.

  • Typescript photo Typescript

    TypeScript is a superset of JavaScript that compiles to clean JavaScript output.

  • TensorFlow photo TensorFlow

    An Open Source Machine Learning Framework for Everyone

  • Django photo Django

    The Web framework for perfectionists with deadlines.

  • D3 photo D3

    Bring data to life with SVG, Canvas and HTML. ๐Ÿ“Š๐Ÿ“ˆ๐ŸŽ‰

Recommend Topics

  • javascript

    JavaScript (JS) is a lightweight interpreted programming language with first-class functions.

  • web

    Some thing interesting about web. New door for the world.

  • server

    A server is a program made to process requests and deliver data to clients.

  • Machine learning

    Machine learning is a way of modeling and interpreting data that allows a piece of software to respond intelligently.

  • Game

    Some thing interesting about game, make everyone happy.

Recommend Org

  • Facebook photo Facebook

    We are working to build community through open source technology. NB: members must have two-factor auth.

  • Microsoft photo Microsoft

    Open source projects and samples from Microsoft.

  • Google photo Google

    Google โค๏ธ Open Source for everyone.

  • D3 photo D3

    Data-Driven Documents codes.