sbrl-github/research-rainfallradar
1
0
Fork 0
mirror of https://github.com/sbrl/research-rainfallradar synced 2024-11-16 14:43:01 +00:00
Code Issues Projects Releases Packages Wiki Activity

README: finish filling out

Browse source
This commit is contained in:
Starbeamrainbowlabs 2023-11-30 16:32:46 +00:00
parent 13ae4df725
commit 60674fb6b3
Signed by: sbrl
GPG key ID: 1BE5172E637709C2
1 changed files with 73 additions and 4 deletions
Show stats Download patch file Download diff file Expand all files Collapse all files

77
README.md
View file

@ -4,7 +4,9 @@
This is the 3rd major version of this model.
Unfortunately using this model is rather complicated and involves a large number of steps. There is no way around this. This README (will) explain it the best I can though.
Unfortunately using this model is rather complicated and involves a large number of steps. There is no way around this. This README explains it the best I can though.
Should anything be unclear, please [open an issue](https://github.com/sbrl/research-rainfallradar/issues/new)
> [!WARNING]
> This README is currently under construction!
@ -31,6 +33,11 @@ By modelling the task as an image segmentation problem, an alternative approach
- 1TiB disk space free
- Lots of time and patience
> [!NOTE]
> The format that HAIL-CAESAR accepts data in results in a ~450GiB rainfall radar file O.o
>
> Thankfully the format that `nimrod-data-downloader` downloads in is only a couple of GiB in the end, and the `.tfrecord` files that the model accepts is only ~70GiB.
## Overview
The process of using this model is as as illustrated:
@ -110,10 +117,72 @@ After all of the above steps are completed, a model can now be trained.
The current state of the art (that was presented in the above paper!) is based on DeepLabV3+. A note of caution: this repository contains some older models, so it can be easy to mix them up. Hence this documentation :-)
<------ WRITING HERE
This model is located in the file [`aimodel/src/deeplabv3_plus_test_rainfall.py`](./aimodel/src/deeplabv3_plus_test_rainfall.py), and is controlled via a system of environment variables. Before using it, you must first install any dependencies you're missing:
TODO: Continue the guide here.
```bash
pip3 install --user -r aimodel/requirements.txt
```
The model should work with any recent version of Tensorflow. See the [version table](https://www.tensorflow.org/install/source#gpu) if you are having trouble with CUDA and/or CuDNN.
With requirements installed, we can train a model. The general form this is done is like so:
```bash
cd aimodel
[ENVIRONMENT_VARIABLES_HERE] src/deeplabv3_plus_test_rainfall.py
```
This model has mainly been tested and trained on the [University of Hull's Viper HPC](), which runs [Slurm](). As such, a Slurm job file is available in [`aimodel/slurm-TEST-deeplabv3p-rainfall.job`](./aimodel/slurm-TEST-deeplabv3p-rainfall.job), which wraps the aforementioned script.
The following environment variables are supported:
Environment Variable | Meaning
----------------------------|-------------------------------------------------
IMAGE_SIZE=128 | Optional. Sets the size of the 'images' that the DeepLabV3+ model will work with.
BATCH_SIZE=64 | Optional. Sets the batch size to train the model with.
DIR_RAINFALLWATER | The path to the directory the .tfrecord files containing the rainfall radar / water depth data.
PATH_HEIGHTMAP | The path to the heightmap jsonl file to read in.
PATH_COLOURMAP | The path to the colourmap for predictive purposes.
DIR_OUTPUT | The directory to write output files to. Automatically calculated in the Slurm job files unless manually set. See POSTFIX to alter DIR_OUTPUT without disrupting the automatic calculation. If you are calling `slurm-TEST-deeplabv3p-rainfall.job` directly then you MUST set this environment variable manually.
PARALLEL_READS | Multiplier for the number of files to read in parallel. 1 = number of CPU cores available. Very useful on high-read-latency systems (e.g. HPC like Viper) to avoid starving the GPU of data. WILL MANGLE THE ORDERING OF DATA. Set to 0 to disable and read data sequentially. WILL ONLY NOT MANGLE DATA IF PREDICT_AS_ONE IS SET. Defaults to 1.5.
STEPS_PER_EPOCH | The number of steps to consider an epoch. Defaults to None, which means use the entire dataset.
NO_REMOVE_ISOLATED_PIXELS | Set to any value to avoid the engine from removing isolated pixels - that is, water pixels with no other surrounding pixels, either side to side to diagonally.
EPOCHS=50 | The number of epochs to train for.
LOSS="cross-entropy" | The loss function to use. Default: cross-entropy (possible values: cross-entropy, cross-entropy-dice).
DICE_LOG_COSH | When in cross-entropy-dice mode, in addition do loss = cel + log(cosh(dice_loss)) instead of just loss = cel + dice_loss. Default: unset
WATER_THRESHOLD=0.1 | The threshold to cut water off at when training, in metres. Default: 0.1
PATH_CHECKPOINT | The path to a checkpoint to load. If specified, a model will be loaded instead of being trained.
LEARNING_RATE=0.001 | The learning rate to use. Default: 0.001.
UPSAMPLE=2 | How much to upsample by at the beginning of the model. A value of disables upscaling. Default: 2.
STEPS_PER_EXECUTION=1 | How many steps to perform before surfacing from the GPU to e.g. do callbacks. Default: 1.
RANDSEED | The random seed to use when shuffling filepaths. Default: unset, which means use a random value.
JIT_COMPILE | Set to any value to compile the model with XLA. Defaults to unset; set to any value to enable.
PREDICT_COUNT=25 | The number of items from the (SCRAMBLED) dataset to make a prediction for.
PREDICT_AS_ONE | [prediction only] Set to any value to avoid splitting the input dataset into training/validation and instead treat it as a single dataset. Default: False (treat it as training/validation)
POSTFIX | Postfix to append to the output directory name (primarily auto calculated if DIR_OUTPUT is not specified, but this allows adjustments to be made without setting DIR_OUTPUT).
ARGS | Optional. Any additional arguments to pass to the python program.
> [!IMPORTANT]
> It is strongly advised that all filepaths do **NOT** contain spaces.
**Making predictions:** Set `PATH_CHECKPOINT` to point to a checkpoint file to make predictions with an existing model that you trained earlier instead of training a new one. Data is pulled from the given dataset, same as during training. The first `PREDICT_COUNT` items in the dataset are picked to make a prediction.
> [!NOTE] The dataset pipeline is naturally non-deterministic with respect to the order in which samples are read. Ensuring the ordering of samples is not mangled is only possible when making predictions, and requires a number of environment variables to be set:
>
> - **`PREDICT_AS_ONE`:** Set to any value to disable the training / validation split
> - **`PARALLEL_READS`:** Set to `0` to reading input files sequentially.
## Contributing
Contributions are very welcome - both issues and pull requests! Please mention in any pull requests that you release your work under the AGPL-3 (see below).
## License
All the code in this repository is released under the GNU Affero General Public License unless otherwise specified. The full license text is included in the [`LICENSE.md` file](./LICENSE.md) in this repository. GNU [have a great summary of the licence](https://www.gnu.org/licenses/#AGPL) which I strongly recommend reading before using this software.
All the code in this repository is released under the GNU Affero General Public License 3.0 unless otherwise specified. The full license text is included in the [`LICENSE.md` file](./LICENSE.md) in this repository. GNU [have a great summary of the licence](https://www.gnu.org/licenses/#AGPL) which I strongly recommend reading before using this software.
> [!NOTE] AGPL 3.0 was chosen for a number of reasons. The code in this repository has taken a very large amount of effort to put together, and to this end it is my greatest wish that this code and all derivatives be open-source. Open-source AI models enable the benefits thereof to be distributed and shared to all, and ensure transparency surrounding methodology, process, and limitations.
>
> You may contact me to negotiate a different licence, but do not hold out hope.
>
> --Starbeamrainbowlabs, aka Lydia Bryan-Smith
> Primary author