This project is used for training PVNet and running PVNet on live data.
PVNet2 is a multi-modal late-fusion model that largely inherits the same architecture from PVNet1.0. The NWP (Numerical Weather Prediction) and satellite data are sent through some neural network which encodes them down to 1D intermediate representations. These are concatenated together with the GSP (Grid Supply Point) output history, the calculated solar coordinates (azimuth and elevation) and the GSP ID which has been put through an embedding layer. This 1D concatenated feature vector is put through an output network which outputs predictions of the future GSP yield. National forecasts are made by adding all the GSP forecasts together.
Our paper based on this repo was accepted into the Tackling Climate Change with Machine Learning workshop at ICLR 2024 and can be viewed here.
Some slightly more structured notes on deliberate experiments we have performed with PVNet are here.
Some very rough, early working notes on this model are here. These are now somewhat out of date.
git clone https://github.com/openclimatefix/PVNet.git
cd PVNet
pip install .
The commit history is extensive. To save download time, use a depth of 1:
git clone --depth 1 https://github.com/openclimatefix/PVNet.git
This means only the latest commit and its associated files will be downloaded.
Next, in the PVNet repo, install PVNet as an editable package:
pip install -e .
pip install ".[dev]"
Before running any code in PVNet, copy the example configuration to a configs directory:
cp -r configs.example configs
You will be making local amendments to these configs. See the README in
configs.example
for more info.
As a minimum, in order to create batches of data/run PVNet, you will need to supply paths to NWP and GSP data. PV data can also be used. We list some suggested locations for downloading such datasets below:
GSP (Grid Supply Point) - Regional PV generation data\ The University of Sheffield provides API access to download this data: https://www.solar.sheffield.ac.uk/api/
Documentation for querying generation data aggregated by GSP region can be found here: https://docs.google.com/document/d/e/2PACX-1vSDFb-6dJ2kIFZnsl-pBQvcH4inNQCA4lYL9cwo80bEHQeTK8fONLOgDf6Wm4ze_fxonqK3EVBVoAIz/pub#h.9d97iox3wzmd
NWP (Numerical weather predictions)\ OCF maintains a Zarr formatted version of the German Weather Service's (DWD) ICON-EU NWP model here: https://huggingface.co/datasets/openclimatefix/dwd-icon-eu which includes the UK
Please note that the current version of ICON loader supports a different format. If you want to use our ICON-EU dataset or your own NWP source, you can create a loader for it using the instructions here.
PV\ OCF maintains a dataset of PV generation from 1311 private PV installations here: https://huggingface.co/datasets/openclimatefix/uk_pv
Outside the PVNet repo, clone the ocf-datapipes repo and exit the conda env created for PVNet: https://github.com/openclimatefix/ocf_datapipes
git clone --depth 1 https://github.com/openclimatefix/ocf_datapipes.git
conda create -n ocf_datapipes python=3.10
Then go inside the ocf_datapipes repo to add packages
pip install -r requirements.txt -r requirements-dev.txt
Then exit this environment, and enter back into the pvnet conda environment and install ocf_datapies in editable mode (-e). This means the package is directly linked to the source code in the ocf_datapies repo.
pip install -e <PATH-TO-ocf_datapipes-REPO>
PVNet contains a script for generating batches of data suitable for training the PVNet models. To run the script you will need to make some modifications to the datamodule configuration.
Make sure you have copied the example configs (as already stated above):
cp -r configs.example configs
We will use the following example config file for creating batches: /PVNet/configs/datamodule/configuration/example_configuration.yaml
. Ensure that the file paths are set to the correct locations in example_configuration.yaml
: search for PLACEHOLDER
to find where to input the location of the files. You will need to comment out or delete the parts of example_configuration.yaml
pertaining to the data you are not using.
When creating batches, an additional datamodule config located in PVNet/configs/datamodule
is passed into the batch creation script: streamed_batches.yaml
. Like before, a placeholder variable is used when specifying which configuration to use:
configuration: "PLACEHOLDER.yaml"
This should be given the whole path to the config on your local machine, for example:
configuration: "/FULL-PATH-TO-REPO/PVNet/configs/datamodule/configuration/example_configuration.yaml"
Where FULL-PATH-TO-REPO
represent the whole path to the PVNet repo on your local machine.
This is also where you can update the train, val & test periods to cover the data you have access to.
Run the save_batches.py
script to create batches with the parameters specified in the datamodule config (streamed_batches.yaml
in this example):
python scripts/save_batches.py
PVNet uses
hydra which enables us to pass variables via the command
line that will override the configuration defined in the ./configs
directory, like this:
python scripts/save_batches.py datamodule=streamed_batches datamodule.batch_output_dir="./output" datamodule.num_train_batches=10 datamodule.num_val_batches=5
scripts/save_batches.py
needs a config under PVNet/configs/datamodule
. You can adapt streamed_batches.yaml
or create your own in the same folder.
If downloading private data from a GCP bucket make sure to authenticate gcloud (the public satellite data does not need authentication):
gcloud auth login
Files stored in multiple locations can be added as a list. For example, in the example_configuration.yaml
file we can supply a path to satellite data stored on a bucket:
satellite:
satellite_zarr_path: gs://solar-pv-nowcasting-data/satellite/EUMETSAT/SEVIRI_RSS/v4/2020_nonhrv.zarr
Or to satellite data hosted by Google:
satellite:
satellite_zarr_paths:
- "gs://public-datasets-eumetsat-solar-forecasting/satellite/EUMETSAT/SEVIRI_RSS/v4/2020_nonhrv.zarr"
- "gs://public-datasets-eumetsat-solar-forecasting/satellite/EUMETSAT/SEVIRI_RSS/v4/2021_nonhrv.zarr"
Datapipes are currently set up to use 11 channels from the satellite data, the 12th of which is HRV and is not included in these.
How PVNet is run is determined by the extensive configuration in the config
files. The configs stored in PVNet/configs.example
should work with batches created using the steps and batch creation config mentioned above.
Make sure to update the following config files before training your model:
configs/datamodule/local_premade_batches.yaml
:
batch_dir
to point to the directory you stored your batches in during batch creationconfigs/model/local_multimodal.yaml
:
in_channels
: number of variables your NWP source suppliesimage_size_pixels
: spatial crop of your NWP data. It depends on the spatial resolution of your NWP; should match nwp_image_size_pixels_height
and/or nwp_image_size_pixels_width
in datamodule/example_configs.yaml
, unless transformations such as coarsening was applied (e. g. as for ECMWF data)configs/local_trainer.yaml
:
accelerator: 0
if running on a system without a supported GPUIf creating copies of the config files instead of modifying existing ones, update defaults
in the main ./configs/config.yaml
file to use
your customised config files:
defaults:
- trainer: local_trainer.yaml
- model: local_multimodal.yaml
- datamodule: local_premade_batches.yaml
- callbacks: null
- logger: csv.yaml
- experiment: null
- hparams_search: null
- hydra: default.yaml
Assuming you ran the save_batches.py
script to generate some premade train and
val data batches, you can now train PVNet by running:
python run.py
If you have successfully trained a PVNet model and have a saved model checkpoint you can create a backtest using this, e.g. forecasts on historical data to evaluate forecast accuracy/skill. This can be done by running one of the scripts in this repo such as the UK GSP backtest script or the the pv site backtest script, further info on how to run these are in each backtest file.
You can use python -m pytest tests
to run tests