Model Card for ESFM/ESFM_s_nm_pre

Released intermediate checkpoint in the no-masking ERA5 lineage, initialized from the knowledge-distilled ESFM encoder. It forecasts six hours ahead from complete, dense ERA5 inputs.

Checkpoint selection: Use for reproducing the released no-masking training lineage or investigating the checkpoint before its final continuation. Prefer ESFM_s_nm for the final released dense-input baseline.

Model Details

Developed by: The ESFM research team, with the full contributor and author lists linked below.
Shared by: ESFM on Hugging Face
Model type: Intermediate deterministic ERA5 checkpoint; modified 3D Swin-UNet encoder-decoder
Model size: Approximately 115 million parameters
Masking protocol: No observation masking
Forecast lead time: 6 hours
License: MIT
Repository: https://huggingface.co/ESFM/ESFM_s_nm_pre

Model Sources

Code: https://github.com/swiss-ai/ESFM
Paper: https://arxiv.org/abs/2605.00850
Project page: https://swiss-ai.github.io/ESFM/

The paper is currently available as an arXiv preprint.

Uses

Direct Use

Use for reproducing the released no-masking training lineage or investigating the checkpoint before its final continuation. Prefer ESFM_s_nm for the final released dense-input baseline.

Downstream Use

Base checkpoint for ESFM_s_nm and, through that lineage, ESFM_s_nm_ens.

Out-of-Scope Use

Do not use with absent variables, missing pressure levels, arbitrary NaN regions, or sparse station/satellite layouts; this lineage was not trained for those conditions.

Bias, Risks, and Limitations

The checkpoint assumes the ERA5 variable set and dense 0.25-degree gridded inputs. It inherits ERA5 biases and is not rollout-finetuned for long-range operational forecasting.

All ESFM checkpoints are research artifacts. Users should validate forecasts for their variables, regions, seasons, lead times, missingness pattern, and decision context. Do not use the model as the sole basis for safety-critical decisions.

How to Get Started

The checkpoint is not packaged as a Hugging Face Transformers from_pretrained model. Construct the ESFM architecture with the matching repository config, then load the state dictionary. The released notebook contains the complete download, model-construction, normalization, and inference workflow.

git clone https://github.com/swiss-ai/ESFM.git
cd ESFM
# Open notebooks/inference_ESFMs_on_ERA5.ipynb

In the notebook, set:

EXPERIMENT_NAME = "ESFM_s_nm_pre"

To download the weights directly:

from huggingface_hub import hf_hub_download

model_name = "ESFM_s_nm_pre"
weights_path = hf_hub_download(
    repo_id=f"ESFM/{model_name}",
    filename=f"{model_name}.safetensors",
)
print(weights_path)

Set EXPERIMENT_NAME = "ESFM_s_nm_pre" in notebooks/inference_ESFMs_on_ERA5.ipynb, or use configs/config_ESFM_s_nm_pre.yaml in the released inference code.

Training Details

Training Data

WeatherBench2 ERA5 at 0.25-degree resolution, trained on 1979 through 2020. The standard configuration uses four surface variables, five atmospheric variables on 13 pressure levels, and three static fields.

Dataset preprocessing and the exact variable registry are documented in the ESFM repository and preprint.

Training Procedure

Initialized from ESFM_s_enc_KD_nm and trained for 100,000 steps on ERA5 using MAE-based deterministic training without the missing-data masking protocol. This experiment was run on 16 GPUs.

Training objective: Six-hour forecast learning, as specified above
Nominal architecture: ESFM small, approximately 115M parameters
Software environment: PyTorch/Lightning in the released NVIDIA PhysicsNeMo 25.03 container; lightning==2.5.1 is pinned in the Dockerfile
Training regime: Lightning precision="32-true" with FP32 parameters and optimizer state; selected model forward operations use CUDA BF16 autocasting through torch.autocast(dtype=torch.bfloat16).

Evaluation

The manuscript reports evaluation for the completed no-masking lineage as a dense-reanalysis reference. This intermediate checkpoint is not separately tabulated; use the linked preprint for the final-lineage evaluation protocol.

The manuscript uses held-out temporal data and reports task-appropriate metrics: latitude-weighted MAE and Pearson correlation for gridded deterministic forecasts, relative MAE for MODIS comparisons, station metrics for station models, and CRPS for ensembles. Detailed values are intentionally not copied into this card.

Technical Specifications

ESFM retains Aurora's 3D Swin-UNet backbone and adds variable-specific tokenization, axial attention across variables, perceiver aggregation across variables and pressure levels, learnable NaN tokens for missing patches, resolution-specific tokenizers where configured, and a decoder queried at target pressure levels. The small configuration uses a 256-dimensional embedding and approximately 115M parameters.

Environmental Impact

Hardware type: NVIDIA GH200 systems with four GPUs per node. This experiment was run on four nodes, totaling 16 GPUs.
Total training time: 368 hours
Compute location: Training used CSCS Alps infrastructure.

Citation

@misc{ozdemir2026esfm,
  title={Earth System Foundation Model (ESFM): A unified framework for heterogeneous data integration and forecasting},
  author={Firat Ozdemir and Yun Cheng and Salman Mohebi and Fanny Lehmann and Simon Adamov and Zhenyi Zhang and Leonardo Trentini and Dana Grund and Oliver Fuhrer and Torsten Hoefler and Siddhartha Mishra and Sebastian Schemm and Benedikt Soja and Mathieu Salzmann},
  year={2026},
  eprint={2605.00850},
  archivePrefix={arXiv},
  primaryClass={physics.ao-ph},
  url={https://arxiv.org/abs/2605.00850}
}