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The dataset viewer is not available for this split.
Cannot load the dataset split (in streaming mode) to extract the first rows.
Error code:   StreamingRowsError
Exception:    ArrowInvalid
Message:      Mismatching child array lengths
Traceback:    Traceback (most recent call last):
                File "/src/services/worker/src/worker/utils.py", line 147, in get_rows_or_raise
                  return get_rows(
                      dataset=dataset,
                  ...<4 lines>...
                      column_names=column_names,
                  )
                File "/src/libs/libcommon/src/libcommon/utils.py", line 272, in decorator
                  return func(*args, **kwargs)
                File "/src/services/worker/src/worker/utils.py", line 127, in get_rows
                  rows_plus_one = list(itertools.islice(safe_iter(ds, dataset=dataset), rows_max_number + 1))
                File "/src/services/worker/src/worker/utils.py", line 483, in safe_iter
                  yield from ds.decode(False) if ds.features else ds
                File "/usr/local/lib/python3.14/site-packages/datasets/iterable_dataset.py", line 2951, in __iter__
                  for key, example in ex_iterable:
                                      ^^^^^^^^^^^
                File "/usr/local/lib/python3.14/site-packages/datasets/iterable_dataset.py", line 2461, in __iter__
                  for key, pa_table in self._iter_arrow():
                                       ~~~~~~~~~~~~~~~~^^
                File "/usr/local/lib/python3.14/site-packages/datasets/iterable_dataset.py", line 2486, in _iter_arrow
                  for key, pa_table in self.ex_iterable._iter_arrow():
                                       ~~~~~~~~~~~~~~~~~~~~~~~~~~~~^^
                File "/usr/local/lib/python3.14/site-packages/datasets/iterable_dataset.py", line 547, in _iter_arrow
                  for key, pa_table in iterator:
                                       ^^^^^^^^
                File "/usr/local/lib/python3.14/site-packages/datasets/iterable_dataset.py", line 430, in _iter_arrow
                  for key, pa_table in self.generate_tables_fn(**gen_kwags):
                                       ~~~~~~~~~~~~~~~~~~~~~~~^^^^^^^^^^^^^
                File "/usr/local/lib/python3.14/site-packages/datasets/packaged_modules/hdf5/hdf5.py", line 83, in _generate_tables
                  pa_table = _recursive_load_arrays(h5, self.info.features, start, end)
                File "/usr/local/lib/python3.14/site-packages/datasets/packaged_modules/hdf5/hdf5.py", line 267, in _recursive_load_arrays
                  arr = _recursive_load_arrays(obj, features[path], start, end)
                File "/usr/local/lib/python3.14/site-packages/datasets/packaged_modules/hdf5/hdf5.py", line 288, in _recursive_load_arrays
                  sarr = pa.StructArray.from_arrays(values, names=keys)
                File "pyarrow/array.pxi", line 4385, in pyarrow.lib.StructArray.from_arrays
                File "pyarrow/error.pxi", line 155, in pyarrow.lib.pyarrow_internal_check_status
                File "pyarrow/error.pxi", line 92, in pyarrow.lib.check_status
                  raise convert_status(status)
              pyarrow.lib.ArrowInvalid: Mismatching child array lengths

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Held–Suarez Dry Atmosphere (dry-atmosphere-3D)

One line description of the data: 162 3D Held–Suarez dry-atmosphere simulations on 8 pressure levels.

Longer description of the data: Held–Suarez is the standard benchmark for the dynamical cores of atmospheric general circulation models. It is a dry atmosphere with no topography, forced by relaxing temperature toward a zonally symmetric equilibrium and damped by Rayleigh friction near the surface. Baroclinic instability produces eddy-driven jets and storm tracks. We vary the rotation rate Ω\Omega, the equator-to-pole temperature contrast ΔTy\Delta T_y, and the static stability Δθz\Delta\theta_z, which changes the number, latitude, and width of the jets. This dataset is of particular relevance since it serves as a simple proxy for the complex atmospheric dynamics that drive weather forecasting.

Code or software used to generate the data: ClimaAtmos.jl, the atmospheric component of the CliMA software stack.

Visualization:

About the data

Dimension of discretized data: 1461 snapshots per trajectory (365 days, 6-hourly) on an 8×144×2888 \times 144 \times 288 (level × lat × lon) grid, plus surface pressure.

Fields available in the data:

HDF5 path Shape Units Description
t0_fields/T (1, 1461, 8, 144, 288) K Air temperature
t0_fields/ps (1, 1461, 1, 144, 288) Pa Surface pressure
t1_fields/velocity (1, 1461, 8, 144, 288, 2) m/s Horizontal wind; last axis is [u, v] (zonal, meridional)
scalars/{omega_factor, delta_T_y, delta_theta_z, seed} () — Run parameters (seed is stored as a float)
dimensions/{time, level, lat, lon} — s, hPa, °, ° Coordinates

Number of trajectories: 162: 3×3×33 \times 3 \times 3 parameter combinations, each with 6 seeds.

Estimated size of the ensemble of all simulations: 667 GB (compressed HDF5).

Grid type: 8×144×2888 \times 144 \times 288 level-lat-lon grid (equiangular). Levels are given by pressure from 50 hPa to 1000 hPa. If the surface pressure is below 1000 hPa, ClimaAtmos.jl fills the 1000 hPa level with the values at the lowest z-level of the simulation.

Initial conditions: An atmosphere at rest with a decaying temperature profile, plus a small seeded temperature perturbation below 5 km. The first 200 days are discarded as spin-up.

Boundary conditions: Spherical; flat and homogeneous lower boundary (no topography, no surface fluxes).

Simulation time-step (Δt)(\Delta t): 100 s.

Data are stored separated by (δt)(\delta t): 6 hours.

Total time range (tmin(t_{min} to tmax)t_{max}): Day 200 to day 565 of each run. (time coordinate counts seconds from the start of the simulation, so the runs begin at 17,280,000 s).

Set of coefficients or non-dimensional parameters evaluated:

  • omega_factor =Ω/Ωearth∈{0.5,1.0,2.0}= \Omega/\Omega_{\rm earth} \in \{0.5, 1.0, 2.0\}, where Ωearth=7.292×10−5 s−1\Omega_{\rm earth} = 7.292 \times 10^{-5}\,\mathrm{s}^{-1}
  • delta_T_y =ΔTy∈{40,60,80}= \Delta T_y \in \{40, 60, 80\} K, the equator-to-pole contrast in equilibrium temperature
  • delta_theta_z =Δθz∈{5,10,20}= \Delta\theta_z \in \{5, 10, 20\} K, the vertical potential-temperature contrast (sets the static stability)
  • seed ∈{0,…,5}\in \{0, \ldots, 5\}, the initial perturbation

The canonical Held–Suarez setting is at the center point (1.0, 60, 10).

Approximate time to generate the data: Per-run wall-time on the order of six hours.

Hardware used to generate the data: GPU-accelerated generation, using one GPU per run (either an NVIDIA RTX 4090, NVIDIA L40S, or NVIDIA A100).

Loading

It's important to load hdf5plugin before h5py to make sure the filters are registered properly.

Download a single run (≈4.3 GB) and read it with h5py:

import hdf5plugin  # registers the LZ4 filter, must come before reading
import h5py
from huggingface_hub import hf_hub_download

path = hf_hub_download("sada-group/dry-atmosphere-3D", "data/test/run_0014.h5", repo_type="dataset")
with h5py.File(path, "r") as f:
    T = f["t0_fields/T"][0, :8]              # (8 steps, 8 levels, 144, 288)
    u, v = f["t1_fields/velocity"][0, :8].transpose(4, 0, 1, 2, 3)
    params = {k: f["scalars"][k][()] for k in f["scalars"]}

The full dataset is 667 GB. To download a subset, e.g. the 16 test runs (≈70 GB), use snapshot_download with allow_patterns:

from huggingface_hub import snapshot_download

root = snapshot_download(
    "sada-group/dry-atmosphere-3D",
    repo_type="dataset",
    allow_patterns=["data/test/*", "stats.yaml"],  # drop allow_patterns for everything
)

Please cite the associated paper if you use this data in your research:

@misc{muser2026dandelionsphericalflowerneural,
      title={Dandelion: A Spherical Flower for Neural Simulation of Planetary Dynamics}, 
      author={Till Muser and Giovanni Abati and Ivan Dokmanić},
      year={2026},
      eprint={2608.27521},
      archivePrefix={arXiv},
      primaryClass={cs.LG},
      url={https://arxiv.org/abs/2608.27521}, 
}

as well as the original benchmark and the solver:

@article{held1994proposal,
  title={A proposal for the intercomparison of the dynamical cores of atmospheric general circulation models},
  author={Held, Isaac M and Suarez, Max J},
  journal={Bulletin of the American Meteorological society},
  volume={75},
  number={10},
  pages={1825--1830},
  year={1994},
  publisher={American Meteorological Society}

}

@article{yatunin2026climate,
  title={The climate modeling alliance atmosphere dynamical core: Concepts, numerics, and scaling},
  author={Yatunin, Dennis and Byrne, Simon and Kawczynski, Charles and Kandala, Sriharsha and Bozzola, Gabriele and Sridhar, Akshay and Shen, Zhaoyi and Jaruga, Anna and Sloan, Julia and He, Jia and others},
  journal={Journal of Advances in Modeling Earth Systems},
  volume={18},
  number={3},
  pages={e2025MS005014},
  year={2026},
  publisher={Wiley Online Library}
}
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