The dataset viewer is not available for this dataset.
Error code: ConfigNamesError
Exception: ValueError
Message: Some splits are duplicated in data_files: ['train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'validation', 'validation', 'validation', 'test', 'test']
Traceback: Traceback (most recent call last):
File "/src/services/worker/src/worker/job_runners/dataset/config_names.py", line 67, in compute_config_names_response
config_names = get_dataset_config_names(
path=dataset,
token=hf_token,
)
File "/usr/local/lib/python3.14/site-packages/datasets/inspect.py", line 161, in get_dataset_config_names
dataset_module = dataset_module_factory(
path,
...<4 lines>...
**download_kwargs,
)
File "/usr/local/lib/python3.14/site-packages/datasets/load.py", line 1215, in dataset_module_factory
raise e1 from None
File "/usr/local/lib/python3.14/site-packages/datasets/load.py", line 1190, in dataset_module_factory
).get_module()
~~~~~~~~~~^^
File "/usr/local/lib/python3.14/site-packages/datasets/load.py", line 646, in get_module
patterns = sanitize_patterns(next(iter(metadata_configs.values()))["data_files"])
File "/usr/local/lib/python3.14/site-packages/datasets/data_files.py", line 151, in sanitize_patterns
raise ValueError(f"Some splits are duplicated in data_files: {splits}")
ValueError: Some splits are duplicated in data_files: ['train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'train', 'validation', 'validation', 'validation', 'test', 'test']Need help to make the dataset viewer work? Make sure to review how to configure the dataset viewer, and open a discussion for direct support.
GOES–OMNI >2 MeV Electron Flux Forecasting
This dataset combines cross-calibrated NOAA GOES-14/GOES-16 >2 MeV electron flux with NASA/GSFC OMNI solar-wind and geomagnetic drivers on a uniform five-minute UTC grid.
It provides two configurations:
ml-ready(default): scaled causal features, validity flags, unscaled 30-minute/6-hour/12-hour targets, and leakage-safe chronological splits.scientific-master: unscaled source measurements, instrument context, calibration factors, and explicit missingness.
Load the data
from datasets import load_dataset
ml = load_dataset(
"snowsadh/goes-omni-electron-flux-forecasting",
"ml-ready",
)
master = load_dataset(
"snowsadh/goes-omni-electron-flux-forecasting",
"scientific-master",
split="full",
)
Size and coverage
| Configuration / split | Rows | Coverage |
|---|---|---|
| Scientific master | 1,326,459 | 2013-05-23 to 2025-12-31 |
| ML train | 978,265 | 2014-01-01 to 2023-06-30 11:55 UTC |
| ML validation | 102,186 | 2023-07-01 to 2024-06-30 11:55 UTC |
| ML test | 80,612 | 2024-07-01 to 2025-04-07 07:50 UTC |
GOES flux ends on 2025-04-07; later scientific-master rows contain OMNI data only. Every ML target remains inside the same temporal split as its features.
Processing
GOES-14 one-minute observations are normalized to exact minutes and aggregated
in log space. GOES-14 and GOES-16 are cross-calibrated in one-hour magnetic
local-time bins over their 2017 overlap. The corrected series is combined with
five-minute means of OMNI drivers. ML features use only causal information;
missing inputs are carried forward for at most one hour and then replaced with
a training-only median. RobustScaler is fitted on the training split only.
Full definitions are in DATA_DICTIONARY.md; preprocessing parameters are in
preprocessing_meta.json; source-level provenance is in SOURCES.md.
Intended uses
- Forecasting GEO >2 MeV electron flux 30 minutes, 6 hours, or 12 hours ahead.
- Space-weather time-series analysis and storm case studies.
- Multi-instrument calibration and leakage-safe ML demonstrations.
Limitations
- The data form a GOES-14/GOES-16 time series, not a global radiation-belt map.
- Satellite longitude and detector geometry change across the 2017 splice.
- MLT-bin calibration cannot recover values below the GOES-14 EPEAD noise floor.
- Values below flux 10 are retained and explicitly marked.
- Imputed ML features must not be interpreted as physical observations.
- OMNI combines several upstream spacecraft and maps measurements toward Earth's bow-shock nose.
- No ISRO GRASP data are included, and the series is not validated at Indian GEO longitude.
License
The compiled data and documentation are licensed under CC BY 4.0 to the
extent the creator holds applicable rights. Processing scripts are MIT-licensed.
Upstream public-domain/CC0/source-specific terms remain in force; see
LICENSE-DATA.md and SOURCES.md.
TsFile Conversion
Original dataset:
snowsadh/goes-omni-electron-flux-forecastingModalities: Time-series
Converted data files are listed in the YAML metadata above.
Source README text and dataset-specific metadata are retained; the source Usage section is replaced with the executable TsFile Python SDK example below.
Both source configurations are retained:
ml-readytrain/validation/test andscientific-masterfull.Source
timeis encoded as millisecondTime; satellite/instrument metadata and configuration labels are TAG columns where present.Numeric scientific and ML fields, including validity flags and forecasting targets, are retained.
Usage
Install the Apache TsFile Python SDK (pip install tsfile) and read a converted file:
from pathlib import Path
from tsfile import TsFileReader
path = Path("goes_omni_ml_ready_test_1.tsfile")
with TsFileReader(str(path)) as reader:
schemas = reader.get_all_table_schemas()
print("tables:", list(schemas))
table_name = next(iter(schemas))
table = schemas[table_name]
columns = [column.get_column_name() for column in table.get_columns()]
print("columns:", columns)
field_names = [
column.get_column_name()
for column in table.get_columns()
if column.get_column_name() not in {"Time", "time"}
]
if field_names:
with reader.query_table(table_name, field_names[:3], batch_size=1024) as result:
batch = result.read_arrow_batch()
if batch is not None:
print(batch.to_pandas().head())
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