Datasets:
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']
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']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.
COSMOGONY Multimodal v3 Scaled (TsFile)
Apache TsFile version of cmgyai/cosmogony-multimodal-v3-scaled.
Overview
COSMOGONY Multimodal v3 Scaled is a public, mission-aligned COSMOGONY training
corpus for multimodal space-physics representation learning. It is curated from
public providers and published as a materialized dataset for direct training.
Each row is one observation: a stable identifier, a modality, a named provider
and provenance URL, a time or catalog field, a per-row named feature vector, and
a long task_relevance sentence describing the intended downstream reasoning.
- Rows: 4,446,916 (split
train), published as 6 parquet shards and converted here into 6.tsfilefiles with one shared schema. - Modalities:
space_weather_timeseries,orbital_elements,light_curve,planetary_system_catalog. - Source families: NASA SPDF OMNI hourly products; NASA SPDF OMNI high-resolution minute products (2020–2026); CelesTrak selected public orbital groups; NASA Exoplanet Archive catalog products; NASA DONKI solar event records; GCAT satellite catalog; CelesTrak Consolidated Space Weather; NOAA/CelesTrak space-weather indices; Asteroid Lightcurve Database (LCDB); and an exoplanet-transit detection catalog (Kepler/K2/TESS).
- Time span: observations and catalog epochs from 1957 onward, plus a small set of rows whose source field is not a wall-clock instant (see notes below).
Schema (TsFile structure)
- Time (INT64, milliseconds) — epoch ms derived from the source
timestampcolumn. Rows whose source timestamp is an empty string (50,118) or a bare BJD-like float (15,721) have no true instant; they are kept and assigned a deterministic synthetic placeholder starting at2100-01-01T00:00:00Z. - modality (TAG) — the source one-element
modalitylist joined into a string. Example query:WHERE modality = 'space_weather_timeseries'. - source (TAG) — provider name, e.g.
WHERE source = 'NASA OMNI2 hourly'. - task_relevance (TAG) — the long downstream-task sentence for the row.
- seq (TAG) — disambiguation tag added during conversion. Several catalog
providers publish date-level records, so many rows share the same
(modality, source, task_relevance, Time)key; TsFile does not allow duplicate timestamps inside one device, andseqis the per-key ordinal that keeps every row addressable without changing any source value. - record_id (FIELD, STRING) — stable source identifier (unique per row).
- source_url (FIELD, STRING) — provenance URL exactly as published.
- timestamp_raw (FIELD, STRING) — the original
timestampstring, kept verbatim so no information is lost whenTimecannot be parsed. - feature_names (FIELD, STRING) — JSON array naming the entries of
featuresfor that row. - features_0 … features_19 (FIELD, DOUBLE) — the source
featuresvector exploded into fixed columns.
Heterogeneous feature vectors. features is not homogeneous across the
corpus: its length and meaning depend on modality/source, and
feature_names records that meaning per row (observed lengths 7, 8, 10, 11,
12, 14, 16 and 20). To produce one consistent TsFile schema, every row was
padded to the global maximum length of 20 before exploding, so
features_0 … features_19 exist in every file. Shorter rows are NaN-padded
(written as null) in the extra columns; nothing is truncated and no feature
entry is dropped. Always read feature_names together with the row's
modality/source before interpreting a features_i column.
FAIR-oriented curation notes
The original dataset follows repository guidelines for findability, accessibility, interoperability and reusability:
- Findable: each row has a stable
record_id, explicitsource, andsource_url. - Accessible: source access methods remain transparent via provider URLs.
- Interoperable: normalized schema and modality vocabulary across source families.
- Reusable: fixed provenance fields and explicit task-intent metadata
(
task_relevance).
Quality controls applied before publication include non-empty modality,
aligned feature_names/features lengths, required identity/time fields,
deterministic ordering by record_id, and duplicate record_id removal.
Intended uses
- self-supervised representation learning for space-physics signals
- masked reconstruction and forecasting pretraining
- multimodal encoder warm-start for downstream COSMOGONY models
Limitations
- This release is not a complete mirror of all upstream archives.
- License posture is source-specific, so the repository-level license remains
other. - Modal coverage is weighted toward space-weather time series in this version.
- Raw catalog records (empty or BJD-like timestamps) are preserved but their
TsFile
Timeis a synthetic placeholder rather than a true observation time.
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("cosmogony_multimodal_v3_scaled_part00.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())
Source & license
- Original dataset: https://huggingface.co/datasets/cmgyai/cosmogony-multimodal-v3-scaled
- Author / publisher: COSMOGONY (cmgyai); curated from public space-physics providers
- License: other — licensing is source-specific. The original card declares
repository-level
license: otherand each row keeps its ownsource/source_urlprovenance; please defer to the original providers for the terms of individual records.
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