Datasets:
The dataset viewer is not available for this subset.
Exception: SplitsNotFoundError
Message: The split names could not be parsed from the dataset config.
Traceback: Traceback (most recent call last):
File "/usr/local/lib/python3.12/site-packages/datasets/inspect.py", line 286, in get_dataset_config_info
for split_generator in builder._split_generators(
^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/packaged_modules/tsfile/tsfile.py", line 271, in _split_generators
scan = self._scan_metadata(all_files)
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/packaged_modules/tsfile/tsfile.py", line 304, in _scan_metadata
from tsfile.constants import TIME_COLUMN, ColumnCategory
ModuleNotFoundError: No module named 'tsfile'
The above exception was the direct cause of the following exception:
Traceback (most recent call last):
File "/src/services/worker/src/worker/job_runners/config/split_names.py", line 66, in compute_split_names_from_streaming_response
for split in get_dataset_split_names(
^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/inspect.py", line 340, in get_dataset_split_names
info = get_dataset_config_info(
^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/inspect.py", line 291, in get_dataset_config_info
raise SplitsNotFoundError("The split names could not be parsed from the dataset config.") from err
datasets.inspect.SplitsNotFoundError: The split names could not be parsed from the dataset config.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.
Deep Space Probes -- Merged Hourly Data (TsFile)
This dataset is a lossless conversion to the Apache TsFile
format of the HuggingFace dataset
juliensimon/deep-space-probes.
The original observations come from the NASA Space Physics Data Facility
(SPDF).
Original dataset
- Source dataset: juliensimon/deep-space-probes
- Author: Julien Simon
- Data origin: NASA SPDF (https://spdf.gsfc.nasa.gov/)
- License: CC-BY-4.0
- Content: Merged hourly measurements of magnetic field, solar-wind plasma, and energetic-particle fluxes from humanity's four most distant spacecraft (Voyager 1/2, Pioneer 10/11), spanning 1972-01-01 .. 2025-12-31 (UTC).
Scale
- 1,183,368 hourly records, 49 columns
- 4 spacecraft (each stored as an independent device / TAG):
- Voyager 1: 403,224 rows
- Voyager 2: 385,704 rows
- Pioneer 10: 210,384 rows
- Pioneer 11: 184,056 rows
TsFile storage mapping (table model)
| Role | Column | Type | Description |
|---|---|---|---|
| TAG | spacecraft |
STRING | Spacecraft identifier; one spacecraft = one independent device/series (voyager_1 / voyager_2 / pioneer_10 / pioneer_11) |
| Time | source datetime |
INT64 (ms) | Hourly UTC timestamp, no gaps; used as the time primary key |
| FIELD | the other 47 columns | DOUBLE | All measurement columns: position (heliocentric_distance_au, hgi_*deg), magnetic field (b*rtn_nt, b_magnitude*), solar wind (flow*, proton), and energetic-particle fluxes per energy channel (flux_h_crs_ / crt_* / lecp_*) |
Conversion notes
- No columns were dropped: all 47 original measurement columns are preserved as DOUBLE.
- Nulls are kept as-is (not filled, not removed). The spacecraft carry different instrument suites, so some columns are entirely null for a given spacecraft (e.g. CRS channels exist only on the Voyagers, CRT channels only on the Pioneers). This is a property of the data itself; when stored per-device, a column that is all-null for a device is simply not written for that device — this is not an active column drop.
- Time precision is
ms(the sourcedatetimeis on exact hour boundaries, so milliseconds are lossless). - Within each spacecraft, rows are sorted ascending by Time;
(spacecraft, datetime)is already unique and free of duplicates in the source.
Data integrity / read-back notes
The converted files were verified timestamp-by-timestamp and value-by-value against the source and match exactly (max absolute difference on matched values = 0.0, null vs. 0.0 distinguished correctly, per-spacecraft row counts identical to the source parquet, 1,183,368 in total).
⚠️ Read-back tip: this dataset is highly sparse (a given timestamp usually has only a few populated columns, and some columns have long leading runs of nulls). When using the TsFile Python SDK
query_table, querying on a single sparse column alone may return fewer rows than expected (a known query-layer behaviour; the file contents themselves are complete). Include one almost-always-populated column (e.g.heliocentric_distance_au) in the query to reliably obtain the full set of device rows.
Layout
The TsFiles live under data/. The tool emits the data as multiple .tsfile
shards (one new shard per 1,000,000 rows), which together form the complete dataset:
data/
├── deep_space_probes_1.tsfile
└── deep_space_probes_2.tsfile
Usage
from tsfile import TsFileReader
reader = TsFileReader("data/deep_space_probes_1.tsfile")
schemas = reader.get_all_table_schemas()
tname = next(iter(schemas))
# Include a dense column to avoid row truncation on sparse-column queries
cols = ["spacecraft", "heliocentric_distance_au", "b_magnitude_nt", "flow_speed_kms"]
with reader.query_table(tname, cols, batch_size=65536) as rs:
while (batch := rs.read_arrow_batch()) is not None:
df = batch.to_pandas()
# ... process ...
reader.close()
Citation
@dataset{deep_space_probes,
title = {Deep Space Probes -- Merged Hourly Data},
author = {juliensimon},
year = {2026},
url = {https://huggingface.co/datasets/juliensimon/deep-space-probes},
publisher = {Hugging Face}
}
Data origin: NASA Space Physics Data Facility (SPDF, https://spdf.gsfc.nasa.gov/). Original dataset licensed under CC-BY-4.0.
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