Dataset Viewer
The dataset viewer is not available for this subset.
Cannot get the split names for the config 'default' of the dataset.
Exception:    SplitsNotFoundError
Message:      The split names could not be parsed from the dataset config.
Traceback:    Traceback (most recent call last):
                File "/usr/local/lib/python3.14/site-packages/datasets/inspect.py", line 286, in get_dataset_config_info
                  for split_generator in builder._split_generators(
                                         ~~~~~~~~~~~~~~~~~~~~~~~~~^
                      StreamingDownloadManager(base_path=builder.base_path, download_config=download_config)
                      ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
                  )
                  ^
                File "/usr/local/lib/python3.14/site-packages/datasets/packaged_modules/webdataset/webdataset.py", line 81, in _split_generators
                  first_examples = list(islice(pipeline, self.NUM_EXAMPLES_FOR_FEATURES_INFERENCE))
                File "/usr/local/lib/python3.14/site-packages/datasets/packaged_modules/webdataset/webdataset.py", line 32, in _get_pipeline_from_tar
                  fs: fsspec.AbstractFileSystem = fsspec.filesystem("memory")
                                                  ~~~~~~~~~~~~~~~~~^^^^^^^^^^
                File "/usr/local/lib/python3.14/site-packages/fsspec/registry.py", line 302, in filesystem
                  cls = get_filesystem_class(protocol)
                File "/usr/local/lib/python3.14/site-packages/fsspec/registry.py", line 239, in get_filesystem_class
                  raise ValueError(f"Protocol not known: {protocol}")
              ValueError: Protocol not known: memory
              
              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(
                               ~~~~~~~~~~~~~~~~~~~~~~~^
                      path=dataset,
                      ^^^^^^^^^^^^^
                      config_name=config,
                      ^^^^^^^^^^^^^^^^^^^
                      token=hf_token,
                      ^^^^^^^^^^^^^^^
                  )
                  ^
                File "/usr/local/lib/python3.14/site-packages/datasets/inspect.py", line 340, in get_dataset_split_names
                  info = get_dataset_config_info(
                      path,
                  ...<6 lines>...
                      **config_kwargs,
                  )
                File "/usr/local/lib/python3.14/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.

TwinnableAgent C-MAPSS Processed Parquet Data

This dataset hosts the processed NASA C-MAPSS turbofan degradation files used by TwinnableAgent. It includes FD001 through FD004 as parquet files plus the conversion script used to derive them from the NASA raw training text files.

Raw NASA zip and text dumps are intentionally not mirrored here. The raw source of record is the NASA Prognostics Center of Excellence C-MAPSS Turbofan Engine Degradation dataset, currently distributed through NASA Open Data as CMAPSSData.zip.

Files

File Rows Units Operating conditions Fault modes
FD001_processed.parquet 20,631 100 1 1
FD002_processed.parquet 53,759 260 6 1
FD003_processed.parquet 24,720 100 1 2
FD004_processed.parquet 61,249 249 6 2
scripts/convert_cmapss_to_parquet.py - - - -

Conversion

Each processed parquet is derived from the matching NASA training file:

train_FD001.txt -> FD001_processed.parquet
train_FD002.txt -> FD002_processed.parquet
train_FD003.txt -> FD003_processed.parquet
train_FD004.txt -> FD004_processed.parquet

The conversion keeps the NASA column order, assigns explicit column names, and adds a per-row remaining-useful-life label:

rul = max(cycle for unit) - cycle

The conversion command used by TwinnableAgent is:

python scripts/convert_cmapss_to_parquet.py --datasets FD001 FD002 FD003 FD004

Schema

All four parquet files use the same schema:

Column Type Meaning
unit integer Engine trajectory identifier.
cycle integer Time-cycle index within the trajectory.
op1, op2, op3 float NASA operating setting columns.
s1 through s21 float NASA sensor channels. Sensor units are anonymized by C-MAPSS.
rul integer Remaining useful life in cycles, derived during conversion.

Operating-condition clusters

TwinnableAgent PAL resolves FD002 and FD004 into six operating-condition groups by rounding the three operating settings to the nearest integer and assigning a stable label by sorted tuple order.

FD002 mapping:

Cluster Rounded (op1, op2, op3) Rows Units represented
op_cluster_0 (0, 0, 100) 8,044 260
op_cluster_1 (10, 0, 100) 8,096 260
op_cluster_2 (20, 1, 100) 8,122 260
op_cluster_3 (25, 1, 60) 8,002 260
op_cluster_4 (35, 1, 100) 8,037 260
op_cluster_5 (42, 1, 100) 13,458 260

FD004 mapping:

Cluster Rounded (op1, op2, op3) Rows Units represented
op_cluster_0 (0, 0, 100) 9,238 249
op_cluster_1 (10, 0, 100) 9,224 249
op_cluster_2 (20, 1, 100) 9,091 249
op_cluster_3 (25, 1, 60) 9,139 249
op_cluster_4 (35, 1, 100) 9,162 249
op_cluster_5 (42, 1, 100) 15,395 249

Provenance note: FD004 unit count

The NASA readme describes FD004 training data as 248 trajectories, but the raw train_FD004.txt file contains 249 distinct unit identifiers. This repository preserves the raw file as authoritative and reports FD004 as 249 units.

Intended use

These files support TwinnableAgent reproducibility, PAL adapter validation, cross-dataset predictive-maintenance experiments, and C-MAPSS RUL benchmark work. They are processed training trajectories, not raw NASA archives.

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