Skip to main content

Decode scientific file headers (MRC cryo-EM, extensible) into typed context for agents — pure, zero-dependency, with bounded parallel readers.

Project description

scigantic-headers

Read the metadata of a scientific file and return its fields (dimensions, data type, pixel size, columns, row count) as a dict, without reading the rest of the file. Decodes MRC, NPY, NIfTI, CryoSPARC .cs, and Parquet. The decode functions have no dependencies; separate reader functions fetch the bytes from a file or a URL (the leading bytes for most formats, the trailing bytes for Parquet, whose schema is in a footer).

from scigantic_headers import decode_file
hdr = decode_file("session/frame.mrc")
hdr.summary            # "MRC stack 4096x4096x16, float32"
hdr.fields["dtype"]    # "float32"
hdr.fields["nz"]       # 16   (frames)

One implementation, shared. The cloud probe's TypeScript twin (backend/src/services/headerDecoders.ts), the notebook, and the edge context-producer describe a file the same way. Same byte offsets, same mode -> dtype table, held to the same test fixtures so they cannot drift.

Edge use: the context-producer (infrastructure/edge/context-producer) runs this next to an instrument, with no network, on amd64 or arm64. The zero dependencies and header-only reads are what let it run there.

Install

Published to PyPI on a scigantic-headers-vX.Y.Z tag (see .github/workflows/scigantic-headers.yml):

pip install scigantic-headers

It has zero runtime dependencies, so it also installs from source into an air-gapped image with no package index at build time. The notebook and edge-producer images bundle it this way:

COPY infrastructure/python/scigantic-headers /tmp/scigantic-headers
RUN pip install /tmp/scigantic-headers

Both paths install the same version pinned in pyproject.toml. Consumers that install from an index should pin it (scigantic-headers==X.Y.Z).

Why it exists

A schema card or context record wants to say what a file is without opening it over a FUSE mount. A scientific file's first ~1 KiB is a structured header that already says so. This reads that, and nothing more.

Decoders today:

  • MRC / MRCS: cryo-EM micrographs, movie stacks, tilt series, EMDB maps.
  • NPY: NumPy arrays (ML, genomics, materials, not cryo-EM). Cross-checked against numpy.
  • NIfTI-1: neuroimaging volumes, .nii and .nii.gz (not cryo-EM). Cross-checked against nibabel. Big- and little-endian.
  • CryoSPARC .cs: a structured-array dataset. Reports record count and the field schema.
  • Parquet: reads the footer, not a leading header, and returns the column names, physical types, and row count. Cross-checked against pyarrow.

.gz is transparent. The reader decompresses just the leading block, so a gzipped .nii.gz or .mrc.gz decodes without inflating the whole file, and dispatch sees the inner format.

Adding a format is a pure bytes -> DecodedHeader | None function plus one register_decoder call. Nothing about the dispatch, the readers, or the batch path is cryo-EM-specific. NPY and NIfTI landed with zero plumbing changes.

Pixel size for raw movies

A raw MRC movie header has no pixel size: CELLA is 0, so decode_* returns pixelSizeA as None. The value is in the RELION STAR or CryoSPARC .cs file the workflow writes in the session, and the library reads it. read_session_optics finds that file next to (or above) the data file and returns the optics:

from scigantic_headers import decode_file, read_session_optics

hdr = decode_file("Movies/frame.mrc")       # header fields; pixelSizeA is None
opt = read_session_optics("Movies/frame.mrc")
# {'pixelSizeA': 1.05, 'voltageKv': 300.0, 'source': 'relion-star:particles.star'}

read_star_optics(path) and read_cryosparc_optics(path) read a specific optics file when you already know which one. The RELION 3.1 data_optics loop, the older key-value form, optics columns in the main data loop, and the legacy detector-pixel-size / magnification pair are all handled.

Layout

src/scigantic_headers/
  decoders.py   pure core: registry + MRC / NPY / NIfTI / .cs decoders
  parquet.py    Parquet footer decode (small Thrift-compact reader)
  sources.py    read leading bytes from file or URL; bounded parallel batch
  star.py       RELION STAR optics reader
  cryosparc.py  CryoSPARC .cs optics reader
  optics.py     read_session_optics: find a data file's optics file
  cli.py        scigantic-headers <file|url|--dir>
  benchmark.py  scigantic-headers-bench, measures the speed levers
tests/          pytest (117 tests, incl. fuzz + golden fixtures)

Robustness

A decoder is handed the leading bytes of arbitrary files, so it must be total: for any input it returns None or a valid, JSON-safe DecodedHeader. It never raises and never emits NaN or inf. This is enforced, not assumed.

  • Fuzz (test_fuzz.py): thousands of random and magic-seeded byte buffers through every decoder. Each result must serialize with allow_nan=False.
  • Golden fixtures (fixtures/mrc-cases.json): hex input to exact decode. This is the single source of truth the three MRC decoders (this library, the TypeScript twin, scigantic_empiar) are all held to, so none can silently diverge.
  • Non-finite floats (a garbage NIfTI pixdim, an inf MRC cell) sanitize to null.

Speed

The decode is microseconds: a 1 KiB read and a few struct unpacks. Optimizing that is a rounding error. All the speed is in I/O, and two things carry it. Both are measured, not asserted (run scigantic-headers-bench).

Read the header, not the file. The read is exactly HEADER_BYTES (1 KiB), so its cost is independent of file size and a multi-GB movie decodes as fast as a small one.

header read + decode (1 KiB):        15 us
full-file read + decode (200 MB):  22.7 ms      (about 1,500x cheaper)

Parallelize the I/O, bounded. Header reads across files are independent and I/O-bound, so a thread pool overlaps their latency (the read releases the GIL). Measured over 8 real EMPIAR headers pulled by HTTP Range:

serial   (1 worker):   25.7 s
parallel (8 workers):   0.7 s        (about 35x)

That 35x is large because EBI's per-request latency is about 3 s, so overlapping eight requests recovers a lot of dead wait. On low-latency local storage the speedup is smaller. The win scales with per-read latency, which is why the pool is bounded and tunable (default 8, the EMPIAR sweet spot; past a point more connections hit server throttling or disk-queue thrash and get slower).

Two more, by construction:

  • Filter before I/O. has_decoder_for is a cheap extension check. The batch and walk paths use it to skip a file before any syscall.
  • Zero deps, fast import. The dtype table is a plain dict, not numpy. There is nothing to install and nothing to import, and it runs air-gapped.

The biggest system-level lever lives in the caller, not here: decode once when a file lands, write the context record, and answer every later query from the tiny record without re-decoding. The edge context-producer and the cloud probe both do this.

Use

from scigantic_headers import decode_file, decode_paths, decode_urls, iter_decodable_files

decode_file("s/frame.mrc")                              # one local file
decode_paths(iter_decodable_files("/mnt/sessions"))     # a tree, parallel
decode_urls([...], workers=8)                           # remote, by Range

# CLI
scigantic-headers session/frame.mrc
scigantic-headers https://ftp.ebi.ac.uk/empiar/.../img.mrcs
scigantic-headers --dir /mnt/flashblade/sessions --workers 8

pytest
scigantic-headers-bench --empiar   # reproduce the numbers above

Limitations

  • Pointer-based formats are not supported. HDF5 and TIFF store their layout behind internal pointers, so reading the header or footer alone is not enough. Parquet (a footer) is supported; formats that need to chase offsets through the file are not. Plain gzip is handled (the reader inflates the leading block), but BAM's BGZF framing and per-record structure are not.
  • Output is not a standard. The fields are an ad-hoc dict, not an interchange format such as Allotrope ASM. Map the dict to a standard if you need one.

Repository

This is the standalone home of the library. It is also vendored into the Scigantic monorepo, where the paths above (backend/..., infrastructure/...) point at the TypeScript twin, the notebook, and the edge context-producer that use it.

Project details


Download files

Download the file for your platform. If you're not sure which to choose, learn more about installing packages.

Source Distribution

scigantic_headers-0.1.0.tar.gz (35.0 kB view details)

Uploaded Source

Built Distribution

If you're not sure about the file name format, learn more about wheel file names.

scigantic_headers-0.1.0-py3-none-any.whl (26.2 kB view details)

Uploaded Python 3

File details

Details for the file scigantic_headers-0.1.0.tar.gz.

File metadata

  • Download URL: scigantic_headers-0.1.0.tar.gz
  • Upload date:
  • Size: 35.0 kB
  • Tags: Source
  • Uploaded using Trusted Publishing? No
  • Uploaded via: twine/6.2.0 CPython/3.11.15

File hashes

Hashes for scigantic_headers-0.1.0.tar.gz
Algorithm Hash digest
SHA256 16254d31f85949fa2eb87c8acacd7dc76c1771d3d2038940bae4b63121a4fdbe
MD5 72bc56f1f210e0245626cde0a8075e14
BLAKE2b-256 e86eed531080ffb81fcd1c77669494138ea8ac541f327729615efabbe604cf5d

See more details on using hashes here.

File details

Details for the file scigantic_headers-0.1.0-py3-none-any.whl.

File metadata

File hashes

Hashes for scigantic_headers-0.1.0-py3-none-any.whl
Algorithm Hash digest
SHA256 faa55f95a06bc0cdd735b8dd482d3a2d7dc106d596e7199b55d3ce54d52256cf
MD5 f3b73cf3aa0d48e858f8040e4e5d9ce6
BLAKE2b-256 97051716cd688a50c91ba9cf258c1dc83eb17f7bfd0129063b22e633e6671360

See more details on using hashes here.

Supported by

AWS Cloud computing and Security Sponsor Datadog Monitoring Depot Continuous Integration Fastly CDN Google Download Analytics Pingdom Monitoring Sentry Error logging StatusPage Status page