Skip to main content
Pre-release

This release is a pre-release and may not be stable for production use.

PYSTILT

Tests Documentation Code Quality codecov PyPI version Python Version License: MIT DOI Ruff Pyright

PYSTILT is a Python implementation of the STILT Lagrangian atmospheric transport model. It runs backward trajectories with HYSPLIT and computes receptor footprints that map where upwind surface fluxes influence a measurement.

The project is in alpha and focused on a unified execution model that works for one-off runs, large batch runs, and streaming queue workers.

Status

PYSTILT is in alpha development. No backward compatibility guarantees before v1.0.

The core transport is stable: HYSPLIT execution, trajectory and footprint generation, numerical STILT-R parity, and the local and SLURM execution paths are all exercised by the test suite. The public API may change while the package settles.

Choose a workflow

  • One-off transport runs for local analysis and notebooks: use Model.run() or stilt run.
  • Queue-backed batch or service runs for cloud execution: use Model.register(), stilt register, stilt pull-worker, and stilt serve with a PostgreSQL work queue configured via PYSTILT_DB_URL. Slurm needs no database: stilt run --backend slurm.
  • Column and satellite workflows for science-facing code: use stilt.observations to group, select, and lay out soundings as Receptor objects, and a per-receptor averaging-kernel table to weight them inside the same runtime.

Roadmap

PYSTILT draws design and science inspiration from two sister projects: X-STILT for column and satellite science workflows, and stiltctl for cloud-native execution patterns. The tables below track what has been absorbed and what remains in scope. See the full roadmap for more details.

Execution and orchestration (from stiltctl)

Feature Status
Pull-mode queue workers (stilt pull-worker) Implemented
Long-lived streaming mode (stilt serve) Implemented
PostgreSQL-backed work queue for distributed coordination Implemented
Thin CLI → Model → worker call path Implemented
Kubernetes worker deployment Partial
Cloud object store outputs (GCS, S3) In scope

Column and satellite science (from X-STILT)

Full X-STILT feature parity is not a goal. PYSTILT absorbs X-STILT's observation-layer design and column-weighting concepts without trying to replicate every script.

Feature Status
stilt.observations helpers (overpass grouping, sounding selection, jitter, slant geometry) Implemented
Column receptor support Implemented
Averaging-kernel and pressure-weighting particle transforms Implemented
First-order lifetime decay transform Implemented
Declarative per-footprint transforms in config Implemented
Slant-column receptor support Implemented
User-defined transforms (kind: my.module.Class) Implemented
Per-sounding averaging kernels in batch runs (averaging_kernel with table:) Implemented
Product readers (OCO-2/3, TROPOMI, TCCON) Out of scope: your reader produces a table of soundings
Transport error on the modelled enhancement (transport_error) Implemented
Modelled enhancement from a flux field (Footprint.enhancement) Implemented
Inventory coupling and background estimation Deferred

Installation

pip install pystilt

For Slurm, Kubernetes, projections, plotting, and cloud object stores:

pip install "pystilt[complete]"

Quickstart: one-off run

Define a receptor, configure meteorology and footprint grid, then run:

import pandas as pd
import stilt

receptor = stilt.Receptor(
    time=pd.Timestamp("2023-07-15 18:00", tz="UTC"),
    latitude=40.766,
    longitude=-111.848,
    altitude=10,
)

model = stilt.Model(
    project="./my_project",
    receptors=[receptor],
    config=stilt.ModelConfig(
        n_hours=-24,
        numpar=100,
        mets={
            "hrrr": stilt.MetConfig(
                directory="/data/hrrr",
                file_format="hrrr_%Y%m%d.arl",
                file_tres="1h",
            )
        },
        footprints={
            "default": stilt.FootprintConfig(
                grid=stilt.Grid(
                    xmin=-113.0,
                    xmax=-110.5,
                    ymin=40.0,
                    ymax=42.0,
                    xres=0.01,
                    yres=0.01,
                )
            )
        },
    ),
)

handle = model.run()
handle.wait()

sim = list(model.simulations.values())[0]
traj = sim.trajectories
foot = sim.get_footprint("default")

Quickstart: queue/service runtime

# Queue workers require a PostgreSQL work queue.
export PYSTILT_DB_URL=postgresql://user:pass@host:5432/pystilt

# Initialize project files (config.yaml and receptors.csv)
stilt init ./my_project

# Run with local workers (blocks until complete)
stilt run ./my_project --backend local --n-workers 8

# Persist inputs and enqueue every simulation (receptors x mets)
stilt register ./my_project

# Drain queue from worker processes (batch mode)
stilt pull-worker ./my_project

# Long-lived queue workers (streaming mode)
stilt serve ./my_project

# Check project status
stilt status ./my_project

The same queue model is available in Python:

import stilt
from stilt.execution import pull_simulations

model = stilt.Model(project="./my_project")
model.register()
pull_simulations(model, follow=False)  # batch mode
print(model.status())

Workers claim simulations from the queue and record done/failed there; whether outputs exist is always read from the project itself.

Quickstart: column and satellite soundings

Your reader produces a table with one row per sounding. stilt.observations groups and selects rows, each row becomes a Receptor, and each sounding's averaging kernel goes into a table in the project so every runner applies the right kernel to the right receptor:

import stilt
from stilt.observations import group_by_overpass
from stilt.transforms import averaging_kernel_table

df = read_my_product(path)                       # your reader: time, longitude, latitude, ak_pressure, ak, ...
df["overpass"] = group_by_overpass(df["time"])   # label rows by overpass; thin with pandas or select_observations_spatial

model = stilt.Model(project="./my_project")      # existing project config on disk
receptors = [stilt.ColumnReceptor(r.time, r.longitude, r.latitude, 0, 3000) for r in df.itertuples()]
model.register(receptors=receptors)

averaging_kernel_table(receptors, levels=df.ak_pressure, values=df.ak).to_parquet(
    model.project.directory / "kernels.parquet"
)
model.run()

with the footprint declared once in config.yaml:

footprints:
  column:
    grid: slv
    transforms:
      - kind: averaging_kernel
        table: kernels.parquet
        coordinate: pres
      - kind: pressure_weighting

Slant paths come from slant_points and Receptor.from_points. See the observations guide and the slant columns guide.

Particle transforms

Per-footprint transforms rescale each particle's influence before the footprint is rasterized. Declare them in config, or pass them in Python:

footprints:
  column:
    grid: slv
    transforms:
      - kind: averaging_kernel
        levels: [0.0, 1000.0, 2000.0]
        values: [1.0, 0.8, 0.5]
      - kind: pressure_weighting      # derived from the particles, X-STILT style
      - kind: first_order_lifetime
        lifetime_hours: 4.0
      - kind: mypkg.transforms.MyWeighting   # your own pydantic class with apply()
        some_field: 3

A transform is any object with apply(particles, context). See the transforms guide for the column-weighting science and for writing your own.

Accessing results

import pandas as pd

for sim in model.simulations.values():
    traj = sim.trajectories
    foot = sim.get_footprint("default")

# Load footprints across all matching simulations
footprints = model.footprints["default"].load(
    time_range=("2023-01-01", "2023-01-31")
)

coords = [(-111.9, 40.7), (-111.8, 40.8)]
time_bins = pd.interval_range(
    start=pd.Timestamp("2023-01-01 00:00", tz="UTC"),
    end=pd.Timestamp("2023-01-02 00:00", tz="UTC"),
    freq="1h",
)

for footprint in footprints:
    hourly = footprint.aggregate(target=coords, time_bins=time_bins)

If a footprint is tracked as complete-empty, no NetCDF file is expected for that footprint. The model APIs treat it as a successful terminal outcome while skipping missing file loads.

STILT-R parity

PYSTILT footprints match the uataq/stilt R implementation on numerical values at rtol=1e-7 per cell, validated by end-to-end fidelity scenarios against a pinned upstream commit. NetCDF output is not byte-compatible with STILT-R; it should be read as generic CF-1.8 NetCDF. See STILT-R.md for more details.

Documentation

Full documentation is available at https://jmineau.github.io/PYSTILT/

Contributing

Contributions are welcome! Please see CONTRIBUTING.md for guidelines.

License

This project is licensed under the MIT License - see the LICENSE file for details.

Author

James Mineau - jmineau

Release files for pystilt 0.1.0a16

For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.

Source distribution (sdist)

Source distribution for pystilt 0.1.0a16
File Size Uploaded
pystilt-0.1.0a16.tar.gz 1.9 MB Details

Built distribution (wheel)

Table of built distributions (wheels) for pystilt 0.1.0a16
File Interpreter ABI Platform
pystilt-0.1.0a16-py3-none-any.whl Python 3 none any Details

Total release size: 3.7 MB

Release files / pystilt-0.1.0a16.tar.gz

Download URL pystilt-0.1.0a16.tar.gz
Size 1.9 MB
Tags Source
SHA-256 checksum
How to use checksums
461107d0dda7e9f7e578c054c1ea493bc1e5451e5907b948b173b88fec5dfaf4
BLAKE2b-256 checksum
How to use checksums
d9770f508081ea35e866b171ae8c74e243d8662fd6f843f97cbb2e0b651e27a9
Upload date
Uploaded using Trusted Publishing?
What is trusted publishing?
Yes
Uploaded via twine/7.0.0 CPython/3.13.14

Provenance

Provenance describes where a file came from. On PyPI, provenance is shared via attestations, which provide a verifiable record of the build or publishing details. View details, limitations and caveats.

PyPI Publish Attestation

PyPI verified that this artifact, at this checksum, originated from the publisher listed below.

Signed by GitHub Actions, verified by PyPI on Sep 22, 2026.

Transparency log

Release files / pystilt-0.1.0a16-py3-none-any.whl

Download URL pystilt-0.1.0a16-py3-none-any.whl
Size 1.8 MB
Tags Python 3
SHA-256 checksum
How to use checksums
e42c289897f3b5433893be4588493e1f1866ad0d3fc830c01394bf257551a01a
BLAKE2b-256 checksum
How to use checksums
df270968b6b3afce335e2f433ae7c9213a434bec436a50a2fb47070577ad5a76
Upload date
Uploaded using Trusted Publishing?
What is trusted publishing?
Yes
Uploaded via twine/7.0.0 CPython/3.13.14

Provenance

Provenance describes where a file came from. On PyPI, provenance is shared via attestations, which provide a verifiable record of the build or publishing details. View details, limitations and caveats.

PyPI Publish Attestation

PyPI verified that this artifact, at this checksum, originated from the publisher listed below.

Signed by GitHub Actions, verified by PyPI on Sep 22, 2026.

Transparency log
Anthropic, PBC Visionary sponsor Bloomberg Visionary sponsor Hudson River Trading Visionary sponsor Meta Visionary sponsor NVIDIA Visionary sponsor Microsoft Sustainability sponsor Depot Continuous Integration AWS Cloud computing and Security Sponsor Datadog Monitoring Fastly CDN Google Download Analytics Sentry Error logging StatusPage Status page