EUV instrument response tools for the SunCAST Python ecosystem
Project description
pyEUVTools: EUV Instrument Response Tools
Overview
pyEUVTools is a SunCAST Python package for building, inspecting, and exporting EUV instrument response products.
The project is designed to become a reusable response-function layer for the
broader SunCAST Python ecosystem, including packages such as pyCHMP and
pyGXrender, while remaining usable as a standalone scientific library.
The first backend focus is SDO/AIA. The immediate goal is to provide a clean
Python interface to the time-dependent AIA instrument response machinery already
available through aiapy, and then build toward GX-compatible temperature
response tables on top of that foundation.
Project Status
pyEUVTools 0.1.0 is publicly released on PyPI and tagged on GitHub.
The next patch release, 0.1.1, is reserved for publication-metadata cleanup so the PyPI long description and Zenodo archival path match the live release state.
The concrete 0.1.0 release gate is documented in docs/dev_workflow.md.
In short, the first release must include a documented usable AIA API, validated
scientific behavior, at least one downstream-consumable output path, and tests
for the shipped public surface.
Current Scope
- AIA wavelength-response wrappers powered by
aiapy - raw AIA temperature-response folding equivalent to the numerical step in SSW
aia_bp_make_tresp.pro - optional
fiascobackend introspection and database bootstrap helpers for Python-native CHIANTI access - IDL fixture comparison helpers for assessing structural parity against GX-style AIA response SAV files
- canonical benchmark planning for raw IDL AIA temperature-response fixtures with full provenance
- response-table data models for future multi-instrument support
- a package layout intended to grow into a generalized EUV response toolkit
Planned Scope
- AIA temperature-response builder compatible with GX-style response tables
- export/import helpers for GX-compatible response structures
- support for additional instruments such as TRACE, EUVI, EUI, and SXT
Installation
Install the published package from PyPI:
python -m pip install pyeuvtools
For local development, use an editable install:
git clone https://github.com/suncast-org/pyEUVTools.git
cd pyEUVTools
python -m pip install -e .[dev]
For a runtime-only editable install:
git clone https://github.com/suncast-org/pyEUVTools.git
cd pyEUVTools
python -m pip install -e .
For the optional Python-native CHIANTI prototype backend:
python -m pip install -e .[chianti]
The fiasco/CHIANTI path is currently a provisional backend rather than the
default production route. Installing the optional chianti extra is therefore
not required for normal package use.
Contributor Artifact Policy
This repository may ship committed reference artifacts for documentation, benchmark parity, and reviewable contributor refreshes, but ordinary user runs should not write into the clone by default.
- User-generated benchmark outputs and hybrid exports default to user-local locations under
~/.pyeuvtools/or a system temp directory fallback whenHOMEis unavailable. - Repo-local writes are intentional contributor actions and should use explicit paths such as
--artifact-dir benchmark-results/...or IDLoutdir='benchmark-data/...'. - The currently shipped runtime AIA V9 exports live under
src/pyeuvtools/data/aia/. - The currently committed benchmark/provenance copy of the AIA V9 hybrid export remains at
benchmark-data/aia/genx-exports/aia_V9/aia_hybrid_genx_export_v1.sav.
For a backend-local note describing what this prototype already covers, what was
validated, and why active development paused in favor of the hybrid
genx-derived approach, see src/pyeuvtools/response/README.md.
Default test runs also exclude the provisional CHIANTI backend tests. To run them explicitly:
python -m pytest -m chianti_backend
Quick Example
from astropy.time import Time
from pyeuvtools.response.aia import build_aia_wavelength_response
response = build_aia_wavelength_response(171, Time("2020-11-26T19:58:31"))
table = response.to_table()
print(response.channel)
print(response.response.unit)
print(table.colnames)
Documentation
Project documentation lives in the docs/ directory and is intended to be published with GitHub Pages.
- Project overview
- Installation
- Usage
- Development workflow
- API notes
- Dependency plan
- Benchmark specification
- Hybrid backend design
Versioning and Releases
- Package versioning is managed with
bumpver - PyPI publishing remains disabled locally until the final release approval is given
- Zenodo metadata is tracked in
.zenodo.jsonand intended to mint a DOI for releases - Release-facing API changes are summarized in
CHANGELOG.md
For this repository, Zenodo and PyPI are intentionally decoupled:
- a GitHub release under
suncast-org/pyEUVToolsis the event intended for Zenodo archival - PyPI publishing is a separate manual GitHub Actions workflow and is not triggered automatically by a tag or GitHub release
- the current Zenodo metadata credits Gelu M. Nita as the named software creator while explicitly acknowledging maintenance in the
suncast-orgGitHub organization
Status
This repository now ships a usable compact AIA response API and the public GX
bridge helper needed for downstream ComputeEUV packing. In particular, the
Python aia_get_response wrapper covers compact effective_area,
emissivity, and temperature responses with explicit non-interactive
correction states: raw, evenorm, and evenorm_chiantifix.
The local metadata now targets 0.1.0, but the release is still intentionally
held pending explicit approval. Remaining broader SSW surface coverage such as
full, all, and uv stays documented as later-milestone work rather than as
part of the compact 0.1.0 promise.
Project details
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