pyAMPP is a Python implementation of the Automatic Model Production Pipeline (AMPP) for solar coronal modeling. It streamlines the process of generating realistic 3D solar atmosphere models with minimal user input.
Full documentation is available at: https://pyampp.readthedocs.io/en/latest/
Format and viewer references:
- Upgraded HDF5 stage format (NONE/BND/POT/NAS/NAS.GEN/NAS.CHR):
docs/model_hdf5_format.rst - GUI workflow and command mapping:
docs/gui_workflow.rst - Viewer guide (
gxbox-viewandgxrefmap-view):docs/viewers.rst - Release notes:
CHANGELOG.rst
AMPP automates the production of 3D solar models by:
- Downloading vector magnetic field data from the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO)
- Optionally downloading contextual Atmospheric Imaging Assembly (AIA) data
- Performing magnetic field extrapolations (Potential and/or Nonlinear Force-Free Field)
- Generating synthetic plasma emission models assuming either steady-state or impulsive heating
- Producing non-LTE chromospheric models constrained by photospheric measurements
- Enabling interactive 3D inspection and customization through user-friendly GUIs
pyAMPP can be installed directly from PyPI.
- Setting up a Python 3.10 Environment (Recommended)
We strongly recommend running pyAMPP in a dedicated Python 3.10 environment. You may use any of the following tools to install Python and create an isolated environment:
- Miniforge: https://github.com/conda-forge/miniforge
- Miniconda: https://www.anaconda.com/docs/getting-started/miniconda/install
- Anaconda: https://www.anaconda.com/docs/getting-started/anaconda/install
- Conda: https://docs.conda.io/projects/conda/en/latest/user-guide/install/index.html
- pyenv: https://github.com/pyenv/pyenv?tab=readme-ov-file#installation
Please refer to the official installation instructions for your chosen tool. Their documentation is comprehensive and up to date, so we will not repeat it here.
You can skip this environment setup section if you already have a suitable Python environment.
The instructions below use Conda as an example:
Install Conda If you don’t have Conda yet, follow the instructions for your platform here: https://docs.conda.io/projects/conda/en/latest/user-guide/install/index.html
Create and activate your environment Open an Anaconda Prompt or Command Prompt and run:
conda create -n suncast python=3.10 conda activate suncast
Upgrade pip and install pyampp
pip install -U pip setuptools wheel pip install -U pyampp
(Optional) Install additional dependencies
For a full scientific Python stack (e.g., SunPy and related tools):
pip install -U sunpy[all]
pyAMPP provides a GUI for building a reproducible CLI command and separate tools for model generation and visualization:
- pyampp – Launches a GUI to select observation time, coordinates, and options. It generates a gx-fov2box CLI command (shown above the Run button) and can launch it.
- gx-fov2box – Pure CLI model generator (IDL gx_fov2box equivalent). It saves the requested stages and records the full command in metadata/execute.
- gxbox – Launches the map GUI and 3D visualization for browsing existing models.
1. Launch the time/coord selector (pyampp)
pyampp2. Generate a model via CLI (gx-fov2box)
gx-fov2box \
--time "2022-03-30T17:22:37" \
--coords 34.44988566346035 14.26110705696788 \
--hgs \
--box-dims 360 180 200 \
--dx-km 1400 \
--pad-frac 0.25 \
--data-dir /path/to/download_dir \
--gxmodel-dir /path/to/gx_models_dir \
--save-potential \
--save-bounds3. Launch the modeling GUI directly (Gxbox Map Viewer)
gxbox \
--time "2022-03-30T17:22:37" \
--coords 34.44988566346035 14.26110705696788 \
--hgs \
--box-dims 360 180 200 \
--box-res 0.729 \
--pad-frac 0.25 \
--data-dir /path/to/download_dir \
--gxmodel-dir /path/to/gx_models_dir \
--external-box /path/to/boxfile.gxboxThe Gxbox Map Viewer GUI automatically downloads the required solar data and builds the 3D model based on the user's input. The resulting model can be visualized in a VTK-based viewer (Gxbox 3D Viewer) that supports interactive exploration of the magnetic field structure.
Additionally, users can trace and extract magnetic field lines within the 3D model and send them back to the gxbox GUI, where they can be overlaid on solar images for contextual visualization.
Notes:
- --coords takes two floats, separated by space (no brackets or commas).
- One of --hpc, --hgc, or --hgs must be specified to define the coordinate system.
- Remaining parameters are optional and have default values.
- Set
PYAMPP_JSOC_NOTIFY_EMAILto override the JSOC export notification email (default:suncasa-group@njit.edu).
gx-fov2box supports --entry-box with .h5 or .sav input for stage-aware resume/recompute.
--rebuild: ignore stage payload and recompute fromNONEusing resolved entry parameters.--clone-only: convert/copy an entry box to normalized HDF5 without recomputation (useful asconvert-from-sav).- Without
--jump2*, the pipeline starts from the detected entry stage. - When
--entry-boxcontainsmetadata/execute,--data-dirand--gxmodel-dirdefault from that execute string. - Explicit CLI values for
--data-dir/--gxmodel-diralways override execute-derived defaults. - Jump validation rules are enforced:
- backward jumps are allowed,
- forward jumps are allowed by one stage,
-
POT -> NASis explicitly allowed (implicitPOT -> BND -> NAS), -POT -> GENis explicitly allowed (skip bothBNDandNAS/NLFFF; keep true POT vectors). - Save requests for stages before the selected start stage are ignored with a warning.
- In
--clone-onlymode, only no-jump or jump-to-self is allowed.
After installation, the following commands become available:
pyampp: Launch the command-builder GUI.gx-fov2box: Run the model-generation pipeline headlessly.gxbox: Launch the modeling/visualization GUI.gxbox-view: Open an existing HDF5 model in the 3D viewer.gxrefmap-view: Open base/refmaps from an HDF5 model in a 2D map browser.gx-idl2fov2box: Translate IDLgx_fov2boxexecute strings (or SAVEXECUTE) into Pythongx-fov2boxcommands.
Copyright (c) 2024, SUNCAST team. Released under the 3-clause BSD license.


