rxn-location 0.2.0

Statistical comparison between X-line location predicted by various models for dayside terrestrial magnetopause

Reconnection line location (rxn_location)

Introduction

rxn_location is a Python package for predicting and analyzing the X-line location at the dayside terrestrial magnetopause. It provides tools to analyze individual reconnection jets via an interactive GUI, as well as CLI tools for automated, large-scale statistical batch processing.

The package predicts the X-line location based on four primary models:

1. Maximum Shear Model

2. Maximum Reconnection Energy

3. Maximum Exhaust Velocity

4. Maximum Bisection Field

The MMS data used by this software is automatically fetched from the MMS mission, and OMNI solar wind data is fetched from OMNIWeb.

The repository is archived using Zenodo with the following DOI:

Documentation

Full documentation, including API reference, CLI usage guides, and theoretical background, is available at: rxn_location

Description

This package originally started as the repository for generating the figures in the paper "Statistical comparison of various dayside magnetopause reconnection X-line prediction models" (by Ramiz A. Qudsi, Brian Walsh, Jeff Broll, Emil Atz, Stein Haaland). It has since evolved into a software tool suite for both individual jet event analysis and aggregated statistical modeling.

Code

The code is written for Python 3.11 or later. All dependencies are managed automatically via pyproject.toml and will be installed when you install the package.

Key scientific and visualization libraries used by rxn_location include:

• spacepy & pyspedas (for MMS and OMNI data retrieval and physics algorithms)
• streamlit (for the interactive graphical interface)
• plotly, seaborn, & matplotlib (for interactive 3D and statistical visualizations)
• scikit-image (for ridge-finding models)
• joblib (for parallelized batch processing)

Installation & Setup

Since the code has many dependencies (including SpacePy and PySPEDAS, which can sometimes be tricky to install), we highly recommend using a virtual environment. You can install the package directly from PyPI (recommended), from GitHub, or by cloning the repository to install it locally.

Option 1: Install from PyPI (Recommended)

The easiest way to get started and use the rxn-location-gui and rxn-batch tools is to install the latest stable release directly from PyPI into a virtual environment:

python3 -m venv venv
source venv/bin/activate  # On Windows: venv\Scripts\activate
pip install rxn-location

Option 2: Install Directly from GitHub

If you want the absolute latest development version without modifying the source code, you can install directly from the GitHub repository:

pip install git+https://github.com/qudsiramiz/rxn_location.git

Option 3: Clone and Install Locally (Standard Python)

If you want to explore the source code, run examples, or contribute, you should clone the repository first:

git clone https://github.com/qudsiramiz/rxn_location.git
cd rxn_location

# Create and activate a virtual environment
python3 -m venv venv
source venv/bin/activate  # On Windows: venv\Scripts\activate

# Install the package in editable mode
pip install -e .

Option 4: Clone and Install Locally (Poetry)

If you prefer using Poetry for dependency management:

git clone https://github.com/qudsiramiz/rxn_location.git
cd rxn_location

# Install Poetry (if you don't have it)
pip install poetry

# Install dependencies and start the environment
poetry install
poetry shell

Interactive GUI

The easiest way to use rxn_location is via the interactive Streamlit graphical user interface. This interface allows you to run Jet Reversal checks, visualize 3D reconnection models, run automated statistical batch modes, and generate statistical plots dynamically.

Recent GUI Features include:

• Master Jet List: Persistent JSON storage of detected jets with automatic 2-minute deduplication across sessions. Now automatically fetches and saves contextual Solar Wind parameters (B_IMF, V_IMF, Np, Tp, Sym-H, Clock Angle, P_dyn).
• Interactive Data Table: View, sort, manually prune, and export (CSV/JSON/Pickle) your master jet list. Features high-quality Unicode formatting for variables.
• Duplicate Jet Dialog: Safety checks when generating models to prevent processing the same jet multiple times.
• Parameter Presets: Save and load your favorite sidebar configurations.
• Data Cache Dashboard: Monitor and clean up the local PySPEDAS data cache directly from the sidebar.
• Dynamic Plot Filtering: Filter statistics by IMF Bz, dynamic pressure, and shear angle before plotting.
• Quick Re-run & Auto-Run: Instantly load parameters from a previously saved jet into the dashboard ("Load into Dashboard"), or use the new "Load & Run Models" button to auto-execute the entire pipeline in one click.
• Batch Processing from File Upload: In addition to time-range and target-count batch processing, "Statistics Mode" now accepts uploaded .csv or .txt files containing custom lists of timestamps. It leverages robust parsing to seamlessly run the jet reversal check and models on every timestamp provided.

To launch the GUI, run the following command from the root directory:

rxn-location-gui

In order to check for jet locations and process statistics from the command line, we recommend using the new automated batch script:

1. Prepare your input file: Create a .txt or .csv file (e.g. times_list.txt) containing the timestamps you want to check, one per line.

   2015-09-02 16:45:00
   2015-09-02 17:30:00
   2015-10-16 13:07:00
   

2. Run the script: Run rxn-batch and pass your input file.

   rxn-batch --input times_list.txt --probe 3 --format html --outdir ./my_batch_figures
   

Available Options:

• -i, --input: (Required) Path to your .txt or .csv list of times.
• --probe: MMS probe number (1-4). Defaults to 3.
• --tsy_model: Tsyganenko model to use. Defaults to T96.
• --data_rate: MMS data rate (fast or brst). Defaults to fast.
• --format: Format for the saved plots (html for interactive Plotly, or pdf/png for static Matplotlib). Defaults to html.
• --outdir: Directory to save the generated plots and CSV. Defaults to ./figures.
• --verbosity: Set the terminal output verbosity (0 to 3). Defaults to 2.

When run, the script will output its default configurations, process each time, fetch Solar Wind parameters, generate the required plots, and intelligently skip logging duplicate jets to your persistent ~/.rxn_location_master_jets.json file.

For more examples and advanced usage (including configuration files), see the CLI Usage Guide.

NOTE: Sometimes, the MMS data is not downloaded properly by PySPEDAS. In that case, please check your internet connection or use the GUI's Data Cache Dashboard to manage corrupted files.

Data

All the data used to generate the figures in the paper are available in the data/study_data directory.

Contact

If you have any questions, please contact Ramiz A. Qudsi at [e-mail]