sir-analysis-tools
This repository contains a series of analysis tools for studying the bulk and turbulent properties of stream interaction regions in solar wind data at 1 au, as well as implications for galactic cosmic ray transport, using a superposed epoch approach.
Science Score: 67.0%
This score indicates how likely this project is to be science-related based on various indicators:
-
✓CITATION.cff file
Found CITATION.cff file -
✓codemeta.json file
Found codemeta.json file -
✓.zenodo.json file
Found .zenodo.json file -
✓DOI references
Found 3 DOI reference(s) in README -
✓Academic publication links
Links to: zenodo.org -
○Academic email domains
-
○Institutional organization owner
-
○JOSS paper metadata
-
○Scientific vocabulary similarity
Low similarity (7.5%) to scientific vocabulary
Repository
This repository contains a series of analysis tools for studying the bulk and turbulent properties of stream interaction regions in solar wind data at 1 au, as well as implications for galactic cosmic ray transport, using a superposed epoch approach.
Basic Info
- Host: GitHub
- Owner: jgaloguz
- License: apache-2.0
- Language: Python
- Default Branch: main
- Size: 170 KB
Statistics
- Stars: 0
- Watchers: 1
- Forks: 0
- Open Issues: 0
- Releases: 2
Metadata Files
README.md
This repository contains a series of analysis tools for studying the bulk and turbulent properties of stream interaction regions in solar wind and magnetic field data at 1 au, as well as implications for galactic cosmic ray transport, using a superposed epoch approach.
These codes were used to analyze data from the Advanced Composition Explorer (ACE) spacecraft, freely available at https://izw1.caltech.edu/ACE/ASC/level2/index.html and https://izw1.caltech.edu/ACE/ASC/DATA/level3/index.html, for a JGR: Space Physics publication (Alonso Guzman at al. 2025). Specifically, the data analyzed was 64s Level 2 (Verified) data from the Magnetic Field Experiment (MAG) and the Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM) instruments, and 1-hour Level 3 (Contributed) data from the Cosmic Ray Isotope Spectrometer (CRIS). The code ran without errors using Python 3.13.1 on linux and equipped with the following additional modules: matplotlib 3.10.0, numpy 2.2.1, and scipy 1.15.1.
See the README.md files within each folder and comments within each program for more information.
Owner
- Name: Juan G Alonso Guzman
- Login: jgaloguz
- Kind: user
- Repositories: 1
- Profile: https://github.com/jgaloguz
Citation (CITATION.cff)
abstract: "This software contains a series of analysis tools for studying the bulk and turbulent properties of stream interaction regions in solar wind and magnetic field data at 1 au, as well as implications for galactic cosmic ray transport, using a superposed epoch approach."
authors:
- family-names: Alonso Guzman
given-names: Juan Gabriel
orcid: "https://orcid.org/0000-0001-9581-3167"
cff-version: 1.2.0
date-released: "2025-01-17"
identifiers:
- description: "Archived snapshot of version 1.0.1 of SIR Analysis Tools"
type: doi
value: 10.5281/zenodo.14867883
keywords:
- "stream interaction regions"
- "solar wind"
- "turbulence"
- "galactic cosmic rays"
- "spacecraft data analysis"
- "superposed epoch analysis"
license: Apache-2.0
message: "If you use this software, please cite it using these metadata."
repository-code: "https://github.com/jgaloguz/SIR-analysis-tools"
title: "SIR Analysis Tools"
version: 1.0.1
GitHub Events
Total
- Release event: 2
- Push event: 18
- Create event: 4
Last Year
- Release event: 2
- Push event: 18
- Create event: 4