magnetosphericswcx
Code used to produce the results in a publication on separating out the magnetospheric SWCX X-ray spectral contribution in astrophysical observations of dark fields.
Science Score: 67.0%
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✓codemeta.json file
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✓.zenodo.json file
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✓DOI references
Found 4 DOI reference(s) in README -
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○Scientific vocabulary similarity
Low similarity (7.5%) to scientific vocabulary
Repository
Code used to produce the results in a publication on separating out the magnetospheric SWCX X-ray spectral contribution in astrophysical observations of dark fields.
Basic Info
- Host: GitHub
- Owner: rebeccaringuette
- License: mit
- Language: Python
- Default Branch: main
- Size: 1.29 MB
Statistics
- Stars: 0
- Watchers: 1
- Forks: 0
- Open Issues: 0
- Releases: 2
Metadata Files
README.md
MagnetosphericSWCX
This repository contains the code used to produce the results in a publication separating out the magnetospheric SWCX X-ray spectral contribution in astrophysical observations of dark fields. The final codes used to produce the publication results are in the PaperAnalysisCode directory, while most of the code iterations along the way are included in the OlderVersions directory. These codes include PyXSPEC code (.py files), XSPEC scripts (.xcm files) and other input files (e.g. the predicted heliospheric SWCX line intensities and the arf/rmfs used). All python code was written in python 2.7.15, and all XSPEC code was written using XSPEC 12.11.1. A few example input files are included in the ExampleData directory, and the spreadsheets produced by the scripts are included in the Results directory. Please see the associated publication for official results. If you have questions or would like to collaborate, please feel free to create an issue to get my attention.
For historical purposes, the codes used to perform the analysis of the heliospheric SWCX published in Ringuette et al. (2021) are also included in the 'HSWCXPaperCode' and 'HSWCXOlderCode' directories, which have similar code types. The 2021 publication is accessible at https://doi.org/10.3847/1538-4357/ac0e33.
Please cite this repository as:
Ringuette, R. (2023). Magnetospheric SWCX. Zenodo. https://www.doi.org/10.5281/zenodo.8252998
Owner
- Login: rebeccaringuette
- Kind: user
- Company: Community Coordinated Modeling Center / ADNET Systems Inc
- Website: https://orcid.org/0000-0003-0875-2023
- Repositories: 2
- Profile: https://github.com/rebeccaringuette
Citation (Citation.cff)
abstract: <p>Code used to produce the results in a publication on separating out the magnetospheric SWCX X-ray spectral contribution in astrophysical observations of dark fields.</p> authors: - affiliation: Heliophysics Digital Resource Library / ADNET Systems Inc family-names: Ringuette given-names: Rebecca orcid: 0000-0003-0875-2023 cff-version: 1.2.0 date-released: '2023-08-16' doi: 10.5281/zenodo.8253002 keywords: - Heliophysics - Solar Wind - Charge Exchange - Heliosphere - Magnetosphere - csv - analysis license: - apache-2.0 repository-code: https://github.com/rebeccaringuette/MagnetosphericSWCX/tree/MSWCX title: 'rebeccaringuette/MagnetosphericSWCX: PublicationCode_v1.0' type: software version: MSWCX