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| Format: | Recurso digital |
| Langue: | anglais |
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Zenodo
2025
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| Accès en ligne: | https://doi.org/10.5281/zenodo.15081593 |
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| _version_ | 1866902154076225536 |
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| author | DAKEYO, Jean-Baptiste |
| author_facet | DAKEYO, Jean-Baptiste |
| contents | <p>BipolySolarWind is a set of Python codes modeling Parker's like solar wind solutions (bipoly solutions), including expansion factor effects.</p> <p>There are three main files : <code>function_to_run_bipoly_dakeyo2025a</code>, <code>bipoly_solar_wind_solve_and_plot</code> and <code>main_bipoly_dakeyo2025a</code>. All the files must be stored in the same respository for the execution. The former contains the functions to solve the equations themselves, the second file runs the solver and plots the solution, and the latter is the main code for the user, which takes the inputs of the model, runs the first two files to display the solutions, and provides the output bipoly parameters. Examples of the use of the main code <code>main_bipoly_dakeyo2025a</code> are provided in the Jupyter Notebook <code>BipolyNotebookExample.ipynb</code>. Another code <code>stream_calc_dakeyo2024a</code> allows to trace the Parker's like spiral (streamline) associated with the computed solution.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_15081593 |
| institution | Zenodo |
| language | eng |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | BipolySolarWind DAKEYO, Jean-Baptiste Solar wind Modeling <p>BipolySolarWind is a set of Python codes modeling Parker's like solar wind solutions (bipoly solutions), including expansion factor effects.</p> <p>There are three main files : <code>function_to_run_bipoly_dakeyo2025a</code>, <code>bipoly_solar_wind_solve_and_plot</code> and <code>main_bipoly_dakeyo2025a</code>. All the files must be stored in the same respository for the execution. The former contains the functions to solve the equations themselves, the second file runs the solver and plots the solution, and the latter is the main code for the user, which takes the inputs of the model, runs the first two files to display the solutions, and provides the output bipoly parameters. Examples of the use of the main code <code>main_bipoly_dakeyo2025a</code> are provided in the Jupyter Notebook <code>BipolyNotebookExample.ipynb</code>. Another code <code>stream_calc_dakeyo2024a</code> allows to trace the Parker's like spiral (streamline) associated with the computed solution.</p> |
| title | BipolySolarWind |
| topic | Solar wind Modeling |
| url | https://doi.org/10.5281/zenodo.15081593 |