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Zenodo
2025
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| Online Access: | https://doi.org/10.5281/zenodo.15397720 |
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| _version_ | 1866901877300396032 |
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| author | Le Saux, Arthur Leclerc, Armand |
| author_facet | Le Saux, Arthur Leclerc, Armand |
| contents | <p dir="auto">This repository holds the data and scripts used to support the article written by A. Le Saux, A. Leclerc, G. Laibe, P. Delplace, A. Venaille.</p> <p dir="auto">profile_1D_sun_r15140_Z0p02.data.FGONG is the 1D model of the interior of the Sun used in this study.</p> <p dir="auto">solar_linear_modes.ipynb is a Jupyter notebook which computes the linear modes using Dedalus (v2).</p> <p dir="auto">rotation_kernels.ipynb is a Jupyter notebook which computes the rotation kernel and the frequency splitting of the solar mixed mode. The linear modes are already computed and loaded from the file mixedMode_acousticMode_forKernels.npy.</p> <p dir="auto">The output of the MUSIC hydrodynamical simulation used to support this article is available in release v1.0.0 of this repository. A Python script named plot_PS_MUSIC.py is provided to open and read these outputs (power spectra). They show the displacements of the f-modes, which are compared to the ones calculated by the linear theory and read from fmodes_simu_0.15-0.9_ells_4-13_r15140_Z0p02.npy.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_15397720 |
| institution | Zenodo |
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| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Scripts and data for Solar f modes Le Saux, Arthur Leclerc, Armand <p dir="auto">This repository holds the data and scripts used to support the article written by A. Le Saux, A. Leclerc, G. Laibe, P. Delplace, A. Venaille.</p> <p dir="auto">profile_1D_sun_r15140_Z0p02.data.FGONG is the 1D model of the interior of the Sun used in this study.</p> <p dir="auto">solar_linear_modes.ipynb is a Jupyter notebook which computes the linear modes using Dedalus (v2).</p> <p dir="auto">rotation_kernels.ipynb is a Jupyter notebook which computes the rotation kernel and the frequency splitting of the solar mixed mode. The linear modes are already computed and loaded from the file mixedMode_acousticMode_forKernels.npy.</p> <p dir="auto">The output of the MUSIC hydrodynamical simulation used to support this article is available in release v1.0.0 of this repository. A Python script named plot_PS_MUSIC.py is provided to open and read these outputs (power spectra). They show the displacements of the f-modes, which are compared to the ones calculated by the linear theory and read from fmodes_simu_0.15-0.9_ells_4-13_r15140_Z0p02.npy.</p> |
| title | Scripts and data for Solar f modes |
| url | https://doi.org/10.5281/zenodo.15397720 |