File:3D view of the magnetised stellar wind of GJ 436.tif
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Size of this JPG preview of this TIF file: 800 × 356 pixels. Other resolutions: 320 × 142 pixels | 640 × 284 pixels | 1,024 × 455 pixels | 1,280 × 569 pixels | 3,301 × 1,467 pixels.
Original file (3,301 × 1,467 pixels, file size: 1.95 MB, MIME type: image/tiff)
Captions
Captions
3D view of the magnetised stellar wind for GJ 436 for Models I and II. The contour shows the wind velocity, and the Alfvén surface is shown by the translucent outer surface.
Summary
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English: 3D view of the magnetised stellar wind for Models I and II. The surface magnetic field from March-June 2016 reconstructed by Bellotti et al. (2023) is used at the boundary of the models. The grey streamlines are the magnetic field lines embedded in the wind. The rotation axis of the star is along the z⋆-axis. The 2D cut is placed at the x⋆z⋆ plane, and for reference the orbital distance of the planet is shown with the translucent sphere at 14.56 R⋆ ≃ 0.028 au. The contour shows the wind velocity, and the Alfvén surface is shown by the translucent outer surface. Models I and II predict stellar wind mass-loss rates of 1.1 × 10−15 M⊙ yr−1 and 2.5 × 10−14 M⊙ yr−1. |
| Date | |
| Source | https://www.aanda.org/articles/aa/full_html/2023/10/aa47237-23/aa47237-23.html |
| Author | A. A. Vidotto, V. Bourrier, R. Fares, S. Bellotti, J. F. Donati, P. Petit, G. A. J. Hussain and J. Morin |
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This file is licensed under the Creative Commons Attribution 4.0 International license.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:17, 30 October 2023 |  | 3,301 × 1,467 (1.95 MB) | Artem.G (talk | contribs) | Uploaded a work by A. A. Vidotto, V. Bourrier, R. Fares, S. Bellotti, J. F. Donati, P. Petit, G. A. J. Hussain and J. Morin from https://www.aanda.org/articles/aa/full_html/2023/10/aa47237-23/aa47237-23.html with UploadWizard |
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