File:Simulated stellar wind environment for AU Mic driven by the different ZDI maps of the star.jpg
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Summary
| Description |
English: Simulated stellar wind environment for AU Mic driven by the different ZDI maps of the star. A common color scale denotes the equatorial distribution of the stellar wind dynamic pressure (Pdyn) normalized to the average Sun–Earth value Pdyn. Solid and dashed lines indicate the orbits of AU Mic b and c, respectively. A translucent shade shows the resulting Alfvén surface (AS) of the stellar wind in each case (see text for details). The equatorial projection of the AS (white solid line) and its average radius are indicated. Selected closed (magenta) and open (black with arrows) magnetic field lines are shown. The field of view on each panel has been adjusted to show the entire SC domain for the respective case. |
| Date | |
| Source | https://iopscience.iop.org/article/10.3847/1538-4357/ac54b8 |
| Author | Julián D. Alvarado-Gómez, Ofer Cohen, Jeremy J. Drake, Federico Fraschetti, Katja Poppenhaeger, Cecilia Garraffo, Judy Chebly, Ekaterina Ilin, Laura Harbach, and Oleg Kochukhov |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 06:50, 18 May 2023 | | 2,170 × 1,930 (1.53 MB) | Artem.G | Uploaded a work by Julián D. Alvarado-Gómez, Ofer Cohen, Jeremy J. Drake, Federico Fraschetti, Katja Poppenhaeger, Cecilia Garraffo, Judy Chebly, Ekaterina Ilin, Laura Harbach, and Oleg Kochukhov from https://iopscience.iop.org/article/10.3847/1538-4357/ac54b8 with UploadWizard |
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