Animations of stellar magnetoconvection simulations
Benjamin Beeck1, Manfred Schüssler1, Robert H. Cameron1, and Ansgar Reiners2
1 Max-Planck-Institute für Sonnensystemforschung, Justus-von-Liebig-Weg 2, D-37077 Göttingen
2 Institut für Astrophysik, Universität Göttingen, Friedrich-Hund-Platz 1, D-37077 Göttingen
With the paper Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations (accepted for publication in A&A, arXiv preprint) we publish animations of six stellar magnetoconvection simulations as online material. These animations show the evolution of the bolometric intensity, the vertical velocity (at τR=1) and the magnetic field strength (at τR=1) over a (stellar) time of about 10-15 minutes. On this page, you can download not only the six animations published with A&A but animations of all 18 magnetic simulations which are analysed in that paper.
- F3V, B0=20G, mpeg, 17.9 MiB, 9.3s (= 932s stellar time)
- F3V, B0=100G, mpeg, 17.2 MiB, 8.9s (= 892s stellar time) — published as online material in A&A
- F3V, B0=500G, mpeg, 18.9 MiB, 9.8s (= 980s stellar time)
- G2V, B0=20G, mpeg, 21.4 MiB, 11.1s (= 1112s stellar time)
- G2V, B0=100G, mpeg, 20.6 MiB, 10.7s (= 1072s stellar time) — published as online material in A&A
- G2V, B0=500G, mpeg, 20.7 MiB, 10.8s (= 1076s stellar time) — published as online material in A&A
- K0V, B0=20G, mpeg, 22.7 MiB, 11.8s (= 888s stellar time)
- K0V, B0=100G, mpeg, 19.5 MiB, 10.1s (= 756s stellar time)
- K0V, B0=500G, mpeg, 18.8 MiB, 9.8s (= 732s stellar time) — published as online material in A&A
- K5V, B0=20G, mpeg, 17.4 MiB, 9.1s (= 681s stellar time)
- K5V, B0=100G, mpeg, 15.5 MiB, 8.0s (= 603s stellar time)
- K5V, B0=500G, mpeg, 15.4 MiB, 8.0s (= 600s stellar time)
- M0V, B0=20G, mpeg, 19.5 MiB, 10.1s (= 759s stellar time)
- M0V, B0=100G, mpeg, 14.1 MiB, 7.3s (= 546s stellar time)
- M0V, B0=500G, mpeg, 13.1 MiB, 6.8s (= 507s stellar time)
- M2V, B0=20G, mpeg, 23.8 MiB, 12.4s (= 930s stellar time)
- M2V, B0=100G, mpeg, 11.5 MiB, 6.0s (= 447s stellar time) — published as online material in A&A
- M2V, B0=500G, mpeg, 10.4 MiB, 5.4s (= 402s stellar time) — published as online material in A&A
Also see:
Acknowledgements: The authors acknowledge research funding by the Deutsche Forschungsgemeinschaft (DFG) under the grant SFB 963/1, project A16. AR has received research funding from the DFG under DFG 1664/9-2.