File:AOriSim2004.png
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Three-dimensional color visualization of the magnetic field (field lines in white, magnetic isosurface in blue and temperature surface in red) resulting from a numerical MHD simulation of hydromagnetic dynamo action in the red supergiant star "Betelgeuse" (a.k.a. alpha Orionis). Source: S. B. F. Dorch, the Niels Bohr Institute, Copenhagen University. Originally published in the journal Astronomy and Astrophysics, volume 423, page 1101-1107 (2004).
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:14, 3 January 2007 | | 486 × 416 (226 KB) | Søren Bertil F. Dorch (Talk | contribs) | Three-dimensional color visualization of the magnetic field (field lines in white, magnetic isosurface in blue and temperature surface in red) resulting from a numerical MHD simulation of hydromagnetic dynamo action in the red supergiant star "Betelgeuse" |
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