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Titlebook: Dynamo and Dynamics, a Mathematical Challenge; P. Chossat,D. Ambruster,I. Oprea (Faculty of Mathe Book 2001 Springer Science+Business Medi

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樓主: Coolidge
41#
發(fā)表于 2025-3-28 14:51:06 | 只看該作者
https://doi.org/10.1007/978-3-642-18962-3homogeneous electroconducting fluid of celestial bodies. Such are fields of the Earth, most of the planets, Sun, another stars and even galaxies. The believe is based on the theory and numerical simulation. Until very recently no direct laboratory experiment was supporting this important point.
42#
發(fā)表于 2025-3-28 20:13:47 | 只看該作者
https://doi.org/10.1007/978-3-642-18962-3tion .) which follows from Maxwell equations and Ohm’s law. The solution . = 0 may become unstable for some critical value Re. of the magnetic Reynolds number, .) . and . being respectively typical length and velocity scales.
43#
發(fā)表于 2025-3-28 23:23:15 | 只看該作者
44#
發(fā)表于 2025-3-29 05:04:44 | 只看該作者
Federico Trucco,Patrick J. Tranelagnetic field (1b) were investigated in dependence on Elsasser, Ekman, Roberts numbers and stratification parameter (7) for various mechanical and electrically conductive boundaries (8, 9). Among corresponding MC-waves the westward ones significantly determined by viscosity were revealed.
45#
發(fā)表于 2025-3-29 10:12:42 | 只看該作者
https://doi.org/10.1007/978-94-010-0788-7Magnetohydrodynamics; convection; linear optimization; model; simulation; fluid- and aerodynamics
46#
發(fā)表于 2025-3-29 11:41:10 | 只看該作者
978-0-7923-7070-3Springer Science+Business Media Dordrecht 2001
47#
發(fā)表于 2025-3-29 17:01:28 | 只看該作者
48#
發(fā)表于 2025-3-29 22:57:05 | 只看該作者
49#
發(fā)表于 2025-3-30 00:39:26 | 只看該作者
50#
發(fā)表于 2025-3-30 05:49:40 | 只看該作者
https://doi.org/10.1007/978-3-642-18962-3 at magnetic Reynolds numbers R. greater than a few tens. While the first numerical evidence of this phenomenon has been obtained since almost 45 years, it was only at the end of the year 1999 that it could be experimentally verified in liquid sodium flows. There is still a great gap between such ex
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