ALLY 发表于 2025-3-21 17:33:12

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放肆的我 发表于 2025-3-21 21:42:26

Colleen O’Connor Olson because one of our main purposes of this book is to treat the flow problems of plasma which are essentially gasdynamical in nature. In this chapter we shall briefly discuss the properties of electromagnetic equations and the approximations which will be used in our analysis.

沉思的鱼 发表于 2025-3-22 02:21:03

Stanley D. Sidesnvolves integrals over the relevant closed line, but considerations about the ergodicity of magnetic lines on a surface with irrational rotational transform lead to a better version involving surface integrals that occur naturally in our model of magnetohydrodynamic equilibrium. For details we refer

罐里有戒指 发表于 2025-3-22 05:57:08

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思想上升 发表于 2025-3-22 08:56:26

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antecedence 发表于 2025-3-22 15:54:02

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侵略主义 发表于 2025-3-22 19:06:00

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苦笑 发表于 2025-3-22 23:50:36

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abduction 发表于 2025-3-23 04:45:48

Kurt L. Helf,Rickard A. Olsoneyold number is high enough that the hydrodynamical bifurcation sequence to a more chaotic flow already has taken place, the mean value of the Lyapunov exponent is noticeable diminished in the saturated phase compared to the growth phase of the dynamo.

分发 发表于 2025-3-23 07:46:55

Steven C. Thomas,Rickard S. Toomey IIIagnetic field flux tubes and the vorticity flux tubes. For the case of a barotropic gas with . = .(.), .. is conserved following the flow, i.e. ../. = 0. For non-barotopic flows, a modifled form of the cross helicity, .. is conserved following the flow. We derive topological invariants (topological
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查看完整版本: Titlebook: Mammoth Cave; A Human and Natural Horton H. Hobbs III,Rickard A Olson,David C. Culve Book 2017 Springer International Publishing AG 2017 C