Wilson 发表于 2025-3-21 18:24:14

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Obstreperous 发表于 2025-3-21 22:01:36

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精致 发表于 2025-3-22 03:53:56

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dura-mater 发表于 2025-3-22 06:24:10

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荧光 发表于 2025-3-22 09:58:21

2190-5053 acroscopic fluid flow to kinetic scales.Discusses dissipatioThis book revisits the long-standing puzzle of cross-scale energy transfer and dissipation in plasma turbulence and introduces new perspectives based on both magnetohydrodynamic (MHD) and Vlasov models. The classical energy cascade scenario

奇思怪想 发表于 2025-3-22 13:34:02

Bernhard Swoboda,Sandra Schwarzooth region ensures the accuracy, while WENO scheme applied in the shock region captures discontinuities robustly. In order to maintain numerical stability and eliminate spurious oscillations, we utilize a pentadiagonal filter.

奇思怪想 发表于 2025-3-22 17:35:33

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极端的正确性 发表于 2025-3-23 00:42:52

Book 2019eraction is of great significance in producing internal energy. This analysis, in contrast to many other recent studies, does not make assumptions about wave-modes, instability or other specific mechanisms responsible for the dynamics – the results are direct consequences of the Vlasov–Maxwell syste

证明无罪 发表于 2025-3-23 01:56:35

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凶兆 发表于 2025-3-23 06:01:44

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查看完整版本: Titlebook: Energy Transfer and Dissipation in Plasma Turbulence; From Compressible MH Yan Yang Book 2019 The Editor(s) (if applicable) and The Author(