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

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發(fā)表于 2025-3-21 18:24:14 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Energy Transfer and Dissipation in Plasma Turbulence
副標(biāo)題From Compressible MH
編輯Yan Yang
視頻videohttp://file.papertrans.cn/311/310461/310461.mp4
概述Nominated by Peking University as an outstanding Ph.D. thesis.Presents a systematic study on energy transfer and dissipation spanning from macroscopic fluid flow to kinetic scales.Discusses dissipatio
叢書名稱Springer Theses
圖書封面Titlebook: Energy Transfer and Dissipation in Plasma Turbulence; From Compressible MH Yan Yang Book 2019 The Editor(s) (if applicable) and The Author(
描述This 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 is key in explaining the heating of corona and solar wind. By employing a high-resolution hybrid (compact finite difference & WENO) scheme, the book studies the features of compressible MHD cascade in detail, for example, in order to approximate a real plasma cascade as “Kolmogorov-like” and to understand features that go beyond the usual simplified theories based on incompressible models. When approaching kinetic scales where plasma effects must be considered, it uses an elementary analysis of the Vlasov–Maxwell equations to help identify the channels through which energy transfer must be dissipated. In addition, it shows that the pressure–strain interaction 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
出版日期Book 2019
關(guān)鍵詞Compressible magnetohydrodynamic turbulence; High-resolution hybrid compact-WENO scheme; Plasma turbul
版次1
doihttps://doi.org/10.1007/978-981-13-8149-2
isbn_ebook978-981-13-8149-2Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor
The information of publication is updating

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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
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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.
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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
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