標題: Titlebook: Energy Transfer and Dissipation in Plasma Turbulence; From Compressible MH Yan Yang Book 2019 The Editor(s) (if applicable) and The Author( [打印本頁] 作者: Wilson 時間: 2025-3-21 18:24
書目名稱Energy Transfer and Dissipation in Plasma Turbulence影響因子(影響力)
書目名稱Energy Transfer and Dissipation in Plasma Turbulence影響因子(影響力)學科排名
書目名稱Energy Transfer and Dissipation in Plasma Turbulence網(wǎng)絡公開度
書目名稱Energy Transfer and Dissipation in Plasma Turbulence網(wǎng)絡公開度學科排名
書目名稱Energy Transfer and Dissipation in Plasma Turbulence被引頻次
書目名稱Energy Transfer and Dissipation in Plasma Turbulence被引頻次學科排名
書目名稱Energy Transfer and Dissipation in Plasma Turbulence年度引用
書目名稱Energy Transfer and Dissipation in Plasma Turbulence年度引用學科排名
書目名稱Energy Transfer and Dissipation in Plasma Turbulence讀者反饋
書目名稱Energy Transfer and Dissipation in Plasma Turbulence讀者反饋學科排名
作者: Obstreperous 時間: 2025-3-21 22:01 作者: 精致 時間: 2025-3-22 03:53 作者: dura-mater 時間: 2025-3-22 06:24 作者: 熒光 時間: 2025-3-22 09:58
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作者: 奇思怪想 時間: 2025-3-22 13:34
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.作者: 奇思怪想 時間: 2025-3-22 17:35 作者: 極端的正確性 時間: 2025-3-23 00:42
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作者: 證明無罪 時間: 2025-3-23 01:56 作者: 兇兆 時間: 2025-3-23 06:01 作者: febrile 時間: 2025-3-23 12:21
Claudia Lucia Velandia Gomez,Michele Girottoery detail of plasmas from the largest to the smallest spatial and temporal scales. The amount of information contained in the many-body distribution function is vast, and as a consequence it is very hard to directly deal with the Liouville equation.作者: extemporaneous 時間: 2025-3-23 17:31
Torsten Tomczak,Sven Reinecke,Alfred Kussr than the MHD fluid scales, i.e., at kinetic scales, means that characterizing the properties with MHD approximation does not work, but rather more refined models embodying kinetic plasma effects are required.作者: Omniscient 時間: 2025-3-23 19:47
Theoretical Modelling,ery detail of plasmas from the largest to the smallest spatial and temporal scales. The amount of information contained in the many-body distribution function is vast, and as a consequence it is very hard to directly deal with the Liouville equation.作者: Tailor 時間: 2025-3-24 01:30
,Energy Transfer and Dissipation in?Collisionless Plasma Turbulence,r than the MHD fluid scales, i.e., at kinetic scales, means that characterizing the properties with MHD approximation does not work, but rather more refined models embodying kinetic plasma effects are required.作者: 切割 時間: 2025-3-24 05:07 作者: 個人長篇演說 時間: 2025-3-24 07:22 作者: 本土 時間: 2025-3-24 11:05 作者: glowing 時間: 2025-3-24 16:03 作者: 流出 時間: 2025-3-24 22:34 作者: LATHE 時間: 2025-3-25 02:08
Introduction,Plasma turbulence is ubiquitous in space and astrophysical flows. For example, the solar wind emitting from the sun into interplanetary space, one of the most studied natural plasmas, is in a turbulent state.作者: Stress 時間: 2025-3-25 05:39
Energy Cascade in Compressible MHD Turbulence,The most commonly studied turbulent flows are assumed that the incompressibility holds. As mentioned at the outset, for some cases, the validity of incompressibility might be deemed questionable, but rather, compressibility effects are invoked.作者: Fecal-Impaction 時間: 2025-3-25 11:27 作者: anachronistic 時間: 2025-3-25 12:05
Claudia Lucia Velandia Gomez,Michele Girottoery detail of plasmas from the largest to the smallest spatial and temporal scales. The amount of information contained in the many-body distribution function is vast, and as a consequence it is very hard to directly deal with the Liouville equation.作者: infatuation 時間: 2025-3-25 18:48 作者: ingenue 時間: 2025-3-25 22:07
Torsten Tomczak,Sven Reinecke,Alfred Kussr than the MHD fluid scales, i.e., at kinetic scales, means that characterizing the properties with MHD approximation does not work, but rather more refined models embodying kinetic plasma effects are required.作者: 哎呦 時間: 2025-3-26 02:54 作者: grudging 時間: 2025-3-26 04:56
Springer Theseshttp://image.papertrans.cn/e/image/310461.jpg作者: 轎車 時間: 2025-3-26 09:20 作者: 緩和 時間: 2025-3-26 16:20
Filterability of leucocyte suspensionse pressure-time curve of fraction I indicates the behavior of a relatively homogeneous cell population. The pressure-time curve of fraction II can be analyzed to distinguish the effect of the more numerous and more deformable lymphocytes (early part) from the sparser but less deformable monocytes (later part).作者: 物質 時間: 2025-3-26 20:48 作者: 高度 時間: 2025-3-26 22:52
Steve Marshalling, quadratic optimization, utility maximization, indifference pricing, ambiguity risk minimization, no-good-deal pricing and dynamic risk measures. Part III presents some other useful classes of BSDEs and their applications..This book will make BSDEs more accessible to those who are interested in 作者: ECG769 時間: 2025-3-27 04:20 作者: arrogant 時間: 2025-3-27 06:26 作者: MURAL 時間: 2025-3-27 09:32 作者: 偉大 時間: 2025-3-27 15:44 作者: 騷動 時間: 2025-3-27 18:39
