febrile
发表于 2025-3-23 12:21:38
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.
extemporaneous
发表于 2025-3-23 17:31:46
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.
Omniscient
发表于 2025-3-23 19:47:52
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.
Tailor
发表于 2025-3-24 01:30:10
,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.
切割
发表于 2025-3-24 05:07:56
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个人长篇演说
发表于 2025-3-24 07:22:58
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本土
发表于 2025-3-24 11:05:33
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glowing
发表于 2025-3-24 16:03:47
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流出
发表于 2025-3-24 22:34:53
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LATHE
发表于 2025-3-25 02:08:38
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.