03676nam 22005295 450 991035022880332120200630013713.0981-13-8149-610.1007/978-981-13-8149-2(CKB)4100000008525969(DE-He213)978-981-13-8149-2(MiAaPQ)EBC5776241(PPN)236523287(EXLCZ)99410000000852596920190502d2019 u| 0engurnn|008mamaatxtrdacontentcrdamediacrrdacarrierEnergy Transfer and Dissipation in Plasma Turbulence [electronic resource] From Compressible MHD to Collisionless Plasma /by Yan Yang1st ed. 2019.Singapore :Springer Singapore :Imprint: Springer,2019.1 online resource (XIX, 134 p. 55 illus., 52 illus. in color.) Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053981-13-8148-8 Introduction -- Elements of Plasma Physics -- Numerical Algorithm for Compressible Magnetohydrodynamic Turbulence -- Energy Cascade in Compressible Magnetohydrodynamic Turbulence -- Energy Transfer and Dissipation in Collisionless Plasma Turbulence -- Discussion and Conclusions.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 system of equations. This is an important step toward understanding dissipation in turbulent collisionless plasma in space and astrophysics.Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053Plasma (Ionized gases)Fluid mechanicsNumerical analysisPlasma Physicshttps://scigraph.springernature.com/ontologies/product-market-codes/P24040Engineering Fluid Dynamicshttps://scigraph.springernature.com/ontologies/product-market-codes/T15044Numerical Analysishttps://scigraph.springernature.com/ontologies/product-market-codes/M14050Plasma (Ionized gases).Fluid mechanics.Numerical analysis.Plasma Physics.Engineering Fluid Dynamics.Numerical Analysis.530.44Yang Yanauthttp://id.loc.gov/vocabulary/relators/aut838755BOOK9910350228803321Energy transfer and dissipation in plasma turbulence1873373UNINA