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Energy transfer and dissipation in p...

Yang, Yan.

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Energy transfer and dissipation in plasma turbulence = from compressible MHD to collisionless plasma /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Energy transfer and dissipation in plasma turbulence/ by Yan Yang.
Reminder of title:	from compressible MHD to collisionless plasma /
Author:	Yang, Yan.
Published:	Singapore :Springer Singapore : : 2019.,
Description:	xix, 134 p. :ill. (some col.), digital ;24 cm.
[NT 15003449]:	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.
Contained By:	Springer Nature eBook
Subject:	Plasma turbulence. -
Online resource:	https://doi.org/10.1007/978-981-13-8149-2
ISBN:	9789811381492

Energy transfer and dissipation in plasma turbulence = from compressible MHD to collisionless plasma /
Yang, Yan.

Energy transfer and dissipation in plasma turbulencefrom compressible MHD to collisionless plasma /[electronic resource] :by Yan Yang. - Singapore :Springer Singapore :2019. - xix, 134 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

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.

ISBN: 9789811381492

Standard No.: 10.1007/978-981-13-8149-2doiSubjects--Topical Terms:

1568180
Plasma turbulence.

LC Class. No.: QC718.5.T8 / Y35 2019

Dewey Class. No.: 530.442

Energy transfer and dissipation in plasma turbulence = from compressible MHD to collisionless plasma /
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300 $a xix, 134 p. : $b ill. (some col.), digital ; $c 24 cm.
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505 0 $a 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.
520 $a 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.
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