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Energy Transfer and Dissipation in Plasma Turbulence

Energy Transfer and Dissipation in Plasma Turbulence
Author: Yan Yang
Publisher: Springer
Total Pages: 134
Release: 2019-05-02
Genre: Science
ISBN: 9811381496

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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.


An Introduction to the Theory of Plasma Turbulence

An Introduction to the Theory of Plasma Turbulence
Author: V. N. Tsytovich
Publisher: Elsevier
Total Pages: 144
Release: 2016-07-29
Genre: Science
ISBN: 1483139921

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An Introduction to the Theory of Plasma Turbulence is a collection of lectures given by the author at Culham laboratory. The book deals with developments on the theory of plasma turbulence. The author describes plasma properties in the turbulent regions as mostly non-linear in nature, and notes that these properties can be regarded as a universal spectrum independent of any type of instability. The text then discusses the general problems of the theory of plasma turbulence. The author also shows that elementary excitation of ""dressed"" particles have a finite lifetime associated with non-linear interactions. The book then discusses the excitation of ion-sound turbulence using different processes, for example, shock waves; the text also analyzes the kind of non-linear interactions present in such energy transfer. The author also explains the Langmuir plasma oscillations — a typical collective plasma motion that can be excited using different types of mechanism such as an electron beam. The book then describes the electromagnetic properties of turbulent plasma and relates the state of turbulent plasma as a natural occurrence in the universe. The book notes the problem of cosmic rays, not as an energy transfer to faster particles, but as an energy distribution between particles. The text will prove valuable for nuclear physicists, scientists, and academicians in the field of quantum mechanics.


Turbulent Heating in Space Plasmas

Turbulent Heating in Space Plasmas
Author: Riddhi Bandyopadhyay
Publisher:
Total Pages: 311
Release: 2021
Genre:
ISBN:

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A turbulent system transfers energy from large scales to progressively smaller scales until it is ultimately dissipated as heat. At intermediate length scales, this energy transfer mostly occurs from larger scales to smaller scales, without any loss of energy. This process is known as the energy cascade. Most space and astrophysical plasmas are considered to exist in a turbulent state. Turbulent energy cascade and dissipation have significant effects on the dynamics of the plasma. However, the nature of energy dissipation is not well understood in weakly-collisional plasmas. Several mechanisms have been proposed as candidates for energy dissipation in these systems. Examples include magnetic reconnection, Landau damping, damping of waves, and heating by microinstabilities, all of which can contribute to plasma heating. A complementary point of view treats the plasma as a statistically homogeneous system with all the aforementioned processes embedded ab inito in an ensemble. From this perspective, an important question is how to quantitatively estimate the average rates of energy transfer and dissipation. In this dissertation, we attempt to answer this and related questions, with a focus on heliospheric plasmas, although the same understandings apply in other turbulent plasmas in laboratory, geophysical, and astrophysical systems.


Plasma Turbulence

Plasma Turbulence
Author: Leslie S. G. Kovásznay
Publisher:
Total Pages: 50
Release: 1960
Genre: Plasma (Ionized gases)
ISBN:

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Anomalous Electron-ion Energy Coupling in Electron Drift Wave Turbulence

Anomalous Electron-ion Energy Coupling in Electron Drift Wave Turbulence
Author: Lei Zhao
Publisher:
Total Pages: 96
Release: 2013
Genre:
ISBN: 9781303212482

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Turbulence is a ubiquitous phenomenon in nature, and it is well known that turbulence couples energy input to dissipation by cascade processes. Plasma turbulence play a critical role in tokamak confinement. Magnetized plasma turbulence is quasi 2D, anisotropic, wave like and two fluid (i.e. electrons and ions) in structure. Thus, weakly collisional plasma turbulence can mediate electron and ion energy transfer. The issue of anomalous electron and ion energy coupling is particularly important for low collisionality, electron heated plasmas, such as ITER. In this work, we reconsider the classic problem of turbulent heating and energy transfer pathways in drift wave turbulence. The total turbulent heating, composed of quasilinear electron cooling, quasilinear ion heating, nonlinear ion heating and zonal flow frictional heating, is analyzed. In Chapter 2, the electron and ion energy exchange via linear wave and particle resonance will be computed. To address net heating, we show the turbulent heating in an annulus arises due to a wave energy flux differential across this region. We show this net heating is proportional to the Reynolds work on the zonal flow. Zonal flow friction heats ions, thus the turbulence and zonal flow interaction enters as an important energy transfer channel. Since zonal flows are nonlinearly generated, it follows that we should apply weak turbulence theory to calculate the nonlinear ion turbulent heating via the virtual mode resonance in the electron drift wave turbulence, which will be discussed in Chapter 3. We defines a new collisionless turbulent energy transfer channel through nonlinear Landau damping in the electron and ion energy coupling process. The result shows that nonlinear ion heating can exceed quasilinear ion heating, so that nonlinear heating becomes the principal collisionless wave energy dissipation channel in electron drift wave turbulence. This follows since the beat mode resonates with the bulk of the ion distribution, in contrast to the linear resonance which is located on the tail. This result also suggests that zonal flow shearing is not necessarily the only saturation mechanism of importance, especially for very low collisionality. This observation brings a new perspective on electron heat transport where ions, play a role as an energy "sink" in a collisionless plasma, such as ITER. In addition, it is shown that the electron turbulent energy transfer to ions in a collisionless plasma can be the same order as electron heat transport losses. Thus, it is necessary to consider the influence of collisionless energy transfer to determine the total energy budget in ITER.


Turbulence in the Solar Wind

Turbulence in the Solar Wind
Author: Roberto Bruno
Publisher: Springer
Total Pages: 270
Release: 2016-10-07
Genre: Science
ISBN: 3319434403

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This book provides an overview of solar wind turbulence from both the theoretical and observational perspective. It argues that the interplanetary medium offers the best opportunity to directly study turbulent fluctuations in collisionless plasmas. In fact, during expansion, the solar wind evolves towards a state characterized by large-amplitude fluctuations in all observed parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence. This text starts with historical references to past observations and experiments on turbulent flows. It then introduces the Navier-Stokes equations for a magnetized plasma whose low-frequency turbulence evolution is described within the framework of the MHD approximation. It also considers the scaling of plasma and magnetic field fluctuations and the study of nonlinear energy cascades within the same framework. It reports observations of turbulence in the ecliptic and at high latitude, treating Alfvénic and compressive fluctuations separately in order to explain the transport of mass, momentum and energy during the expansion. Further, existing models are compared with direct observations in the heliosphere. The problem of self-similar and anomalous fluctuations in the solar wind is then addressed using tools provided by dynamical system theory and discussed on the basis of available models and observations. The book highlights observations of Yaglom’s law in solar wind turbulence, which is one of the most important findings in fully developed turbulence and directly related to the long-lasting and still unsolved problem of solar wind plasma heating. Lastly, it includes a short chapter dedicated to the kinetic range of fluctuations, which has recently been receiving more attention from the space plasma community, since this is inherently related to turbulent energy dissipation and consequent plasma heating. It particularly focuses on the nature and role of the fluctuations populating this frequency range, and discusses several model predictions and recent observational findings in this context.


Plasma Physics of the Local Cosmos

Plasma Physics of the Local Cosmos
Author: National Research Council
Publisher: National Academies Press
Total Pages: 100
Release: 2004-06-06
Genre: Science
ISBN: 9780309092159

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Solar and space physics is the study of solar system phenomena that occur in the plasma state. Examples include sunspots, the solar wind, planetary magnetospheres, radiation belts, and the aurora. While each is a distinct phenomenon, there are commonalities among them. To help define and systematize these universal aspects of the field of space physics, the National Research Council was asked by NASA's Office of Space Science to provide a scientific assessment and strategy for the study of magnetized plasmas in the solar system. This report presents that assessment. It covers a number of important research goals for solar and space physics. The report is complementary to the NRC report, The Sun to the Earthâ€"and Beyond: A Decadal Research Strategy for Solar and Space Physics, which presents priorities and strategies for future program activities.


Handbook of Single-Phase Convective Heat Transfer

Handbook of Single-Phase Convective Heat Transfer
Author: Sadik Kakaç
Publisher: Wiley-Interscience
Total Pages: 1268
Release: 1987-11-03
Genre: Science
ISBN:

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Very Good,No Highlights or Markup,all pages are intact.


Study of Nonlinear Energy Transfer Between Drift Wave Turbulence and Spontaneously Generated Sheared Flows in a Laboratory Plasma

Study of Nonlinear Energy Transfer Between Drift Wave Turbulence and Spontaneously Generated Sheared Flows in a Laboratory Plasma
Author: Min Xu
Publisher:
Total Pages: 316
Release: 2010
Genre:
ISBN: 9781124201375

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Experiments in a laboratory plasma are used to identify how small-scale turbulent structures give rise to large-scale sheared zonal flows. A new technique based on cross-bispectral analysis has been developed and applied to directly measure the nonlinear energy transfer rates between drift wave turbulence and sheared flows. In addition fast imaging is used to directly observe the turbulent structure dynamics. A combined study using both Langmiur probe arrays and fast visible light imaging shows that the sheared zonal flow is sustained by the emission of drift vortices in the central plasma which then propagate in a spiral trajectory, approach the shear layer, and then merge into the sheared flow, thereby transferring their momentum and kinetic energy to it. The shear flow is then amplified. The results are consistent with previous probe measurements of the turbulent Reynolds stress, and provide a detailed confirmation of the basic theoretical expectations for the turbulent drive of zonal flows in magnetized plasmas.


Magnetohydrodynamic Turbulence

Magnetohydrodynamic Turbulence
Author: Dieter Biskamp
Publisher: Cambridge University Press
Total Pages: 313
Release: 2003-07-31
Genre: Science
ISBN: 1139441671

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This book presents an introduction to, and modern account of, magnetohydrodynamic (MHD) turbulence, an active field both in general turbulence theory and in various areas of astrophysics. The book starts by introducing the MHD equations, certain useful approximations and the transition to turbulence. The second part of the book covers incompressible MHD turbulence, the macroscopic aspects connected with the different self-organization processes, the phenomenology of the turbulence spectra, two-point closure theory, and intermittency. The third considers two-dimensional turbulence and compressible (in particular, supersonic) turbulence. Because of the similarities in the theoretical approach, these chapters start with a brief account of the corresponding methods developed in hydrodynamic turbulence. The final part of the book is devoted to astrophysical applications: turbulence in the solar wind, in accretion disks, and in the interstellar medium. This book is suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.