Plasma Turbulence in the Solar System - read free eBook in online reader or directly download on the web page. Select files or add your book in reader. Download and read online ebook Plasma Turbulence in the Solar System write by Yasuhito Narita. This book was released on 2012-01-19. Plasma Turbulence in the Solar System available in PDF, EPUB and Kindle. Dynamics of astrophysical systems is often described by plasma physics, yet understanding the nature of plasma turbulence remains as a challenge in physics in both theories and experiments. This book is an up-to-date summary and review of recent results in research on waves and turbulence in near-Earth space plasma turbulence, obtained by Cluster, the multi-spacecraft mission. Spatial and temporal structures of solar wind turbulence as well as its interaction with the bow shock ahead of the Earth are presented using Cluster data. The book presents (1) historical developments, (2) theoretical background of plasma physics, turbulence theories, and the plasma physical picture of the solar system, (3) analysis methods for multi-spacecraft data, (4) results of Cluster data analysis, and (5) impacts on astrophysics and Earth sciences.
Plasma Turbulence in the Solar System
Plasma Turbulence in the Solar System - read free eBook in online reader or directly download on the web page. Select files or add your book in reader. Download and read online ebook Plasma Turbulence in the Solar System write by Yasuhito Narita. This book was released on 2012-01-21. Plasma Turbulence in the Solar System available in PDF, EPUB and Kindle. Dynamics of astrophysical systems is often described by plasma physics, yet understanding the nature of plasma turbulence remains as a challenge in physics in both theories and experiments. This book is an up-to-date summary and review of recent results in research on waves and turbulence in near-Earth space plasma turbulence, obtained by Cluster, the multi-spacecraft mission. Spatial and temporal structures of solar wind turbulence as well as its interaction with the bow shock ahead of the Earth are presented using Cluster data. The book presents (1) historical developments, (2) theoretical background of plasma physics, turbulence theories, and the plasma physical picture of the solar system, (3) analysis methods for multi-spacecraft data, (4) results of Cluster data analysis, and (5) impacts on astrophysics and Earth sciences.
Solar System Plasma Processes
Solar System Plasma Processes - read free eBook in online reader or directly download on the web page. Select files or add your book in reader. Download and read online ebook Solar System Plasma Processes write by Louis J. Lanzerotti. This book was released on 1979. Solar System Plasma Processes available in PDF, EPUB and Kindle.
Turbulence in Space Plasmas
Turbulence in Space Plasmas - read free eBook in online reader or directly download on the web page. Select files or add your book in reader. Download and read online ebook Turbulence in Space Plasmas write by Loukas Vlahos. This book was released on 2009-06-12. Turbulence in Space Plasmas available in PDF, EPUB and Kindle. Over the years, many leading European graduate schools in the field of astrophysical and space plasmas have operated within the framework of the research network, "Theory, Observations, and Simulations in Turbulence in Space Plasmas." This text is a set of lectures and tutorial reviews culled from the relevant work of all those schools. It emphasizes applications on solar coronae, solar flares, and the solar wind. In bridging the gap between standard textbook material and state-of-the-art research, this text offers a broad flavor to postgraduate and postdoctoral students just coming to the field. And because of its unique mix, it will also be useful to lecturers looking for advanced teaching material for their seminars and courses.
Turbulence in the Solar Wind
Turbulence in the Solar Wind - read free eBook in online reader or directly download on the web page. Select files or add your book in reader. Download and read online ebook Turbulence in the Solar Wind write by Roberto Bruno. This book was released on 2016-10-07. Turbulence in the Solar Wind available in PDF, EPUB and Kindle. 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.
