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Plasma turbulence in the solar system

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-Ea...

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Autor principal: Narita, Yasuhito
Lenguaje:eng
Publicado: Springer 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-642-25667-7
http://cds.cern.ch/record/1433765
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author Narita, Yasuhito
author_facet Narita, Yasuhito
author_sort Narita, Yasuhito
collection CERN
description 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.
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spelling cern-14337652021-04-22T00:35:34Zdoi:10.1007/978-3-642-25667-7http://cds.cern.ch/record/1433765engNarita, YasuhitoPlasma turbulence in the solar systemAstrophysics and AstronomyDynamics 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.Springeroai:cds.cern.ch:14337652012
spellingShingle Astrophysics and Astronomy
Narita, Yasuhito
Plasma turbulence in the solar system
title Plasma turbulence in the solar system
title_full Plasma turbulence in the solar system
title_fullStr Plasma turbulence in the solar system
title_full_unstemmed Plasma turbulence in the solar system
title_short Plasma turbulence in the solar system
title_sort plasma turbulence in the solar system
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1007/978-3-642-25667-7
http://cds.cern.ch/record/1433765
work_keys_str_mv AT naritayasuhito plasmaturbulenceinthesolarsystem