| 書目名稱 | Turbulence in the Solar Wind |
| 編輯 | Roberto Bruno,Vincenzo Carbone |
| 視頻video | http://file.papertrans.cn/932/931026/931026.mp4 |
| 概述 | Serves as modern and concise introduction to the subject matter.Combines theory and observation throughout.Offers a self-contained and tutorial presentation |
| 叢書名稱 | Lecture Notes in Physics |
| 圖書封面 |  |
| 描述 | .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parameters, which resembles, at least at large scales, the well-known hydrodynamic turbulence..This text starts with historical references to past observations and experiments on turbulent flows.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 andcompressive 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 proble |
| 出版日期 | Book 2016 |
| 關(guān)鍵詞 | MHD approximation; MHD turbulence; Transport processes in space plasmas; Yaglom’s law; Solar wind plasma |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-319-43440-7 |
| isbn_softcover | 978-3-319-43439-1 |
| isbn_ebook | 978-3-319-43440-7Series ISSN 0075-8450 Series E-ISSN 1616-6361 |
| issn_series | 0075-8450 |
| copyright | Springer International Publishing Switzerland 2016 |
|Archiver|手機(jī)版|小黑屋|
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