| 書目名稱 | Fast Solar Wind Driven by Parametric Decay Instability and Alfvén Wave Turbulence | | 編輯 | Munehito Shoda | | 視頻video | http://file.papertrans.cn/342/341318/341318.mp4 | | 概述 | Nominated as an outstanding PhD thesis by the University of Tokyo, Tokyo, Japan.Is a winner of the 2019 International Astronomical Union Division E Ph.D. prize.Includes the first-ever 3D simulation of | | 叢書名稱 | Springer Theses | | 圖書封面 |  | | 描述 | This book discusses key theoretical aspects concerning the formation of the solar wind: the most essential building block in the heliosphere, in which planets orbit. To understand the influence of solar activity on planetary magnetospheres and atmospheres, we need to first understand the origin of the solar wind, which is still under debate. This book presents the outcomes of state-of-the-art numerical simulations of solar wind acceleration, including the first three-dimensional simulation of the turbulence-driven solar wind model. One of the book’s goals is to include compressional effects in the dynamics of solar wind turbulence; accordingly, it discusses parametric decay instability in detail. Several key aspects that are relevant to the Parker Solar Probe observations are also discussed. Given its scope, the book plays a key role in bridging the gap between the theory of magnetohydrodynamic turbulence and current/future in-situ observations of the solar wind.?This book is based on the Ph.D. thesis by the author, which won the 2019 International Astronomical Union Division E Ph.D. prize. | | 出版日期 | Book 2021 | | 關(guān)鍵詞 | Coronal Heating and Solar Wind Acceleration; Compressible Magnetohydrodynamic Turbulence; Alfvén Wave | | 版次 | 1 | | doi | https://doi.org/10.1007/978-981-16-1030-1 | | isbn_softcover | 978-981-16-1032-5 | | isbn_ebook | 978-981-16-1030-1Series ISSN 2190-5053 Series E-ISSN 2190-5061 | | issn_series | 2190-5053 | | copyright | The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor |
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