Fluid Mechanics of Planets and Stars
https://images.springer.com/sgw/books/medium/9783030220730.jpg标题：Fluid Mechanics of Planets and Stars
作者：Michael Le Bars, Daniel Lecoanet
年份：2020
版本：1st ed.
语言：english
ISBN 13: 978-3-030-22073-0;978-3-030-22074-7
格式: PDF
简介：
This book explores the dynamics of planetary and stellar fluid layers, including atmospheres, oceans, iron cores, and convective and radiative zones in stars, describing the different theoretical, computational and experimental methods used to study these problems in fluid mechanics, including the advantages and limitations of each method for different problems. This scientific domain is by nature interdisciplinary and multi-method, but while much effort has been devoted to solving open questions within the various fields of mechanics, applied mathematics, physics, earth sciences and astrophysics, and while much progress has been made within each domain using theoretical, numerical and experimental approaches, cross-fertilizations have remained marginal. Going beyond the state of the art, the book provides readers with a global introduction and an up-to-date overview of relevant studies, fully addressing the wide range of disciplines and methods involved.本书探讨行星和恒星流体层的动力学，包括大气、海洋、铁核以及恒星中的对流和辐射带，描述用于研究流体力学中这些问题的不同理论、计算和实验方法，包括每种方法对不同问题的优点和局限性。这一科学领域本质上是跨学科和多方法的，但在力学、应用数学、物理学、地球科学和天体物理学的各个领域内，虽然已作出了很大的努力来解决公开的问题，虽然各领域使用理论、数值和实验的方法取得了很大的进展，但交叉施肥仍然是微不足道的。超越了最先进的水平，这本书为读者提供了一个全球性的介绍和最新的概述相关的研究，充分涉及广泛的学科和方法所涉及的。The content builds on the CISM course “Fluid mechanics of planets and stars”, held in April 2018, which was part of the research project FLUDYCO, supported by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program.这些内容以2018年4月举办的CISM课程“行星和恒星流体力学”为基础，该课程是FLUDYCO研究项目的一部分，该项目得到了欧洲研究理事会(ERC)在欧洲联盟Horizon 2020研究和创新项目下的支持。
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