对流区和速斜的大尺度动力学

IF 20.9 1区 物理与天体物理
Mark S. Miesch
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引用次数: 300

摘要

在过去的几十年里,我们对太阳内部动力学的理解取得了巨大的进步,这是由相对较新的日震学和日益复杂的数值模型所推动的。作为太阳变率和空间天气的最终驱动因素,全球尺度的对流运动从实践和理论的角度来看都是特别有趣的。在旋转和分层的影响下,湍流对流重新分配动量和能量,通过水力发电机过程产生微分旋转、经向环流和磁场。在靠近对流区底部的太阳速斜中,强角速度切变进一步放大了随后上升到地表形成活动区的场。穿透性对流、不稳定性、分层湍流和波浪都增加了速斜区域的动力丰富性,并提出了特殊的建模挑战。在这篇文章中,我们回顾了太阳内部全球尺度动力学的观测、理论和计算研究。特别强调的是太阳对流的高分辨率全球模拟,强调我们从中学到的东西以及如何改进它们。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Large-Scale Dynamics of the Convection Zone and Tachocline

Large-Scale Dynamics of the Convection Zone and Tachocline

The past few decades have seen dramatic progress in our understanding of solar interior dynamics, prompted by the relatively new science of helioseismology and increasingly sophisticated numerical models. As the ultimate driver of solar variability and space weather, global-scale convective motions are of particular interest from a practical as well as a theoretical perspective. Turbulent convection under the influence of rotation and stratification redistributes momentum and energy, generating differential rotation, meridional circulation, and magnetic fields through hydromagnetic dynamo processes. In the solar tachocline near the base of the convection zone, strong angular velocity shear further amplifies fields which subsequently rise to the surface to form active regions. Penetrative convection, instabilities, stratified turbulence, and waves all add to the dynamical richness of the tachocline region and pose particular modeling challenges. In this article we review observational, theoretical, and computational investigations of global-scale dynamics in the solar interior. Particular emphasis is placed on high-resolution global simulations of solar convection, highlighting what we have learned from them and how they may be improved.

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来源期刊
Living Reviews in Solar Physics
Living Reviews in Solar Physics ASTRONOMY & ASTROPHYSICS-
自引率
1.40%
发文量
3
期刊介绍: Living Reviews in Solar Physics, a platinum open-access journal, publishes invited reviews covering research across all areas of solar and heliospheric physics. It distinguishes itself by maintaining a collection of high-quality reviews regularly updated by the authors. Established in 2004, it was founded by the Max Planck Institute for Solar System Research (MPS). "Living Reviews®" is a registered trademark of Springer International Publishing AG.
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