Collaborative Research: Models of the deep circulation of gas giants: solar heating, convection, and zonal flows

合作研究：气态巨行星的深层循环模型：太阳加热、对流和纬向流

• 批准号: 0708698
• 负责人: Adam Showman
• 金额: $ 1.59万
• 依托单位: University of Arizona
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2007
• 资助国家: 美国
• 起止时间: 2007-07-01 至 2010-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0708698&HistoricalAwards=false
• 关键词: Collaborative; Research; Models; deep; circulation

AST 0708106FlierlAST 0708698ShowmanDrs. Glenn Flierl and Adam Showman will carry out a program of modeling the circulations on gas giant planets (both solar and extra-solar) to understand the role of rotation, internal heat sources, and heating from the star on the dynamics. They have extended the general circulationmodel developed at MIT to include deep spherical geometry, fully non-hydrostatic dynamics, strong density variations using the anelastic approximation, and an equation of state suitable for hydrogenand helium at high pressures. The objective is to understand thermal convection and the productionof columnar zonal flow, the circulations driven by the equatorial heating and polar cooling, the role of eddies, and the interactions between the various kinds of motions. They will study both two- and three-dimensional models and relate them to previous, more idealized models and analytical theories.The flows on gas giants remain a fascinating problem in geophysical fluid dynamics. By examining in detail convective and instability processes and the interactions between the deep and surface circulations, this research team will learn more about the ways in which these processes set the mean thermal structure and the forces which produce the prominent zonal flows. Convection and interactions between eddies and mean flows are general features in atmospheres and oceans. Giant planets offer a laboratory for studying and modeling these processes. This kind of knowledge will be important in interpreting the new data being gathered about the extra-solar gas giants as well. Numerical models offer an approach to understanding geophysical flows, but the most difficult aspect in using them is analyzing the results and understanding the processes, including study of simplified representations. Training students and postdocs in this area is important to advance our capabilities in planetary fluid dynamics (including climate dynamics).***

AST 0708106传单AST 0708698 Showman医生Glenn Flierl和Adam Showman将开展一项模拟气体巨行星（太阳和太阳系外）环流的计划，以了解旋转，内部热源和星星加热对动力学的作用。他们扩展了麻省理工学院开发的一般循环模型，包括深球形几何形状，完全非流体静力学动力学，使用滞弹性近似的强密度变化，以及适用于高压下氢和氦的状态方程。 目的是了解热对流和柱状纬向流的产生，赤道加热和极地冷却驱动的环流，涡旋的作用，以及各种运动之间的相互作用。 他们将研究二维和三维模型，并将其与以前的，更理想化的模型和分析理论。气体巨星上的流动仍然是地球物理流体动力学中一个迷人的问题。通过详细研究对流和不稳定过程以及深层和表层环流之间的相互作用，该研究小组将更多地了解这些过程设定平均热结构的方式以及产生显著纬向流的力。对流以及涡旋和平均流之间的相互作用是大气和海洋中的一般特征。巨行星为研究和模拟这些过程提供了实验室。这类知识对于解释收集的关于太阳系外气体巨星的新数据也很重要。数值模型提供了一种理解地球物理流动的方法，但使用它们最困难的方面是分析结果和理解过程，包括简化表示的研究。 在这一领域培训学生和博士后对于提高我们在行星流体动力学（包括气候动力学）方面的能力非常重要。*