Wang Guiquan, Santelli Luca, Lohse Detlef, Verzicco Roberto, Stevens Richard J A M
Department of Science and Technology Physics of Fluids Group and Twente Max Planck Center, Mesa+ Institute J. M. Burgers Center for Fluid Dynamics University of Twente Enschede The Netherlands.
Gran Sasso Science Institute L'Aquila Italy.
Geophys Res Lett. 2021 Oct 28;48(20):e2021GL095017. doi: 10.1029/2021GL095017. Epub 2021 Oct 21.
Direct numerical simulations are employed to reveal three distinctly different flow regions in rotating spherical Rayleigh-Bénard convection. In the high-latitude region vertical (parallel to the axis of rotation) convective columns are generated between the hot inner and the cold outer sphere. The mid-latitude region is dominated by vertically aligned convective columns formed between the Northern and Southern hemispheres of the outer sphere. The diffusion-free scaling, which indicates bulk-dominated convection, originates from this mid-latitude region. In the equator region , the vortices are affected by the outer spherical boundary and are much shorter than in region .
采用直接数值模拟来揭示旋转球形瑞利-贝纳德对流中三个明显不同的流动区域。在高纬度区域,在热的内球和冷的外球之间产生垂直(平行于旋转轴)对流柱。中纬度区域由在外球的北半球和南半球之间形成的垂直排列的对流柱主导。表明整体主导对流的无扩散标度起源于这个中纬度区域。在赤道区域,涡旋受到外球边界的影响,并且比在其他区域短得多。