{"title":"Multiplicity in an optimised kinematic dynamo","authors":"Long Chen","doi":"10.1080/03091929.2022.2098284","DOIUrl":null,"url":null,"abstract":"Multiplicity in optimal kinematic dynamos exists for certain types of symmetry classes and boundary conditions, at least near the lowest dynamo onset . Here we investigate the NNT type dynamo generated by steady flows with impermeable boundary conditions in a cube, where the letter N or T stands for pseudo-vacuum or superconducting boundary conditions along x, y, z directions, respectively. We find the top two of the three branches in the neighbourhood of have their growth rates crossed over at . Within each branch, the spatial structure of the optimal velocity field gradually shifts with respect to . At about above , the original optimal branch has developed distinct combinations of dominant Fourier modes. In contrast, the first suboptimal branch shows the least change in structure. We then follow the evolution of selected optimised solutions when varies until it becomes unstable. Specific modes in the flow that can destabilise the dynamo are identified. Within the range surveyed, we find that there can be one to two dynamo windows. All three branches generate a steady dynamo near , but the first suboptimal branch can generate an oscillatory dynamo at about eight times , and for both suboptimal branches, the growth rate reaches saturation approximately at . We find the two suboptimal branches create a more robust dynamo action supercritically.","PeriodicalId":56132,"journal":{"name":"Geophysical and Astrophysical Fluid Dynamics","volume":"67 1","pages":"290 - 304"},"PeriodicalIF":1.1000,"publicationDate":"2022-07-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Geophysical and Astrophysical Fluid Dynamics","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.1080/03091929.2022.2098284","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Multiplicity in optimal kinematic dynamos exists for certain types of symmetry classes and boundary conditions, at least near the lowest dynamo onset . Here we investigate the NNT type dynamo generated by steady flows with impermeable boundary conditions in a cube, where the letter N or T stands for pseudo-vacuum or superconducting boundary conditions along x, y, z directions, respectively. We find the top two of the three branches in the neighbourhood of have their growth rates crossed over at . Within each branch, the spatial structure of the optimal velocity field gradually shifts with respect to . At about above , the original optimal branch has developed distinct combinations of dominant Fourier modes. In contrast, the first suboptimal branch shows the least change in structure. We then follow the evolution of selected optimised solutions when varies until it becomes unstable. Specific modes in the flow that can destabilise the dynamo are identified. Within the range surveyed, we find that there can be one to two dynamo windows. All three branches generate a steady dynamo near , but the first suboptimal branch can generate an oscillatory dynamo at about eight times , and for both suboptimal branches, the growth rate reaches saturation approximately at . We find the two suboptimal branches create a more robust dynamo action supercritically.
在某些对称类和边界条件下,最优运动发电机存在多重性,至少在最低发电机起点附近存在多重性。在这里,我们研究了由立方体中具有不渗透边界条件的稳定流动产生的NNT型发电机,其中字母N或T分别代表沿x, y, z方向的伪真空或超导边界条件。我们发现在附近的三个分支中,最上面的两个的增长率相交于。在各支路内,最优速度场的空间结构相对于。大约在上面,原始的最优分支已经发展出不同的主要傅立叶模式组合。相比之下,第一个次优分支的结构变化最小。然后,当选择的优化解决方案发生变化时,我们遵循其演变,直到它变得不稳定。确定了流动中可能破坏发电机稳定的特定模式。在测量范围内,我们发现可以有一到两个发电机窗口。所有三个分支都在附近产生稳定的发电机,但第一个次优分支可以在大约8倍的时间内产生振荡发电机,并且对于两个次优分支,增长率大约达到饱和。我们发现两个次优分支超临界地创造了一个更鲁棒的发电机作用。
期刊介绍:
Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects.
In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.