Kazantsev dynamo in turbulent compressible flows

Author:

Martins Afonso Marco1,Mitra Dhrubaditya2,Vincenzi Dario3ORCID

Affiliation:

1. Centro de Matemática (Faculdade de Ciências) da Universidade do Porto, Rua do Campo Alegre 687, Porto 4169-007, Portugal

2. Nordita, KTH Royal Institute of Technology and Stockholm University, Stockholm, Sweden

3. Université Côte d'Azur, CNRS, LJAD, Nice 06100, France

Abstract

We consider the kinematic fluctuation dynamo problem in a flow that is random, white-in-time, with both solenoidal and potential components. This model is a generalization of the well-studied Kazantsev model. If both the solenoidal and potential parts have the same scaling exponent, then, as the compressibility of the flow increases, the growth rate decreases but remains positive. If the scaling exponents for the solenoidal and potential parts differ, in particular if they correspond to typical Kolmogorov and Burgers values, we again find that an increase in compressibility slows down the growth rate but does not turn it off. The slow down is, however, weaker and the critical magnetic Reynolds number is lower than when both the solenoidal and potential components display the Kolmogorov scaling. Intriguingly, we find that there exist cases, when the potential part is smoother than the solenoidal part, for which an increase in compressibility increases the growth rate. We also find that the critical value of the scaling exponent above which a dynamo is seen is unity irrespective of the compressibility. Finally, we realize that the dimension d  = 3 is special, as for all other values of d the critical exponent is higher and depends on the compressibility.

Funder

Faculdade de Ciências e Tecnologia, Universidade Nova de Lisboa

Vetenskapsrådet

European Regional Development Fund

Centro de Matemática Universidade do Porto

Publisher

The Royal Society

Subject

General Physics and Astronomy,General Engineering,General Mathematics

Cited by 10 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Simulating small-scale dynamo action in cool main-sequence stars;Astronomy & Astrophysics;2024-03-29

2. Small-scale dynamo with finite correlation times;Physical Review E;2023-06-27

3. Dissipative magnetic structures and scales in small-scale dynamos;Monthly Notices of the Royal Astronomical Society;2022-12-05

4. Fundamental scales in the kinematic phase of the turbulent dynamo;Monthly Notices of the Royal Astronomical Society;2022-04-09

5. Astrophysical Magnetic Fields;CAM ASTROPH;2021-12-23

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3