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Dynamos in rotating compressible convection

Dynamos in rotating compressible convection
旋转可压缩对流发电机
批准号:
EP/H006842/1
负责人:
Paul Bushby
金额:
$12.42万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2010
资助国家:
英国
项目状态:
已结题
起止时间:
2010 至 --

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中文摘要
翻译
磁流体发电机理论描述了由于导电流体的运动而产生的磁场再生。发电机有许多物理例子,特别是在天体物理学和天体物理学中,最近的液态金属实验室实验中发现了发电机作用。热对流是驱动许多这些自然发电机的原因,其中绝大多数还取决于旋转的动力学影响。以前大多数关于旋转对流发电机作用的研究都采用了Boussinesq近似,这意味着忽略了层结的影响。通过进行一系列的数值模拟,我们建议调查发电机在旋转可压缩对流的行动,特别是侧重于对流驱动发电机分层后的影响。具体地说,我们将解决的问题,发电机行动在高度超临界可压缩对流是否可以导致大规模磁场的形成(等效Boussinesq发电机未能做到这一点)。我们还将建立是否有一个最佳的旋转速率和分层发电机行动的最佳水平在弱超临界参数制度(接近对流不稳定性的发病)。最后,受Boussinesq对流先前结果的启发,我们将在亚临界参数范围内寻找发电机作用,即在没有磁场的情况下不会发生对流不稳定性的参数空间区域。
英文摘要
Hydromagnetic dynamo theory describes the regeneration of magnetic fields as the result of the motions of an electrically-conducting fluid. There are many physical examples of dynamos, particularly in geophysics and astrophysics, and dynamo action has been found in recent liquid metal laboratory experiments. Thermal convection is responsible for driving many of these natural dynamos, the vast majority of which also depend upon the dynamical influence of rotation. Most previous studies of dynamo action in rotating convection have adopted the Boussinesq approximation, which means (amongst other things) that the effects of stratification are ignored. By carrying out a series of numerical simulations, we propose to investigate dynamo action in rotating compressible convection, focusing particularly upon the effects that stratification has upon convectively-driven dynamos. Specifically, we shall address the question of whether or not dynamo action in highly-supercritical compressible convection can lead to the formation of large-scale magnetic fields (something that equivalent Boussinesq dynamos fail to do). We shall also establish whether there is an optimal rotation rate and an optimal level of stratification for dynamo action in the weakly-supercritical parameter regime (close to the onset of convective instabilities). Finally, motivated by previous results from Boussinesq convection, we will look for dynamo action in the subcritical parameter regime, i.e. a region of parameter space in which no convective instabilities would occur in the absence of a magnetic field.
期刊论文(7)
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会议论文
DOI: 10.1017/jfm.2011.429
发表时间: 2011-10
期刊: Journal of Fluid Mechanics
影响因子: 3.7
作者: [B. Favier;P. Bushby]
通讯作者: B. Favier;P. Bushby
DOI: 10.1017/jfm.2013.132
发表时间: 2013
期刊: Journal of Fluid Mechanics
影响因子: 3.7
作者: [Favier B]
通讯作者: Favier B
Convectively driven dynamo action in the quiet Sun
在安静的阳光下对流驱动的发电机动作
DOI: 10.1080/03091929.2011.638067
发表时间: 2012
期刊: Geophysical & Astrophysical Fluid Dynamics
影响因子: 1.3
作者: [Bushby P]
通讯作者: Bushby P
The Astrophysics Research Programme at Newcastle University
  • 批准号:
    ST/K001019/1
  • 项目类别:
    Research Grant
  • 资助金额:
    $11.61万
  • 财政年份:
    2013
  • 负责人:
    Paul Bushby
  • 依托单位:
Cosmic rays in the multi-phase interstellar medium with dynamo-generated magnetic fields
  • 批准号:
    ST/L005549/1
  • 项目类别:
    Research Grant
  • 资助金额:
    $25.13万
  • 财政年份:
    2013
  • 负责人:
    Paul Bushby
  • 依托单位:
国内基金
海外基金
圆柱形阳极层霍尔等离子体推进器中的Rotating Spoke研究
  • 批准号:
    11275063
  • 项目类别:
    面上项目
  • 资助金额:
    80.0万元
  • 批准年份:
    2012
  • 负责人:
    唐德礼
  • 依托单位: