Accretion discs, Astrophysical dynamos, Planetary formation, Exoplanet systems, Solar and stellar phenomena and non equilibrium physical processes
Accretion discs, Astrophysical dynamos, Planetary formation, Exoplanet systems, Solar and stellar phenomena and non equilibrium physical processes
批准号:
ST/G002584/1
负责人:
John Papaloizou
金额:
$214.79万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2009
资助国家:
英国
项目状态:
已结题
起止时间:
2009 至 --
中文摘要
这是一项研究一些现象的提议:第一个是天体物理盘。这些天体很常见,存在于紧密的双星系统、活动星系核和新形成的恒星周围。在那里它们为行星的形成提供了环境。我们建议对这些物体进行深入研究,以确定适用的物理条件,例如湍流程度、磁场强度、异常传输量以及圆盘是否保持圆形。然后,我们打算研究这种环境对行星形成和轨道迁移的影响。如果向内,这自然会导致考虑与中央恒星的潮汐相互作用,这可能会导致加热和膨胀,这似乎是常见的,甚至与中央恒星合并。这样的研究需要一个我们打算发展的关于一般轨道的完全非线性潮汐理论。第二项研究涉及太阳系外行星围绕其运行的太阳型恒星。因此,它与潮汐相互作用的研究相联系。这项研究旨在了解太阳能发电机的行为以及磁通量如何出现在表面。这可以从活动区的Hinode观测中确定。对发电机过程的分析和数值研究将与改进的太阳跃层模型一起进行,后者可能在产生浮升到地表的环形场方面发挥重要作用。
英文摘要
This is a proposal to investigate a number of phenomena: The first is astrophysical discs. These objects are common, being found in close binary systems, active galactic nuclei, and around newly formed stars. There they provide the environment for planet formation. We propose in depth studies of these objects to establish the physical conditions that apply, for instance the degree of turbulence, the magnetic field strength, the amount of anomalous transport and whether the discs remain circular. We then intend to investigate the effects of this environment on forming planets and their orbital migration. If inward, this natuarlly leads on to a consideration of tidal interaction with the central star which may cause heating and inflation, which appears to be common, or even coallescence with the central star. Such a study requires a fully nonlinear tidal theory for general orbits that we intend to develop. The second investigation relates to solar type stars which many extrasolar planets orbit. It accordingly connects with the investigation of tidal interaction. This investigation is directed towards understanding the behaviour of the solar dynamo and how magnetic flux emerges at the surface. This can be determined from Hinode obsrvations of active regions. Both analytic and numerical studies of dynamo processes will be undertaken together with improved modeling of the solar tachocline which may play an important role in generating toroidal field that rises buoyantly to the surface.
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Stellar and galactic environment survey (SAGE)
恒星和银河环境调查(SAGE)
DOI:
10.1007/s10509-008-9792-9
发表时间:
2008
期刊:
Astrophysics and Space Science
影响因子:
1.9
作者:
[Barstow M]
通讯作者:
Barstow M
MIGRATION OF A MOONLET IN A RING OF SOLID PARTICLES: THEORY AND APPLICATION TO SATURN'S PROPELLERS
固体粒子环中小卫星的迁移:理论及其在土星螺旋桨中的应用
DOI:
10.1088/0004-6256/140/4/944
发表时间:
2010
期刊:
The Astronomical Journal
影响因子:
--
作者:
[Crida A]
通讯作者:
Crida A
A self-consistent treatment of the electromotive force in magnetohydrodynamics for large diffusivities
大扩散率磁流体动力学电动势的自洽处理
DOI:
10.1002/asna.201011358
发表时间:
2010
期刊:
Astronomische Nachrichten
影响因子:
0.9
作者:
[Courvoisier A]
通讯作者:
Courvoisier A
On internal wave breaking and tidal dissipation near the centre of a solar-type star
太阳型恒星中心附近的内波破碎和潮汐耗散
DOI:
10.1111/j.1365-2966.2010.16400.x
发表时间:
2010
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Barker A]
通讯作者:
Barker A
Differential rotation in fully convective stars
全对流恒星中的差分旋转
DOI:
10.1111/j.1365-2966.2010.16380.x
发表时间:
2010
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Balbus S]
通讯作者:
Balbus S
共 10 条
Solar and stellar physics, MHD, astrophysical dynamos, planet formation and processes in galaxy clusters
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批准号:PP/D001072/1
-
项目类别:Research Grant
-
资助金额:$123.73万
-
财政年份:2006
-
负责人:John Papaloizou
-
依托单位:
国内基金
海外基金
果蝇泛素连接酶Hyd (Hyperplastic discs)对Wingless信号通路的调控机理
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批准号:31401235
-
项目类别:青年科学基金项目
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资助金额:24.0万元
-
批准年份:2014
-
负责人:刘淑君
-
依托单位:
基因discs large在果蝇卵母细胞的后端定位及其体轴极性形成中的作用机制
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批准号:30800648
-
项目类别:青年科学基金项目
-
资助金额:20.0万元
-
批准年份:2008
-
负责人:于玲珠
-
依托单位: