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Rapidly Rotating Lenses: Repeating features in the lightcurves of short period binary microlenses
gravitational lensing: micro – celestial mechanics – binaries: general –planetary systems – Galaxy: bulge
2011/9/29
Microlensing is most sensitive to binary lenses with relatively large orbital separations, and as such, typical binary microlensing events show little or no orbital motion during the event. However, d...
Rossby waves and polar spots in rapidly rotating stars: Implications for stellar wind evolution
magnetic fi eld – Stars: activity – Stars: starspots – Stars: oscillations – Physical data and processes: Magnetohydrodynamics
2011/10/10
Rapidly rotating stars show short-period oscillations in magnetic activity and polar appearance of starspots. The aim of this paper is to study large-scale shallow water waves in the tachoclines of ra...
Modeling of differential rotation in rapidly rotating solar-type stars
Modeling differential rotation rapidly rotating solar-type stars
2011/10/9
We investigate differential rotation in rapidly rotating solar-type stars by means of an axisymmetric mean field model that was previously applied to the sun. This allows us to calculate the latitudin...
Global magnetic cycles in rapidly rotating younger suns
Global magnetic cycles rapidly rotating younger suns
2011/1/13
Observations of sun-like stars rotating faster than our current sun tend to exhibit increased magnetic activity as well as magnetic cycles spanning multiple years. Using global simulations in spherica...
Rotation and differential rotation in rapidly rotating field stars
differential rotation rapidly rotating field stars
2011/1/13
We continue our studies on stellar latitudinal differential rotation. The presented work is a sequel of the work of Reiners et al. who studied the spectral line broadening profile of hundreds of stars...
Persistent Magnetic Wreaths in a Rapidly Rotating Sun
convection – MHD – stars:interiors – stars rotation – stars magnetic fields – Sun:interior
2010/11/15
When our Sun was young it rotated much more rapidly than now. Observations of young, rapidly rotating stars indicate that many possess substantial magnetic activity and strong axisymmetric magnetic fi...
Rossby-wave turbulence in a rapidly rotating sphere
Rossby-wave turbulence rapidly rotating sphere
2009/11/11
We use a quasi-geostrophic numerical model to study the turbulence of rotating flows in a sphere, with realistic Ekman friction and bulk viscous dissipation. The forcing is caused by the destabilizati...
Topological Numbers and Edge State of Hierarchical State in Rapidly
Rotating Ultracold Atoms
edge state topological number
2007/8/15
2005Vol.43No.2pp.225-228DOI:
Topological Numbers and Edge State of Hierarchical State in Rapidly
Rotating Ultracold Atoms
ZHAO Bo and CHEN Zeng-Bing
Department of Moder...
专著信息
书名
A new asymptotic method for the analysis of convection in a rapidly rotating sphere
语种
英文
撰写或编译
作者
Zhang Keke,Xinhao Liao
第一作者单位
出版社
Journal of Fluid Mechanics, 2004,Vol. 504: 327-340
出版地
出版日期...
期刊信息
篇名
Convective instability in a rapidly rotating fluid layer layer in the presence of a non-uniform magnetic field
语种
英文
撰写或编译
作者
陈出新,郭孝城
第一作者单位
刊物名称
力学学报
页面
19(6)，527-534, 2003.
出版日期
2003年
月
日
文章...