A comparison of local simulations and reduced models of MRI-induced turbulence

We run mean-field shearing-box numerical simulations with a temperature-dependent resistivity and compare them to a reduced dynamical model. Our simulations reveal the co-existence of two quasi-steady states, a 'quiet' state and an 'active' turbulent state, confirming the predictions of the reduced model. The initial conditions determine on which state the simulation ultimately settles. The active state is strongly influenced by the geometry of the computational box and the thermal properties of the gas. Cubic domains support permanent channel flows, bar-shaped domains exhibit eruptive behaviour, and horizontal slabs give rise to infrequent channels. Meanwhile, longer cooling time-scales lead to higher saturation amplitudes.     

Preliminary Analysis of Photometric Variations of the Central Star of the Planetary Nebula Sh 2-71

We confirm the presence of regular UBV(RI)_C light variations of the object in the center of the planetary nebula Sh 2-71, with an improved period of P = 68.132 ± 0.005 days. The shapes and amplitudes of light curves, in particular colours, are briefly discussed.     

冲击反循环工程钻机自动同步机构的原理

采用行星齿轮差速机构作为ＧＣＦ－１５００型冲击反循环工程钻机的自动同步机构，已经获得成功。分析了该机构的运动学原理和力平衡原理。该机构具有结构简单、工作可不的特点。     

热带东风急流显著偏强和偏弱期平流层绕极反气旋及波动的差异

首先采用150～100 hPa气层20 °W～180 °,15 °S～35 °N区域的平均东风和单位面积东风贡献的动能两种办法定义了热带东风急流(TEJ)指数,并分析了1948—2010年TEJ随时间的变化。然后利用谐波分析方法分析了急流显著偏强和偏弱期平流层10 hPa绕极反气旋和波动的差异。分析表明,在急流显著偏强期平流层10 hPa 40 °N以北的绕极反气旋偏弱,而急流显著偏弱期则偏强,差值约为100～150位势米。45 °N以北1波占绝对优势,1波从春到夏的季节转换与TEJ的快速发展紧密相连,急流显著偏强期1波的季节性调整早于显著偏弱期。急流显著偏强和偏弱期相比,极区65～85 °N 1波平均槽脊位置有较大差异。45～60 °N纬带1波在急流显著偏强期振幅明显加强,变化相对稳定,而急流显著偏弱期1波振幅和位相的变化要强烈得多。      

M型恒星周围系外行星统计研究

M型恒星(M dwarf)是主序星中质量较小的恒星,也是银河系中数量最多的恒星类型,在其周围形成的行星通常距离主星较近,宜居带也比F、G、K型恒星更靠近主星,更有利于发现系外宜居行星.研究表明, M型恒星周围平均存在2.5颗小质量行星,约为F、 G、 K型恒星的3.5倍,但M型恒星周围巨行星的出现率(occurrence rate)则比F、 G、K型小一个量级.基于M型恒星周围发现的401颗行星的参数开展了统计研究,发现质量越大的行星平均轨道半长径越大.类地行星约占行星总数的74%,且轨道半长径均小于1 au,其中28颗行星具有潜在宜居性.根据行星质量-半径关系,在质量等于4倍地球质量(M⊕)处存在一拐点,除少数几颗行星外,大部分小于该质量的行星可能都是由约65%的硅酸盐和约35%的铁组成,大于该质量的行星半径则随质量增加而迅速增大.约60%的M型恒星周围的行星位于多行星系统且轨道分布紧密,相邻行星轨道在3:2、5:3及2:1等平运动共振位置处存在峰值. M型恒星的多行星系统形成与演化等问题对现今的行星形成理论提出了新挑战.     

Late Eocene pollen records and palaeoenvironmental changes in northern Tibetan Plateau

The Eocene palaeovegetation landscape and palaeoclimate reconstructed from the pollen records in the Jiuquan Basin, northwest China provide some important information on the early uplift of the Tibetan Plateau and the origin and evolution of the aridification in northwest China. The records show the arid-semiarid scrubs with open forest palynofloras controlled by the subtropical high existed in northwest China during the 40.2–33.4 Ma. Four pollen assemblages are found: Nitrariadites-Cheno-podipollis-Pinaceae assemblage (40.2–37.9 Ma) is followed by Chenopodipollis-Nitrariadites assemblage (37.9–34.6 Ma), Pinuspollenites & Abietineaepollenites-Chenopodipollis assemblage (34.6–33.9 Ma), and Chenopodipollis-Nitrariadites assemblage (33.9–33.4 Ma). The percentage of thermophilic types is in anti-correlation with that of the dry types, which means the palaeoclimate is relatively warm-wet or cold-dry during most of that time. Such aridity may be related to the water vapor reduction and the planetary wind system movement northward in response to the cooling caused by small-ephemeral ice-sheets. Supported by the National Key Program for Developing Basic Sciences (Grant No. 2005CB422001), the National Science Foundation of China (Grant Nos. 40334038, 40421101) and the President Fund of Chinese Academy of Sciences     

移动性热岛边界层特征的数值研究

用二维非静力完全弹性的中－γ尺度数值模式模拟了移动性热岛的大气边界层特征。试验中，热岛移速取为４ｍ·ｓ＾－１，热岛强度取△θｇ＝６０Ｋ和３０Ｋ两种。△θｇ＝６０Ｋ时，在热岛后方出现了强烈的垂直运动并形成了水平尺度为３－５ｋｍ的局地环流，最大上升速度１００ｃｍ·ｓ＾－１，出现在低层３００－４００ｍ高度；△θｇ＝３０Ｋ时，移动热岛的边界效应比前大为减弱，且不再出现闭合的局地环流。     

适用于GRAPES模式C-P边界层方案的设计和实现

基于K廓线闭合方案,通过考虑不稳定边界层和稳定边界层中热量交换系数在半层上求取及下边界条件的设置,将温湿倾向在整层上直接计算,设计了Charney-Phillips跳点（简称C-P跳点）的边界层方案,使之与GRAPES全球模式的C-P跳点相协调,解决了Lorenz跳点物理过程与C-P跳点动力框架耦合时插值造成的不协调问题,同时避免了耦合时反复插值造成的误差,提高了边界层物理过程参数化方案及其反馈的准确性和合理性。试验表明:C-P跳点边界层方案因为避免了温度和湿度在垂直方向上的插值,消除了温湿变量在垂直方向上的锯齿状抖动,使温湿廓线分布更合理,减小了模式预报误差,形势场的预报效果也得到一定改善。C-P边界层方案的应用提升了GRAPES全球模式的总体预报性能。