登陆热带风暴Bilis（2006）暴雨特征及其可能原因   总被引：3，自引：1，他引：2  

滕代高  罗哲贤  代刊  黄新晴 《南京气象学院学报》2008,31(3):369-380

利用NCEP/NCAR 1°×1°格点再分析资料、FY-2C TBB（black bright temperature）资料及中国740站降水资料,对0604号强热带风暴Bilis登陆后的暴雨特征及其可能原因进行诊断分析,结果表明：（1）Bilis登陆过程中强降水中心位于风暴中心西北侧沿岸,主要影响福建和浙江两省;进入内陆后强降水中心向风暴中心以西转移,最后在风暴中心西南侧聚集,主要影响广东东北部、福建、江西和湖南南部。（2）西北太平洋副热带高压的稳定少动为Bilis陆上西行过程中产生持续性降水提供了稳定的背景场。（3）Bilis西南部季风环流的发展增强为Bilis登陆后强降水的产生提供了必要的水汽条件。（4）涡合并和自激增长形成的中尺度系统与风暴涡旋的相互作用,是Bilis登陆后产生强降水的可能机制。  相似文献   

The influence of obliquity on europan cycloid formation     

T.A. Hurford  A.R. Sarid  B.G. Bills 《Icarus》2009,202(1):197-215

Tectonic patterns on Europa are influenced by tidal stress. An important well-recognized component is associated with the orbital eccentricity, which produces a diurnally varying stress as Jupiter's apparent position in Europa's sky oscillates in longitude. Cycloidal lineaments seem to have formed as cracks propagated in this diurnally varying stress field. Maps of theoretical cycloid patterns capture many of the characteristics of the observed distribution on Europa. However, a few details of the observed cycloid distribution have not been reproduced by previous models. Recently, it has been shown that Europa has a finite forced obliquity, so Jupiter's apparent position in Europa's sky will also oscillate in latitude. We explore this new type of diurnal effect on cycloid formation. We find that stress from obliquity may be the key to explaining several characteristics of observed cycloids such as the shape of equator-crossing cycloids and the shift in the crack patterns in the Argadnel Regio region. All of these improvements of the fit between observation and theory seem to require Jupiter crossing Europa's equatorial plane 45° to 180° after perijove passage, suggestive of complex orbital dynamics that locks the direction of Europa's pericenter with the direction of the ascending node at the time these cycloids were formed.  相似文献   

The interior structure of Mercury and its core sulfur content     

A. Rivoldini  T. Van Hoolst  O. Verhoeven 《Icarus》2009,201(1):12-30

Depth-dependent interior structure models of Mercury are calculated for several plausible chemical compositions of the core and of the mantle. For those models, we compute the associated libration amplitude, obliquity, tidal deformation, and tidal changes in the external potential. In particular we study the relation between the interior structure parameters for five different mantle mineralogies and two different temperature profiles together with two extreme crust density values. We investigate the influence of the core light element concentration, temperature, and melting law on core state and inner and outer core size. We show that a sulfur concentration above 10 wt% is unlikely if the temperature at the core-mantle boundary is above 1850 K and the silicate shell at least 240 km thick. The interior models can only have an inner core if the sulfur weight fraction is below 5 wt% for core-mantle boundary temperature in the 1850-2200 K range. Within our modeling hypotheses, we show that with the expected precision on the moment of inertia the core size can be estimated to a precision of about 50 km and the core sulfur concentration with an error of about 2 wt%. This uncertainty can only be reduced when more information on the mantle mineralogy of Mercury becomes available. However, we show that the uncertainty on the core size estimation can be greatly reduced, to about 25 km, if tidal surface displacements and tidal variations in the external potential are considered.  相似文献   

On the homeostasis and bistability on a Gaian planet     

Peter Nørtoft Nielsen 《Planetary and Space Science》2009,57(4):491-497

Geochemical disequilibrium of Earth's atmosphere is a sign of life. The fact that Earth's atmosphere is just right for life led Lovelock to propose the Gaia hypothesis: life itself regulates the environment on planetary scale in order to maintain habitability. This hypothesis is supported by the so-called Daisyworld parable, which illustrates a possible mechanism for such a self regulation. Here we revisit Daisyworld and challenge some of its conclusions from a closer examination of the model. We find that even within this simple, conceptual model of a Gaian planet there are regimes where climate is less homeostatic than on a dead planet. Furthermore, in other regimes, bistability between two climate states is found to exist due to the presence of life. This indicates that even if the Gaian stability might describe life in some planetary conditions, it need not be generic to all inhabited planets.  相似文献   

A numerical study of the orbits of second species of the planar circular RTBP     

Joaquim Font  Ana Nunes  Carles Simó 《Celestial Mechanics and Dynamical Astronomy》2009,103(2):143-162

We present a numerical study of the set of orbits of the planar circular restricted three body problem which undergo consecutive close encounters with the small primary, or orbits of second species. The value of the Jacobi constant is fixed, and we restrict the study to consecutive close encounters which occur within a maximal time interval. With these restrictions, the full set of orbits of second species is found numerically from the intersections of the stable and unstable manifolds of the collision singularity on the surface of section that corresponds to passage through the pericentre. A ‘skeleton’ of this set of curves can be computed from the solutions of the two-body problem. The set of intersection points found in this limit corresponds to the S-arcs and T-arcs of Hénon’s classification which verify the energy and time constraints, and can be used to construct an alphabet to describe the orbits of second species. We give numerical evidence for the existence of a shift on this alphabet that describes all the orbits with infinitely many close encounters with the small primary, and sketch a proof of the symbolic dynamics. In particular, we find periodic orbits that combine S-type and T-type quasi-homoclinic arcs.  相似文献   

Artificial halo orbits for low-thrust propulsion spacecraft     

Shahid Baig  Colin R. McInnes 《Celestial Mechanics and Dynamical Astronomy》2009,104(4):321-335

We consider periodic halo orbits about artificial equilibrium points (AEP) near to the Lagrange points L ₁ and L ₂ in the circular restricted three body problem, where the third body is a low-thrust propulsion spacecraft in the Sun–Earth system. Although such halo orbits about artificial equilibrium points can be generated using a solar sail, there are points inside L ₁ and beyond L ₂ where a solar sail cannot be placed, so low-thrust, such as solar electric propulsion, is the only option to generate artificial halo orbits around points inaccessible to a solar sail. Analytical and numerical halo orbits for such low-thrust propulsion systems are obtained by using the Lindstedt Poincaré and differential corrector method respectively. Both the period and minimum amplitude of halo orbits about artificial equilibrium points inside L ₁ decreases with an increase in low-thrust acceleration. The halo orbits about artificial equilibrium points beyond L ₂ in contrast show an increase in period with an increase in low-thrust acceleration. However, the minimum amplitude first increases and then decreases after the thrust acceleration exceeds 0.415 mm/s². Using a continuation method, we also find stable artificial halo orbits which can be sustained for long integration times and require a reasonably small low-thrust acceleration 0.0593 mm/s².  相似文献   

Trees, lateral shrinkage and building damage     

Vicente Navarro  Miguel Candel  ngel Yustres  Juan Alonso  Beatriz García 《Engineering Geology》2009,108(3-4):189-198

This article presents the study conducted and the actions taken to stabilise the foundations of 25 low-rise (two/three-storey) buildings in Alcázar de San Juan (Ciudad Real, central Spain). Owing to the immediate attention required, it was decided that the study would focus on procuring a synthetic model that would be able to provide a satisfactory explanation for the tendency of the movements, overlooking the detailed model of each building. This analysis pointed out that the mobilisation was probably due to both the shrinkage caused by the existing trees during the dry-growing seasons, and to the loss of lateral confinement caused by the excavation of a service trench adjacent to the footings of the buildings. In keeping with this mechanism, stabilization was carried out by transplanting the trees growing near the damaged buildings and installing a line of piles to provide lateral support to the footings. The evolution of the damage was therefore stopped.  相似文献   

云南剑川金河岩体中地幔流体交代特征及其成矿意义   总被引：5，自引：0，他引：5  

刘显凡  赵甫峰  陶专  宋祥峰  蔡永文  蔡飞跃 《矿床地质》2009,28(2):185-194

云南剑川金河岩体中的硅化霓辉正长斑岩含有较多的镁铁-超镁铁质深源岩石包体.岩相学研究表明,伴随交代蚀变,其主岩和各类包体岩石中普遍发育沿矿物粒间和矿物晶体裂隙或解离纹贯入或穿插的呈网状和细脉浸染状分布的黑色不透明物质.对该物质进行了电子探针及扫描电镜和能谱分析,发现其组成以微晶硅酸盐矿物为主,含少量微晶石英,尤其是含有微晶地幔标型矿物--含钛磁铁矿(或镜铁矿)和含铬自然铁;后两者与硅酸盐矿物构成超显微熔离结构交生.研究认为,这种物质组成和特征,是具超临界和熔浆性质的地幔流体的微观表现,其活动所引发的交代蚀变表现为硅化、钠化及深源包体中的暗色矿物由辉石→角闪石→黑云母的退变序列.这一地幔流体作用微观踪迹的揭示,对于分析和论证滇西地区新生代多金属成矿的深部地质作用规律具有重要的理论和现实意义.  相似文献   

东秦岭金堆城大型斑岩钼矿床同位素及元素地球化学研究   总被引：9，自引：2，他引：7  

郭波  朱赖民  李犇  许江  王建其  弓虎军 《矿床地质》2009,28(3):265-281

文章系统研究了金堆城钼矿床的含矿钾长斑岩、围岩、矿石、矿石中的黄铁矿及矿化围岩的地球化学特征,深入探讨了矿区成矿物质的来源.金堆城含矿斑岩的稀土元素分布和特征地球化学参数显示,金堆城含矿斑岩富集LREE(LaN/YbN=540～1684),轻、重稀土元素分馏较明显,Eu异常不明显或无Eu异常(δEu=070～096).矿石中黄铁矿富集LREE(LaN/YbN=315～2628),具有弱的Eu负异常,无Ce异常(δEu=064～081, δCe=088～103),并与金堆城含矿钾长斑岩和矿石具有一致的球粒陨石标准化配分曲线和特征的地球化学参数,显示金堆城钼矿床的成矿物质来源与钾长斑岩同源.矿床铅、硫、碳和氢-氧同位素地球化学综合研究表明,成矿物质来源于深部,与钾长斑岩同源.围岩在矿化和蚀变过程中元素的迁移计算结果表明,在热液成矿过程中Mo随成矿流体加入到围岩并使围岩发生蚀变和矿化.钼矿床的成矿物质主要来自钾长斑岩,围岩不提供成矿物质.金堆城含矿斑岩和钼矿化的发生处于秦岭造山带在中新生代的挤压-伸展转变期,受板片断离作用和壳幔边界附近发生的基性岩浆底侵作用影响,加厚的华北地块南缘下地壳物质发生熔融形成花岗质岩浆,并沿构造薄弱带上升到浅部侵位,形成金堆城等同熔型斑岩和斑岩型矿床.  相似文献   

铁矿床深部矿体定位预测的一种新途径 ———以西藏恰功铁矿为例   总被引：2，自引：0，他引：2  

李志华 《地质与勘探》2009,45(2):90-97

恰功铁矿是近几年新发现的矿山,矿体的形态、大小、位置、产状、边界等几何特征还没有清楚的认识,为了弄清这些问题,文章首先通过小渡多尺度分析方法将恰功铁矿磁异常资料进行了位场信号分离,然后应用欧拉反褶积方法反演了异常与其场源深度的对应定量关系,最后把位场分离后的异常场源深度叠加起来,就可以对矿山深部找矿提供一种全新的思路.  相似文献