相对论多方球的稳定性

本文从理论的角度，讨论了静态相对论多方球的稳定性问题，给出稳定性对球体物质的绝热指数的依赖关系．     

地形动力作用对华北暴雨和云系影响的数值研究

为了进一步研究地形对华北暴雨的影响,本文从云微物理学的角度出发,选取了2005年7月22～24日的一次华北暴雨过程为研究对象,利用中尺度数值模式ARPS,通过地形高度敏感性试验,详细讨论了地形高度变化对流场、云及降水微物理过程的影响.结果表明:地形高度变化对水平和垂直流场的大小和分布都有较大影响;地形高度增加有利于迎风坡附近水平风场辐合和垂直上升运动发展,这对云的垂直和水平发展影响都很大,尤其是对中高层云的发展影响最明显,并且能明显扩大地面降水的分布范围,地面最大降水量也有所增多.这主要是由于地形高度增加后能促进中高层云水的产生,尤其是零度层之上的过冷云水含量的增多,这大大促进了冰相粒子(雪和霰)的增多,从而使得以冷云过程为主的此次降水过程中,冰相粒子融化形成的雨水含量增多.虽然地形高度的增加会抑制云系发展前期的暖云过程,但对冷云过程有持续加强作用,而且不会明显改变云内降水的形成机制,冷云过程依然是降水的最大贡献项,总体上促进了云和降水的发展.     

A search for infrared stellar objects in Vela

In a search for infrared excess objects near the galactic plane, a star field of 28.5 square degrees in Vela has been measured on UK Schmidt plates R4272 and 14183 with the Cosmos machine at Royal Observatory, Edinburgh. The magnitude limit is around 20 in R and around 19 in I. 131 infrared excess objects with colour index R-I > 2.5 are discovered in the field, and 3 red stellar objects have been identified as the optical counterparts of IRAS point sources.     

Periodic orbits based on geometric structure of center manifold around Lagrange points

This study proposes an analytical method that determines the center manifold and identifies the reduced system on the center manifold. The proposed method expresses the center manifold through general equations containing only state variables, and not functions with respect to time. This is the so-called geometric structure of the center manifold. The location of periodic or quasi-periodic orbits is identified after the geometric structure of the center manifold is determined. The reduced system on the center manifold is described using ordinary differential equations, so that periodic or quasi-periodic orbits can be computed by numerically integrating the reduced system. The results indicate that the analytical method proposed in this study has higher precision compared with the Lindstedt-Poincaré method of the same order.     

兴隆60 cm望远镜主焦CCD系统测光性能的研究

对兴隆６０ｃｍ望远镜主焦ＣＣＤ系统的测光性能进行了测试和研究．测定了ＣＣＤ快门时间函数,讨论了快门延迟效应对短时间曝光观测的可能影响．通过观测大批Ｌａｎｄｏｌｔ标准星,较准确地定出了ＢＶＲＩ宽带测光的星等系统转换关系,结果表明本系统与标准ＢＶＲＩ系统很接近．对ＣＣＤ系统的天文测光精度作了仔细的检验和分析,并对ＰＳＦ拟合测光和孔径测光两种方法进行了比较     

准噶尔盆地深层致密油储层特征及致密化成因——以莫索湾—莫北地区侏罗系八道湾组为例

综合利用岩心、岩石薄片、扫描电镜及测井等资料,对准噶尔盆地莫索湾—莫北地区侏罗系八道湾组致密油储层特征及其致密化成因进行研究。结果表明:八道湾组储层为低—特低孔、低—特低渗储层,属典型的深层致密砂岩储层;储层砂体主要为三角洲前缘水下分流河道细砂岩、中—细砂岩,成分成熟度低,具有岩屑和塑性岩屑含量高及胶结物含量低的"两高一低"特征;垂向上以4 100和4 500m为界,可划分为减小原生孔、稳定混合孔及增加次生孔3个孔隙演化带;孔隙主要为中—小孔,孔喉类型以分选较差的中-细孔—细喉型为主,连通性和渗流能力相对较差,结构相对较差。储层致密化主要受控于沉积环境相对稳定性、岩石主要成分、储层埋藏深度及胶结物赋存状态4个因素,构成了致密化的背景、内因和外因;相对稳定的沉积环境、低成分成熟度、高岩屑和塑性岩屑含量、储层埋深大、压溶作用大量减孔,以及不同类型胶结物以4种状态充填孔喉,形成了八道湾组致密储层。     

NanoSIMS analysis of organic carbon from the Tissint Martian meteorite: Evidence for the past existence of subsurface organic‐bearing fluids on Mars

Two petrographic settings of carbonaceous components, mainly filling open fractures and occasionally enclosed in shock‐melt veins, were found in the recently fallen Tissint Martian meteorite. The presence in shock‐melt veins and the deuterium enrichments (δD up to +1183‰) of these components clearly indicate a pristine Martian origin. The carbonaceous components are kerogen‐like, based on micro‐Raman spectra and multielemental ratios, and were probably deposited from fluids in shock‐induced fractures in the parent rock of Tissint. After precipitation of the organic matter, the rock experienced another severe shock event, producing the melt veins that encapsulated a part of the organic matter. The C isotopic compositions of the organic matter (δ¹³C = ?12.8 to ?33.1‰) are significantly lighter than Martian atmospheric CO₂ and carbonate, providing a tantalizing hint for a possible biotic process. Alternatively, the organic matter could be derived from carbonaceous chondrites, as insoluble organic matter from the latter has similar chemical and isotopic compositions. The presence of organic‐rich fluids that infiltrated rocks near the surface of Mars has significant implications for the study of Martian paleoenvironment and perhaps to search for possible ancient biological activities on Mars.