Focal mechanism dependence of static stress triggering of earthquakes

We perform a global statistical investigation into the problem of Coulomb stress triggering of earthquakes by using the Harvard CMT catalogue of shallow earthquakes from 1976 to 2001. We consider ‘earthquake pairs’, i.e., pairs of successive earthquakes occurring near each other with similar focal mechanisms, and address the problem of whether or not the change of the Coulomb failure stress (CFS) produced by the first earthquake of the pair ‘encourages’ the occurrence of the second one. An interesting feature is that such a Coulomb stress-triggering phenomenon has an apparent focal mechanism dependence: for thrust earthquakes, a more evident triggering effect can be observed.     

一种地方与区域地震震源机制反演技术:广义极性振幅技术(二)——对实际震例的应用

为了检验广义极性振幅技术(GPAT)的实用性,我们利用GPAT反演确定了49次实际地震的震源机制、矩震级和震源深度.为了检验GPAT对地方地震、区域地震以及远震的实用性,我们选用了震级范围约为ML0.2~MS7.0之间的地震与震中距范围约在5~8000km之间的观测资料.对反演结果的分析表明,利用GPAT获取的震源机制结果在合理误差范围内是正确的,利用GPAT获取的矩震级结果是可靠的,而利用GPAT获取的震源深度总体上似乎比常规定位深度深约0.6km.总体而言,GPAT在震源机制、矩震级和震源深度的反演方面表现出良好的实用性.     

冬季北半球风暴轴的多尺度能量变化特征及其可能机制

基于1971—2016年NCEP/NCAR(美国环境预报中心和国家大气研究中心)的逐日再分析资料及NCPC(美国国家海洋和大气管理局气候预报中心)的海温、大气环流及海洋指数等资料通过多尺度能量分析(MS-EVA)等方法,把冬季北半球风暴轴看做一整体,分析了风暴轴区域多尺度的能量变化特征及其可能机制。主要结论概括如下:(1)多年气候平均状态下,风暴轴的动能来源主要表现为在风暴轴中上游先由低频尺度向天气尺度输送有效位能,随后在风暴轴主体区再由天气尺度有效位能转换为天气尺度动能,其中风暴轴西端可直接由低频尺度向天气尺度输送动能。(2)北半球三大风暴轴联合EOF结果表明:第一模态下,主要体现了北西伯利亚风暴轴与北太平洋风暴轴强度的减弱(增强),同时伴随着北大西洋风暴轴位置北抬(南压);第二模态下,主要体现了北西伯利亚风暴轴强度减弱(增强),同时北太平洋风暴轴位置北抬(南压)中东部强度增强(减弱),而北大西洋风暴轴位置南压(北抬)。(3)回归分析表明:北半球风暴轴异常在不同模态下与低频尺度环流联系密切。低频尺度波动可通过海温及西风急流等异常变化先影响风暴轴区域多尺度间的能量转换,进而影响风暴轴整体的异常变化。     

On the Dynamics of Dust Grains in a Hierarchical Environment

Most main sequence stars are binaries or higher multiplicity Systems and it appears that at birth most stars have circumstellar disks. It is commonly accepted that planetary systems arise from the material of these disks; consequently, binary and multiple systems may have a main role in planet formation. In this paper, we study the stage of planetary formation during which the particulate material is still dispersed as centimetre-to-metre sized primordial aggregates. We investigate the response of the particles, in a protoplanetary disk with radius R_D = 100 AU around a solar-like star, to the gravitational field of bound perturbing companions in a moderately wide (300–1600 AU) orbit. For this purpose, we have carried out a series of simulations of coplanar hierarchical configurations using a direct integration code that models gravitational and viscous forces. The massive protoplanetary disk is around one of the components of the binary. The evolution in time of the dust sub-disk depends mainly on the nature (prograde or retrograde) of the relative revolution of the stellar companion, and on the temperature and mass of the circumstellar disk. Our results show that for binary companions near the limit of tidal truncation of the disk, the perturbation leads to an enhanced accretion rate onto the primary, decreasing the lifetime of the particles in the protoplanetary disk with respect to the case of a single star. As a consequence of an enhanced accretion rate the mass of the disk decreases faster, which leads to a longer resultant lifetime for particles in the disk. On the other hand, binary companions may induce tidal arms in the dust phase of protoplanetary disks. Spiral perturbations with m = 1 may increase in a factor 10 or more the dust surface density in the neighbourhood of the arm, facilitating the growth of the particles. Moreover, in a massive disk (0.01M⊙) the survival time of particles is significantly shorter than in a less massive nebula (0.001M⊙) and the temperature of the disk severely influences the spiral-in time of particles. The rapid evolution of the dust component found in post T Tauri stars can be explained as a result of their binary nature. Binarity may also influence the evolution of circumpulsar disks. This revised version was published online in July 2006 with corrections to the Cover Date.     

塔里木盆地地貌过程对绿洲形成演变的影响

第三纪末以来，天山、昆仑山强烈隆起使塔里木盆地相对下沉，山盆高差悬殊大，白山顶至盆地腹部地貌外力作用过程依次由冰川作用→冰缘作用→流水作用→干燥作用→冲→洪积作用→湖积作用→风沙作用过渡。在山区河谷平原、平原区冲积扇、冲积平原、湖积平原等地方形成条带状、串珠状、扇形状绿洲，绿洲平面几何形状与适宜绿洲形成与发展的地貌类型空间分布基本吻合。绿洲荒漠化和荒漠绿洲化与地貌过程的关系密切。纵观区内地貌过程发展趋势可预测，区内流水、风沙和人类活动三大地貌过程将有增无减，流水侵蚀与风蚀风积作用将对绿洲产生不良作用。山区流水侵蚀过程加强导致山麓地带绿洲山洪泥石流危害加重。平原河流下游地区流水作用减弱，风蚀风积过程加剧，由绿洲→荒漠演变，而人类活动可分建设作用与破坏作用两方面，前者可稳定绿洲乃至促进荒漠绿洲化而后者则导致绿洲荒漠化。因此，改善山区、山麓地带，特别是盆地南缘与塔河中、下游等重要地区地貌过程并防止绿洲荒漠化，是保障区域可持续发展的有效途径。     

珍珠囊发育中马氏珠母贝血清免疫因子的变化规律

马氏珠母贝育珠贝插核手术后的第1、第2、第3、第10、第15、第20、第30和第60天,抽取育珠贝血清,并研究其非特异性免疫因子酸性磷酸酶(ACP)、碱性磷酸酶(AKP)、过氧化氢酶(CAT)、超氧化物歧化酶(SOD)和溶菌酶(LSZ)的活性变化。结果表明:在珍珠囊发育初期(插核后3～10d),育珠贝血清的免疫因子ACP、AKP、CAT、SOD均比对照组(未经插核的马氏珠母贝)显著性增大(P<0.05),LSZ在插核后1～3d比对照组LSZ活性显著性增大(P<0.05);在珍珠囊发育中期(插核后第15～20天),各种免疫酶活性都逐渐降低;珍珠囊发育后期(插核30d后),育珠贝血清中的各种免疫酶活性都已恢复到对照组水平。     

论构造成矿规律及其动力学机制

本文在简述构造成矿学概念的演进之后.着重论述了构造成矿的对称性、等距性、递变性和侧向迁聚性等规律,对构造成矿的动力机制进行了初步分析.作者指出.构造动力成矿作用,是构造应力场、构造地球牾场和构造地球化学场的综合作用;构造成矿过程,是构造运动和成矿物质运动的全过程:是一种不断存在物质交换和能量交换的开放体系中的不可逆过程.构造动力作用能促使成矿元素活化.驱动含矿溶液运移.改变成矿的物理化学条件,导致成矿物质聚集.构造成矿动力学机制的研究.是构造成矿学的关键问題.随着构造成矿学研究的深入发展.逐渐形成了构造成矿学的基础理沦系统.     

双核结构模式形成的自然基础

The dual-nuclei spatial structurs is composed of a regional central city,a port city and their spatial relations in certain regions.In general,this spatial structure could be found in most of the coastal regions or regions along big rivers.In terms of the mechanism,the dual-nuclei structure is the result of the spatial interaction and the complementary characteristics of the center city and the port city.The “marginal function” of the port city and its relationship with the central city has long been discussed in the literature.On the one hand,drainage area is the main natural grographical background of the formation of the dual-nuclei spatial structure;therefore,we can build a theoretical geographic structure that is based on the drainage area.On the other hand,vicissitude of the coastline also has important influence on the formation of the dual-nuclei spatial structure.It is especially meaningful if we can notice this when we examine deeply the research on the spatial structure of delta.     

四川盆地东北部三叠系飞仙关组碳酸盐岩成岩作用和白云岩成因的研究现状和存在问题

四川盆地东北部三叠系飞仙关组是我国重要的天然气储集层，优质储层形成机制直接与碳酸盐岩成岩作用、尤其是白云岩化作用相关，但飞仙关组碳酸盐岩在锰含量、锶含量、阴极发光性等特征上反映其成岩过程与经典成岩理论相悖；碳酸盐岩的锶同位素组成和锰、锶含量的关系也表明与大气水有关的成岩过程和作为重要储集岩的结晶白云岩的形成机制无关，传统的白云岩化机制难以解释结晶白云岩的成因。具有海源色彩的高锶、低锰成岩流体在很大程度上控制了飞仙关组碳酸盐的成岩作用，其来源与成因值得进一步关注，控制其运移、封存和发生水—岩反应的时空机制有待回答。整个海相三叠纪时间段盆地尺度碳酸盐岩和蒸发岩的沉积地球化学研究、尤其是不同结构组分碳酸盐的锶同位素组成、锶和锰含量研究（包括碳酸盐岩中不同结构组分的阴极发光性研究），可为四川盆地东北部飞仙关组碳酸盐岩成岩作用（尤其是白云岩化作用和作为重要储集岩的结晶白云岩的成因研究），天青石矿床成因研究和四川盆地三叠系深层富钾、锶、硼、溴卤水的成因研究提供重要的线索。     

塔里木盆地凝析气田的地质特征及其形成机制

塔里木盆地凝析油气资源丰富,已发现了二十余个凝析气田,包括库车坳陷的陆相油气来源的凝析气田和台盆区海相烃源岩来源的凝析气田;储层有碎屑岩,也有碳酸盐岩;时代自奥陶系至新生代均有分布。这些凝析气田的气油比分布在600~19900m³/m³,凝析油含量40~750g/m³;储层温度在78~155℃;地层压力在37~111MPa。研究认为,塔里木盆地凝析气藏的成因类型可以分为原生凝析气藏和次生凝析气藏。其中,以库车坳陷迪那2凝析气田为代表的煤系烃源岩在高演化阶段(镜质体反射率Ro为1.2%~2.0%),即凝析油和湿气生成带所形成的原生腐植型凝析气藏或煤成型凝析气藏。次生凝析气藏包括两类:陆相油气来源的多期充注,晚期干气对早期油藏发生混合改造,形成了以牙哈为代表的陆相油气成因的次生凝析气藏;以海相油气来源,多期油气充注与晚期干气气侵,造成蒸发分馏,在运移、聚集和成藏过程中烃体系分异、富化,发生反凝析作用,从而导致次生凝析气藏的形成。随着塔里木盆地勘探向深层转化,地层的温度和压力逐渐增高,烃类演化程度的升高,不同生烃阶段的烃体系混合也将更为普遍,次生凝析气藏也将更为普遍,因此,以海相油气来源的次生成因型凝析气藏将成为勘探的主体。