0907号热带风暴“天鹅”登陆后异常路径和陆上维持机制的诊断分析

2009年第7号热带风暴"天鹅"在广东省台山沿海登陆,登陆后在粤西上空长时间停留、强度维持,后期路径异常,针对这几方面在预报上的难点进行分析。结果表明:热带气旋在陆上长时间维持与低空水汽通道的连结,高空弱的风场切变有关;热带风暴后期路径第一次西南转向是由于周围环境流场出现变化转向西南的,第二次路径再次产生转向,是受到离它较近的台风"莫拉克"的牵引作用,另外,925 hPa附近θse的高值区或高能轴也可意示"天鹅"的趋向。     

高温海水钻井液现状及关键技术研究

在重点介绍国内外抗高温海水钻井液处理剂及钻井液体系的研究与应用情况的基础上,提出了几点针对高温海水钻井液未来研究方向的建议,抗200 ℃以上抗盐关键处理剂（如抗盐降滤失剂、增粘剂、防塌抑制剂、润滑剂等）、海水体系、检测仪器、高温环保等是超高温海水钻井液技术研究的方向。     

Formation mechanism for the anomalous anticyclonic circulation over Northeast Asia and the Japan Sea in boreal winter 1997/98 and the spring of 1998

A robust anomalous anticyclonic circulation (AAC) was observed over Northeast Asia and the Japan Sea in boreal win-ter 1997/98 and over the Japan Sea in spring 1998. The formation mechanism is investigated. On the background of the vertically sheared winter monsoonal flow, anomalous rainfall in the tropical Indo-Western Pacific warm pool excited a wave train towards East Asia in the upper troposphere during boreal winter of 1997/98. The AAC over Northeast Asia and the Japan Sea is part of the wave train of equivalent barotropic structure. The AAC over the Japan Sea persisted from winter to spring and even intensified in spring 1998. The diagnostic calculations show that the vorticity and temperature fluxes by synoptic eddies are an important mechanism for the AAC over the Japan Sea in spring 1998.     

基于频变AVO技术对多尺度裂缝内流体属性反演与识别（英文）

通过地震数据获取裂缝储藏中流体的性质并对流体类型进行识别,是地震勘探岩性反演的重要问题之一。由于地震波的速度、储层的密度等弹性参数对某些流体不具有很强的敏感性,使只依赖振幅信息进行流体识别的传统AVO方法面临困境。作为传统叠前振幅反演的一个拓展,频变AVO（FDAVO）技术进一步考虑了振幅对频率的依赖关系,将这种依赖关系与地下裂缝结构、流体填充对应起来,能带来更丰富的流体信息。利用该技术,本文提出了一种基于地震数据参数化Chapman模型的贝叶斯反演新方法（BIDCMP）,它包含两步算法,即,FDAVO反演储层的非弹性属性和贝叶斯框架下的流体识别。首先,通过匹配观测数据和模型数据,构造差函数反演裂缝储层非弹性参数。随后,在贝叶斯框架下,使用马尔科夫随机场（MRF）作为先验模型,联合多参数场识别流体。本方法在计算过程中,除综合考虑了弹性参数场、测井资料等常规信息外,还特别地加人了第一步中反演得的非弹性参数的约束,从而充分利用了流体粘性差异,最后在最大后验概率（MAP）准则下输出最佳岩性一流体识别结果。分别对合成地震记录和模拟岩性—流体剖面验证本文方法的有效性,结果证明本文方法获得的流体识别结果准确可信。     

石嘴山地震台伸缩仪典型异常图像及形成原因浅析

通过对石嘴山台伸缩仪2008年至今资料的分析,绘制一系列典型异常图像,主要从自然、仪器、人为、不明原因等四方面简要总结了各种干扰的形成原因,此外从同震记录方面分析总结了伸缩仪典型异常图像形成的机理。     

临汾地震台数字水平摆曲线畸变与地震关系

对记录到的震前典型畸变图像进行分类,对未来准确利用观测资料识别震兆,研究中强地震具有一定的参考意义.     

Can zonally symmetric inertial waves drive an oscillating zonal mean flow?

In the present paper zonal mean flow excitation by inertial waves is studied in analogy to mean flow excitation by gravity waves that plays an important role for the quasi-biennial oscillation in the equatorial atmosphere. In geophysical flows that are stratified and rotating, pure gravity and inertial waves correspond to the two limiting cases: gravity waves neglect rotation, inertial waves neglect stratification. The former are more relevant for fluids like the atmosphere, where stratification is dominant, the latter for the deep oceans or planet cores, where rotation dominates. In the present study a hierarchy of simple analytical and numerical models of zonally symmetric inertial wave-mean flow interactions is considered and the results are compared with data from a laboratory experiment. The main findings can be summarised as follows: (i) when the waves are decoupled from the mean flow they just drive a retrograde (eastward) zonal mean flow, independent of the sign of the meridional phase speed; (ii) when coupling is present and the zonal mean flow is assumed to be steady, the waves can drive vertically alternating jets, but still, in contrast to the gravity wave case, the structure is independent of the sign of the meridional phase speed; (iii) when coupling is present and time-dependent zonal mean flows are considered the waves can drive vertically and temporarily oscillating mean flows. The comparison with laboratory data from a rotating annulus experiment shows a qualitative agreement. It appears that the experiment captures the basic elements of the inertial wave mean flow coupling. The results might be relevant to understand how the Equatorial Deep Jets can be maintained against dissipation, a process currently discussed controversially.     

辽宁榛子沟铅锌矿床热液叠加成矿作用特征及成矿流体来源

榛子沟铅锌矿矿床是青城子矿田代表性矿床之一,矿体赋存于高家峪组和大石桥组之中,呈层状、似层状和脉状产出,受地层、岩浆和构造联合控制。矿床的形成经历了海底喷流、变质变形和热液叠加三期成矿作用,其中热液叠加成矿作用对脉状矿体的形成与层状矿体的局部热液改造起到了重要作用,可划分为Ⅰ黄铁矿-方铅矿-闪锌矿-石英和Ⅱ黄铁矿-方铅矿-石英-方解石两个阶段。流体包裹体和碳、氢、氧同位素研究表明:I阶段石英中发育气液两相和少量的富气相、CO₂三相流体包裹体,成矿流体属中高温、低盐度、低密度的CO₂-H₂O-NaCl体系热液,含H₂O、CO₂、CH₄和N₂,流体包裹体的δD_H2O-SMOW为-96.5‰和-95.4‰、δ¹⁸O_H2O-SMOW为-0.62‰和0.04‰、δ¹³C为-4.8‰和-4.4‰,具有大气降水与岩浆水混合流体的特点;Ⅱ阶段石英中主要发育气液两相包裹体,成矿流体属低温、低盐度和低密度的H₂O-NaCl体系热液,流体包裹体δD_H2O-SMOW为-88.4‰~-80.0‰、δ¹⁸O_H2O-SMOW为-7.93‰~-5.57‰,具有大气降水的特点,δ¹³C为-12.6‰~-7.9‰,具有岩浆水特点。综合分析表明,热液叠加成矿期成矿流体来源于岩浆水与大气降水的混合热液,且成矿后期大气降水的混入比例增加。     

On the nature,formation and diversity of particulate coherent structures in microgravity conditions and their relevance to materials science and problems of astrophysical interest

Different phenomena related to the spontaneous accumulation of solid particles dispersed in a fluid medium in microgravity conditions are discussed, with an emphasis on recent discoveries and potential links with the general field of astrophysical fluid-dynamics on the one hand, and with terrestrial applications in the field of materials science on the other hand. With special attention to the typical physical forces at play in such an environment, namely, surface-tension gradients, oscillatory residual gravity components, inertial disturbances and forces of an electrostatic nature, specific experimental and numerical examples are presented to provide inputs for an increased understanding of the underlying cause-and-effect relationships. Studying these systems can be seen as a matter of understanding how macroscopic scenarios arise from the cooperative behaviour of sub-parts or competing mechanisms (nonlinearities and interdependencies on various spatial and temporal scales). Through a critical assessment of the properties displayed by the resulting structures (which appear in the form of one-dimensional circuits formed by aligned particles, planar accumulation surfaces, three-dimensional compact structures resembling “quadrics”, micro-crystallites or fractal aggregates), we discuss a possible classification of the related particle attractors in the space of parameters according to the prevailing effect.     

四川牦牛坪稀土矿床地幔流体成矿的碳、氢、氧、硫同位素证据

选取2种主要矿石类型——碳酸岩伟晶岩型矿石和重晶石伟晶岩型矿石进行了成矿流体的C、H、O、S同位素测试，获得δ^13CV-PDB值为-3．0‰～-5．6‰，δDV-SMOW值为-57‰～-88‰，δ^18OH2O-VSMOW值为8．0‰～13．3‰，δ^34SV-CDT值为3．3‰～5．9‰，以及方解石的δ^13CV-PDB值为-6．9‰和δ^18OV-SMOW值为7．3‰～7．4‰。所有这些数据表明，四川牦牛坪稀土矿床在成矿过程中有大量地幔物质参与。