凡纳对虾引进亲本及其子代对也P分析

运用PCR-RFIJ技术分析凡纳对虾两个引进亲本群体及其各自子一代的遗传变异情况。用一对引物对这四个群体进行mtDNA-细胞色素氧化酶Ⅰ部分片段的PCR扩增，扩增结果为一条约1．25kb的条带。用19种限制性内切酶对该扩增条带进行酶切分析，其中HinfⅠ，StyⅠ，TaqⅠ这3种酶有酶切位点。用这3种酶进行限制性片段长度多态性(RFlP)分析，共获得2种限制性类型(基因型)。而且内切酶StyⅠ在两个不同的引进亲本群体及其各自的子一代的扩增产物的酶切中，表现出明显的差异。     

大气对外强迫低频遥响应的数值模拟 Ⅰ:对赤道东太平洋SSTA的响应

本文通过在IAP-GCM上实现的数值模拟,研究了大气对赤道东太平洋地区暖SSTA的响应,着重讨论了大气遥响应的性质和演变过程. 数值模拟清楚地表明,大气对异常外源的响应主要是一种具有30—60天周期的低频遥响应.分析不同地区和不同季节这种强迫响应的30—60天低频振荡的结构及活动,可以清楚看到它与大气中实际存在着的30—60天振荡极为相似.因此也可以认为,大气对海温异常的强迫遥响应是激发产生全球大气30—60天振荡的重要机制.     

土库曼斯坦阿姆河右岸卡洛夫—牛津阶储层流体包裹体特征及成藏期

基于阿姆河右岸中部中上侏罗统卡洛夫—牛津阶碳酸盐岩储层流体包裹体的镜下观察、均一温度测定,结合烃源岩生排烃史、地层埋藏史、热史及构造演化史,恢复阿姆河右岸中部油气藏的成藏过程。结果表明:第一期为早白垩世阿尔必期(120～105 Ma),穆尔加勃坳陷的中下侏罗统烃源岩进入生烃门限,早白垩世晚期,生成的油气沿不整合面及查尔朱基底断裂运移至桑迪克雷隆起的碳酸盐岩礁滩体而聚集成藏,对应的包裹体为赋存于二世代方解石胶结物的、具有定向排列的叶黄色荧光包裹体;第二期为晚白垩世土伦期(75～65 Ma),盆地东南部中下侏罗统生成的凝析气继续充注桑迪克雷隆起的圈闭,中下侏罗统达到生烃高峰,生成的油气开始充注中部油气藏,对应的包裹体为赋存于半自形晶簇状及自形连晶状方解石胶结物的、略具有定向性的绿色荧光包裹体;第三期为晚渐新世—中新世(30～20 Ma),在穆尔加勃坳陷的油气持续充注的背景下,烃源岩对中部油气藏的充注强度不断增加,并在喜山期构造挤压的影响下,对古油气藏进行调整定形,对应的包裹体为与大量气体包裹体共生的杂乱无章的蓝色荧光包裹体。     

低阶煤熔融体系电化学转化过程

为解决低阶煤转化的高耗能、高污染与分级转化调控难问题,提出一种基于电化学过程的低阶煤转化方法,以镍作为电化学反应阴极与阳极,在熔融体系中,采用热—电化学协同反应过程电解低阶煤进行提质转化。结果表明:低阶煤在熔融体系中能够进行电化学氧化还原反应,随温度的升高,能够有效降低氧化还原电位;低阶煤的电化学转化随反应时间的改变而呈现阶段性变化;电压/电流、温度是低阶煤转化的关键影响因素,通过调控电压/电流与反应度匹配,能够获得理想的低阶煤转化率;在反应温度为360℃、电压为2.0 V、反应时间为4 h条件下,低阶煤电化学转化率可以达到87.3%,其中液体转化率为48.8%,气体转化率为38.5%。     

测量上海产业网络的点入度和点出度——超越后工业化社会的迷思北大核心CSCDCSSCI

利用上海市2007年144个部门投入产出表,计算基于投入产出完全消耗系数的点入度和点出度,将产业划分为Ⅰ型(高点入度、高点出度),Ⅱ型(低点入度、高点出度),Ⅲ型(低点入度、低点出度),Ⅳ型(高点入度、低点出度)。研究发现:1Ⅰ型、Ⅱ型、Ⅲ型和Ⅳ型制造业点入度均值分别比各类型服务业高0.52、0.45、0.04、0.27,表明制造业相对服务业具有更强的后向拉动效应。2Ⅱ型和Ⅳ型服务业点出度均值分别高于Ⅱ型和Ⅳ型制造业0.29、0.16,而Ⅰ型和Ⅲ型服务业点出度均值分别小于Ⅰ型和Ⅲ型制造业0.32、0.17,表明服务业的前向拉动效应存在着分异。3Ⅰ型、Ⅳ型制造业及服务业的点出度对GDP均具有正向的相关性,提高对这些产业的使用有利于提升GDP。Ⅱ型服务业的点入度对GDP具有负向的相关性,点入度较低的房地产开发经营业、银行业、证券业GDP分别为该类服务业前3名。Ⅱ型服务业点出度、Ⅲ型制造业和服务业点入度和点出度对GDP的回归系数均未通过显著性检验。尽管制造业GDP占比下降,制造业仍在上海产业网络中发挥着重要的作用。上海应超越后工业化的迷思,降低对房地产业的依赖,加强制造业与服务业的融合发展,特别是加强金融对制造业等实体经济的支持,提升产业网络关联多样性和非关联多样性,促进航空、航天、机器人等新兴产业的发展。     

东海陆架南部邻近陆域晚三叠世—早侏罗世沉积古环境分析

东海陆架盆地南部邻近陆域主要包括福建东南部以及广东东北部的广大地区。结合野外地质考察、岩石薄片镜鉴及样品地球化学测试结果等资料,研究了该地区晚三叠世—早侏罗世沉积古环境。研究区晚三叠世—早侏罗世时期,属于温湿气候环境,南部的粤东地区沉积水体深度较大,因此,大部分样品指示厌氧环境。晚三叠世时,整个东海陆架南部邻近陆域自南向北水体逐渐变浅,南部主要为滨海—浅海陆棚—深水陆棚环境,北部主要表现为受海侵作用影响的海陆过渡相环境;早侏罗世时,南部主要表现为水体较深的深水陆棚环境,北部主要表现为海陆过渡相—陆相沉积环境。通过对具有相同大地构造背景的邻近陆域沉积古环境的研究,从而可以推断缺乏钻井资料的东海陆架盆地南部沉积古环境自北向南由陆及海,为后续开展海域中生界油气地质条件研究提供依据。     

A Kinematical Calibration of the Galactocentric Distance

1 INTRODUCTION The distance to the Galactic center R0 is a fundamental constant for astronomy and astrophysics. Most determinations of astronomical quantities are directly connected with the Galactic distance scale, e.g., the rotational speed of our Galax…     

Excitation of Annual Polar Motion by the Pacific,Atlantic and Indian Oceans

The global oceans play important roles in exciting the annual polar motion besides the atmosphere. However,it is still unclear about how large the regional oceans contribute to the annual polar motion. We investigate systemically the contributions of the Pacific,Atlantic and Indian Oceans to the excitation of the annual polar motion,based on the output data of ocean current velocity field and ocean bottom pressure field from "Estimating the Circulation and Climate of the Ocean (ECCO)" ocean circulation model over the period 1993-2005. The result shows that due to its particular location and shape,the Atlantic Ocean makes a less significant contribution to the x-component of the annual polar motion excitation than the Pacific and Indian Oceans,while all these three oceans contribute to the y-component of the annual polar motion excitation to some extent.     

An Infrared Photometric Study of Galaxies with Extragalactic H2O Maser Sources

All galaxies with extragalactic H_2O maser sources observed so far are collected. With the 2MASS and the IRAS photometric data an infrared study is performed on those galaxies.By a comparison between the H_2O maser detected sources and non-detected sources in the infrared it is indicated that infrared properties in the IRAS 12-25μm and 60-100μm are important for producing H_2O masers in galaxies.It is also found that the H_2O maser galaxies with different nuclear activity types have rather different infrared properties mainly in the IRAS 12-60μm region.     

Shallow Decay of X-ray Afterglows in Short GRBs： Energy Injection from a Millisecond Magnetar？

With the successful launch of Swift satellite,more and more data of early X-ray afterglows from short gamma-ray bursts have been collected.Some interesting features such as unusual afterglow light curves and unexpected X-ray flares are revealed.Especially,in some cases,there is a fiat segment in the X-ray afterglow light curve.Here we present a simplified model in which we believe that the flattening part is due to energy injection from the central engine.We assume that this energy injection arises from the magnetic dipole radiation of a millisecond pulsar formed after the merger of two neutron stars.We check this model with the short GRB 060313.Our numerical results suggest that energy injection from a millisecond magnetar could make part of the X-ray afterglow light curve flat.