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积雨云中微物理过程的数值模拟——(二)阵雨、冰雹、暴雨的个例研究

用文(一)的微物理模式在一维时变动力学框架里模拟了江西阵雨云,75·8暴雨和张家口冰雹云。用实测探空作为输入,计算结果同实测的云降水和雷达回波特征相比,在很多方面相当一致。它展示了暴雨云的持续性和冰雹云的低降水效率等,表明了在这些云底较暖的积雨云中贝吉隆过程对降水作用不大,而暖雨过程则是启动降水的主要环节。     

MM5模式中不同对流参数化方案的比较试验

应用MM5中尺度模式, 在60、20和10 km模式分辨率下, 分别选用4种不同对流参数化方案 (KUO方案、GRELL方案、KAIN-FRITSCH方案和BETTS-MILLER方案, 以下简称KU、GR、KF和BM方案) 对1996年8月3~4日石家庄暴雨过程进行数值模拟试验.模拟结果的对比分析及其与观测的比较表明:主要雨带位置对参数化方案并不是十分敏感, 但随分辨率提高, 雨带分布特征的模拟更接近实况; 当分辨率提高到10 km时, 虚假的降水中心也明显增加; 模拟的暴雨中心强度随分辨率的提高而增强并随参数化方案的不同有所变化, 但均比实况偏弱.分析还发现, MM5模式的GR、KF及BM方案的次网格降水对总降水的贡献率随分辨率的提高而减小, 而KU方案的情况则呈现出不合理的缓慢增加态势.虽然4种方案下模拟的水平环流特征有较好的一致性, 但模拟的云物理特征和垂直运动特征还是存在一定差别的, 这种差别对定点、定量降水和天空状况、地面气温、湿度等要素的准确预报都会产生影响.因此, 在预报和模拟中应考虑预报和研究对象的特点来选择对流参数化方案.     

国产旋转导向及随钻测井系统在渤海某油田的应用

旋转导向和随钻测井系统可在精确、高效控制井眼轨迹和快速识别地层性质的同时大幅度提高作业效率,降低作业成本。尤其在海上油气开发过程中具有较好的提效效果,但是长期以来该领域均被国外石油公司垄断且租赁价格高昂。中海油国产化研制的Welleader旋转导向系统、Drilog随钻测井系统经过多次试验达到了入井应用要求,在渤海某平台调整井钻井作业中进行了应用,结果表明该套系统旋转导向系统轨迹控制满足定向井轨迹要求、测斜数据准确、测井质量符合标准要求,能够实现钻井过程中的轨迹控制和测井要求。     

Chronology and cooling history of the Tianmenshan pluton in South Jiangxi Province and their geological significance

Geochronological studies on the crust-derived Tianmenshan pluton were undertaken by SHRIMP zircon U-Pb dating and Ar-Ar dating of biotite, muscovite and K-feldspar, giving a petrogenetic age of 167 Ma. Owing to the closure systems in different minerals, the cooling history of the pluton can be determined with an age-temperature diagram. The late hydrothermal event has been recognized, which is related probably with mineralization. In terms of the comparative geochronological and petrologic records, it is concluded that there are some constrains on tectonic evolution and that the formation of the Tianmenshan pluton proceeded in a transition period from Indosinian post-orogeny extension to strong compressive tectonics. And the timing of the hydrothermal event matches the compressive climax of the Yanshanian orogeny. The temporal gap between granite emplacement and wolframite mineralization could last 10-20 Ma owing to the low cooling rate of the pluton.     

洛川黄土剖面的粉砂与粘粒比值及粒度旋回

洛川黑木沟黄土剖面发育了一套完整的黄土地层。据剖面百余块标本粒度资料阐述了Kd=(粉砂(0.05-0.01mm％))/(粘粒(<0.005mm)％)的地质及物理意义。它反映了受风化的粉尘粒组与次生粒组之间的消长关系,Kd值变化既受风尘来源区干湿状况或生物气候条件的制约,又受风化成壤作用的制约。因此,Kd值可视为黄土、古土壤生成环境的一个指标。据Mφ(平均值)由粗到细的变化划为一个粒度旋回,全剖面共分11个旋回。每个旋回反映了一定的岩性地层组合及生物气候环境的变化。     

热动力条件对白云凹陷深水区珠海组砂岩成岩演化过程的影响

珠江口盆地白云凹陷位于中国南海北部,是目前我国深水油气勘探研究的重要区域.盆地现今大地热流值为24.2～121.0mW/m^2,单井现今地温梯度(Gra)最高可达6.64℃/100m,具"热盆"属性.白云凹陷裂后沉降阶段,特别是白云运动(23.8Ma)发生之后,盆地由断裂控盆转变为断裂、热作用共同控盆,热作用及热动力条件成为控制研究区储层成岩演化过程的重要因素,珠海组地层的镜质体反射率值、砂岩中次生流体包裹体均一温度、热液成因自生矿物等热流背景及岩石学记录为这一观点提供了有力证据.通过铸体薄片显微镜下观察与定量统计、电镜扫描观察、X-射线衍射分析等,发现白云凹陷北部中-低地温梯度(LGR,Gra≤4.5℃/100m)和南部高地温梯度(HGR,Gra>4.5℃/100m)两个地区珠海组砂岩的成岩作用特征、成岩演化过程存在以下差异:(1)中-低地温梯度地区珠海组砂岩的压实作用主要是静岩压实作用;高地温梯度地区珠海组砂岩的原生孔隙受静岩压实作用和热压实作用的共同控制,压实减孔速率高,等孔隙度埋深显著变浅;(2)地层升温速率的增大加快了储层中粘土矿物转化的速率,高地温梯度地区高岭石消失的埋深界限较中-低地温梯度地区浅,I/S(伊利石/蒙皂石混层)有序化进程较中-低地温梯度地区有所加快;(3)中-低地温梯度地区珠海组砂岩成岩演化过程属正常有序演变,高地温梯度地区受构造热事件的影响明显,深部流体参与了高地温梯度地区珠海组砂岩的成岩演化过程,地层孔隙水物质交换过程复杂,成岩演化进程加快,改变了碳酸盐矿物溶解-沉淀热平衡状态,各成岩作用过程活跃并出现一些典型的热液成因自生矿物组合.     

The evolutionary status of HD 104237, ε Cha and HD 100546

Using the new data from Hipparcos and the TD-1 UV data, we fix the positions of three objects, HD 104237, HD 100546 and ε Cha in the HR diagram and discuss their theoretical evolutionary status.     

中国遥感卫星辐射校正场气溶胶光学特性观测研究

1999年6月28日~7月19日在敦煌场, 7月25日~7月31日在青海湖水面场进行了一次大规模综合野外测量试验, 其中采用3台先进的法国CIMEL太阳辐射计对两个场地大气光学特性进行了系统全面测量, 获得大量晴空天气条件下的大气光学数据。利用Langley法处理气溶胶通道数据得到气溶胶光学厚度及其光谱变化。测量结果显示550 nm波长平均气溶胶光学厚度分别为0.12、0.18, 由气溶胶光学厚度的波长变化得到气溶胶Junge参数分别为2.6、3.0, 并与几种典型气溶胶类型比较。结果表明两地在晴空天气里, 气溶胶含量较小, 符合遥感卫星传感器辐射定标的大气条件。     

Near-field effects of Cherenkov radiation induced by ultra high energy cosmic neutrinos

The radio approach based on the Askaryan effect for detecting the ultra-high energy cosmic neutrinos has become a mature experimental technique. So far the existing calculations of the Cherenkov radiation associated with the Askaryan effect has been mostly based on the far-field approximation, whose validity maybe challenged when the detector is close to the event. In this paper we present an alternative approach to calculate the Cherenkov pulse by a numerical code based on the finite difference time-domain (FDTD) method. This approach has the advantage of providing the solution everywhere in space, contrary to other methods that rely on the far-field approximation. We also present a one-dimensional theoretical model for the shower with analytical solution, which helps to elucidate our nonzero-width simulation results. We show that for a shower with symmetric longitudinal development, the resulting near-field waveform would be asymmetric in time. In addition, we demonstrate that for a shower elongated by the LPM (Landau-Pomeranchuk-Migdal) effect and thus with a multi-peak structure, a bipolar, asymmetric waveform is still preserved in the near-field regime irrespective of the specific variations of the multi-peak structure, which makes it a generic, distinctive feature. This should provide an important characteristic signature for the identification of ultra-high energy cosmogenic neutrinos.