南海东北陆缘的地壳速度结构及其构造意义: 来自广角地震剖面的约束

南海东北部深部地壳结构蕴含着南海陆缘伸展张裂过程的重要信息。在南海东北陆缘布设的一条广角地震测线(DP13)沿NW-SE方向依次穿过东沙隆起和台西南盆地。本文利用射线追踪和正演走时拟合软件RayInvr构建地壳纵波速度结构,模型表明：沉积层速度1.6～4.6 km/s,厚度0.5～3.8 km,横向分布不均匀,沉积基底起伏剧烈;莫霍面埋藏深度由陆架区的25.5 km急剧减小到陆坡下方的13 km,随后向下陆坡远端增深至16 km;陆架处东沙隆起下方地壳厚度从～25 km减薄到～21 km,下陆坡远端地壳厚约10～13 km,地壳拉张因子分别为1.3～1.5和2.6～3.1,表现为轻微和中等减薄;陆坡区台西南盆地内地壳厚度从17 km急剧减薄至7～8 km,地壳拉张因子高达4.6,呈超伸展减薄;地壳厚度由陆向海非单调减薄,地壳伸展具有明显的空间差异性;陆架-上陆坡和下陆坡下地壳底部发现两个相对孤立的不连续高速体,速度分别为7.0～7.5 km/s和7.0～7.3 km/s,厚度分别3～5 km和1～3 km,前者位于古太平洋俯冲带前缘,几乎与南海东北部高磁异常重叠,推测由中生代古太平洋板...     

CMIP5西北太平洋气候变率的模拟评估

利用观测海温资料和CMIP5模式模拟结果分析西北太平洋(120°E~120°W,20~60°N)海表温度的气候态和年代际变化特征。结果表明,所选22个模式可以较好地模拟出西北太平洋海表温度的气候特征及其年际、年代际变化特征;模式模拟的海表温度总体标准偏差在黑潮延伸体区域最大;绝大多数模式能模拟出海表温度的第一EOF模态;西北太平洋海表温度具有较明显的年代际振荡现象,13/22的模式模拟的海表温度存在明显的年代际振荡,同时海表温度气候态的模拟偏差对其周期振荡模拟的影响较大,尤其在黑潮延伸体区域。     

Influence of positive and negative Indian Ocean Dipoles on ENSO via the Indonesian Throughflow: Results from sensitivity experiments

The role of the Indonesian Throughflow(ITF) in the influence of the Indian Ocean Dipole(IOD) on ENSO is investigated using version 2 of the Parallel Ocean Program(POP2) ocean general circulation model. We demonstrate the results through sensitivity experiments on both positive and negative IOD events from observations and coupled general circulation model simulations. By shutting down the atmospheric bridge while maintaining the tropical oceanic channel, the IOD forcing is shown to influence the ENSO event in the following year, and the role of the ITF is emphasized. During positive IOD events,negative sea surface height anomalies(SSHAs) occur in the eastern Indian Ocean, indicating the existence of upwelling.These upwelling anomalies pass through the Indonesian seas and enter the western tropical Pacific, resulting in cold anomalies there. These cold temperature anomalies further propagate to the eastern equatorial Pacific, and ultimately induce a La Nia-like mode in the following year. In contrast, during negative IOD events, positive SSHAs are established in the eastern Indian Ocean, leading to downwelling anomalies that can also propagate into the subsurface of the western Pacific Ocean and travel further eastward. These downwelling anomalies induce negative ITF transport anomalies, and an El Nio-like mode in the tropical eastern Pacific Ocean that persists into the following year. The effects of negative and positive IOD events on ENSO via the ITF are symmetric. Finally, we also estimate the contribution of IOD forcing in explaining the Pacific variability associated with ENSO via ITF.     

基于模糊逻辑的大气云粒子相态反演和效果分析

为了探究8mm云雷达探测到的大气云粒子相态特征,根据Shupe总结得到云雷达探测参量:反射率因子、Doppler径向速度、线性退偏振比以及温度在不同相态水凝物对应的云雷达产品特征阈值,采用不对称T型的隶属函数,成员函数包括:反射率因子、线性退偏振比、径向速度以及垂直温度廓线,反演出的粒子相态包括:雪、冰晶、混合相态、液水、毛毛雨、雨等6种。通过联合分析中国气象科学研究院灾害天气国家重点实验室的偏振云雷达探测资料和GTS1型探空仪温度数据,结果表明;通过模糊逻辑法对云雷达探测的参量反演出的大气粒子相态结果与探空实时数据一致性较好,对现阶段常规天气预报参考、人工影响天气作业指挥以及效果评估来说具有较好指导性。     

甘肃武威市一次局地大到暴雨天气成因分析

利用常规天气图、FY-2D卫星云图、单站地面资料、NCEP再分析物理量场资料,对2013年8月6日发生在甘肃武威市对流性强降雨天气成因进行了诊断分析。结果表明:强降雨是在一定的大尺度环流背景下高低层天气系统共同作用下发生的,地面气象要素的剧烈变化是强对流天气能量的释放过程;湿度条件和水汽在本地辐合为大到暴雨提供了充沛的水汽;高层辐散、低层辐合以及强烈的上升气流是大到暴雨发生的动力条件;强烈的不稳定能量和不稳定层结是对流增强、雨强较大的必要条件;对流云团的发展和加强是降雨强度较大的直接原因。     

改进影像匹配点云滤波方法的下沉盆地建模

针对受地表植被物候性特征的影响,无人机影像匹配点云所生成DEM精度偏低的问题,该文提出了一种基于坡度阈值和相邻点高差阈值相结合的地面种子点选取方法,改进了移动曲面拟合点云滤波算法.以林南仓煤矿西四采区为例,基于无人机测绘技术获取实验区地表三维点云,结合实测数据,分别采用 目视检验、定量评价和DEM精度分析等验证了滤波算...     

基于飞机观测资料的石家庄秋季对流层CH4垂直分布特征

为研究石家庄秋季对流层内CH₄垂直分布特征,2018年9月使用“空中国王350”飞机搭载Picarro温室气体在线观测仪和气象要素观测设备,对石家庄上空（600—5500 m）CH₄浓度进行探测。探测期间共飞行7架次,取得7条CH₄浓度廓线数据。结果表明: 石家庄上空近地面层（1000 m以下）CH₄平均浓度与同时间段区域背景站上甸子站CH₄浓度呈显著正相关（r=0.81,P < 0.03）。探测到的CH₄浓度最小值为1898×10^-9摩尔分数,最大值为2219×10^-9摩尔分数,平均浓度为1981×10^-9摩尔分数。观测得到的7条廓线均有较好的一致性,2000 m以上,浓度均随高度呈先增大后减小的趋势。利用后向轨迹模式（HYSPLIT）对探测时段内石家庄上空不同高度层主要气流传输路径进行统计分析表明,600 m高度输送路径较短,CH₄浓度受本地排放影响较大; 3000 m受输送作用影响较大,偏西和西南路径可能将较高CH₄浓度气团输送至石家庄上空; 5000 m气团传输对CH₄浓度影响较小,浓度相对较稳定,对传输路径的变化不敏感。     

The analytic properties of the flapping current sheets in the earth magnetotail

The current sheet in Earth’s magnetotail often flaps, and the flapping waves could be induced propagating towards the dawn and dusk flanks, which could make the current sheet dynamic. To explore the dynamic characteristics of current sheet associated with the flapping motion holistically and provide reasonable physical interpretations, detailed direct calculation and analysis have been applied to one approximate analytic model of magnetic field in the flapping current sheet. The main results from the model demonstrate: (1) the magnetic fluctuation amplitude is attenuated from the center of current sheet to the lobe regions; The larger wave amplitude would induce the larger magnetic amplitude; (2) the curvature of magnetic field lines (MFLs), with maximum at the center of current sheet, is only dependent on the displacement Z along the south-north direction from the center of current sheet, regardless of the tilt of current sheet; (3) the half-thickness of neutral sheet, h, the minimum curvature radius of MFLs, R_cmin, and the tilt angle of current sheet, δ, satisfies h=R_cmin cos δ; (4) the gradient of magnetic strength forms a double-peak profile, and the peak value would be more intense if the local current sheet is more tilted; (5) current density j and its j_y, j_z components reach the extremum at the center of CS. j and j_z would be more intense if the local current sheet is more tilted, but it is not the case for j_y; and (6) the field-aligned component of current density mainly appears in the neutral sheet, and the sign of it would change alternatively as the flapping waves passing by. To check the validity of the model, one simulation on the virtual measurements has been made, and the results are in well consistence with actual observations of Cluster.     

关于Fe-C(H)系高温高压合成金刚石多晶形成机制的一些思考

Fe-C(H)系高温高压金刚石多晶在合成片上呈成堆聚集状、不均匀分布.多晶中的金刚石晶粒多为八面体晶形、随机定向、大小无规律,表面发育"锯齿状"生长台阶,普遍发育塑性形变等缺陷.多晶中的金刚石晶粒间接触界线清晰、呈突变状.无论是利用品体成核、还是晶体长大理论都只能解释多晶中存在的部分现象.利用碳原子配位四面体生长基元模型分析多晶的形成机制值得探索.深入分析Fe-C(H)系高温高压合成金刚石多晶的形成机制不但有利于改善金刚石合成的工艺、提高合成金刚石多晶的品级.而且有利于为人们探讨天然金刚石多晶的形成机制及其深部意义提供科学线索.     

大气折射指数的结构参数与北方5～9月降雨的强相关现象

基于中荷合作项目"建立关于荒漠化和粮食保障的中国能量与水平衡监测系统"(CEWBMS),在国家卫星气象中心和国家林业总局的支持下,乾安大孔径闪烁仪于1999年10月安装并正式运行.利用2000-2005年5～9月大孔径闪烁仪(LAS)观测的大气折射指数的结构参数Cn2,采用独立性检验,证实了Cn2的高低与未来32h是否出现降雨(晴雨)存在显著相关关系.结合乾安气象站的有关气象观测数据,初步选择Cn2白天值以及夜间值以Cn2的24 h变量作为预报依据,建立基于Cn2预报未来32h晴雨的预报流程;并利用2006年Cn2的观测数据,依照预报流程对2006年进行了回报预报试验,正确率为42/47.