多尺度非静力通用模式框架的设计策略

针对目前国际上数值预报模式的最新发展趋势,综述了新形势下多尺度非静力通用数值预报模式框架的设计策略。目前世界上开发通用模式主要有两个途经,一是建立一个离散化方案和源程序代码共享的、全球和有限区通用的模式,二是建立一个单一的全球可变分辨率的模式。还从通用模式方程组的选取策略、模式网格属性的构造,时间积分方案、空间离散方案,垂直坐标的选取等方面进行了分析。     

加密自动站资料质量保障体系分析

加密自动站（IAws）观测网随着我国观测系统的加强日趋完善,许多省市都有IAWS局域网。IAWS观测资料的应用也日益受到重视。但由于IAWS观测资料的特殊性,其质量问题不同程度地阻碍了它的使用。为了促进我国IAWS观测资料质量保障体系的建立,首先通过对比IAWS观测资料和以往的天气尺度常规地面人工站（CMWS）观测资料的特点,分析了IAWS资料的特殊性,然后从国际上IAWS观测资料质量保障体系的经验和方法着手,对IAWS观测资料和CMwS观测资料质量保障体系的差别以及建立IAWS观测资料质量保障体系应注意的重点和问题进行了分析。分析结果表明：IAWS观测资料质量保障体系不同于CMWS观测资料质量保障体系,应特别重视观测业务管理体制建立和台站级自动质量控制、人工干预、监测评估等技术的应用。     

Processes of initial collision and suturing between India and Asia

The initial collision between Indian and Asian continents marked the starting point for transformation of land-sea thermal contrast, uplift of the Tibet-Himalaya orogen, and climate change in Asia. In this paper, we review the published literatures from the past 30 years in order to draw consensus on the processes of initial collision and suturing that took place between the Indian and Asian plates. Following a comparison of the different methods that have been used to constrain the initial timing of collision, we propose that the tectono-sedimentary response in the peripheral foreland basin provides the most sensitive index of this event, and that paleomagnetism presents independent evidence as an alternative, reliable, and quantitative research method. In contrast to previous studies that have suggested collision between India and Asia started in Pakistan between ca. 55 Ma and 50 Ma and progressively closed eastwards, more recent researches have indicated that this major event first occurred in the center of the Yarlung Tsangpo suture zone (YTSZ) between ca. 65 Ma and 63 Ma and then spreading both eastwards and westwards. While continental collision is a complicated process, including the processes of deformation, sedimentation, metamorphism, and magmatism, different researchers have tended to define the nature of this event based on their own understanding, an intuitive bias that has meant that its initial timing has remained controversial for decades. Here, we recommend the use of reconstructions of each geological event within the orogenic evolution sequence as this will allow interpretation of collision timing on the basis of multidisciplinary methods.     

PRB数字地质填图中的遥感技术应用研究——以云南1:5万罗平幅区域地质调查为例

区域地质调查是一项基础性、公益性、综合性的调查研究工作,是国民经济建设和社会可持续发展中最重要的基础工作(李超岭等,2003;中国地质调查局①).     

The structure of the mid- and high-latitude ionosphere during the November 2004 storm event obtained from GPS observations

GPS data from the International GNSS Service (IGS) network were used to study the development of the severe geomagnetic storm of November 7–12, 2004, in the total electron content (TEC) on a global scale. The TEC maps were produced for analyzing the storm. For producing the maps over European and North American sectors, GPS measurements from more than 100 stations were used. The dense network of GPS stations provided TEC measurements with a high temporal and spatial resolution. To present the temporal and spatial variation of TEC during the storm, differential TEC maps relative to a quiet day (November 6, 2004) were created. The features of geomagnetic storm attributed to the complex development of ionospheric storm depend on latitude, longitude and local time. The positive, as well as negative effects were detected in TEC variations as a consequence of the evolution of the geomagnetic storm. The maximal effect was registered in the subauroral/auroral ionosphere during substorm activity in the evening and night period. The latitudinal profiles obtained from TEC maps for Europe gave rise to the storm-time dynamic of the ionospheric trough, which was detected on November 7 and 9 at latitudes below 50°N. In the report, features of the response of TEC to the storm for European and North American sectors are analyzed.     

Lateral tidal mixing in the Antarctic marginal seas

Tidal mixing plays an important role in the modification of dense water masses around the Antarctic continent. In addition to the vertical (diapycnal) mixing in the near-bottom layers, lateral mixing can also be of relevance in some areas. A numerical tide simulation shows that lateral tidal mixing is not uniformly distributed along the shelf break. In particular, strong mixing occurs all along the Ross Sea and Southern Weddell Sea shelf breaks, while other regions (e.g., the western Weddell Sea) are relatively quiet. The latter regions correspond surprisingly well to areas where indications for cross-shelf exchange of dense water masses have been found. The results suggest that lateral tidal mixing may account for the relatively small contribution of Ross Sea dense water masses to Antarctic Bottom Water.     

阶段性干旱胁迫对小麦光合生理特性及产量结构的影响

在人工遮雨的条件下,采用盆栽的种植方式探究"皖麦68"营养生长期(返青期—开花期)及生殖生长期(开花期—成熟期)轻度干旱胁迫(土壤相对含水量为55%±5%)及复水(土壤相对含水量为70%±5%)对其光合生理特性及产量结构的影响。结果表明:返青期至成熟期充分供水(CK)的小麦旗叶光合参数和产量最高。开花至成熟期复水(DN)的小麦叶片在复水后光合能力迅速恢复,表现出了超补偿效应:光合速率(16.43μmol/(m~2·s))甚至超过了CK(15.01μmol/(m~2·s));采用非直角双曲线模型拟合小麦旗叶的光响应曲线,其中DN的曲角θ最大;DN产量较CK略有降低但千粒重为34.51 g,高于CK(34.44 g)。开花至成熟期轻度干旱(ND)及全生育期轻度干旱(DD)的小麦光合特征参数与产量均显著降低。DD产量最低、品质最差,但其收获指数I_H高于CK、仅次于DN。在小麦返青期—开花期进行水分管理适量减少灌溉,开花期—成熟期复水能够提升籽粒的干物质积累量,获得较高的产量及品质。     

木本植被覆盖岸坡上波浪爬升过程的数值模拟研究

近岸木本植物构成的生态缓冲带作为新型的海岸软防护结构,兼具功能性和生态友好性,在沿海工程建设中愈发受到关注,如何深入开展其防护效果的机理研究是目前亟待解决的问题。本文采用数值模拟方法,在N-S方程中分别考虑树枝和树干的拖曳力影响,提出了木本植被作用下波浪沿斜坡爬升的表面波衰减的连续介质等效模型,并采用MAC法来跟踪自由曲面上的水颗粒轨迹。本文以波浪沿1/30的斜坡爬升为算例,对比讨论了有无植被作用下波浪的传播过程,并将算例结果与以往试验结果规律进行对照,验证了数值模型的有效性。最后,分别讨论了植物枝干的高度、密度、树枝倾斜角度等植被特性和波浪因素对植被消浪效果的影响,得到植被消浪的基本规律。文中的计算结果也可为实际的护岸工程和生态景观设计提供参考。     

国产磁通门磁力仪稳定性分析

国产磁通门磁力仪(GM-3磁通门磁力仪)在全国各地磁台站推广应用,两年来,该仪器在武汉地震台工作比较稳定。本文对该仪器的基线值进行了多层线性回归分析。结果表明仪器性能比较稳定。     

Space Weather: Physics,Effects and Predictability

The time varying conditions in the near-Earth space environment that may affect space-borne or ground-based technological systems and may endanger human health or life are referred to as space weather. Space weather effects arise from the dynamic and highly variable conditions in the geospace environment starting from explosive events on the Sun (solar flares), Coronal Mass Ejections near the Sun in the interplanetary medium, and various energetic effects in the magnetosphere–ionosphere–atmosphere system. As the utilization of space has become part of our everyday lives, and as our lives have become increasingly dependent on technological systems vulnerable to the space weather influences, the understanding and prediction of hazards posed by these active solar events have grown in importance. In this paper, we review the processes of the Sun–Earth interactions, the dynamic conditions within the magnetosphere, and the predictability of space weather effects on radio waves, satellites and ground-based technological systems today.