风云三号C星微波全球地表温度产品精度评估

地表温度是衡量地表水热平衡的关键参数,微波地表温度因其范围大、全天候等独特的优势,在气候、农业和环境等领域得到广泛应用。基于经质量控制的MODIS地表温度产品对风云三号卫星C星的微波地表温度日产品和月平均产品进行验证评估,结果显示:FY-3C卫星升轨(夜晚)和降轨(白天)微波地表温度日产品平均分别高估8. 7 K、低估13. 2 K,月平均产品平均分别高估7. 9 K、低估12. 0 K,日产品和月平均产品的反演误差都在15K以内。在全球空间分布上,升轨(夜晚)和降轨(白天)月产品误差分别呈现高估和低估,热带雨林区和沙漠、荒漠区域在夜晚分别高估5 K以内和30 K以内,白天则分别低估10 K以内和10～30 K。不同土地覆盖类型间FY-3C微波地表温度反演精度存在差异,总体上升轨(夜晚)比降轨(白天)的精度高,反演精度最高和最低的土地类型分别是常绿阔叶林和荒漠、稀疏植被,不同土地覆盖类型间的地表温度反演精度在季节上存在明显差异。根据分析结果,改进FY-3C微波地表温度的反演算法,可进一步提高微波地表温度的反演精度。     

京西北地区地应变观测与小震震源机制解一致性研究

以京西北地区作为研究区域,采用应变参数方法解算定点地应变观测数据,将所得应变参数时间序列作为研究对象,利用该结果与研究区内同期小震震源机制解进行一致性分析,研究得出呈拉张性质的定点观测最大主应变方位与震源机制解最大拉张变形方向（T轴）水平投影具有良好的对应性,整体以NNW—NE向为主,且自西向东排布的测点最大主应变方位与震源机制解最大拉张变形方向均表现为逐渐东向偏移的趋势,与华北平原块体北部发生顺时针旋转活动的特征相吻合,结果进一步检验了地应变观测反映区域应变场信息的能力。     

Processes of the deposition and vicissitude of Mu Us Desert, China since 150 ka B.P.

“Milanggouwan stratigraphical section” named lately takes down 27 cycles of alternately evolutionary histories of desert depositions in the Mu Us area with the fluviolacustrine facies and palaeosols since 150 ka B. P. Studies show that the sedimentary form was induced by the growth and decline and confrontation each other between the winter monsoon and the summer monsoon of East Asia in the past 150 ka. Project supported by the National Natural Science Foundation of China (Grant No. 49473192).     

Simulation of spatially correlated earthquake ground motions for engineering purposes

A new model to simulate spatially correlated earthquake ground motions is developed. In the model, the main factors that characterize three distinct effects of spatial variability, namely, the incoherency effect, the wave-passage effect and the site-response effect, are taken into account, and corresponding terms/parameters are incorporated into the well known model of uniform ground motions. Some of these terms/parameters can be determined by the root operation, and others can be calculated directly. The proposed model is fi rst verif ied theoretically, and examples of ground motion simulations are provided as a further illustration. It is proven that the ensemble expected value and the ensemble auto-/cross-spectral density functions of the simulated ground motions are identical to the target spectral density functions. The proposed model can also be used to simulate other correlated stochastic processes, such as wave and wind loads.     

南海台风生成前48 h环流特征及热力与动力条件

利用1979—2019年4—11月中国气象局上海台风研究所热带气旋最佳路径资料和静止卫星红外云图资料,筛选出189例南海台风,结合欧洲中期天气预报中心1°×1°再分析资料,分析南海台风生成前48 h至生成时刻的天气环流和动力、热力条件。结果表明：南海台风生成于热带洋面大范围的高海表温度、高水汽含量和高不稳定层结区,其生成前的主要环境背景环流是赤道辐合带、西南季风或东风波等;台风生成前扰动中心常常处于其北侧风切变小而南侧风切变大的过渡带中,少数扰动中心倾向于风切变小值中心附近,风切变与扰动的发展之间无显著相关;扰动中心一般与垂直涡度中心重合,垂直涡度中心是表征扰动自身强弱的物理量,但垂直涡度自身的大小与未来扰动发展趋势关系不明显,而Okubo-Weiss（OW）指数则对于扰动的发展以及扰动位置确定有较好的指示意义;在扰动发展过程中,扰动中心附近存在一个贯穿整个对流层的位涡柱,低层扰动部分与位涡柱中的中低层位涡相互作用,有利于扰动发展。     

The down-faulted basin zone and high disaster risk zone in Shanxi Province, China

Introduction Since 1920s, with increasing awareness of disaster prevention and reduction in various as-pects and gradually deepened development of International Decade for Natural Disaster Reduction (IDNDR) activities in China, the role and position of disaster risk analysis and risk management work are increasingly prominent. In the final report of the IDNDR activities in 1999, the Science and Technology Committee of IDNDR had presented 5 challenge fields, which the international dis…     

光轴角近90°时二轴晶光性正负的判别

二轴晶光率体光性正负有两种判别方法：一种是根据光轴角（２Ｖ）的锐角平分线（Ｂｘａ）与Ｎｇ一致还是与Ｎｐ一致来判别，其临界点是２ｙ＝９０°；另一种是根据三个主拆射率的相对大小来判别．由于二轴晶光率体为三轴椭球体，在其临界点Ｎｇ一Ｎｍ＝Ｎｍ一Ｎｐ时，光轴角并不等于９０°。就是说，两种判别方法的临界点不一致。本文从光率体几何特性研究入手，通过几何及数学方法，着重讨论上述两种判别方法在其临界点时的相对关系，并结合实际例证，认为二轴晶光率体光性正负的临界点不能只确定为一个点，而应限定在一个范围，即２Ｖ＝９０°到Ｎｇ－Ｎｍ＝Ｎｍ－Ｎｐ之间。     

Fatigue-Damage Evolution Characteristics of Interbeded Marble Subjected to Dynamic Uniaxial Cyclic Loads

In this work, uniaxial fatigue tests combined with post-test X-ray computed tomography (CT) scanning were conducted on marble samples with different interbed orientations, in order to reveal the anisotropic damage evolution characteristics during rock failure. The dynamic elastic modulus, damping ratio, fatigue deformation, damage evolution, accumulative damage modeling and crack pattern were systematically analyzed. The testing results indicate that the interbed structure in marble affects the damage evolution and the associated dynamic mechanical behaviors. The damage curve in “S” style indicates three-stage trend, namely, initial damage stage, steady damage stage and the accelerated damage stage. The damage index during cyclic deformation for marble presents obvious discrepancy. In addition, a fatigue damage prediction models was employed numerically as double-term power equations based on the experimental data. It is found that the selected damage model is suitable in modeling the rapid damage growth in the early and final stage of rock fatigue lifetime. Moreover, post-test CT scanning further reveals the anisotropic damage characteristics of marble, the crack pattern in the fractured sample is controlled by the interbed structure. What is more, the most striking founding is that the fracture degree is in consistent with the damage accumulation within the steady damage stage. Through a series of damage mechanical behavior analysis, the internal mechanism of the effect of interbed orientation on damage evolution of marble is firstly documented.

     

The physical origin of optical flares following GRB 110205A and the nature of the outflow

The optical emission of GRB 110205A is distinguished by two flares.We examine two possible scenarios for the optical afterglow emission.In the first scenario,the first optical flare is the reverse shock emission of the main outflow and the second one is powered by the prolonged activity of the central engine.However,we find that it is rather hard to reasonably interpret the late(t > 0.1 d) afterglow data unless the GRB efficiency is very high(～ 0.95).In the second scenario,the first optical flare is the low...     

A Statistical Study on the Geomagnetically Induced Current Events Driven by Earth-directed Full-Halo Coronal Mass Ejections

Solar activities can cause the anomalies of electric power transmission systems, especially, for an extra-long distance transmission system. Using the data of coronal mass ejection (CME) from SOHO/LASCO (Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph), and the data of the geomagnetically induced current (GIC) and geomagnetic storm from the North China Electric Power University and Finnish Meteorological Institute, respectively, we analyze some important observational features and physical properties of the earth-directed halo CMEs associated with the GIC events. After classifying the observed halo CMEs according to their symmetry, it is found that the halo CMEs associated with GIC events are mainly the 3 types: completely symmetric, brightness-asymmetric, and outline-asymmetric. The geomagnetically induced current events driven by the three different types of halo CMEs have different characteristics in the intensity, duration, and period. We ?nd that the brightness-asymmetric halo CMEs are most likely to cause the major damage to the transmission systems. And that the geomagnetically induced current has also a good correlation with the time variation of geomagnetic ?eld.