2014年2月12日于田7.3级地震序列震源机制特征分析

基于新疆及西藏区域数字地震台网的宽频带资料,采用CAP方法反演了2014年2月12日于田7.3级地震的前震、主震及早期MS≥3.5余震序列的震源机制解。结果显示,此次7.3级强震为带有正断分量的走滑型地震,结合震源区的构造和余震分布,节面I走向241°/倾角90°/滑动角-22°,判定该节面代表了主震的发震断层面。主震主压力轴方位为194o,与该区历史中强震主压应力P轴方位近NS向较为接近。其5.4级前震和主震震源机制解具有较高的一致性。18次余震中有10次为走滑型地震,其中6次为正断型,2次为逆断型,且70%的地震具有近SN向的P轴方位。此次7.3级地震序列震源深度范围5~28km,而大部分地震为15~20km,略大于本文计算得到的主震震源深度10km。     

A method characterizing urban expansion based on land cover map at 30 m resolution

Based on the global land cover data at 30 m resolution (GlobeLand30) in the year 2000 and 2010, the urban expansion process of 320 cities in China was analyzed using lognormal regression, and the expansion model were established. Three metrics were presented for the models, including the peak position, the full width at half maximum, and the skewness. It was found that the three metrics could reveal different patterns of the urban expansion process of cities with different sizes. Specifically, cities with larger size tend to expand outward strongly, and their expansion intensity and influence are likely to be higher. Moreover, most cities’ expansion occurs around the urban core with spatially limited influence. In addition, it was also found that the city’s expansion intensity is related to the city size. These results showed that the lognormal regression model could describe the distribution of urban expansion with effectiveness and robustness.     

JYZ11A钻孔记录的居延泽演化历史

我国内陆干旱区在末次冰期(含深海氧同位素第3阶段)是否存在古大湖近年来持续存在争论。居延泽是黑河的尾闾湖之一, 位于我国典型干旱区, 是开展这项研究的理想区域。依据居延泽盆地最低处的JYZ11A钻孔(全孔长61.13m, 本文侧重上部27m岩芯), 使用石英光释光测年获得3个可靠释光年龄并据此建立年代框架。全孔10cm间距测量沉积物粒度, 钻孔上部16.7m以2cm间距测量低频磁化率, 本文侧重分析JYZ11A钻孔上部10m的指标记录。综合岩性地层、沉积物粒度分布特征和粒度、磁化率指标记录, 并与前人已有研究进行对比, 本研究发现末次冰期时居延泽盆地主要堆积棕色冲洪积物和风沙沉积物, 早全新世为风沙沉积, 中全新世出现浅灰色湖相沉积与风沙交替沉积, 而稳定湖泊只在约3ka时才逐渐形成, 可能存在多次湖面波动并留下古湖岸堤。因此, 居延泽盆地在末次冰期包括深海氧同位素第3阶段晚期并不存在稳定大湖。居延泽早全新世干涸、中晚全新世湖泊较稳定发育的全新世成湖模式与季风区湖泊演化模式明显不同, 而与许多中亚干旱区的湖泊、风成沉积等古环境记录相似, 它们可能共同指示了一种有别于中国季风区的全新世区域湿度演化模式。     

ANSYS软件中修正剑桥模型的二次开发

ANSYS软件具有很强的非线性计算功能和前、后处理能力,是目前世界上最强大的通用分析程序之一。标准ANSYS程序中包含众多的材料本构模型,但尚缺少岩土工程数值计算中常用的修正剑桥模型。为扩展ANSYS在岩土工程领域的计算能力,利用二次开发工具UPFs和数据接口将修正剑桥模型连接到标准ANSYS程序中。二次开发的核心是本构模型子程序UMAT.F的编制。子程序的编写一方面要符合修正剑桥模型的本构关系式和弹塑性有限元计算的特点;另一方面变量名和输入输出格式必须和标准ANSYS程序一致。对二次开发后的ANSYS程序进行了典型算例的验证。结果表明,在ANSYS中加入修正剑桥模型的方法是可行的,可推广到ANSYS对于其他材料本构模型的二次开发中。     

基于遗传算法优化的小波神经网络在地下水位预测中的应用

地下水位是衡量生态环境优劣和地下水资源的一个重要指标.地下水位下降,将引发地面沉降、地面塌陷和降落漏斗等.因此,地下水位预测对保护地质生态环境和实现地下水资源严格管理至关重要.由于BP算法存在极易收敛于局部极小点与过拟合等缺点,导致网络泛化能力不足,本文在构建小波神经网络基础上并引入遗传算法加以优化,以解决上述不足,并与BP和WNN对比预测了天津市深层承压水水位.预测结果表明,GA-WNN模型拟合精度较高,模型的预测能力有较大幅度提高.     

辽河三角洲滨海湿地水域初级生产力研究进展

滨海湿地位于海洋与陆地生态系统的交错过渡带,具有极高的生产力和光合固碳效率,是海岸带蓝色碳汇的重要组成部分。滨海湿地生产力不仅由芦苇、翅碱蓬、红树林等陆上植被提供,水体中浮游植物的光合固碳也是提供初级生产力的重要途径。以往较多的调查和研究集中在陆上植被,而对于滨海湿地水域浮游植物和底栖微藻的报道较少。近年来随着各国政府和学者对二氧化碳排放和气候变化的关注,滨海湿地多圈层生态系统的碳循环和碳汇过程成为研究热点,而湿地水域生产力和光合固碳过程作为多圈层碳循环中重要的一个环节亦应受到足够的重视。以中国北方典型的盐沼湿地区域——辽河三角洲滨海湿地为案例,对湿地水域生产力研究进展进行综述,并对其影响因素进行讨论,以期为国家碳循环与碳中和目标调查提供参考资料。     

国际地球自转服务(IERS)评介

回顾了建立国际地球自转服务(IERS)的历史过程,简述了IERS机构各部门的设置及其作用。着重介绍了IERS重建的理由和过程以及新IERS机构的组成。最后给出IERS成果对现有科学研究的作用和意义。     

Astrophysical constraints on the gravitational constant

We study the astrophysical bounds on the change of the gravitational constant with time. We found that |/G|<10^–12yr^–1 is the condition that has to be satisfied in order not to cause a conflict with the observations. We find the condition to be in accord with the lower limits, the superstring theory predicts.     

Flare-induced signals in polarization measurements during the X2.6 flare on 2005 January 15

Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two questions: can we distinguish the flare-induced signals from real magnetic changes during flares, and what we can learn about flare energy release from the flare-induced signals? We select the X2.6 flare that occurred on 2005 January 15, for further study. The flare took place in NOAA active re-gion (AR) 10720 at approximately the central meridian, which makes the interpretation of the vector magnetograms less ambiguous. We have identified that flare-induced signals during this flare appeared in six zones. The zones are located within an average distance of 5 Mm from their weight center to the main magnetic neutral line, have an average size of (0.6±0.4)×1017 cm2, duration of 13±4 min, and flux density change of 181±125 G in the area of reversed polarity. The following new facts have been revealed by this study: (1) the flare-induced signal is also seen in the transverse magnetograms but with smaller magnitude, e.g., about 50 G; (2) the flare-induced signal mainly manifests itself as apparent polarity reversal, but the signal starts and ends as a weakening of flux density; (3) The flare-induced signals appear in phase with the peaks of hard X-ray emission as observed by the Ramaty High Energy Solar Spectroscopic lmager (RHESSI), and mostly trace the position of RHESSI hard X-ray footpoint sources. (4) in four zones, it takes place cotemporally with real magnetic changes which persist after the flare. Only for the other two zones does the flux density recover to the pre-flare level immediately after the flare.The physical implications of the flare-induced signal are discussed in view of its relevance to the non-thermal electron precipitation and primary energy release in the flare.     

水脉泽寄主活动星系核的吸积率(英文)

水超脉泽辐射( 各向同性光度超过 10 个太阳光度) 通常在星系中心最内部的核区( 小于几个秒差距) 被发现,因而活动星系核被认为是其唯一的能量源。同其它没有检测到水脉泽辐射的活动星系核相比,水脉泽寄主活动星系核可能隐含着某种或某些特殊性质。基于此我们调研了已经公开发表的所有水脉泽源的 X 射线观测情况,得到了一个有 X 射线观测研究结果的子样本( 39 个源) 。由它们的 X 射线光度以及估算的黑洞质量,导出了它们的无量纲吸积率( logL2-10keV /LEdd,其中 L2-10keV和 LEdd分别是 2 - 10keV 的固有光度和爱丁顿光度) ; 与距离范围相当的、没有检测到水脉泽的活动星系核样本相比,发现脉泽寄主活动星系核有较高的吸积率。进一步分析比较这两个活动星系核样本的质量吸积率,也发现类似的趋势。此外,为了探索吸积率和水脉泽辐射间可能的内在联系,我们对它们的脉泽光度和吸积率进行了统计分析,然而结果显示二者之间没有明显的相关性。