绥中某电力设备站场区地震危险性分析

绥中某电力设备站是东北地区较重要的电力设施,场址位于长期隆起的绥中剥蚀丘陵上。通过现场实地勘察,获得区域、近区域地震活动、地质构造、地球物理场等资料,并对工程场址进行了地震危险性分析。按工程建筑物抗震设计规范要求,分别给出了50年63%、10%和2%超越概率水平的基岩峰值加速度及反应谱,计算出地震动参数,为该电力设备站建设提供了抗震设计依据。     

球状星团M79天区169颗恒星的位置和自行归算及其成员概率

使用上海天文台佘山40cm折射望远镜拍摄的底片资料,对球状星团M79中心附近15’×15’天区内106颗恒星和63颗Tycho-2星,以《Tycho-2星表》中M79附近1°×1°天区内上述63颗Ty cho-2星的位置和自行为参考,归算得到了所有169颗恒星的位置和自行,并估计了其成员概率。     

冬季一次南支槽活动对川南城市群空气重污染过程影响研究

针对四川盆地大气污染防治工作的需要,应用2016年12月26日至2017年1月11日川南城市群(宜宾、自贡、泸州、内江、乐山)大气污染物浓度观测数据和气象数据,采用数理统计和污染天气诊断分析等方法,分析了这次川南城市群跨年度空气重污染过程的污染变化特征及其气象成因.结果表明:南支槽加强并引导其槽前西南干暖气流北上,致使...     

强震作用下地铁车站结构损伤破坏的高效分析方法

地下结构的关键构件(如柱子等)在地震作用下可能发生破坏,进而影响结构体系的整体稳定性。在借鉴传统反应位移法的基础上,提出了一种新的位移时程反应分析方法,采用该方法对日本神户大开地铁车站进行地震响应分析。结果表明:位移时程反应分析方法能够考虑土-结构相互作用、材料非线性、几何非线性、水平地震与竖向地震的耦合作用及地震动传播的时空效应,适用于地下结构地震反应分析,利用该方法得出的地铁车站结构变形及损伤破坏与实际震害观察具有较好的一致性,并指出大开地铁车站结构的整体垮塌是由于柱子剪坏和高轴压联合作用所致。     

卧龙自然保护区内海拔梯度上林窗如何影响植物多样性?（英文）

Understanding the underlying ecological processes that control plant diversity within(α-diversity) and among(β-diversity) forest gaps is important for managing natural forest ecosystems, and it is also a prerequisite for identifying the formation and maintenance mechanisms of forest plant communities. In this study, we focused on the interrelationships among habitat type(gap/non-gap plots), gap size, elevation and environmental factors, and we explored their effects on plant diversity(α-diversity and β-diversity). To do this, a total of 21 non-gap(i.e., closed canopy) plots(100 m2) and 63 gap plots, including 21 with large gaps(200–410 m2), 21 with medium gaps(100–200 m2) and 21 with small gaps(38.5– 100 m2),were selected along an elevational gradient in a subalpine coniferous forest of southwestern China. Using structural equation models(SEMs), we analyzed how forest gaps affected plant diversity(α-diversity and β-diversity) along an elevational gradient. The results showed that(1) as elevation increased, unimodal patterns of α-diversity were found in different-sized gaps, and β-diversity showed a consistent sinusoidal function pattern in different-sized gaps. The gap size was positively related to α-diversity, but this effect disappeared above 3500 masl. Moreover, the patterns of α-diversity and β-diversity in non-gap plots were irregular along the elevational gradient.(2) SEMs demonstrated that many environmental factors, such as the annual mean air temperature(AMAT), ultraviolet-A radiation(365 nm, UV-A365), ultraviolet-B1 radiation(297 nm, UV-B297), moss thickness(MT), soil carbon/nitrogen ratio(C/N ratio), NH4-N and NO3-N, were significantly affected by elevation, which then affected α-diversity and β-diversity. The photosynthetic photon flux density(PPFD), UV-A365 and UV-B297 were significantly higher in plots with forest gaps than in the non-gap plots. Moreover, the PPFD and UV-A365 were positively and directly affected by gap size. Surprisingly, except for the NH4-N and the C/N ratios, the below-ground environmental factors showed little or no relationships with forest gaps. All of these effects contributed to plant diversity. Overall, the above-ground environmental factors were more sensitive to gap-forming disturbances than the below-ground environmental factors, which affected α-diversity and β-diversity. The predicted pathway in the SEMs of the elevational effects on α-diversity andβ-diversity was relatively complicated compared with the effects of forest gaps. These results can provide valuable insights into the underlying mechanisms driving the diversity-habitat relationship in the subalpine coniferous forests of southwestern China.     

海底地下水和海水混合营养盐变化的模拟实验研究

1 引言 海底地下水排泄(submarine groundwater dis-charge,SGD)早在几世纪前就被发现,直到20世纪80年代,LOCIZ工作组成立并通过一系列的研究,让人们才逐渐认识地下水向沿海海域排泄是海岸带陆海相互作用的一个重要过程[1-2].近年来随着监测技术的发展,特别是同位素示踪剂技术的应用[3-4],已证实SGD是一个全球性的现象.     

第二代天体测量卫星及后依巴谷地面天体测量的进展

简述了后依巴谷的天体测量工作。首先给出了第二个天体测量卫星Gaia的最新进展、最近提出的JAMSE和OBSS计划的简介,以及包含天体测量内容的SIM PlanetQuest计划的情况; 叙述了多波段天体参考架的建立和维持,特别是依巴谷星表向暗星方向的扩充和数字巡天,以及其他地面观测计划,如双星和聚星、太阳系天体的观测等;介绍了天体测量与天体物理结合的几个研究课题的进展;最后对我国自然科学基金会“十一五”天体测量优先发展的方向与内容提出建议。     

HST WFPC2天体测量和测光方法最新进展

对于哈勃空间望远镜(HST)来说，其广角行星照相机(WFPC2)的CCD性能的数据处理校正对提高天体测量和测光结果的精度有着重要意义。最近几年由于WFPC2对精度要求越来越高，其数据处理方法和校正方法包括点扩散函数、行误差和畸变修正等各个方面的研究都有了很大改进和进展。对近年来上述方面的最新进展作了介绍，并评价了其优缺点，提出了一些有待解决的问题。     

疏散星团NGC6530的成员研究和空间运动

利用上海天文台40厘米折射望远镜照相观测资料所得出的恒星自行,按最大似然原理确定了疏散星团NGC6530天区内恒星的成员概率．分析表明星团成员确定是非常有效的,成员概率p≥0．9的恒星计有250颗．最后,确定了星团的空间运动,并作了简单的讨论．