紫坪铺水库水位变化对剪切波分裂参数的影响

本文通过对2006—2009年四川紫坪铺水库库区8个地震台站记录的地震事件,采用剪切波分裂方法获得了水库库区剪切波分裂参数,并结合地震活动性与水库水位之间的变化关系,分析了紫坪铺水库库区地壳应力的变化特征.剪切波分裂结果显示该研究区域快波偏振方向有两个,分别为北东向和北西向,充分体现了紫坪铺水库地区地壳应力是由北西向的区域主压应力与南东走向的龙门山断裂带综合作用的结果.慢波延迟时间平均值为5.8ms·km-1,慢波延迟时间较大的地区位于库坝和库尾,分别是水库蓄水排水引起地壳应力变化最大的区域.对比慢波延迟时间的变化和水库水位的变化显示了慢波延迟时间与水库水位之间的一致变化关系,揭示了水库的蓄水排水对地壳应力的影响.     

两种精化的对流层延迟改正模型

对流层延迟是全球导航卫星系统(Global Navigation Satellite System,GNSS)导航定位中的重要误差源,其量值主要受气象条件影响.采用传统对流层建模思路,利用GPT2模型来提供相对准确的气温、气压和相对湿度,然后利用Saastamoinen模型来计算天顶对流层延迟,由此构建了GPT2+Saas模型;采用新的对流层建模思路,直接针对天顶对流层延迟的时空特性建模,构建了与GPT2+Saas模型相匹配的GZTDS格网模型.以GGOS Atmosphere格网数据为参考,GPT2+Saas模型(Bias:0.2cm;RMS:4.2cm)和GZTDS模型(Bias:0.2cm;RMS:3.7cm)较UNB3m模型精度分别提升34%和43%.以IGS(International GNSS Service)数据为参考,GPT2+Saas(Bias:0.5cm;RMS:4.7cm)和GZTDS(Bias:-0.3cm;RMS:3.8cm)相对UNB3m模型精度分别提升10%和27%.针对GPT2+Saas模型在少数测站出现精度异常的情况进行了研究,探讨了可能的原因.在两种不同思路构建的精化对流层模型中,GZTDS模型不仅表现出更高的精度,而且在时间稳定性和地理稳定性上也表现出优越性.     

基于二维三分量伪谱法模拟数据的EDA介质中横波分裂研究

为了检测定向裂隙介质中横波分裂的方位属性特征,分析地震属性随裂隙密度和方位变化,采用人工吸收边界和反周期扩展边界,用伪谱法获得不同裂隙密度和不同方位地质模型三分量地面记录;应用时频分析和剪切波偏振分析研究由于裂隙方位和密度引起的横波分裂.结果显示,裂隙密度和方位决定着横波分裂的时差和偏振.快慢横波的延迟时间随裂隙密度增大而增加,不同方位相同裂隙密度的横波分裂时差有微小的变化.在45°方位检测时间延迟时间最大.通过时频分析,可以看到不同方位的瞬时主频有显著的变化,在横波分裂处瞬时主频有明显变化.因此,瞬时主频和快横波的偏振以及延迟时间可以作为裂隙方位和密度的指示.     

由Saastamoinen和Hopfield模型推算水汽含量的比较与分析

详细介绍利用ＧＰＡ数据推算大气水汽含量的过程。根据Ｓａａｓｔａｍｏｉｎｅｎ和Ｈｏｐｆｉｅｌｄ两种模型利用实测数据对大气水汽含量进行了推算,并对其结果进行了比较和分析,得到了一些有益的结论。     

Groundbased Doas UV/visible measurements at Kiruna (Sweden) during the sesame winters 1993/94 and 1994/95.

Zenith sky observations of O3, NO2, OClO and BrO are reported, which were performed at Kiruna (67.9°N, 21.1°E) within the SESAME winters 1993/1994 and 1994/95. For both winters large total amounts of OClO were observed inside the polar vortex at twilight, indicating the degree and the temporal variation of the halogen activation of the polar stratosphere. Occasionally OClO could also be observed outside the polar vortex, most likely due to export of halogen activated vortex air masses into the ambient stratosphere. BrO could also be detected in winter 1994/95, with the largest slant column amounts (5·1014/cm2) occuring in the polar vortex in mid-winter. Similar abundances of stratospheric BrO were observed at dusk and dawn, for both, air masses inside and outside the vortex. This observation is in reasonable agreement with previous studies on stratospheric BrO (observations and models) of Wahner et al. (1992), Arpag et al. (1994), Krug et al. (1996), and Lary et al. (1996a,b), but partly in disagreement with those of Solomon et al. (1989), Fish et al. (1995), and Sessler et al. (1996).     

射电源结构对VLBI天体测量的影响

目前利用VLBIMK3系统确定的延迟测量的精度约为30ps,在这样的精度下,改善计算延迟的理论模型,考虑各种微扰改正（包含30ps量级）是非常重要的。在VLBI天休测量和测地计算的各种软件中,至今尚未计及射电源结构对延迟的影响。本文利用两子源模型对源结构延迟的大小及随时间的变化进行了计算,讨论了源结构延迟对VLBI天测和测地参数的影响,指出：（1）除对某些VLBI天测的射电源作长期的监测与研究,给出它们的双频综合图外,对大多数源可采用简单的两子源模型;（2）源结构对延迟的影响主要依赖于基线相对于源形态的主要特征的空间投影;（3）源结构延迟对天测和测地参数的影响达厘米和亚毫角秒量级。     

一个偶数阶时滞微分方程的振动准则

讨论了一类偶数阶时滞微分方程x~(n)(t)+p(t)f(x(g(t)))=0的振动性。通过转化到一个一阶时滞微分不等式,得到了该方程的一切解振动的一个新的充分性条件。作为n=2的情况,它包含了魏俊杰最近的结果。     

Astronomical-topographic levelling using high-precision astrogeodetic vertical deflections and digital terrain model data

At the beginning of the twenty-first century, a technological change took place in geodetic astronomy by the development of Digital Zenith Camera Systems (DZCS). Such instruments provide vertical deflection data at an angular accuracy level of 0.̋1 and better. Recently, DZCS have been employed for the collection of dense sets of astrogeodetic vertical deflection data in several test areas in Germany with high-resolution digital terrain model (DTM) data (10–50 m resolution) available. These considerable advancements motivate a new analysis of the method of astronomical-topographic levelling, which uses DTM data for the interpolation between the astrogeodetic stations. We present and analyse a least-squares collocation technique that uses DTM data for the accurate interpolation of vertical deflection data. The combination of both data sets allows a precise determination of the gravity field along profiles, even in regions with a rugged topography. The accuracy of the method is studied with particular attention on the density of astrogeodetic stations. The error propagation rule of astronomical levelling is empirically derived. It accounts for the signal omission that increases with the station spacing. In a test area located in the German Alps, the method was successfully applied to the determination of a quasigeoid profile of 23 km length. For a station spacing from a few 100 m to about 2 km, the accuracy of the quasigeoid was found to be about 1–2 mm, which corresponds to a relative accuracy of about 0.05−0.1 ppm. Application examples are given, such as the local and regional validation of gravity field models computed from gravimetric data and the economic gravity field determination in geodetically less covered regions.     

Accuracy analysis of vertical deflection data observed with the Hannover Digital Zenith Camera System TZK2-D

This paper analyses the accuracy of vertical deflection measurements carried out with the Digital Zenith Camera System TZK2-D, an astrogeodetic state-of-the-art instrumentation developed at the University of Hannover. During 107 nights over a period of 3.5 years, the system was used for repeated vertical deflection observations at a selected station in Hannover. The acquired data set consists of about 27,300 single measurements and covers 276 h of observation time, respectively. For the data collected at an earlier stage of development (2003 to 2004), the accuracy of the nightly mean values has been found to be about 0′′.10−0′′.12. Due to applying a refined observation strategy since 2005, the accuracy of the vertical deflection measurements was enhanced into the unprecedented range of 0′′.05 − 0′′.08. Accessing the accuracy level of 0′′.05 requires usually 1 h of observational data, while the 0′′.08 accuracy level is attained after 20 min measurement time. In comparison to the analogue era of geodetic astronomy, the accuracy of vertical deflection observations is significantly improved by about one order of magnitude.     

2005年-2014年京津冀对流层NO2柱浓度时空变化及影响因素

基于臭氧监测仪OMI对流层NO₂柱浓度产品研究了京津冀城市群2005年-2014年NO₂时空变化及影响因素:(1)10年柱浓度年均增长率为3.35%,且年度波动较大。忽略2008年国家奥运会的环境治理所引起的变化,2005年-2011年NO₂呈逐渐升高趋势;2012年-2014年呈逐渐降低趋势,以2014年下降最为显著。(2)呈西北低东南高的趋势。燕山-太行山山系以北的承德和张家口市浓度较低,山系以南主要有北京-天津-唐山与石家庄-邢台-邯郸两个污染中心。(3)京津冀北部三面环山不利于NO₂的扩散,夏季丰富的降水对NO₂具有显著湿沉降作用。(4)通过相关性分析、文献及国家政策印证等方法,发现地区产业及能源结构很大程度上决定了地区的污染来源。北京市10年来第三产业一直处于主导且稳步提高,煤炭消耗量低,但汽车保有量增加了1.5倍,主要来源为机动车尾气排放;天津市第二产业比第三产业比重略高,煤炭消耗量是北京的两倍之余,但汽车保有量仅是北京市的一半,由此可知工业排放和机动车是共同来源;河北省第二产业比重很高,燃煤量占京津冀地区的80.6%,河北省工业排放是NO₂的主要来源,但近几年随着机动车保有量的剧增,其尾气排放分担率不可小觑。