海上E区天然气水合物地质、地震、地球化学特征综合研究与成藏远景预测

本文提出一种将地质、地震、地球化学分析相结合的方法,以研究海区天然气水合物的成藏条件,首先用物源、构造、沉积和地温等资料进行地质分析,确定海区天然气水合物成藏的地质条件;然后根据对水合物的地震属性（BSR,AVO,BZ等）分析和正演模拟研究,预测水合物及其游离气的存在,结合地质条件,圈定出水合物成藏的有利区带;最后结合对水合物主要成分（甲烷及烃类等）的地球化学异常分析,对研究区天然气水合物成藏的远景作出评价．野外实践结果表明,这种综合研究方法是有效可行的,为海区天然气水合物勘探提供了一种新的研究途径．     

基于图像分析的双台面波相速度频散曲线快速提取方法

双台波形的互相关方法是面波相速度频散曲线提取的一种常用方法。传统的方法精度不高,效率较低。本文提出了一种基于图像分析的频散曲线快速提取方法,采用图像显示互相关振幅矩阵,且提出了快速追踪整条频散曲线的算法,并用Matlab编写了交互式的处理软件。基于这种方法编写的资料处理软件提高了双台相速度频散曲线提取的速度和精度,为大批量处理地震数据资料提供了坚实的软件基础。基于图像分析的方法可以更为清晰地展现出双台问的面波频散曲线的特征,对频散曲线的识别和分析也提供了更为有效的研究工具。     

化学与稳定同位素指纹示踪原油类污染:以广东南海两次小型溢油事件为例

化学和稳定同位素指纹是目前国际上用于示踪石油类污染来源及其环境命运的有效技术。通过气相色谱-质谱(GC—MS)分析可疑重油与被污染水体及植物表面污染物的饱和烃和芳烃分布以及生物标志化合物姥姣烷、植烷、“不可分辨的混合物”(UCM)等化学指纹特征,对比可疑重油与被污染水体表面漂浮重油的沥青质同位素组成,追踪了发生在广东省南海市的两次小型重油泄漏事件。结果揭示,2002年10月16日晚发生的污染事件源于某饲料公司锅炉房的重油泄漏;而2002年10月25日的泄漏事故则是某加油站重油渗漏所致。     

南梁煤矿多煤层开采地下水系统演化规律

煤层开采对所在矿区地下水系统有着重要影响.以往研究单煤层开采对地下水系统的影响较多,而对多煤层的影响研究甚少,特别对于我国西部缺水矿区.以南梁煤矿为例,运用地下水系统演化理论和岩石力学模拟等,对该矿井水文地质结构、矿井涌水变化规律、矿井地下水流场演变、矿井地下水化学成分变化等方面进行了综合分析研究,重构了多煤层开采条件...     

Simulation of the Unusual Solar Minimum with 3D SIP-CESE MHD Model by Comparison with Multi-Satellite Observations

The observations both near the Sun and in the heliosphere during the activity minimum between solar cycles 23 and 24 exhibit different phenomena from those typical of the previous solar minima. In this paper, we have chosen Carrington rotation 2070 in 2008 to investigate the properties of the background solar wind by using the three-dimensional (3D) Solar?CInterPlanetary Conservation Element/Solution Element Magnetohydrodynamic (MHD) model. We also study the effects of polar magnetic fields on the characteristics of the solar corona and the solar wind by conducting simulations with an axisymmetric polar flux added to the observed magnetic field. The numerical results are compared with the observations from multiple satellites, such as the Solar and Heliospheric Observatory (SOHO), Ulysses, Solar Terrestrial Relations Observatory (STEREO), Wind and the Advanced Composition Explorer (ACE). The comparison demonstrates that the first simulation with the observed magnetic fields reproduces some observed peculiarities near the Sun, such as relatively small polar coronal holes, the presence of mid- and low-latitude holes, a tilted and warped current sheet, and the broad multiple streamers. The numerical results also capture the inconsistency between the locus of the minimum wind speed and the location of the heliospheric current sheet, and predict slightly slower and cooler polar streams with a relatively smaller latitudinal width, broad low-latitude intermediate-speed streams, and globally weak magnetic field and low density in the heliosphere. The second simulation with strengthened polar fields indicates that the weak polar fields in the current minimum play a crucial role in determining the states of the corona and the solar wind.     

UV transit observations of EUV-heated expanded thermospheres of Earth-like exoplanets around M-stars: testing atmosphere evolution scenarios

The detection and investigation of EUV heated, extended and non-hydrostatic upper atmospheres around terrestrial exoplanets would provide important insights into the interaction of the host stars plasma environment as well as the evolution of Earth-type planets their atmospheres and possible magnetic environments. We discuss different scenarios where one can expect that Earth-like planets should experience non-hydrostatic upper atmosphere conditions so that dynamically outward flowing neutral atoms can interact with the stellar plasma flow so that huge hydrogen coronae and energetic neutral atoms (ENA) can be produced via charge exchange. By observing the size of the extended upper atmospheres and related ENA-clouds and by determining the velocities of the surrounding hydrogen atoms, conclusions can be drawn in respect to the origin of these features. Due to the large number of M-type stars in our neighbourhood and their long periods of strong and moderate stellar activity in comparison to G-stars, we expect that M-type stars represent the most promising candidates for the detection of hydrogen ENA-clouds and the subsequent study of the interaction between the host star and the planets?? upper atmosphere. We show that the low mass of M-type stars also makes them preferable targets to observe extended hydrogen clouds around terrestrial exoplanets with a mass as low as one Earth mass. Transit follow-up observations in the UV-range of terrestrial exoplanets around M-type stars with space observatories such as the World Space Observatory-UV (WSO-UV) would provide a unique opportunity to shed more light on the early evolution of Earth-like planets, including those of our own Solar System.     

Radio Observations of the S5 Sample

The S5 sample was monitored on a monthly basis since December 2008 at Urumqi Observatory. Most of the sources are variables and a considerable proportion (about 20%) exhibited a significant inter-month flux variability (modulation index >?4%) during the 1-year observation.     

台湾-吕宋岛弧巴士段火山活动的热模拟

岛弧火山活动的数值热模拟研究是俯冲带构造热演化研究的重要方面,也是验证地表观测结果的重要方法。选取台湾-吕宋岛弧巴士段内东火山链(EVC)的甘米银活火山和西火山链(WVC)的加拉鄢死火山,根据地质和地球物理条件,进行了有限元热模拟计算。在计算模拟甘米银活火山和加拉鄢死火山现今的热流分布的基础上,分析了二者的差异。模拟结果表明,甘米银活火山顶部至周边30km热流值有明显升高,越靠近火山热流值越高且增加速率越快,岩浆房正上方的热流高达310mW.m-2。加拉鄢死火山顶部及周边热流略有升高,热流增量从周边40km处的小于3mW.m-2缓慢增加到火山顶部的15mW.m-2。     

福建中南部沿岸海域潮汐特征分析

利用2004、2007、2010年在福建中南部沿海长期验潮站和临时验潮站获取的实测逐时潮位资料,采用基于最小二乘原理的潮汐调和分析方法,分析了福建中南部沿岸海域18个验潮站的潮汐调和常数,并根据调和常数分析了沿岸海域潮汐特征.结果表明:福建中南部沿岸海域以向南传播的半日分潮为主,传播至浮头湾以南海域后衰减明显,对应平潭至浮头湾海域的潮汐性质为半日潮,古雷半岛以南海域为不规则半日潮混合潮;福建中南部沿岸海域自北部平潭向南至诏安,平均海平面升高约25 cm,潮差减小超过3 m,平均大潮差与平均小潮差之差也减小2 m左右,理论高潮位降低约1.5m,而理论低潮位升高约2 m,潮时推迟约2h.     

弹性液舱内液体晃荡实验研究

通过物理模型实验,对水平简谐激励下弹性矩形液舱内液体晃荡问题进行了研究。实验中给出了不同液深和不同激励振幅下弹性液舱内液体最低阶固有频率。采用影像采集与分析系统获得液舱内自由液面的形状和高度,通过压力采集系统得到舱壁上的压力分布。实验中分析了不同液深、不同激励频率下弹性和刚性液舱内自由液面高度和晃荡压力的变化特性。比较了弹性和刚性液舱内不同位置处自由液面高度随外界激励频率的变化规律,以及舱壁上不同位置处的压力峰值随外界激励频率的变化规律。结果表明:非共振情况下,弹性和刚性实验结果及理论值三者的波高和压力较为接近。共振情况下,弹性和刚性波高基本相等,在近舱壁处二者明显大于理论值,而在远离舱壁处二者与理论值存在一定差别;弹性压力较刚性压力略小,但二者与理论值差别较大。