海温异常对东亚夏季风强度先兆信号的影响

利用ERA-Interim再分析资料、NOAA海温资料、CMAP格点降水资料和中国气象站降水资料,通过合成、相关和回归分析等方法研究了1979—2012年东亚夏季风强度与其先兆信号的关系,并分析了热带海温异常的可能影响。研究表明:东亚夏季风先兆指数反映了2月200 hPa纬向风距平的主要模态特征 (EOF1),前冬热带中东太平洋海温偏低 (高),2月亚洲地区西风急流位置偏北 (偏南),东亚夏季风先兆指数偏强 (弱)。前期热带海温异常对东亚夏季风强度有明显影响,前冬热带中东太平洋海温偏低 (高) 有利于东亚夏季风偏强 (弱)。2月亚洲中纬度地区纬向风异常特征在春季不能持续,先兆信号与东亚夏季风强度的联系主要源自热带海洋。     

基于CEI的飞船交会对接远程导引段的轨道确定方案

探讨了CEI技术在飞船交会对接远程导引段的高精度定轨与实时监控的能力。仿真结果表明:精密定轨中采用可视弧段较长的单站可使相对位置精度达百米以内,速度达厘米/秒级。采用单一绝对扩展卡尔曼滤波器的方案进行实时轨道计算,采用滤波稳定后固定模糊度的方法可以使相对轨道位置精度达十米级,速度精度达厘米/秒级,事后及实时的轨道精度均满足远程导引段的精度指标。     

The Influence of Merges with Various Mass Ratios on the Spins of Black Holes

The distribution of black hole spins in consideration of only the effect of merges is discussed. The angular momentum after merging is treated via the post-Newtonian approximation, and the effects of merges under different conditions are simulated by adopting the Monte Carlo method. The obtained results indicate that the major merge cannot make the distribution of black hole spins stable, but the minor merge can make the black hole spin smoothly slow down. The distribution of black hole spins can stay at a stable level with the overwhelming proportion of small spins, when the mass ratio of merging black holes takes the form of power-law function. In addition, based on the simulated results, the possible relationship between radio-loud active galactic nuclei (AGNs) and black hole spins is also discussed. Finally, the distribution of radio loudness is calculated and presented.     

鲁西新泰孟家屯2.7Ga变质沉积岩与黑云斜长片麻岩锆石Hf同位素特征

对出露于山东新泰孟家屯2.7Ga的孟家屯岩组中石榴石石英岩(M08)、含十字石石榴石黑云母石英片岩(D242-Y2)和黑云斜长片麻岩(M03)(TTG质片麻岩)进行锆石Lu-Hf同位素分析。石榴石石英岩锆石核部176Lu/177Hf、176Hf/177Hf变化范围为0.001730～0.002546、0.281249～0.281360,锆石变质边部176Lu/177Hf、176Hf/177Hf变化范围为0.000123～0.002070、0.281241～0.281318;含十字石石榴石黑云母石英片岩锆石核部176Lu/177Hf、176Hf/177Hf变化范围为0.001334～0.002169、0.281226～0.281324,锆石变质边部176Lu/177Hf、176Hf/177Hf变化范围为0.000445～0.001375、0.281227～0.281309;黑云斜长片麻岩锆石176Lu/177Hf、176Hf/177Hf变化范围为0.000315～0.000847、0.281186～0.281265。孟家屯岩组石榴石英岩、含十字石石榴石黑去母石英片岩中碎屑(岩浆)锆石和黑云斜长片麻岩中岩浆锆石的εHf(t)分别为3.75～7.26、2.31～7.26和3.21～6.27,同时TDM1与其U-Pb年龄非常接近,表明它们起源于新生地壳的部分熔融。结合区域研究资料认为,2.7Ga是鲁西重要的一期构造岩浆热事件,也可能是华北克拉通重要的构造岩浆活动时期。变质沉积岩中许多变质增生锆石相对于核部岩浆锆石低176Lu/177Hf、高176Hf/177Hf,显示变质作用过程中石榴石的存在对锆石的Lu-Hf同位素体系有很大影响。     

Source apportionment and distribution of atmospheric mercury in urban Beijing,China

The concentration of gaseous elemental mercury (GEM) in the atmosphere of urban Beijing was measured from October 2003 to September 2004 to investigate the origins and spatial-temporal variations of atmospheric Hg. The mean value of Hg concentration is 17.1 ng·m-3 (n=653). The atmospheric Hg data showed spatial-temporal variations throughout the duration of our observation. The maximum GEM concentration (53.7 ng·m-3) was observed at Gucheng in the western area of urban Beijing. The GEM concentrations increased from the north to the south of the studied area, and were higher in winter than in summer. The highest and lowest monthly averages of GEM concentrations were measured to be 23.3 and 4.1 ng·m-3 in January and July, respectively. In addition, GEM concentrations are higher in the daytime than at night in Autumn and from 14 March to 15 April, but daily GEM variation showed an inverse pattern from 22 April to 22 May. In winter, two peak values of GEM concentrations occurred at 13:30 and 21:30. Daily variation of GEM concentrations in summer was the lowest in the four seasons. Mercury from coal combustion was estimated to be the main source of anthropogenic emissions in Beijing from October 2003 to September 2004. Additionally, Hg emission from natural gas burning was estimated to be another dominant source of atmospheric Hg in Beijing.     

晋豫间黄河峡谷黄土状沙丘的光释光年代学探讨

通过对风陵渡-三门峡晋豫间黄河峡谷的地貌考察和1:50000 地形图(1970年)的分析,初步查明了黄河南岸黄土状沙丘的分布特征.选取河南省灵宝市豫灵镇阌底约75m高的黄土状沙丘剖面进行了观测和取样.根据该剖面的粒度分布特点,选取中颗粒(40～90μm)石英进行了光释光(OSL)测年研究.采用简化SAR法测量样品的等效剂量(De),其中5个样品与SAR法测量的De值对比,结果在误差范围内一致.对阌底剖面自上而下19个样品运用简化SAR法做了OSL年龄测定,其中8个还进行了4～11μm细颗粒石英简易多测片再生法(SMAR)OSL测年,两个粒级石英的OSL年龄测定值在测量误差范围内一致.初步结果表明,晋豫间黄河峡谷阌底黄土状沙丘发育不晚于距今约5.5万年前,并延续到全新世初期,风沙堆积速率在3.2万年前后曾出现显著变化.     

陕北能源化工基地采煤对地下水资源的影响及对策

陕北能源化工基地侏罗纪煤田是中国煤炭工业战略西移的首选基地,采煤引起的地下水资源及生态环境响应的研究是一个不可逾越的课题。从分析水文地质工程地质条件入手,将煤田区划分为7个水文地质结构类型和5个含水系统,按照排泄基准面进一步将含水系统划分若干地下水流子系统。在经验公式和数值法预测结果的基础上,综合考虑研究区实际,提出了本区能够保障生态、水资源和采煤安全的冒裂带高度为240 m,"三带"安全高度为300 m,并据此将煤采区划分为非导水区、无水导水区、贫水导水区和富水导水区。从水资源的角度提出了"保水采煤"、"煤水共采"和"含水层再造"的煤炭资源开发近期和中远期对策。     

Re–Os age of non-mineralized black shale from the Kupferschiefer, Poland, and implications for metal enrichment

Six samples of non-mineralized black shale from a Kupferschiefer section in the northern part of the Polish Zechstein Basin (Zdrada IG-8 drill hole: 1026.16–1026.90 m) were studied for Re–Os isotopes and selected major and trace elements. These black shales, averaging 5.82 wt.% C_org and 1.69 wt.% S_tot, display very low base metal values (up to 106 ppb Cu, 792 ppb Pb, and 144 ppb Zn) and have abundances of 64–1376 ppb Re and 0.37–1.25 ppb Os, with a ¹⁸⁷Os/¹⁸⁸Os ratio of 6.95–22.5. The regression of all Re–Os data yields an age of 247 ± 20 Ma, which is within the range of uncertainties of previous Rb–Sr and K–Ar geochronological studies. The scatter in the Re–Os data can be explained in terms of fluctuations in sedimentary conditions, i.e., restricted basin with terrestrial influence.