华北克拉通中生代伸展构造研究的几个问题及其在岩石圈减薄研究中的意义

总结了华北克拉通及周边以变质核杂岩和穹隆为代表的伸展构造研究的进展和存在的问题,提出了值得进一步研究的几个重要问题及其在华北克拉通破坏和岩石圈减薄研究中的意义。以变质核杂岩和穹隆为窗口,开展推覆向伸展的转化机制、区域性伸展运动学特征、剪切应变类型、伸展构造发育的时间和过程的研究,有助于深入探讨增厚地壳向伸展减薄转化的起因和过程,确定减薄的区域运动学方式及时限,查明伸展构造变形对地壳及岩石圈减薄的贡献。这方面的研究将提升华北伸展构造研究的水平,有助于查明岩石圈减薄的地壳响应,为探讨华北克拉通破坏和减薄的时限、机制、模式及深部动力学问题提供直接的构造证据。     

基于脉冲星计时的航天器自主定位误差估计方法

目前很多学者希望从"X射线脉冲星自主导航"的导航算法研究入手,利用数据分析或仿真进行验证.其中关于航天器自主定位的误差估计方法、误差量级和各种影响因素的讨论,并没有在给定详细初始条件的基础上系统性地说明问题.为了分析上述问题,需从天体测量学的角度出发,对自主定位的各种误差源及其影响因素进行探讨和误差量级的估计.首先,由...     

系外行星系统掩星周期变化研究进展

在掩星法发现的系外行星系统中,如果存在其他未知的伴星绕同一颗恒星运动,掩星行星由于受到伴星引力的影响,运动轨道将发生变化,轨道周期不再是常数,而是变化的。利用这种变化探测掩星系统中的其他行星,已成为一种新的方法。主要介绍了未知行星与掩星行星之间的引力作用引起的掩星周期变化效应,以及掩星周期变化法探测系外行星的理论和研究进展状况,最后简要讨论了几种影响掩星周期变化的其他因素:共轨行星、卫星、潮汐效应、相对论效应及恒星的引力四极矩等。     

冀北金台子盆地早白垩世酸性火山岩地球化学、锆石年代学及其地质意义

华北克拉通在中生代以来遭受了显著破坏。前人的研究对克拉通破坏的机制和峰期取得了较大共识, 但是关于克拉通破坏的启动时间一直存在争议。本文通过对冀北金台子中生代盆地构造特征及其填充的火山岩地球化学和年代学进行分析, 为华北克拉通破坏启动时间提供新的约束。研究表明, 金台子盆地为一伸展断陷盆地。盆地呈北东-南西向展布, 东侧被正断层控制, 西侧为地层超覆边界。盆地内自下而上发育后城组、白旗组、啕北营组、九佛堂组火山-沉积组合。后城组是一套稳定的河流相红色砂砾岩沉积地层;白旗组和啕北营组主体为巨厚层流纹岩、流纹质凝灰熔岩, 局部夹安山岩和火山碎屑岩;九佛堂组是一套以砾岩、砂砾岩等为主体的碎屑岩。地球化学分析表明金台子盆地中发育的酸性火山岩源于地壳重熔。锆石U-Pb年代学研究显示, 金台子盆地内流纹岩自约145 Ma开始广泛喷发并形成巨厚层的酸性火山岩地层, 表明此时在华北北缘地区的岩石圈减薄和破坏可能就已非常剧烈, 据此华北克拉通在其北缘的破坏至少应早于145 Ma。     

孙吴地区中侏罗世白云母花岗岩的年代学与地球化学:对蒙古-鄂霍茨克洋闭合时间的限定

本文对孙吴地区白云母花岗岩行了锆石LA-ICP-MS U-Pb年代学和岩石地球化学研究,确定其形成时代、岩石成因,从而揭示区域构造背景。孙吴地区白云母花岗岩中的锆石均呈半自形-自形,振荡生长环带明显,暗示其岩浆成因。测年结果显示,白云母花岗岩形成于168Ma,为中侏罗世岩浆事件的产物。岩体具有高硅(Si O2=74.61%~80.16%)、富铝(Al2O3=10.59%~13.90%)、贫铁(Fe2O3=0.11%~0.3%)等特征,在化学上属于准铝质-过铝质(A/CNK=0.97~1.13)系列。孙吴地区白云母花岗相对富集轻稀土元素(LREEs)和大离子亲石元素(LILEs),亏损重稀土元素(HREEs)和高场强元素(HFSEs)。锆石的εHf(168Ma)=+7.53~+11.66,二阶段的模式年龄(tDM2)变化于595~966Ma之间。上述特征表明,孙吴地区中侏罗世白云母花岗岩的岩浆起源于新增生加厚陆壳物质的部分熔融。结合在大兴安岭与小兴安岭衔接地区变质杂岩和冀北-辽西地区区域性地层不整合面的存在,表明大兴安岭西坡-冀北-辽西地区中侏罗世经历了一次与蒙古-鄂霍茨克洋闭合有关的陆壳加厚过程。因此,研究区内中侏罗世白云母花岗岩的形成应与蒙古-鄂霍茨克洋闭合过程中的陆-陆碰撞作用有关,而与古环太平洋向欧亚大陆的俯冲作用无关,其形成时代也限定额尔古纳地块西北部蒙古-鄂霍茨克洋的闭合时间应为中侏罗世。     

基于北斗卫星导航系统的飞行物轨迹标记法

为了实时准确地掌握和了解导航系统飞行物的位置和空间关系,以提高北斗系统的运行准确性,该文根据北斗卫星导航系统不间断授时服务特点,提出一种利用北斗卫星授时信号估计空间飞行物轨迹的方法。卫星下发的授时信号到达用户终端的过程中,受到空间飞行物的遮挡而产生扰动。用户终端将接收的扰动信号的变化量通过各种网络汇聚到数据中心,如果用户终端、空间星座和地面数据中心的时钟同步,在多个用户终端存在的条件下,将数据中心计算出的飞行物的时空参量等信息标注到空间地理信息系统上,连接这些空间点,就可以绘制出空间飞行物的运动轨迹。     

Two-frequency timing of the pulsar B1937+21 in Kalyazin and Kashima in 1997–2002

We present the results from our timing of the millisecond pulsar B1937+21, performed jointly since 1997 on two radio telescopes: the RT-64 in Kalyazin (Russia) at a frequency of 0.6GHz and RT-34 in Kashima (Japan) at a frequency of 2.15 GHz. The rms value of the pulse time of arrival (TOA) residuals for the pulsar at the barycenter of the Solar system is 1.8 μs (the relative variation is ≈10^?14 over the observing period). The TOA residuals are shown to be dominated by white phase noise, which allows this pulsar to be used as an independent time scale keeper. The upper limit for the gravitational background energy density Ω_gh² at frequencies ≈6.5 × 10^?9 Hz is estimated to be no higher than 10^?6. Based on the long-term timing of the pulsar, we have improved its parameters and accurately determined the dispersion measure and its time variation over the period 1984–2002, which was, on average, ?0.00114(3) pc cm^?3 yr^?1.     

Timing characteristics of the hard X-ray emission from bright X-ray pulsars based on INTEGRAL data

We review the results of a timing analysis of the observations for ten bright X-ray pulsars (with fluxes >100 mCrab in the 20–100 keV energy band) that fell within the INTEGRAL field of view from 2003 to 2007. The dependence of the pulse profile on the energy and intrinsic source luminosity has been investigated; particular attention has been paid to searching for changes in the pulse profile near the cyclotron frequency. The dependence of the pulsed fraction for X-ray pulsars on their luminosity and energy band has been studied in detail for the first time.     

Climate Change of 4°C Global Warming above Pre-industrial Levels

Using a set of numerical experiments from 39 CMIP5 climate models, we project the emergence time for 4°C global warming with respect to pre-industrial levels and associated climate changes under the RCP8.5 greenhouse gas concentration scenario. Results show that, according to the 39 models, the median year in which 4°C global warming will occur is 2084. Based on the median results of models that project a 4°C global warming by 2100, land areas will generally exhibit stronger warming than the oceans annually and seasonally, and the strongest enhancement occurs in the Arctic, with the exception of the summer season. Change signals for temperature go outside its natural internal variabilities globally, and the signal-to-noise ratio averages 9.6 for the annual mean and ranges from 6.3 to 7.2 for the seasonal mean over the globe, with the greatest values appearing at low latitudes because of low noise. Decreased precipitation generally occurs in the subtropics, whilst increased precipitation mainly appears at high latitudes. The precipitation changes in most of the high latitudes are greater than the background variability, and the global mean signal-to-noise ratio is 0.5 and ranges from 0.2 to 0.4 for the annual and seasonal means, respectively. Attention should be paid to limiting global warming to 1.5°C, in which case temperature and precipitation will experience a far more moderate change than the natural internal variability. Large inter-model disagreement appears at high latitudes for temperature changes and at mid and low latitudes for precipitation changes. Overall, the inter-model consistency is better for temperature than for precipitation.     

Spatial Distribution of Shelf- and Slope-Dwelling Fishes Collected by Bottom Longline off Lanzarote and Fuerteventura, Canary Islands

Abstract. A total of 1789 fish belonging to 38 families and 73 species were collected at depths between 18 and 1102 m during 216 bottom longline operations off Lanzarote and Fuerteventura, Canary Islands, between February 1994 and December 1995. For each species the depth distribution is provided. Length-weight and depth-size relationships are reported for three shelf-dwelling species. The bigger-deeper relationship found in two of them contrasts with the bigger-shallower pattern of the deeper living trichiurid Lepidopus caudatus . In November 1997, nine additional bottom longline operations were carried out off eastern Fuerteventura at depths between 805 and 1217 m. In this area, after earlier studies in October 1995, a spawning aggregation of the morid Mora moro was encountered for the second time. The catches of 1997 revealed a strongly male-biased sex ratio. Also, the males showed a significantly lower gonadosomal index than two years earlier. These findings indicate slight interannual variations in reproductive timing and an earlier arrival of male Mora moro at the spawning grounds. Clear variations in the number of fish collected at adjacent sites possibly reflect a preference for distinct microhabitats. Preliminary evidence of local upwelling of cold water above the spawning grounds is provided by satellite imagery.