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。     

基于瑞典条分法数值解的边坡蒙特卡罗可靠性分析

本文基于瑞典条分法数值解的基本思想,建立了蒙特卡罗(Monte-Carlo)边坡可靠性分析计算模型,对云南省香格里拉县冷都复杂斜坡体前缘滑动体的稳定性进行了分析,计算结果表明该复杂斜坡体在目前状况下具有较高的稳定系数和可靠度,在降雨和地震作用下稳定性差,需要采取工程措施进行加固。     

重金属离子在胡敏酸-高岭石复合体上的吸附

本文研究了胡敏酸存在下高岭石对重金属离子的吸附行为。实验结果表明:①胡敏酸和Cu2 溶液按先后顺序或同时加入高岭石中反应,在Cu2 平衡浓度<10mg/L时,3种加入顺序对Cu2 的吸附量基本相同,当Cu2 平衡浓度>10mg/L时,(K Cu) HA和(K Cu HA)两种加入顺序对Cu2 的吸附量比(K HA) Cu的略大。②在pH=5时,胡敏酸-高岭石复合体对Cu2 的吸附量明显大于纯高岭石。这是由于胡敏酸含有大量的羧基和酚羟基等活性基团,吸附在高岭石上的胡敏酸增加了其表面吸附位,在复合体表面形成了S—HA—Cu三元配合物,且Cu2 的吸附量与复合体中胡敏酸的含量在一定范围内成正相关;③溶液pH值在4～7之间变化可调控复合体对Cu2 的吸附机制。④在Cu2 和Cd2 共存时,随着金属离子初始浓度的增大,Cu2 的吸附量呈直线上升,而Cd2 的吸附量增加缓慢,表明复合体对Cu2 的吸附能力比对Cd2 强。     

大别山南山岭石榴橄榄岩成因的岩石学研究

大别山罗田穹隆东南侧的南山岭石榴橄榄岩岩体面积小(173×133m~2),由贵橄榄石(75%)。透辉石(10%)和镁铝石榴石(15%)组成。本文通过岩石学及地球化学研究,并与大别山的碧溪岭、毛屋、饶拔寨、芝麻坊岩体以及其他地区的基性岩浆杂岩体(如红格岩体、元宝山岩体、柴北缘岩体)、残留地幔块体(五大连池、鹤壁、山旺)等不同成因的超镁铁岩进行对比后认为,该岩体属于火成成因,是镁铁-超镁铁杂岩体的一部分。表现在:橄榄岩呈块状构造,矿物分布均匀未见定向排列,镜下呈现典型的火成结构;FeO~T含量高(21.36%),Mg~#(0.77)低,Mg Ni/Fe Mn(3.06)<7,V(175.5×10~(-6))含量高于地幔块体成因的橄榄岩;REE总量偏低,LREE弱富集,(La/Yb)_N=3.1,低于饶拔寨、芝麻坊等残留地幔块体成因的橄榄岩。南山岭橄榄岩在微量元素蛛网图中,具有Ba、U、Pb、Zr、Eu的正异常和Nb的负异常,石榴橄榄岩全岩以及透辉石单矿物都具有高~(87)Sr/86 Sr(0.7088,0.7086)和低ε_(Nd)(t)(-6.55～-6.01)的特征,尽管南山岭与碧溪岭岩体距离很近而且都属于火成成因,但岩石的结构构造、变质变形的印记、REE配分形式和同位素特征都有区别,表明二者的源区及演化经历不同,相比之下,南山岭岩浆源区地壳组分的作用更为明显。在ε_(Nd)(t)-(~(87)Sr/~(86)Sr)_t图解中南山岭橄榄岩的投点十分靠近大别山北麓120～130Ma侵位的祝家铺辉石岩-辉长岩岩体群的投点分布范围,暗示可能有与罗田穹窿西北侧祝家铺岩体群的岩浆活动相对应。     

中国云南易门式铜矿床的主要类型及成因

系统地概括了易门铜矿田的成矿地质背景及2种矿床类型的地质特征,在此基础上论证了火山热水沉积作用、构造改造作用、岩浆叠加作用、地下热水再造作用与成矿密切相关。易门式铜矿床为"裂谷成矿背景-火山热水沉积-构造改造富集-深源岩浆叠加-地下热水再造"型多因复成矿床,建立了新的成矿模式,为该类矿床深部及外围的找矿预测指明了方向。     

A review on reflective remote sensing and data assimilation techniques for enhanced agroecosystem modeling

During the last 50 years, the management of agroecosystems has been undergoing major changes to meet the growing demand for food, timber, fibre and fuel. As a result of this intensified use, the ecological status of many agroecosystems has been severely deteriorated. Modeling the behavior of agroecosystems is, therefore, of great help since it allows the definition of management strategies that maximize (crop) production while minimizing the environmental impacts. Remote sensing can support such modeling by offering information on the spatial and temporal variation of important canopy state variables which would be very difficult to obtain otherwise.In this paper, we present an overview of different methods that can be used to derive biophysical and biochemical canopy state variables from optical remote sensing data in the VNIR-SWIR regions. The overview is based on an extensive literature review where both statistical–empirical and physically based methods are discussed. Subsequently, the prevailing techniques of assimilating remote sensing data into agroecosystem models are outlined. The increasing complexity of data assimilation methods and of models describing agroecosystem functioning has significantly increased computational demands. For this reason, we include a short section on the potential of parallel processing to deal with the complex and computationally intensive algorithms described in the preceding sections.The studied literature reveals that many valuable techniques have been developed both for the retrieval of canopy state variables from reflective remote sensing data as for assimilating the retrieved variables in agroecosystem models. However, for agroecosystem modeling and remote sensing data assimilation to be commonly employed on a global operational basis, emphasis will have to be put on bridging the mismatch between data availability and accuracy on one hand, and model and user requirements on the other. This could be achieved by integrating imagery with different spatial, temporal, spectral, and angular resolutions, and the fusion of optical data with data of different origin, such as LIDAR and radar/microwave.     

北半球高纬地区年际尺度循环过程中的气-海-冰相互作用关系

基于一个全球气-海-冰耦合模式数值模拟结果,对北半球高纬度地区年际尺度的气-海-冰相互作用进行了分析。在所使用的全球气-海-冰耦合模式中,大气环流模式和陆面过程模式来自国家气候中心,海洋环流模式和海冰模式来自中国科学院大气物理研究所大气科学和地球流体力学数值模拟国家重点实验室。采用一种逐日通量距平耦合方案实现次网格尺度海冰非均匀条件下大气环流模式和海洋环流模式在高纬地区的耦合。只对50 a模拟结果中的后30 a结果进行了分析。在分析中,首先对滤波后的北半球高纬度地区海平面气压、表面大气温度、海表面温度、海冰密集度及海表面感热通量的标准化距平做联合复经验正交函数分解,取第一模进行重建,然后讨论了在一个循环周期(约4 a)中北半球高纬度地区气-海-冰的作用关系。结果表明:(1)当北大西洋涛动处于正位相时,格陵兰海出现南风异常,使表面大气温度升高,海洋失去感热通量减少,海洋表面温度升高,海冰密集度减小;当北大西洋涛动处于负位相时,格陵兰海出现北风异常,使表面大气温度降低,海洋失去感热通量增多,海洋表面温度降低,海冰密集度增加。巴伦支海变化特点与格陵兰海相似,但在时间上并不完全一致。(2)多年平均而言,北冰洋内部靠近极点区域为冷中心。当北冰洋内部为低压异常时,因异常中心偏向太平洋一侧,使北冰洋内部靠近太平洋部分为暖平流异常,靠近大西洋一侧为冷平流异常。伴随着暖、冷平流异常,这两侧分别出现暖异常和冷异常,海表面给大气的感热通量分别偏少和偏多,上述海区海表面温度分别偏高和偏低,海冰密集度分别偏小和偏大。当北冰洋内部为高压异常时特点正好与上述相反。由上述分析结果可知,在海洋、大气年际循环中,大尺度大气环流变率起主导作用,海洋表面温度和海冰密集度变化主要是对大气环流变化的响应。     

辽北地区早石炭世变质火山岩年代学和地球化学特征:对华北板块北缘东段构造演化的启示

华北板块北缘东段分布的构造混杂岩带为研究古亚洲洋的演化提供了重要的依据,"下二台岩群"作为该构造混杂岩带的重要组成部分,其形成时代和构造属性仍存在争议。详细的研究表明下二台地区变质火山岩原岩包括流纹岩、英安岩、安山岩,为一套钙碱性火山岩,属于准铝质-弱过铝质岩石,根据岩相学和地球化学特征将其分为变质酸性火山岩和变质中性火山岩;二者均相对富集轻稀土元素,亏损重稀土元素,轻重稀土元素分馏明显,Eu负异常不明显,但变质中性火山岩稀土总量低于变质酸性火山岩,变质酸性火山岩明显亏损Sr、P元素,结合野外产出面积和高场强元素相关性特征,认为二者不是同一基性岩浆分异的产物。变质火山岩锆石LA-ICP-MS U-Pb年龄为341～348Ma,代表其原岩结晶年龄。变质酸性火山岩原始岩浆来自于地壳物质的部分熔融,变质中性火山岩原始岩浆来自于俯冲带附近岩石圈地幔,并遭受了地壳物质的混染,二者均形成于活动大陆边缘火山弧环境。最新研究成果表明"下二台岩群"由不同时代、不同构造环境下形成的地质单元叠置混杂而成,称其为"下二台"构造杂岩更为准确。下二台地区变质火山岩表明在早石炭世初,古亚洲洋板块已经南向俯冲,在华北板块北缘形成活动大陆边缘弧环境,早石炭世变质火山岩原岩为这一俯冲阶段的产物。     

An averaging method to study the motion of lunar artificial satellites I: Disturbing Function

We describe a semi-analytical averaging method aimed at the computation of the motion of an artificial satellite of the Moon. In this paper, the first of the two part study, we expand the disturbing function with respect to the small parameters. In particular, a semi-analytic theory of the motion of the Moon around the Earth and the libration of the lunar equatorial plane using different reference frames are introduced. The second part of this article shows that the choice of the canonical Poincaré variables lead to equations in closed form without singularities in e = 0 or I = 0. We introduce new expressions that are sufficiently compact to be used for the study of any artificial satellite. This revised version was published online in July 2006 with corrections to the Cover Date.     

Stream overflow and dwarf nova eruptions

We consider the effects of accretion stream overflow on the viscous dynamics of accretion discs in dwarf novae. If the stream from the secondary star is geometrically thick enough, some fraction of its material can flow over and under the disc. The mass and specific angular momentum of the stream are then deposited not only at the point of collision with the outer disc, but also at those radii in the inner disc with geometric heights that are large enough to intercept the residual stream, or near the radius where the disc has the same specific angular momentum as the stream. The overflowing stream can alter the behaviour of heating fronts and cooling fronts in the disc. If the mass fraction of the overflowing stream is of order tens of per cent, the deposition of mass in the inner parts of the disc is sufficient to change the character of the eruption light curves significantly.