地震前低频事件的实验研究

介绍了几种强震前超低频事件的观测证据,并通过实验,研究了产生和传播机理。初步结果表明,微破裂的集结和断层的破裂起始会出现超低频脉冲,并透射到空气中形成次声波。塑性体的冲击或超临界流体的膨胀比脆性破裂更容易激发（超）低频波,且不伴随明显高频辐射成分。这样可以较为合理地解释震前“平衡”背景下的（超）低频事件。对实验中破坏前的低频脉冲给出了断裂力学解释。断裂力学的实验和膨胀－－扩容理论证明了震前会产生断层的张裂隙,从而为超临界流体提供了运移空间。流体在运移过程中突然涨缩会激发（超）低频辐射波。讨论了改进（超）低频事件的观测条件问题。     

Evolution of relative helicity in active regions

The evolution dH _R/dt of relative helicity H _R provides a gauge-invariant measure of the helicity flow across the open surface S _o of an active region. With the incompressible approximation, reformulation of the evolution reveals that it is determined not only by the widely used cross-helicity h _mvp=A _pv contributed by the vector potential A _p of a reference potential field B _p, where v is the fluid velocity, but by another cross-helicity h _mvo=A _ov contributed by the vector potential A _o of the open field B _o in the region as well. Only under two conditions, (1) A _p=A (A is the transverse component of A _o), (2) v _z=0 (v _z is the longitudinal component of v) or A _z=0 (A _z is the longitudinal component of A _o), can h _mvo be merged into h _mvp to give the pioneering dH _R/dt equation shown in Equation (4) of Berger (1984). Results show that h _mvo originates from vh _o (h _o=A _oB _o is the helicity density of the open field) and should also be considered in dealing with the development of relative helicity in active regions. Finally, the equation to calculate dH _R/dt in active regions is synthesized and presented.     

试论中国重要景观区区域地球化学异常系统评价的量化模型

在对中国5个重要景观区1:20万金、铜表生地球化学异常特征进行总结、对比,并讨论景观、表生因素对区域异常评价标志影响的基础上,进一步充实、完善了区域异常系统评价体系的思路和评价准则,提出了区域地球化学异常系统评价的量化模型。     

Halo Profiles and the Nonlinear Two- and Three-Point Correlation Functions of Cosmological Mass Density

NGC 4945 is one of the brightest Seyfert galaxies on the sky at 100 keV, but is completely absorbed below 10 keV; its absorption column is probably the largest that still allows a direct view of the nucleus at hard X-ray energies. Our observations of it with the Rossi X-Ray Timing Explorer (RXTE) satellite confirm the large absorption, which for a simple phenomenological fit using an absorber with solar abundances implies a column of 4.5+0.4-0.4x1024 cm(-2). Using a more realistic scenario (requiring Monte Carlo modeling of the scattering), we infer the optical depth to Thomson scattering of approximately 2.4. If such a scattering medium were to subtend a large solid angle from the nucleus, it should smear out any intrinsic hard X-ray variability on timescales shorter than the light-travel time through it. The rapid (with a timescale of approximately 1 day) hard X-ray variability of NGC 4945 discovered by us with RXTE implies that the bulk of the extreme absorption in this object does not originate in a parsec-size, geometrically thick molecular torus. Instead, the optically thick material on parsec scales must be rather geometrically thin, subtending a half-angle less than 10 degrees, and it is likely to be the same disk of material that is responsible for the water maser emission observed in NGC 4945. Local number counts of Seyfert 1 and Seyfert 2 galaxies show a large population of heavily obscured active galactic nuclei (AGNs) which are proposed to make up the cosmic X-ray background (CXRB). However, for this to be the case, the absorption geometry in the context of axially symmetric unification schemes must have the obscuring material subtending a large scale height-contrary to our inferences about NGC 4945-implying that NGC 4945 is not a prototype of obscured AGNs postulated to make up the CXRB. The small solid angle of the absorber, together with the black hole mass (of approximately 1.4x106 M( middle dot in circle)) from megamaser measurements, allows a robust determination of the nuclear luminosity, which in turn implies that the source radiates at approximately 10% of the Eddington limit.     

川滇地区地震活动单键群分析

利用单键群（即ＳＬＣ）分析方法,通过有关ＳＬＣ特征参量的时间滑移分析,结合１９７０年以来的区域地震活动和构造环境,分析了川滇西部地区的地震活动。较之７０年代和８０年代,９０年代的地震活动在总体上是处于中等强度的活动水平。文章认为,ＳＬＣ方法考虑了地震事件的时空关联性,可以用来分析地震活动趋势,是研究地震活动性的有用工具。     

陕西二台子铜金床钠长石碳酸（角砾）岩类特征及形成构造背景分析

从岩石学、矿物学、岩石化学、地球化学、稀土元素等方面研究了二台子铜金矿内长石炭酸（角砾）岩类地质地球化学特征。晚泥盆世－石炭纪,在区域幔羽构造作用下,深部热流体沿先存在构造通道上升进入镇安二台子三级热水沉积盆地之中,形成了石英重晶石炭酸角砾岩、碳酸角砾岩、复成分角砾岩、钠长岩、钠长石碳酸岩,受同性断裂及层位控制明显,并构成了金的矿源层及普遍金矿化。燕山期,具有幔源特征的深部含矿热流体在北东、北西向     

微波辅助化学反应制备纳米高岭石

为提高高岭石比表面积、孔隙率和吸附容量，利用微波辅助化学反应制备了尿素-高岭石复合物，进一步微波辐射使层状高岭石完全剥离并粉碎，经分散后得到了纳米高岭石。利用傅立叶红外光谱仪（FT-IR）、X射线粉晶衍射仪（XRD）、扫描电镜（SEM）和透射电镜（硎）进行了过程中样品结构、形貌和尺寸方面的表征。结果表明：同等条件下，通过微波辅助剥离并粉碎层状高岭石，时间只需30min，约为单一球磨的1／20，分散后的纳米高岭石平均粒径约为150nm。     

宁芜盆地凹山和东山铁矿床流体包裹体和氢氧同位素研究

本文对宁芜地区凹山和东山铁矿床中的磷灰石流体包襄体进行了较为系统的测温研究,并测定了不同时期形成的磁铁矿、阳起石和石英的 H、O 同位素组成。凹山和东山铁矿磷灰石含有丰富的流体包裹体,原生气液包裹体包括早期细长管状、针状包裹体(类型Ⅱ)和晚期不规则状包襄体(类型Ⅰ);早期包裹体又可分为单一液相包裹体(类型Ⅱ-a)、气液两相(富气相)包襄体(类型Ⅱ-b)、气液两相(富液相)包裹体(类型Ⅱ-c)和气相、液相及固相多相包裹体(类型Ⅱ-d)四种亚类。包襄体中至少含有五种不同的子矿物。磷灰石包裹体记录了多个峰值温度,从600℃～800℃到～410℃和～270℃,分别对应于磷灰石(磁铁矿 透辉石)、阳起石和石英的形成。流体的盐度随温度的降低而逐渐减小,从高达～80%NaCl equiv。到<20%NaCl equiv。磷灰石形成时流体处于不均匀的状态,流体包裹体为非均一捕获。H、O 同位素研究显示成矿流体早期为演化的初始岩浆(水),在高温下形成了铁矿石;此后,成矿流体有可能与蒸发盆地卤水或大气降水发生混合;晚期则可能有较显著的大气降水加入。     

基于元数据的信息共享机制研究

元数据作为关于数据的数据,是目前信息共享的关键技术,也是当前研究的热点。在对比国际、国内元数据标准的基础上,采用元数据管理的三个层次:元数据子集、元数据实体和元数据元素,建立了“数字成都”元数据标准模板。它主要包括:标识信息、数据质量信息、空间参考信息、数据集的内容信息、分发信息、元数据参考信息。讨论了“数字成都”中基于元数据信息共享系统的结构、模块和特点,实现了分布式数据组织与管理、分布式数据共享、分布式数据快速索引机制以及跨平台数据访问。     

半干旱区内陆湖泊透明度高光谱估测模型研究——以松嫩平原查干湖为例

通过实测查干湖高光谱数据,建立透明度(Secchi Disk Depth,SDD)单波段估测模型、比值估测模型以及神经网络高光谱估测模型,并以确定性系数R2以及剩余残差RMSE为指标进行了验证.通过对单波段估测模型和比值估测模型进行比较发现,单波段模型估测结果与比值模型相差无几,而水体透明度经对数处理有利于模型精度提高,但是神经网络模型是三者中最优的.查干湖透明度高光谱定量估测模型的建立,有利于今后利用遥感影像,对查干湖水体透明度进行全面估测,对于研究和监测查干湖水体水质状况有重要意义.