GIS在大比例尺的城市非点状源污染模型中的应用研究

人们对于与城市雨水有关的非点状源污染的关注，促使更好地规划水质的新工具得到了发展。本文介绍ＧＩＳ在城市水质研究中的应用。这种ＧＩＳ用于管理非点状源污染模型的土地利用数据，还可用于总计各种地理单元之中污染物的负荷量，在土地利用的基础上用水质经验模型来估算污染负荷量。通过判读最新的航空像片更新旧图从而编出土地利用图。这种土地利用图同样也可用来记录每个土地利用多边形的所有污染负荷量。通过对雨水沟图的数字     

黄河下游悬河稳定性因素分析

黄河悬河的形成是自然营力与人为因素综合作用的产物.悬河的稳定性关乎黄河下游广大人民的生命财产安全.从地学角度出发,论证了影响黄河悬河稳定性的因素:①地质构造控制机制;②河流地貌的影响;③河床质与土体结构;④流动力地质作用;⑤治理工程对悬河稳定性的影响.     

无定形氢氧化铝的表面酸度

通过酸碱滴定法以及分析反应后的溶液和反应后固体的XRD表征等方法测定了合成氢氧化铝的表面酸度。XRD结果表现出4个宽峰,说明合成产物是无定形的。滴定实验的固体产物的XRD的分析表明,无定形的氢氧化铝在碱性的环境下(pH>10),迅速转化成为结晶的三羟铝石。滴定过程中和反应后的溶液分析计算出无定形氢氧化铝的溶解度,为1010.3。滴定实验中加入的酸或碱与溶解的铝和其表面羟基发生质子化作用或脱质子化作用。表面酸度常数,表面羟基密度和比表面积用FITEQL4.0进行了评价。无定形氢氧化铝的表面酸度@K.FUKUSHI$Research Center for…     

深反射地震揭示喜马拉雅地区地壳上地幔的复杂结构

报告了中、美两国在喜马拉雅山区进行的第一次深反射地震试验的结果．试验剖面南起喜马拉雅山山脊南亚东县的帕里镇,向北穿过喜马拉雅山脊的荡拉,到达康马南的萨马达．剖面长约１００ｋｍ．共中心点（ＣＭＰ）叠加剖面上显示出：１．在地壳中部有一强反射带,向北缓倾斜下去,延长达１００ｋｍ以上．它可能代表了一个活动的逆冲断裂或是一条巨大的拆离带,印度地壳整体或下地壳沿此拆离层俯冲到藏南之下．２．上部地壳的反射很丰富,显示了上地壳存在着大规模的叠瓦状结构．３．下地壳的反射同相轴呈现短而有规律的分布,显示了塑性流变特征．４．在测线南部莫霍反射明显,深度达７２－７５ｋｍ．发现南部有双莫霍层的存在．５．试验中还取得莫霍层下面３２,３８,４８ｓ等双程走时的多条反射,向北倾斜,反射同相轴延续较长,信息丰富,反映了上地幔的成层结构和变形特征．这些结果对印度大陆地壳整体或其下地壳俯冲到藏南特提斯喜马拉雅地壳之下,并导致西藏南端地壳增厚的观点,给予了实质性的支持．     

Simulation Study on High Energy Cosmic Electron Detection by Shower Image

Many projects have recently been carried out and proposed for observing high energy electrons since it is realized that cosmic ray electrons are very important when studying the dark matter particles and the acceleration mechanism of cosmic rays. An imaging calorimeter, BETS （Balloon-borne Electron Telescope with Scintillator fiber）, has been developed for this purpose. Using pattern analysis of the shower development, the electrons can be selected from those primary cosmic ray proton events with flux heights one-tenth that of the electrons. The Monte-Carlo simulation is indispensable for the instrument design, the signal trigger and the data analysis. We present different shower simulation codes and compare the simulation results with the beam test and the flight data of BETS. We conclude that the code FLUKA2002 gives the most consistent results with the experimental data.     

A Model for the Quiescent Phase of the Recurrent Nova U Scorpii

A theoretical light curve is constructed for the quiescent phase of the recurrent nova U Scorpii in order to resolve the existing distance discrepancy between the outbursts (d approximately 6 kpc) and the quiescences (d approximately 14 kpc). Our U Sco model consists of a very massive white dwarf (WD), an accretion disk (ACDK) with a flaring-up rim, and a lobe-filling, slightly evolved, main-sequence star (MS). The model properly includes an accretion luminosity of the WD, a viscous luminosity of the ACDK, and a reflection effect of the MS and the ACDK irradiated by the WD photosphere. The B light curve is well reproduced by a model of 1.37 M middle dot in circle WD + 1.5 M middle dot in circle MS (0.8-2.0 M middle dot in circle MS is acceptable) with an ACDK having a flaring-up rim and the inclination angle of the orbit i approximately 80&j0;. The calculated color is rather blue (B-V approximately 0.0) for a suggested mass accretion rate of 2.5x10-7 M middle dot in circle yr-1, thus indicating a large color excess of E(B-V) approximately 0.56 with the observational color of B-V=0.56 in quiescence. Such a large color excess corresponds to an absorption of AV approximately 1.8 and AB approximately 2.3, which reduces the distance to 6-8 kpc. This is in good agreement with the distance estimation of 4-6 kpc for the latest outburst. Such a large intrinsic absorption is very consistent with the recently detected period change of U Sco, which is indicating a mass outflow of approximately 3x10-7 M middle dot in circle yr-1 through the outer Lagrangian points in quiescence.     

The Properties of Supernova 1997cy Associated with GRB 970514

The extraordinary SN 1997cy associated with GRB 970514 has been observed photometrically and spectroscopically for nearly 2 yr. At the time of discovery, SN 1997cy was the brightest supernova (SN) ever observed (MV相似文献   

用1Hz GPS观测数据推导中强震震源过程的能力:2008年日本岩手—宫城内陆地震例子

通过反演研究2008年日本岩手—宫城内陆地震（M～6.9）,说明了用1Hz全球定位系统（GPS）观测数据推导中强震（M6级）震源过程的能力。比较了此次地震采样率为1Hz的GPS观测波形,发现与强震仪记录波形有很好的一致性。由于震源区及其周围有足够多的GPS台站很好地记录到了地面运动,因而使我们仅仅采用1Hz的GPS观测数据就可进行波形反演。反演的结果与大地测量和强震仪数据联合反演的结果相当一致,如地震矩（Mw～6.9）、累积滑动量分布和破裂传播等。这种一致性证明,采样率为1Hz的GPS观测数据不仅能用来推导M6级中强震破裂过程的动态特征,而且能用来推导其持久（或静态）的滑动。