含钙铝铁水解聚合产物的矿物学研究Ⅱ:热分解特性

分别以NaOH和Ca(OH)2作为碱化剂,合成了聚合氯化铝铁(PAFCNa,PAFCCa),比较样聚合氯化铝(PACNa,PACCa)、聚合氯化铁(PFCNa,PFCCa),制成低温干燥样进行热分解检测.热重分析证明,PAFCCa中的含水量高,主要是配位水与结晶水.当n(Al)/n(Fe)>5:5后,PAFCCa的含水量平均为42.3%.按Ca6Al2(SO4)3(OH)12·26H2O分子式计算,钙矾石的结构水(含OH水)含量为43.06%,两者含水量相当接近.TG-DTG热分析结果支持XRD对PAFCCa中存在含Ca3Al2(OH)12柱体的类钙矾石结构体的认定.PAFC-Ca根据其DTG曲线上的125℃和180℃两个脱水速率(肩)峰可以判别其中有无钙矾石结构体,以及相对量的多少.     

Using geospatial technology to strengthen data systems in developing countries: The case of agricultural statistics in India

Despite significant progress in the development of quantitative geography techniques and methods and a general recognition of the need to improve the quality of geographic data, few studies have exploited the potential of geospatial tools to augment the quality of available data methods in developing countries. This paper uses data from an extensive deployment of geospatial technology in India to compare crop areas estimated using geospatial technology to crop areas estimated by conventional methods and assess the differences between the methods. The results presented here show that crop area estimates based on geospatial technology generally exceed the estimates obtained using conventional methods. This suggests that conventional methods are unable to respond quickly to changes in cropping patterns and therefore do not accurately record the area under high-value cash crops. This finding has wider implications for commercializing agriculture and the delivery of farm credit and insurance services in developing countries. Significant data errors found in the conventional methods could affect critical policy interventions such as planning for food security. Some research and policy implications are discussed.     

汶川8.0级地震前龙门山断裂带的地震活动性和构造应力场特征

研究了2008年5月12日汶川8.0级地震前龙门山断裂带及其附近地区的地震活动.利用区域地震台网和流动测震台的数字地震波资料,测定了震源机制解.结果表明,震中所在的龙门山断裂带震前地震活动平稳,未出现显著异常增强或平静现象.根据汶川8.0级地震前地震活动求出的震源机制解,其主压应力P轴方位为WNE——ESE向,震源断层面呈NE向与NW 向两组节面走向.其中NE向节面呈N50deg;——70deg;E,断面倾角均陡,达60deg;——70deg;,震源力学作用方式多呈逆倾型,少部分呈走滑型．震前地震活动呈现的主压应力方位、震源断面走向及其错动类型,与汶川8.0级地震给出的解是一致的.巨大地震发生前沿龙门山断裂带微破裂呈现的平均应力场与主震一致．起始破裂区东侧20km内是紫坪铺水库水域区,这一区域发生小震活动增加的现象处于水库放水的卸载阶段.本文研究了汶川8.0级地震起始破裂区附近的小震活动,其震源参数表明,震源位于8.0级地震之上的5——14km深度,其震源参数与8.0级地震给出的解也是一致的．      

汶川8.0级地震序列及相关问题讨论

汶川8.0级地震序列具有明显的分段特性,较强余震分布于茂县、绵竹以南及平武以北。主破裂过程在中南段以逆冲为主,序列逐渐衰减,呈主余型的序列衰减特征;北段是汶川地震破裂过程的终止区域,主破裂过程在该区域以走滑为主,形成多震型的序列特征,也成为汶川序列较大余震的主体活动区域。序列较强余震活动明显受引潮力调制,大多数较强余震发生在固体潮大、小潮时段,并且16时前后是较强余震的优势发震时段。序列衰减系数p值随时间增加而逐渐增大,最终基本稳定在1附近变化。结合以往的研究,对序列类型及最大强余震震级、强余震活动持续时间等进行了初步讨论。初步的统计结果还显示,8级左右强震序列中主震与最大余震之间的震级差正比于主震破裂尺度,这意味着当震级大体接近时,较大的破裂尺度与较为充分的能量释放相对应     

祁连山老虎沟12号冰川冰内结构特征分析

利用探地雷达(Ground Penetration Radar,GPR)调查冰川冰内结构和冰层厚度是一种监测冰川变化常用手段.应用麦克斯维(Maxwell)方程的二维时域有限差分(FDTD)方法,通过将模拟图像与老虎沟12号冰川的实测图像的对比,分析了雷达剖面中的几种反射特征,如冰裂隙、融洞、暖冰等.对比结果表明,GP...     

祁连山老虎沟冰川积累区风速、风向变化特征研究

基于2008年11月-2009年10月祁连山老虎沟12号冰川积累区的风速、风向观测资料, 分析了年内季节和日变化特征. 结果表明: 全年日平均风速波动较大, 介于1～8.8 m·s^-1. 日均值以冬季最大, 春, 秋季次之, 夏季最小, 分别为5.1 m·s^-1, 3.4 m·s^-1, 3.7 m·s^-1, 2.6 m·s^-1, 表现出典型的"高山型"风速特征. 秋, 冬季节, 无论昼夜, 以偏南风为主, 风速始终保持在较为稳定的高值状态, 属于典型的冰川风; 春, 夏季节, 冰川风场依旧强劲, 而且伴有山谷风出现. 受山系-河谷地形及雪冰下垫面的共同作用, 春, 夏, 秋三季表现出一定的偏东风, 柴达木低压可能对此也有贡献.     

新疆和田南部地区矿产地质特征及成矿潜力分析

新疆和田南部地区地质矿产工作程度低,已有的矿产信息十分有限,2008年以矿产路线调查为主的找矿工作取得了一定进展,新发现的矿(化)点对了解本区的成矿特征具有重要意义,并展示出了形成矿集区的成矿潜力.     

The movement features analysis of Laohugou Glacier No. 12 in Qilian Mountains

The Laohugou Glacier No. 12 is the largest valley glacier in Qilian Mountains, which is located in northern Qinghai-Tibet Plateau. Movement is the basic characteristic of glaciers, and is also an important distinction from other terrestrial natural ice. Glacier changes not only reflect climate change, but also play an important role in humanity society. In the arid regions of western China, glaciers are becoming an important water source. We use the GPS receiver (South-Lingrui S82) as data platform with the aid of RTK measurement technology to observe the surface velocity of Laohugou Glacier No. 12. Surface velocity data shows that the maximum value appears at an altitude of 4,750–4,850 m during the period of 2008–2009. During this period, the west branch surface velocity reached 32.6 m per year at an altitude near 4,830 m, the east branch surface velocity reached 32.4 m per year at the altitude near 4,770 m. Comparing the surface velocity data during 2008–2009 with observation results in 1959, the glacier velocity slowed down about 11%.     

云量对祁连山老虎沟12号冰川表面能量平衡的影响

为探讨云量对冰川表面能量平衡(SEB)的影响,利用架设在老虎沟12号冰川(简称12号冰川)消融区(4 550m a. s. l.)的自动气象站资料,结合能量平衡模型计算各能量分量并分析其季节变化,通过云量参数化方案获取云量因子并量化其对冰川表面能量收支的影响。结果表明:净短波辐射为冰川表面主要的能量来源(92%),净长波辐射为主要能量支出(61%),二者均受云量影响,但云的短波辐射效应更强(-37W·m^-2)。云量通过影响辐射收支和湍流通量进而影响冰川表面能量收支,随云量的增加,冰川表面获得的能量减少,冰川消融速率降低。与其他区域的冰川表面能量收支对比,除地理位置、反照率、气温等因素外,海拔和云量的影响也非常显著。     

Starbursts and the triggering of the activity in nearby powerful radio galaxies

We present high-quality long-slit spectra for three nearby powerful radio galaxies – 3C 293, 3C 305 and PKS 1345+12. These were taken with the aim of characterizing the young stellar populations (YSP), and thereby investigating the evolution of the host galaxies, as well as the events that triggered the activity. Isochrone spectral synthesis modelling of the wide wavelength coverage spectra of nuclear and off-nuclear continuum-emitting regions have been used to estimate the ages, masses and luminosities of the YSP component, taking full account of reddening effects and potential contamination by activity-related components. We find that the YSP make a substantial contribution to the continuum flux in the off-nuclear regions on a radial scale of 1–20 kpc in all three objects. Moreover, in two objects we find evidence for reddened post-starburst stellar populations in the near-nuclear regions of the host galaxies. The YSP are relatively old (0.1–2 Gyr), massive  (10⁹ < M _YSP < 2 × 10¹⁰ M_⊙)  and make up a large proportion (∼1–50 per cent) of the total stellar mass in the regions of the galaxies sampled by the observations. Overall, these results are consistent with the idea that the nuclear activity of active galactic nuclei in some radio galaxies is triggered by major gas-rich mergers. Therefore, these radio galaxies form part of the subset of early-type galaxies that is evolving most rapidly in the local Universe. Intriguingly, the results also suggest that the radio jets are triggered relatively late in the merger sequence, and that there is an evolutionary link between radio galaxies and luminous/ultraluminous infrared galaxies.