江苏省入太湖污染量分析(1998-2007年)

近年来,太湖水体受到了严重污染,水环境质量逐年下降,太湖水环境的状况直接影响了地区的经济和社会发展,保护太湖已列为国家重点治理项目。本文根据1998-2007年环太湖水文巡测资料及主要入湖河道水质监测成果,分析入湖水量、入湖河道水质、入湖污染物量及其变化趋势,为太湖地区水环境综合整治提供技术支撑和决策依据。     

地震的感应磁效应（二）

本文是“地震的感应磁效应（一）--三维电磁感应的数值理论”一文的继续。首先从理论和实际计算两个方面证明了三维电磁感应数值方程解的唯一性、收敛性和稳定性,从而充实了作为研究地壳、上地幔电性结构横向不均匀性理论基础的“三维数值方法”。作为这一理论方法的实际应用,文中对不同源场周期和具有不同埋藏深度的三维电导率异常体进行了模拟计算,以研究地震感应磁效应的大小、空间分布特征和频率特性。模拟计算结果表明,对于周期从数秒到数分钟的地磁短周期变化,若电导率异常体的线度与5至7级地震的震源体积大体相当,其电导率较原背景电导率高近一个量级,其感应磁效应主要特征为:在异常体正上方,地面磁场的水平分量变化最大,相对变化量约30％;在异常体于源场方向一致的两侧,垂直分量变化最大,相对变化量约40-50％。因此,观测短周期地磁场的异常变化,有可能是监测地震孕育过程地下电性变化的一种试验途径。但由于上述异常强度在空间上衰减迅速,所以观测必须接近震源区,这对测点的选择是个不利的因素。     

宇宙黎明和再电离时期低频全天总功率探测实验现状

宇宙黎明和再电离时期探测是目前宇宙学最前沿科学研究方向之一.对这一时期的直接探测只能依赖于观测来自这一时期红移后的中性氢21 cm信号,其3种主要探测方式之一是21 cm信号全天总功率测量.在此回顾已有和正在计划中的探测宇宙黎明和再电离时期的低频全天总功率测量实验及其进展,包括地面射电望远镜如BIGHORNS¹、EDGES²、LACE³、LEDA⁴、MIST⁵、REACH⁶、SARAS⁷ 3、SCI-HI⁸、PRI^ZM⁹以及空间低频总功率相关实验如DARE¹⁰、DAPPER¹¹、FARSIDE¹²、鸿蒙计划.其中, EDGES实验是目前唯一声称观测到疑似宇宙黎明信号的实验,然而其实验结果与标准宇宙学模型(Λ Cold Dark Matter,ΛCDM)有不符之处.如果该探测结果被证实,那么这将是人类第1次...     

GIS的语音功能实现

和大多数信息系统一样,地理信息系统(GIS)主要是通过键盘、鼠标和屏幕进行人机信息交流,人机交流方式的增加有可能拓展信息系统的应用空间。通过ArcEngine和Microsoft Speech SDK的结合,笔者建立了一个具有语音功能的校园GIS,实现了GIS语音信息的输入与输出。     

中国60城市站1901—2019年日降水数据集的构建

近年来中国区域降水的极端化问题得到学术界的广泛关注,有关研究也获得了大量成果。但是,目前国内外常用的高分辨率降水资料序列多从1951年左右开始,普遍缺少20世纪早期中国的逐日降水资料,对于近一百多年中国极端降水变化特征及其机理,目前还不清楚。基于多来源的1901—1950年原始观测报表数字化逐日降水资料,补充先前未录入的“无降水”和缺测数据,研发质量控制方案并开展质量控制,补充录入检出的缺失和错误数据并再次质控,结合1951年以来的现代降水日值资料,建立中国60个城市站1901—2019年降水日值数据集。数据集评估结果显示,早期中国东部地区的台站较为密集,数据完整性和正确性较好,但中国西部的台站数量少且完整性和正确性偏低。本数据集构建的年总降水量累积值序列与已有的月降水量数据基本一致。基于该数据集,研究发现重庆站近百年来的降水未出现显著的趋势性变化。该数据集使后续分析研究中国极端降水的百年尺度长期变化特征成为可能。     

风云二号卫星地球观域修正算法

风云二号静止气象卫星在获取图像时, 必须使扫描辐射计的观域对准地球。卫星在轨道上受到各种摄动力的作用, 使轨道和姿态改变, 扫描辐射计的地球观域随之发生变化。卫星扫描辐射计对地球观域的偏差会影响图像定位的精度, 因此对准观域的工作是日常业务工作的一部分, 不仅在卫星定点之初启动观测时, 而且在业务运行的过程中, 都需要通过地面遥控指令进行修正。该文提出了一种风云二号静止气象卫星扫描辐射计地球观域修正量和调整方向的算法, 以替代人工目测卫星原始云图进行的卫星观域调整控制决策。这种算法的实施可以提高风云二号气象卫星云图获取作业的可靠性。     

Biogas charging and dissipating process and its accumulation in the Sebei gasfield,Qaidam Basin,China

The Sebei gasfield is the largest biogas accumulation found in China and many reservoirs and seal rocks superposed on a syndepositional anticline in Quaternary. The biogas charging and dissipating process and its distribution have been a research focus for many years. The authors suggest a diffusing and accumulating model for the biogas, as they find that the shallower the gas producer, the more methane in the biogas, and the lighter stable carbon isotope composition of methane. Based on the diffusing model, diffused biogas is quantitatively estimated for each potential sandy reservoir in the gasfield, and the gas charging quantity for the sandy reservoir is also calculated by the diffused gas quantity plus gas reserve in-place. A ratio of diffusing quantity to charging quantity is postulated to describe biogas accumulating state in a sandy reservoir, if the ratio is less than 0.6, the reservoir forms a good gas-pool and high-production layer in the gasfield, which often occurs in the reservoirs deeper than 900 m; if the ratio is greater than 0.6, a few gas accumulated in the reservoir, which frequently exists in the reservoirs shallower than 900 m. Therefore, a biogas accumulation model is built up as lateral direct charging from gas source for the sands deeper than 900 m and indirect charging from lower gas-bearing sands by diffusion at depth shallower than 900 m. With this charging and diffusion quantitative model, the authors conducted re-evaluation on each wildcat in the central area of the Qaidam Basin, and found many commercial biogas layers.

     

Crytic period analysis model of hydrological process and its application

It is difficult to analyse the crytic period of the hydrological process, because hydrological time series is probably characterized by heteroscedasticity. To find out the crytic period, a model is constructed as follows: (1) after using zero‐mean transformation for the data, to do Augmented Dickey–Fuller stationary test for the sequence, to build the corresponding AR(p) model and then to do ARCH effects test and white noise test for residual series; (2) for those time series that cannot pass through ARCH test, using logarithm transformation to reduce the heteroscedasticity, and then to redo step (1) until they pass through ARCH test and stationary test; (3) using periodogram analysis to determine all the possible the prime periods and further to put forward three kinds of tests to determine significance level of those prime periods. As examples, the hydrological processes of streamflow from 1784 to 1997 for the gauging stations of Alaer and Xinquman along Tarim River are analysed. After reducing their heteroscedasticity, AR(4) and AR(2) models are developed, respectively. Our results show that the streamflows from the two gauging stations have the same cryptic period of 42·7 years. Furthermore, the reliability for the crytic period model is testified by variance analysis, which shows that the crytic period model is useful and reliable. Copyright © 2009 John Wiley & Sons, Ltd.     

鲤JAK2基因分子克隆及组织表达分析

采用同源克隆策略和RACE-PCR技术,克隆得到可能的鲤(Cyprinus carpio)两面神激酶2(JAK2)基因的c DNA全长序列,包括3 378 bp的开放阅读框,732 bp的5'-非编码区,529 bp的3'-非编码区,总长度达4 639bp。开放阅读框可编码1 125个氨基酸,推测分子质量和理论等电点分别为129.33 ku和6.99。同源性分析显示,克隆的鲤鱼基因与斑马鱼(Danio rerio)JAK2同源性最高,其氨基酸序列同一性和相似度分别达89%和95%。结构域预测表明,所编码氨基酸序列包含FERM、SH2及两个酪氨酸激酶结构域,这4个结构域也保守地存在于其他脊椎动物的JAK分子中。高级结构预测显示,鲤JAK2主要包括α-螺旋(α-helix)、β-折叠(β-sheet)和连接环(loop)等3类结构元件。脊椎动物JAK分子系统进化树显示,JAK1、JAK2、JAK3和TYK2等4类JAK分子分别聚类,鲤JAK2处于JAK2支系中,与所有其他的鱼类JAK2聚为一大支,并与两栖类和哺乳类组成的另一大支构成姊妹群,表明它们具有共同的祖先基因,为直系同源关系。实时荧光定量PCR检测结果表明,鲤JAK2在皮肤中表达量最高,其次是肠、血液和脑,而在肌肉、鳃、头肾、心、肝、脾中表达量较低;鲤JAK3在脾中表达量最高,在其他组织中表达量均很低,甚至未检出。     

A cyclical period variation detected in the updated orbital period analysis of TV Columbae

Two CCD photometries of the intermediate polar TV Columbae are made for obtaining two updated eclipse timings with high precision. There is an interval time ～17 yr since the last mid-eclipse time observed in 1991. Thus, the new mid-eclipse times might offer an opportunity to check the previous orbital ephemerides. A calculation indicates that the orbital ephemeris derived by Augusteijn et al. (Astron. Astrophys. Suppl. Ser. 107:219, 1994) should be corrected. Based on the proper linear ephemeris (Hellier in Mon. Not. R. Astron. Soc. 264:132, 1993), the new orbital period analysis suggests a cyclical period variation in the O–C diagram of TV Columbae. Using Applegate’s mechanism to explain the periodic oscillation in the O–C diagram, the required energy is larger than the energy that a M0-type star can afford over a complete variation period of ～31.0(±3.0) yr. Thus, the light travel-time effect indicates that the tertiary component in TV Columbae may be a dwarf with a low mass, which is near the lower mass limit of ～0.08M _⊙ as long as the inclination of the third body is high enough.