GAS参数优化方法在黄河上游非汛期径流预报中的应用

本文采用相关分析与GAS参数优化相结合的方法,对黄河上游非汛期径流预报模型进行了研究,并对2000～2003年的径流进行了实时预报检验,从检验结果来看,这种预报方法具有较高的预报精度.本文为非汛期径流预报研究提供了参考和借鉴,同时,就计算分析手段而言,GAS在参数优化方面具有广泛的应用价值.     

新疆叶尔羌河流域地下水同位素特征及其补给来源分析

笔者以新疆叶尔羌河流域为例,在研究区水文地质调查的基础上,根据不同区域、不同深度D、~(18)O和T值的变化分析地下水补给来源.解决了传统研究方法很难解决的问题.为干旱地区地下水起源及空间分布规律研究提供了新思路。研究结果表明:(1)研究区地下水不是来自大气降水的直接入渗,而是地表水渗漏补给。(2)流域分为两个独立的地下水循环系统,分别接受叶尔羌河与提孜那甫河河水补给。(3)潜水和承压水的起源相同,属统一的地下水系统。(4)地下水径流表现为倾斜平原区径流强烈,地下水以水平运动为主;细土平原区地下水径流迟缓,地下水以垂直蒸发运动为主.径流方向与地表水流向密切相关。     

西秦岭熊山沟岩体地球化学及构造环境分析

在区域地质调查及综合研究的基础上,对位于西秦岭天水东南部地区的原百花岩体进行了详细的岩石学、岩石地球化学、岩体接触关系、同位素年龄研究,从中解体出熊山沟岩体,并初步了解了该岩体的岩浆活动规律。熊山沟岩体早期岩石类型为斜长花岗岩,岩石化学成分K2O含量较低,K2O∕Na2O比值为0.33～0.42;晚期岩石类型为二长花岗岩,岩石相对富集K2O,K2O∕Na2O比值为1.01～1.43,岩石属拉斑-钙碱性系列;微量元素富集Th、Hf、Nb、Zr等元素;稀土元素以富集轻稀土,无铕负异常或铕负异常不明显为主要特征;氧同位素值较低（δ^18O为＋3.32‰）,岩石具Ⅰ型花岗岩的特征,岩浆来源于下地壳物质,形成于大陆弧构造环境。     

内蒙古西河盆地新近纪“红土”记录的沉积环境

笔者从岩性地层、孢粉组合、地层对比等方面,对西河盆地红层的地层时代与沉积环境,进行深入的研究和探讨并追朔其地质演化历程。本区首次发现的孢粉组合是以草本植物蒿属为优势种,松、胡桃及禾本科为次优势种的疏林灌丛草原,其中胡桃属、榆属为典型的古—新近纪属种。根据岩性特征及生物特征综合分析研究,认为西河盆地“红土”地层属于新近系上新统宝格达拉组（N2b）,地层层序类型在平面上体现出从盆地边缘到中心沉积环境由河流、冲积扇、三角洲到湖泊的变化规律。     

深层裂缝性储层防漏堵漏实验评价研究

深层裂缝性气藏具有异常高压、高产等特点,钻井完井过程中易出现又喷又漏等复杂事故,因此需做好“防漏为主、堵漏为辅”的防漏堵漏措施。通过全尺寸堵漏装置进行了高压静态、动态模拟堵漏实验,优选配方组合,并系统评价了防漏、堵漏配方的封堵能力、承压能力以及酸溶性,评价研究出的防漏堵漏配方,具有酸溶率高、堵塞强度高、返排效果好等特点,为防漏、堵漏方案现场实施提供依据。     

地下管线内损伤电视检测系统的研制

介绍了地下管线内损伤电视检测系统的基本结构、工作原理、主要技术参数及其现场试验情况。     

Cyclotron amplification of geomagnetic micropulsations Pc1 in the magnetosphere

A numerical analysis of cyclotron instabilities is carried out by computing the dispersion relation for a three component cold plasma-beam system. Rates of growth and damping for various values of the stream density are calculated from the dispersion relation. The rates of growth and damping increase monotonically as the number density of the proton stream increases. It is found that the frequencies at the rates of maximum growth and the damping decrease slightly to lower frequencies and a sharp peak at these frequencies becomes blunt. The minimum e-folding times of an ion cyclotron wave for (a) σ_s = 10⁻⁴, σ_i = 10⁻² and (b) σ_s = 10⁻¹, σ_i = 10⁻² are about 3·84 and 0·16 sec respectively in the vicinity of the equatorial plane at 6 Re, where σ_s and σ_i are the ratios of the beam density N_s and the helium ion (H₆⁺) density N_i to the total positive ions in the plasma-beam system.     

Variations in exospheric density at heights near 1100km, derived from satellite orbits

In an earlier paper, values of exospheric density were obtained from the orbit of Echo 2 for the years 1964–1965. The results indicated a semi-annual variation in density by a factor of between 2 and 3, considerably larger than predicted by existing atmospheric models.

These studies have now been extended to the beginning of 1967, using both Echo 2 and Calsphere 1, to show how the density is responding to increasing solar activity. Variations in density during 1964 have been analysed in more detail. The long-term variation associated with the solar cycle and the short-term variations associated with magnetic and solar disturbances agree with the variations expected on the basis of current models. The semi-annual variation is persisting to higher levels of solar activity, and although its amplitude is diminishing the factor of variation was still 1.6 in 1966.