中国人工增雨研究进展

随着全球气候变暖的加剧,水资源短缺问题表现得越来越突出,如何有效地开发利用空中水资源已成为人们关注的热点问题之一。本文回顾了人工增雨的发展历史,概述了当今国内外人工增雨的发展状况,归纳了各地区云状、积云特征、液态含水量、冰晶浓度等云物理特征,并在此基础上对我国各地区尤其是西北地区的增雨潜力进行了分析,最后归纳总结了人工增雨的常用手段、经验和检验人工增雨效果的方法。     

“资源一号”卫星星内粒子探测器对扰动事件的观测

本文比较了在太阳平静和扰动时期“资源一号”卫星星内粒子探测器对卫星舱内高能粒子的观测结果，发现在平静时期观测结果很好地反映了辐射带高能粒子在该高度上的分布情况.在扰动时期，粒子探测器观测到高能粒子分布出现重大变化，本文进一步讨论了影响高能粒子在近地空间分布的可能因素.     

库区蓄水型人工增雨效果评估及其应用

通过对降水影响系统分型,给出了以同一影响天气系统下的降水时段为评估单元,对降水前后目标区和控制区的流域面雨量、入库流量和作业前后雷达回波参量进行评估,并对2005年夏季增雨作业个例进行了计算,结果表明,雷达回波参量在作业前后有明显的变化,平均增雨率为19.61%,投入产出比为1:37,经济效益显著。     

一种基于直方图均衡化改进的图像增强算法

本文分析了传统的灰度图像直方图均衡化算法的不足,提出了一种基于概率的灰度图像直方图均衡化的改进算法。该方法给出了较合理的变换关系,使运算结果有较大改善,而且保留了传统算法的快速、自动化的特点。     

柴达木盆地东缘晚更新世气候变化的（古）土壤发生记录

柴达木盆地东缘典型剖面（古）土壤及其黄土线质的宏观特征和理化分析表明,本区晚更新世以来气候曾有几次较大的波动,反映了全球冰量影响的气候波动以及东亚季风气候的强弱变化特征。揭示出气候变化过程中温度和降水并不同步,温度主要受地球轨道变化引起的太阳辐射的影响;降水则主要取决于冬、夏季风的浊弱对比关系,夏季风盛行时,降水丰沛。间冰段古土壤Ｓｍ的土壤发生特征和强度,揭示了除低温引起的蒸发减少外,降水丰沛也是     

人工增雨试验中的反效果问题

该文对人工增雨试验中出现的反效果（减雨）现象及其发生的条件和原因作了概要的评述和分析。根据实例分析,指出人工增雨作业中不适当的催化对象、不适当的催化剂和催化剂量以及不适当的催化部位和催化时机都有可能导致无效或减雨的反效果。在开展人工增雨作业时,应力求在作业有关的各环节提高科学性、减少盲目性,以提高人工增雨实效。文章还简要探讨了人工削弱局地暴雨的可能性,指出这是一个值得认真探索的具有重大潜在社会和经济效益的研究领域。     

缢蛏(Sinonovacula constricta)规模增殖放流对三沙湾滩涂底质环境改良的效果

于2013-2014 年在三沙湾选择增殖放流区Ⅰ区和Ⅱ区, 开展了2 批次的缢蛏增殖放流, 计 放流缢蛏苗数量约3747 万粒。采用对缢蛏生长、生物量动态变化和滩涂底质主要因子跟踪监测的方 法, 开展对缢蛏增殖放流效果的评估。研究结果, 2 个增殖放流区的缢蛏密度和缢蛏生物量都比对照 区有极显著提高, 共收获65 吨缢蛏大规格苗, 增殖放流产出比为1: 8.0-9.0, 获得了一定的资源增 殖效果和经济效益。放流期间, 滩涂底泥中的氧化还原电位、硫化物和有机碳等浓度在增殖区Ⅰ区、 Ⅱ区和对照区之间都无显著差异(P>0.05), 但, 底泥中Ⅰ区、Ⅱ区的氧化还原电位平均值分别比对照 区提高了26%和18%, 硫化物浓度平均值分别比对照区降低了45%和34%, 有机碳浓度平均值分别 比对照区下降了5.8%和6.8%, 表明, 缢蛏增殖放流获得了一定的改良底质环境效果。     

Extracting the subsonic anti-symmetric lamb wave from a submerged thin spherical shell backscattering through iterative time reversal

The extraction of the weakly excited anti-symmetric Lamb wave from a submerged thin spherical shell backscattering is very difficult if the carrier frequency of the incident short tone burst is not at its frequency of greatest enhancement. Based on a single channel iterative time reversal technique, a method for isolating the subsonic anti-symmetric Lamb wave is proposed in this paper. The approach does not depend on the form function of a thin shell and any other priori knowledge, and it is also robust in the presence of some stochastic noise. Both theoretical and numerical results show that the subsonic anti-symmetric Lamb wave can be identified, even when the carrier frequency of the incident short tone burst is away from the frequency of greatest enhancement. The phenomenon may also be observed even in the case that the subsonic anti-symmetric Lamb wave is submerged in the noise, other than the case with the Signal to Noise Ratio being less than 10 dB, when the amplitude of the noise is comparable with the specular wave. In this paper, each iteration process contains a traditional transmission and time reversal transmission steps. The two steps can automatically compensate the time delay of the subsonic anti-symmetric Lamb wave relative to the specular wave and within-mode dispersion in the forward wave propagation.     

Variation of the 0+ ion density during low and high solar activity as measured by the SR0SS-C2 satellite

The O⁺ ion density measured by the SROSS-C2 satellite during solar minima (year 1995, F_10.7 = 77) and maxima (year 2000, F_10.7 = 181) has been analyzed for studying diurnal, seasonal, latitudinal and geomagnetic variations. The study region covers an area encompassed between 5-3 5° N latitude and 65-95° E longitude over India at a ~500 km altitude (F2 region). The year 2000 shows significant enhancement in the annual average of O⁺ ion density and attainment of post sunset secondary enhancement compared to 1995. Attributed to photoionization, daytime shows a maximum ionization compared to nighttime. However, attainment of post sunset secondary maxima is attributed to the strong pre-reversal enhancement in the vertical E x B drift. The effect of geomagnetic activity Kp through the E x B drift dynamic movement on O⁺ ion density distribution studies indicates periodicities of seven and nine days in 1995 and 2000, respectively, and polynomial dependency of the O⁺ ion density on geomagnetic activity Kp. Further on, stratification of the O⁺ ion density according to latitude (5-35° N) indicates high density in mid-latitudes (12-24° N) compared to high and low latitudes, except in the winter of 1995, which shows a distinct trend (i.e., density decreases with increasing latitude).