甘肃第四纪古地理环境

第四纪在全球性冰期和间冰期气候影响下，甘肃气候呈干旱、寒冷与温暖、湿润交替变化。沉积物以灰色格调为主，水平和垂直分带规律明显，成因类型复杂。各地区在小气候影响下植被发育不平衡。总的看来，以干旱区系草本植物为主，喜温暖湿热的木本植物较少，一般呈荒漠草原型和疏林草原型，局部为森林草原型。动物群的分布和古人类的发展受古地理环境影响：早更新世早期以大型哺乳动物为主；早更新世晚期和中更新世以穴居的鼠兔类为主；晚更新世以干旱—半干旱草原型动物群为特征；全新世在适宜条件下人类文化得到发展，部分野生动物在人类豢养下成为家畜     

两系杂交稻制种的气候适应性研究

研究两系杂交稻的首要不育系———培矮64S制种的气候适应性, 一方面可为两系杂交稻的生产提供决策参考, 另一方面也可为其它不育系的研究提供借鉴。分析气候适应性时, 首先利用播种—抽穗天数及其对应的气象资料, 建立发育期模型; 然后利用自交结实率资料及其对应的气象资料建立育性量化模型, 并求出育性转换的光温指标; 最后将我国稻区35个站点42年 (1951~1992年) 的气象资料代入发育期模型, 求出各站点的可能出穗持续期 (最早出穗期—最晚出穗期的历期), 对比育性转换的光温指标, 确定培矮64S在80%、90%和95%保证率下连续不育 (可育) 的初、终日, 将连续不育期作为生产杂交稻种子的季节, 将连续可育期作为繁殖培矮64S的季节。结果显示:培矮64S仅能在海南岛及云贵高原中低海拔地区自交繁殖; 而在东北、云贵高原以外的稻区, 培矮64S均可用于生产两系杂交稻的种子, 各稻区制种季节的长短、起止日期与种植地的纬度、海拔高度相关。     

GPS高程曲面拟合算法的精度分析

在GPS高程测量中需要将大地高转换为正常高。本文对GPS高程的多项式曲面拟合、多面函数拟合和移动曲面函数拟合算法进行了比较分析。结果表明,三种拟合算法均能达到四等几何水准的要求,但移动曲面拟合算法精度最高,多面函数拟合算法精度最低。     

华东地质学院校园网设计方案简介

根据华东地质学院校园网二期建设项目,简要介绍了本院校园网的拓扑结构图、校园网采用的VLAN技术及其第三层交换（路由）技术,阐述了校园网建设中子网划分与IP地址分配方法。     

长河坝水电站开关站工程边坡稳定性三维有限元分析

长河坝水电站开关站边坡的稳定性主要受斜向上游的f24断层控制,其变形破坏方式主要为旋转滑移拉裂型.本文采用三维有限元分析方法对该边坡的稳定性进行了分析,分析结果表明,工程边坡具有从下游往上游稳定性提高的趋势,边坡的稳定性具有一定的分区特征:下游侧0～35 m斜坡处于不稳定状态,35～70 m处于潜在不稳定状态,70 m以上处于基本稳定状态.上述结果为工程边坡的支护措施设计提供了依据.     

高效多路直流开关电源

本文介绍一种新型的直流开关电源,该电源是一种直流电压输入,三种直流电压输出,并能够达到相当高的效率。这种电源适用于数字化设备的无人职守台站。本文也论述了实现的技术思路和达到的技术要求。     

澳门地质概况

对澳门的泥盆系、第三系、第四系地层出露作了叙述，说明了花岗闪长岩、黑云母粗粒花岗石等几篑夺浆岩的分布及岩性特征，详细地论述了区内８条断裂构造，概述了碎石、建筑材料等矿产资料。     

高隔离多路射频转换开关的研制

介绍一个可用于多路信号自动测量系统或自动切换系统的高隔离射频多路转换开关的设计与制作。开关制式为双刀16掷;控制采取本地（利用本机面板控制）和遥控（IEEE—488标准接口）两种方式工作频率范围为DC～100MHz;路与路之间的串扰,隔离度优于120dB（5MHz）[1]。     

On the impact of multiply charged heavy solar wind ions on the surface of Mercury, the Moon and Ceres

We have studied the impact of multiply charged solar wind O⁷⁺ and Fe⁹⁺ ions on the surfaces of Mercury, the Moon and on a Ceres-size asteroid using a quasi-neutral hybrid model.The simulations showed that heavy O⁷⁺ and Fe⁹⁺ ions impact on the surface of Mercury non-homogenously, the highest flux being near the magnetic cusps—much as in the case of impacting solar wind protons. However, in contrast to protons, the analyzed heavy ions do not create high ion impact flux regions near the open-closed magnetic field line boundary. Dawn-dusk asymmetry and the total ion impact flux were each found to increase with respect to the increasing mass per charge ratio for ions, suggesting that the Hermean magnetic field acts as a mass spectrometer for solar wind ions. The Moon, in contrast, does not have a global intrinsic magnetic field and, therefore, solar wind ions can freely impact on its surface when this body is in the solar wind. The same is true for a, non-magnetized, Ceres-size asteroid.The impact of multiply charged ions on a solid surface results in a large variety of physical processes, of often intimately inter-related atomic reactions, e.g. electron exchange between solid and approaching projectile, inelastic scattering of projectile, electronic excitation in the projectile and/or the solid, ejection of electrons, photons, neutral and iodized surface particles, and eventual slowing down and stopping of the projectile in the solid. The electron transfer process between impacting heavy ions and surface constituents can result in soft X-ray (E<1 keV) and extreme ultraviolet (EUV) photon emissions. These processes will eventually damage the target surface. Analysis of the hybrid Mercury model (HYB-Mercury) suggests that, at this planet the damaging processes result in non-homogenous ageing of the surface that is controlled by the intrinsic magnetic field of the planet and by the direction of the interplanetary magnetic field. In the corresponding Lunar model (HYB-Moon) and in the non-magnetized asteroid model (HYB-Ceres), surface ageing is demonstrated to take place on that side of the body that faces toward the flow of the solar wind.