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     

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。     

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.