泥河湾盆地虎头梁剖面河湖相沉积物磁组构特征及其环境意义

泥河湾盆地在第四纪环境变化和古人类演化研究领域占有重要地位。虎头梁剖面记录了中更新世以来泥河湾盆地逐渐消亡的过程。本文对虎头梁天然露头剖面进行了详细的沉积学、岩石磁学和磁组构研究。剖面沉积物中的磁性矿物以假单畴（PSD）的磁铁矿为主,还含有一定量的赤铁矿,磁组构类型为正常沉积磁组构。根据虎头梁剖面沉积相的划分和磁组构参数特征,将泥河湾盆地中-晚更新世晚期的演化过程划分为3个阶段：下部为第Ⅰ阶段（60~53m）,中部为第Ⅱ阶段（53~12m）,上部为第Ⅲ阶段（12~0m）,包含3个完整湖侵旋回,每个旋回由下部灰黄色粗粒三角洲相到中部黄灰色滨湖相再到顶部灰绿色细粒湖相组成,相应的磁组构参数值由大到小的变化规律,中部第Ⅱ阶段推断由气候因素主导,上部第Ⅲ阶段可能主要由构造驱动,长期稳定的优势古水流方向以NW向为主,而东坡遗址时期的古人类可能生活在湖侵阶段的相对短期湖退的滨岸地带。

     

台风作用下的港湾型潮滩沉积过程 以2008年“凤凰”台风对福建省罗源湾的影响为例

通过对"凤凰"台风的现场观测和沉积物样品的分析,结果表明,在台风影响下潮水淹没时间增长,增水达1.1 m;台风期间互花米草盐沼内流速变化较复杂,而且盐沼内部流速大于盐沼边缘的;台风期间盐沼边缘潮周期平均悬沙含量是台风前2 d的7倍;台风期间十分之一波高最大为1.54 m。滩面重复测量结果显示,台风登陆期间整个光滩滩面都发生了侵蚀,盐沼内部有部分地区发生侵蚀,侵蚀深度为4.5~5.5 cm,盐沼边缘的侵蚀深度仅为0.7 cm,侵蚀原因主要是植被在风浪作用下从根部折断,从而带走了滩面的沉积物;随着台风强度的减弱,整个滩面均接受悬沙沉降;台风带来的强降雨是影响滩面沉积物活动的重要因素。     

Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU

Based on the variations of sunspot numbers, we choose a 1-year interval at each solar minimum from the beginning of the acquisition of solar wind measurements in the ecliptic plane and at 1 AU. We take the period of July 2008??C?June 2009 to represent the solar minimum between Solar Cycles 23 and 24. In comparison with the previous three minima, this solar minimum has the slowest, least dense, and coolest solar wind, and the weakest magnetic field. As a result, the solar wind dynamic pressure, dawn?Cdusk electric field, and geomagnetic activity during this minimum are the weakest among the four minima. The weakening trend had already appeared during solar minimum 22/23, and it may continue into the next solar minimum. During this minimum, the galactic cosmic ray intensity reached the highest level in the space age, while the number of solar energetic proton events and the ground level enhancement events were the least. Using solar wind measurements near the Earth over 1995??C?2009, we have surveyed and characterized the large-scale solar wind structures, including fast-slow stream interaction regions (SIRs), interplanetary coronal mass ejections (ICMEs), and interplanetary shocks. Their solar cycle variations over the 15 years are studied comprehensively. In contrast with the previous minimum, we find that there are more SIRs and they recur more often during this minimum, probably because more low- and mid-latitude coronal holes and active regions emerged due to the weaker solar polar field than during the previous minimum. There are more shocks during this solar minimum, probably caused by the slower fast magnetosonic speed of the solar wind. The SIRs, ICMEs, and shocks during this minimum are generally weaker than during the previous minimum, but did not change as much as did the properties of the undisturbed solar wind.     

Lithologic mapping of HED terrains on Vesta using Dawn Framing Camera color data

The surface composition of Vesta, the most massive intact basaltic object in the asteroid belt, is interesting because it provides us with an insight into magmatic differentiation of planetesimals that eventually coalesced to form the terrestrial planets. The distribution of lithologic and compositional units on the surface of Vesta provides important constraints on its petrologic evolution, impact history, and its relationship with vestoids and howardite‐eucrite‐diogenite (HED) meteorites. Using color parameters (band tilt and band curvature) originally developed for analyzing lunar data, we have identified and mapped HED terrains on Vesta in Dawn Framing Camera (FC) color data. The average color spectrum of Vesta is identical to that of howardite regions, suggesting an extensive mixing of surface regolith due to impact gardening over the course of solar system history. Our results confirm the hemispherical dichotomy (east‐west and north‐south) in albedo/color/composition that has been observed by earlier studies. The presence of diogenite‐rich material in the southern hemisphere suggests that it was excavated during the formation of the Rheasilvia and Veneneia basins. Our lithologic mapping of HED regions provides direct evidence for magmatic evolution of Vesta with diogenite units in Rheasilvia forming the lower crust of a differentiated object.     

大管岛多能互补独立发电系统的发电量设计

结合大管岛居民用电需求,论述了当采用波浪能、太阳能、风能多能互补的独立发电系统时的发电量设计,并根据电力需求与波浪能、太阳能、风能能源资源的季节性变化进行了多能互补的供电效果分析.     

基于GWR模型的中国区域旅行社业效率空间分异及动力机制分析

基于DEA模型对中国31个省域的旅行社业效率空间分异特征进行了分析,首次运用GWR模型探索交通、资本、人才、信息化和经济动力对区域旅行社业效率影响的空间差异。结果表明：旅行社业效率在空间上具有正相关性和集聚特征,空间格局从“川”字型向“山”字型转变。各动力因子的系数均存在空间非平稳性。资本和人才动力的回归系数在空间分布上从南向北依次递减;经济动力的分布趋势为从北向南依次递减;交通动力对中西部地区旅行社效率提升的促进作用显著于东部地区;信息化动力则在东部地区表现出较强的促进作用。     

东北三省城乡收入差距空间格局及其分异机制研究

借助多元逐步线性回归、GWR等模型方法,探讨1990年以来东北三省城乡收入差距空间格局、类型特征及其分异机制,最后提出城乡统筹可持续发展建议。结果表明： 1990年以来,东北三省城乡居民收入水平大幅提高,但大部分地区城镇居民可支配收入水平仍低于全国平均水平;城乡收入差距整体有所拉大,呈现出“中间高、两端低”的空间特征。 城乡收入差距空间分布格局受经济发展水平、工业拉动效应、服务业带动力和交通通达程度影响,其中经济发展水平对城乡收入差距由早期的正向拉大作用为主,逐步演变为负向抑制效应。 据此提出对策建议：深化改革开放,加快国有企业改革步伐,优化区域产业结构,提高服务业发展水平和比重,激发市场活力,破解制约区域经济发展的各种障碍;加快实施乡村振兴战略,促进乡村资源开发,开辟致富增收新路径。     

污水-海水混合过程中磷转移的动力学

模拟研究厦门市污水排海时污水-海水混合过程中磷含量和形态的变化,及其在海水-颗粒物界面交换的动力学过程;提供转移模式,确定转移速率,进行磷的容量校正,为厦门西海域环境容量估算和水质控制提供定量参数和理论依据。     

隧道工程地质评价的内容和方法

结合工程隧道实际,首先阐述了隧道工程的基本地质环境和工程地质条件,然后针对隧道工程可能出现的不良地质现象和可采取的工程措施,从大气降水、围岩稳定、围岩压力、洞口稳定、隧道比选等角度探讨隧道工程地质评价的主要方法和一般内容,进行隧道工程地质评价,为隧道施工、支护提供了依据.     

9012号热带气旋维持的卫星云图和垂直结构特征分析

本文根据卫星云图的演变和常规天气分析相结合，对9012号热带气旋登陆后维持水消的成因进行了分析。指出该热带气旋经久不消的重要原因为其西南侧对流云团和东北侧高空槽前对流云带与热带气旋云系相衔接在中低层东北气流引导下卷入，热带气旋内部的两条云带的维持，以及利有的环流条件。