物理过程参数化方案对中国夏季降水日变化模拟的影响

国际耦合模式比较计划第六阶段(CMIP6)新增的高分辨率模式比较计划(HighResMIP)首次提供全球高分辨率(25—50 km)多模式集合的气候模拟试验结果。利用8个CMIP6 HighResMIP模式评估了高分辨率全球气候模式对青藏高原夏季小时降水与极端降水的模拟能力,结果表明：CMIP6高分辨率模式高(低)估了青藏高原地区的降水量和频率(强度),过多的降水量主要来自模式对降水频率的高估,尤其是弱降水(< 2 mm·h^-1)的发生频率。模拟偏差与地形海拔密切相关,偏差大值区主要位于高原南坡和东坡陡峭地形区。模式不能准确再现降水量与海拔之间的关系,高(低)估了高(低)海拔地区的降水量。模式低估了降水强度随海拔升高而降低的变化速率。在日变化方面,模式能够模拟出青藏高原降水傍晚至午夜的峰值特征,但明显低估了降水的日变化振幅。在小时极端降水方面,模式低估了高原区域平均极端降水第95百分位数阈值,仅为观测值的57%。

     

Design and implementation of a 3D ocean virtual reality and visualization engine

In this study,a 3D virtual reality and visualization engine for rendering the ocean,named VV-Ocean,is designed for marine applications.The design goals of VV-Ocean aim at high fidelity simulation of ocean environment,visualization of massive and multidimensional marine data,and imitation of marine lives.VV-Ocean is composed of five modules,i.e.memory management module,resources management module,scene management module,rendering process management module and interaction management module.There are three core functions in VV-Ocean:reconstructing vivid virtual ocean scenes,visualizing real data dynamically in real time,imitating and simulating marine lives intuitively.Based on VV-Ocean,we establish a sea-land integration platform which can reproduce drifting and diffusion processes of oil spilling from sea bottom to surface.Environment factors such as ocean current and wind field have been considered in this simulation.On this platform oil spilling process can be abstracted as movements of abundant oil particles.The result shows that oil particles blend with water well and the platform meets the requirement for real-time and interactive rendering.VV-Ocean can be widely used in ocean applications such as demonstrating marine operations,facilitating maritime communications,developing ocean games,reducing marine hazards,forecasting the weather over oceans,serving marine tourism,and so on.Finally,further technological improvements of VV-Ocean are discussed.     

西藏鄂雅错盐湖砷和汞的分布特征研究

本研究对西藏鄂雅错盐湖和主要支流中不同形态的砷(亚砷酸盐As(Ⅲ)、砷酸盐As(Ⅴ)、一甲基砷酸MMA、二甲基砷酸DMA)和总汞(THg)含量进行了测定,并与主要水质参数进行相关性分析研究,结果表明鄂雅错盐湖As主要以As(Ⅴ)形态存在,其次分别为As(Ⅲ)、DMA和MMA,其中无机砷的含量明显大于有机砷。相比较其他砷的形态,盐湖中As(Ⅲ)与主要水质参数的相关性显著,与总溶解性固体(TDS)、总溶解态氮(DTN)呈显著的强正相关性,与水温、溶解氧 (DO)、氧化还原电位(Eh)、pH呈显著负相关性。总汞浓度较低,且与主要水质参数相关性不显著。通过风险评价发现鄂雅错湖水中砷存在一定的致癌健康风险,汞不存在风险。本研究丰富了西藏盐湖和支流水体中砷、汞分布特征及其环境影响因素的认识,对于环境保护具有一定的意义。     

北太平洋150°E-165 °E海域柔鱼重心渔场的年间变动

利用空间距离和灰色关联度分析方法对1995～2001年间北太平洋150°E—165°E柔鱼作业渔场的重心分布进行比较研究,1995～1997年8～10月份作业渔场的重心与1998～2001年存在着较大的差异,前者基本上在150°E—153°30E的42°30′N以南海域,而后者位于155°E-161°E的42°45′N以北海域。聚类结果表明,8月份作业渔场重心分为三类:1998～2001年为一类,1996～1997年为一类,而1995年为一类。9月份产量重心与作业渔船重心的聚类结果则有所不同,产量重心的聚类结果为四类,即1999～2001年为一类,1997、1996年为一类,1998年和1995年各为一类;而作业渔船重心的聚类结果则分为三类,即1999～2001年为一类,1995～1997年为一类,1998年为一类;10月份作业渔场重心分为三类;1998、2001和1999年为一类,1995～1997年为一类,2000年为一类。年间的渔场变化可能是由海洋环境条件所引起。灰色关联分析表明,产量重心与作业渔船重心存在一定的差异。8～10月份作业渔场重心的总体变化趋势为向东北偏东移动。     

北京市大兴区大气降尘环境磁学特征及其环境意义

应用环境磁学方法对北京市大兴区大气降尘环境磁学特征进行了系统研究,并通过与北京市朝阳区、兰州市大气降尘环境磁学特征的对比,对环境磁学在污染物来源解析及扩散条件研究中的应用机理进行了探讨。结果表明,大兴区大气降尘磁性矿物含量明显高于本区表土,人为源影响显著;降尘样品磁学特征主要受磁铁矿控制,并含有一定数量的磁赤铁矿,磁性矿物为准单畴和多畴颗粒;大兴区降尘样品的磁性矿物含量明显低于朝阳区,且样品颗粒相对较细,表明人口密度、车流量、城市发达度对大气污染程度存在显著影响;大兴区与兰州市大气降尘磁性矿物含量的季节变化差异表明,燃煤取暖对北京大气质量的影响显著减弱,燃煤锅炉改造是大气污染防治的重要措施之一。气象因素对大气颗粒物浓度变化有重要影响,降水、低气压和高风速利于大气颗粒物的清除和扩散,低气温对大气颗粒物污染的负面影响显著。     

2009年夏季极区电离层加热实验观测研究

2009年夏季,中国在挪威特罗姆瑟(Tromsφ)利用非相干散射雷达进行电离层加热实验。实验中发现了处在150km附近的小范围温度增强事件和150—400km之间的大范围温度增强事件。前者的相对增幅明显,后者的绝对增量更大。对这两类加热事件来说,温度增量百分比均随加热功率的增加线性增长,但对比两类加热事件来看,增长速度随加热频率增大而减小。加热效应存在显著的二维分布特征,加热最强方向处在场向附近。加热效应受加热天线波束指向与地磁场的夹角影响明显,随夹角增大温度增强效应减弱。     

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。

     

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.     

Eco-environment range in the source regions of the Yangtze and Yellow rivers

Based on geographical and hydrological extents delimited, four principles are identified, as the bases for delineating the ranges of the source regions of the Yangtze and Yellow rivers in the paper. According to the comprehensive analysis of topographical characteristics, climate conditions, vegetation distribution and hydrological features, the source region ranges for eco-environmental study are defined. The eastern boundary point is Dari hydrological station in the upper reach of the Yellow River. The watershed above Dari hydrological station is the source region of the Yellow River which drains an area of 4.49×104 km2. Natural environment is characterized by the major topographical types of plateau lakes and marshland, gentle landforms, alpine cold semi-arid climate, and steppe and meadow vegetation in the source region of the Yellow River. The eastern boundary point is the convergent site of the Nieqiaqu and the Tongtian River in the upstream of the Yangtze River. The watershed above the convergent site is the source region of the Yangtze River, with a watershed area of 12.24×104 km2. Hills and alpine plain topography, gentle terrain, alpine cold arid and semi-arid climate, and alpine cold grassland and meadow are natural conditions in the source region of the Yangtze River.