甘肃黄土高原水热气候异常阶段特征

利用1960～2004年相关地面实测气象资料,分析甘肃黄土高原地区水热气候异常变化的阶段性特征。结果表明,该地区地表变暖最为突出,夏半年增幅明显大于冬半年,地温随深度加深增温幅度越大;降水日数减少,连阴雨天气时段缩短、过程雨量减少,无雨时段增长,日照出现2次突变、呈现下降趋势;降水日数在1991年后突变减少,最长连续降水日数及过程降水量在1978年后突变减少。     

影响我国北方冬半年气旋的气候特征及年际变率

本文首先对气旋进行了客观定义,实现了气旋的自动识别与跟踪算法,利用NCEP/NCAR再分析资料建立了近60年(1951～2010)我国北方冬半年气旋活动数据集。对气旋的气候特征与年际变率进行了探讨。结果表明:蒙古国中西部、雅布洛诺夫山脉东麓等为主要气旋源地;蒙古国东南部、内蒙古东南部、松嫩平原是气旋活跃区;内蒙古东南部、东北地区中北部为气旋消亡区与快速填塞区;初春、仲秋季节气旋较活跃,冬季气旋最少;随季节推移,气旋活动区域向南、向东推进;气旋移动以偏东路径居多,其次是东南、东北路径;700 hPa风场对气旋移动趋势具有较好的指示意义;24 h标准加深率大于0.5 Bergeron的快速发展气旋,位于内蒙古东部、东北地区中北部、日本海中部等地;爆发性气旋则主要位于日本海附近,我国大陆极少;极端最强气旋主要集中在1980年代以前的仲秋与初春;1980年代以来,气旋频次相对较少,强气旋有逐渐增加的趋势;气旋频次减少与东亚中高纬度大气低层斜压性减弱有关。     

Modelling potential impacts of climate change on water and nitrate export from a mid-sized, semiarid watershed in the US Southwest

The impacts of climate change on water and nitrogen cycles in arid central Arizona (USA) were investigated by integrating the Second Generation Coupled Global Climate Model (CGCM2) and a widely used, physical process-based model, Soil and Water Assessment Tool (SWAT). With statistically downscaled daily climate data from the CGCM2 as model input, SWAT predicted increased potential evapotranspiration and decreased surface runoff, lateral flow, soil water, and groundwater recharge, which suggests serious consequences for the water cycle in this desert catchment in the future. Specifically, stream discharge is projected to decrease by 31 % in the 2020s, 47 % in the 2050s, and 56 % in the 2080s compared to the mean discharge for the base period (0.73 m³/s). A flow-duration analysis reveals that the projected reduction of stream discharge in the future is attributable to significant decreases in mid-range and low-flow conditions; however, flood peaks would show a slight increase in the future. The drier and hotter future also will decrease the rate of nitrogen mineralization in the catchment and ultimately, nitrate export from the stream. Since mean mineralization rate would decrease by 15 % in the 2020s, 28 % in the 2050s, and 35 % in the 2080s compared to the based period (9.3 g N ha^?1 d^?1), the combined impact of reduced catchment mineralization and reduced streamflow would predict declining nitrate export: from today’s mean value of 30 kg N/d, to 20, 15 and 12 kg N/d by the 2020s, 2050s, and 2080s, respectively.     

浙西南热带气旋强降水主要影响因子

对1950-2010年影响浙西南的热带气旋降水的移动路径、影响时间、强度、西风槽、西南季风以及地形等主要因子进行分析.结果表明:在玉环南-厦门一带登陆的热带气旋是影响浙西南的热带气旋中正面影响浙西南的类型,影响时间和最大平均过程降雨量、最大过程雨量存在着正相关关系,热带气旋的强度与其降水强度相关性较高.西风槽的存在不仅影响着热带气旋路径的变化,其槽前的西南气流也为热带气旋降水提供充足的水汽,同时槽后冷空气与热带气旋相结合,使丽水的西北部出现另一个强降水中心.西南季风为登陆后的热带气旋提供了水汽条件,使降水得到增幅.浙西南独特的地形,使在厦门以北到玉环以南登陆后西进、西北行或西北行后在120°E以西转向北上的热带气旋迎着山脉进入,降水强度明显加强.     

地面气象测报业务试题库自动化管理系统

将地面气象观测规范、地面气象观测、气象学等多项知识形成题库,利用VB6编程、Access 2003数据库及Word 2003文字处理软件,研制了地面气象测报业务试题库自动化管理系统,实现了以下主要功能:用户管理、数据库管理、试题库维护、自动生成试卷、试卷编辑打印。着重阐述该系统的设计思路、技术方法、功能实现及使用效果。     

基于三维地质模型的西咸新区地下空间开发 适宜性评价

地下空间开发地质适宜性评价是合理进行地下空间开发、降低开发地质风险的重要手段。传统的评价方法没有考虑地下空间复杂的垂向变化,因而无法满足越来越精确的地下空间规划要求。本文以西咸新区沣东沣西为例,结合该区地质地貌背景、工程地质特征、水文地质条件、不良地质作用以及地下空间开发现状等特点,建立地下空间开发地质适宜性评价因子体系;利用三维精细化剖分的评估单元为载体,综合使用多种三维空间分析方法从多要素地质模型中定量或定性提取各项指标,运用层次分析法模型开展研究区地下空间开发适宜性评价。评价结果表明：研究区60 m以浅地下空间开发利用条件优越,总体适宜开发建设。浅层空间易受文物保护区、地面水体、活动断裂影响,中层空间受城市建成区既有设施及地下构筑物影响较大,深部地下空间主要受断裂影响。该方法能够精细刻画地下空间在垂向上的差异,评估过程与结果能够立体透明化表达,能够定性、定量地为地下空间开发利用提供辅助决策,以达到资源保护优先、协同开发的开发利用格局。     

江西省“三农”服务专项建设现状与思考

通过对江西省24个"三农"服务专项建设实施地的"两个体系"建设情况开展实地调查,分析了江西省"三农"服务专项建设在提高气象为农服务现代化、促进气象工作政府化、惠民利民等三方面取得的成效,总结了各地的建设内容、成功经验、工作亮点和特色,梳理了存在的问题,并结合建设现状和有关要求,对今后江西省"三农"服务专项建设提出了六个方面的具体建议。     

Dynamics of the Jupiter Trojans with Saturn’s perturbation in the present configuration of the two planets

The dynamics of the two Jupiter triangular libration points perturbed by Saturn is studied in this paper. Unlike some previous works that studied the same problem via the pure numerical approach, this study is done in a semianalytic way. Using a literal solution, we are able to explain the asymmetry of two orbits around the two libration points with symmetric initial conditions. The literal solution consists of many frequencies. The amplitudes of each frequency are the same for both libration points, but the initial phase angles are different. This difference causes a temporary spatial asymmetry in the motions around the two points, but this asymmetry gradually disappears when the time goes to infinity. The results show that the two Jupiter triangular libration points should have symmetric spatial stable regions in the present status of Jupiter and Saturn. As a test of the literal solution, we study the resonances that have been extensively studied in Robutel and Gabern (Mon Not R Astron Soc 372:1463–1482, 2006). The resonance structures predicted by our analytic theory agree well with those found in Robutel and Gabern (Mon Not R Astron Soc 372:1463–1482, 2006) via a numerical approach. Two kinds of chaotic orbits are discussed. They have different behaviors in the frequency map. The first kind of chaotic orbits (inner chaotic orbits) is of small to moderate amplitudes, while the second kind of chaotic orbits (outer chaotic orbits) is of relatively larger amplitudes. Using analytical theory, we qualitatively explain the transition process from the inner chaotic orbits to the outer chaotic orbits with increasing amplitudes. A critical value of the diffusion rate is given to separate them in the frequency map. In a forthcoming paper, we will study the same problem but keep the planets in migration. The time asymmetry, which is unimportant in this paper, may cause an observable difference in the two Jupiter Trojan groups during a very fast planet migration process.     

Detection of large color variation in the potentially hazardousasteroid （297274） 1996 SK

Low-inclination near-earth asteroid(NEA)(297274) 1996 SK,which is also classified as a potentially hazardous asteroid,has a highly eccentric orbit.It was studied by multi-wavelength photometry within the framework of an NEA color survey at Lulin Observatory.Here,we report the finding of large color variation across the surface of(297274) 1996 SK within one asteroidal rotation period of4.656 ± 0.122 hours and classify it as an S-type asteroid according to its average colors of B- V = 0.767 ± 0.033,V- R = 0.482 ± 0.021,V- I = 0.801 ± 0.025and the corresponding relative reflectance spectrum.These results might be indicative of differential space weathering or compositional inhomogeneity in the surface materials.     

Disappearance of a coronal hole induced by a filament activation

We present a rare observation of direct magnetic interaction between an activating filament and a coronal hole(CH). The filament was a quiescent one located at the northwest of the CH. It underwent a nonradial activation, during which filament material constantly fell and intruded into the CH. As a result, the CH was clearly destroyed by the intrusion. Brightenings appeared at the boundaries and in the interior of the CH, meanwhile, its west boundaries began to retreat and the area gradually shrank. It is noted that the CH went on shrinking after the end of the intrusion and finally disappeared entirely. Following the filament activation, three coronal dimmings(D1–D3) were formed, among which D1 and D2 persisted throughout the complete disappearance of the CH. The derived coronal magnetic configuration shows that the filament was located below an extended loop system, which obviously linked D1 to D2. By extrapolating this result, our observations imply that the interaction between the filament and the CH involved direct intrusion of the filament material to the CH and the disappearance of the CH might be due to interchange reconnection between the expanding loop system and the CH's open field.