中国南极维多利亚地新站气象特征分析

中国南极新站选择在维多利亚地特拉诺瓦湾难言岛上进行建设,其气象环境状况是开展科学研究的基础工作,也是考察队员生命安全保障的基础资料。因此,通过2013年度难言岛气象站的观测资料,结合附近地区历史气象资料,对该区域气象要素特征进行了分析。结果表明:(1)由于地处罗斯海与东南极冰盖交界处,难言岛年均气压为987.8 h Pa,与中山站非常接近;(2)年均温为-16.1℃,最低气温为-39.3℃,且冬季气温波动较大,标准差可达±6.0℃;(3)年均相对湿度为42.1%,年均比湿为0.6 g·kg-1且冬季比湿极低,空气非常干燥,降水量非常低;(4)盛行风向为WNW,5—7级风出现频率超过50%,但夏季风速明显低于冬季风速,一般不超过8.0 m·s~(-1),有利于中国在夏季开展工程建设和补给;(5)难言岛年总辐射量为3 342.8 MJ·m~(-2),明显低于中山站,但两站反照率非常接近。     

Field determination for roughness length above the different non-erodible surfaces

Non-erodible elements, for its disturbance to the near-surface airflow, have been widely used in arid and semi-arid regions to protect the surface from wind erosion. Roughness length was usually used to evaluate the protection effect of non-erodible elements from wind erosion. In this study, the wind profiles above five types of non-erodible surfaces including gravel, wheat straw checkerboard barriers, cotton stem checkerboard barriers, shrubs, and herbs were measured and analyzed. The wind velocities above these surfaces increased with height approximately in logarithmic functions. The roughness length of different non-erodible surfaces was calculated by the functions of wind profiles. The results reveal that:(1) Roughness length increased with wind velocity in given wind velocity ranges. (2) On vegetative surfaces, wind did not effectively bend the stems. The threshold wind velocity for bending the stems of Achnatherum splendens was 4 m/s, 10 m/s for Agropyron cristatum, and for Artemisia ordosica, no obvious bending of stems even for wind velocity reaching 12 m/s. (3) Correlation analysis results show that the vegetation''s coverage and frontal area affect the roughness length more significantly than the other parameters. (4) The protective results of these non-erodible elements were evaluated. The checkerboard sand barriers made of cotton stem could provide more effective protection than that made of wheat straw. In the same coverage conditions, vegetation could provide more effective protection from wind erosion than gravel, and the blending of different non-erodible elements especially the combination of blending of vegeation and checkerboard sand barriers could provide more effective protection to the surface.     

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。     

气候变化对中国大雾的影响

1 Introduction The global environmental problem caused by climatic warming has attracted increasing attention of the scientific communities, the public and governments of various countries. The mean temperature of the recent decade is the highest of the p…     

乡土地理课程资源在高中地理教学中的应用

乡土地理课程资源对培养中学生地理核心素养具有重要促进作用。乡土地理课程资源在高中地理教学应用中应把握"贴近生活、结合课标、难易适度"的原则,科学运用于编写校本教材、开展案例教学、编制试题、设计野外考察路线、开展研究性学习活动等。     

Under the shadow of the Magellanic Bridge: A measurement of the extragalactic background at ∼ 0.7 keV

We measured the extragalactic 0.7 keV X-ray background by observing the X-ray shadow of a neutral gas cloud in the Magellanic Bridge region. Two ROSAT PSPC observations of total 104 ks were complemented by a detailed H I mapping of the cloud with both the Parkes 64 m telescope and the Australia Telescope Compact Array. From the detected anti-correlation between the observed background intensity and the H I column density of the cloud, we derived the unabsorbed extragalactic background intensity as ∼ 28 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹ at ∼ 0.7 keV. The 95% confidence lower limit 18 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹ is greater than the expected point-like source contribution ? 14 keV s⁻¹ cm⁻² keV⁻¹ sr⁻¹, constrained by the mean source spectrum together with the total background intensity in the 1-2 keV band. A significant fraction of the 0.7 keV background likely arises in a diffuse hot intergalactic medium of a few million degrees, as has been predicted in hydrodynamic simulations of cosmological structure formation.Richard McCray     

人海河流河口及其近海水域盐度分析方法浅析

在水质监测及水环境调查中,盐度分析工作是一个重要环节,根据现行的<水质分析国家标准>,<海洋调查规范>,地表水及生活用水的盐度分析一般采用前者,而海洋水样则采用后者.对于长江口及其近海水域既有适用<水质分析国家标准>(TB11896-89)的区段,又有适用<海洋调查规范>的区域,亦有两者都不适用的部分.本文通过对长江口盐度分析方法的研究.阐述了该区域进行水样盐度分析的各种方法的适用范围及提高效率保证成果质量的办法.最后作者提出的人海河流河口及其近海水域盐度分析的方法是:按取样地点位于河口的具体位置来选择其分析方法.     

浙西北江山─绍兴断裂带构造演化特征

江山—绍兴断裂带是中国南方最重要的构造带之一。它是江南陆块与华夏陆块神功运动形成的碰撞拼贴带。它表现出明显的多期变形、构造叠加的特征：神功运动形成近东西向平卧褶皱；印支运动沿断裂带有向北西强烈的推覆挤压。断裂带不同时期的活动反映了不同特征的构造环境，形成不同的构造变形特征，并对两侧的地质历史具有明显的控制作用。     

极谱法在镉诱导单胞藻和禾草类植物螯合物研究的应用

三角褐指藻（Phaeodactylum tricornutum）和翦股颖草属禾草（A-grostis capillaris）经过处理后再用液相层析法从中提取一种金属结合多肽，极谱分析表明不同的镉结合多肽具有不同的稳定性，金属结合与金属硫蛋白不同，在电位--1.7V附近未出现氧催化峰，金属硫蛋白以及从单胞藻和禾草中提取的多肽在极谱测定过程中都在电位-520mV和-930mV附近出现双峰，在-520mV处，半波电位显示了单个镉硫醇键的还原，在-930mV处的峰是由于镉和硫多齿螯合的还原，因此这通常可用以鉴定镉螯合物。在镉浓度为5umol/dm^3和10umol/dm^3时-930mV的峰高与镉浓度之间存在着对应关系。     

On the Collision Nature of Two Coronal Mass Ejections: A Review

Observational and numerical studies have shown that the kinematic characteristics of two or more coronal mass ejections (CMEs) may change significantly after a CME collision. The collision of CMEs can have a different nature, i.e. inelastic, elastic, and superelastic processes, depending on their initial kinematic characteristics. In this article, we first review the existing definitions of collision types including Newton’s classical definition, the energy definition, Poisson’s definition, and Stronge’s definition, of which the first two were used in the studies of CME–CME collisions. Then, we review the recent research progresses on the nature of CME–CME collisions with the focus on which CME kinematic properties affect the collision nature. It is shown that observational analysis and numerical simulations can both yield an inelastic, perfectly inelastic, merging-like collision, or a high possibility of a superelastic collision. Meanwhile, previous studies based on a 3D collision picture suggested that a low approaching speed of two CMEs is favorable for a superelastic nature. Since CMEs are an expanding magnetized plasma structure, the CME collision process is quite complex, and we discuss this complexity. Moreover, the models used in both observational and numerical studies contain many limitations. All of the previous studies on collisions have not shown the separation of two colliding CMEs after a collision. Therefore the collision between CMEs cannot be considered as an ideal process in the context of a classical Newtonian definition. In addition, many factors are not considered in either observational analysis or numerical studies, e.g. CME-driven shocks and magnetic reconnections. Owing to the complexity of the CME collision process, a more detailed and in-depth observational analysis and simulation work are needed to fully understand the CME collision process.