A Research on the Gravity Deformation of Delingha 13.7m Telescope

Based on digital photogrammetric measurements, the antenna panels of the Delingha 13.7m radio telescope are adjusted to make the main dish have an optimal paraboloidal surface at the elevation of 52°, thus the overall antenna efficiency is optimized for different observing elevations. Observations indicate that the aperture efficiency of the telescope has been improved approximately twice in comparison with the antenna panels adjusted on the basis of theodolite measurements. According to the results of the measurements at different elevations, the models of antenna gravity deformation are built, including the displacement and tilt angle of the subreflector, as well as the focal length and surface error of the main reflector, as functions of elevation angle. In the process of modeling the gravity deformation of the main dish, instead of the direct calculation method, the least square fitting on the measured surface errors at different elevation angles is adopted, in order to reduce the effect of measurement errors on the accuracy of the model.     

Mark 421天体多波段辐射机制研究

基于对数抛物线型电子分布,用单区、均匀同步自康普顿(Synchrotron Self-Compton,SSC)辐射模型计算BL Lac天体S5 0716+714的多波段能谱,并与Paggi等人的结果进行了比较.模型的计算结果与Paggi等人直接用δ函数近似得到的结果不同,导致该差异的主要原因可能是由于单电子同步辐射的δ函数近似丢失了电子的部分能量而影响逆康普顿散射结果.把该模型分别应用于Mark 421天体的高、中、低3种不同状态下的多波段观测结果,理论计算结果能与不同状态下的观测结果符合得很好.分析认为,观测到的Mark 421天体的不同状态可能是由于喷流内电子分布变化引起的.     

Improving the estimate of wind energy input into the Ekman layer within the Antarctic Circumpolar Current

Based on the data and method offered by Liu et al. (2009), the direct wind and Stokes drift-induced energy inputs into the Ekman layer within the Antarctic Circumpolar Current (ACC) area are reestimated since the results of the former have been proved to be underestimated. And the result shows that the total rate of energy input into the Ekman-Stokes layer within the ACC area is 852.41 GW, including 649.75 GW of direct wind energy input (76%) and 202.66 GW of Stoke drift-induced energy input (24%). Total increased energy input, due to wave-induced Coriolis-Stokes forcing added to the classical Ekman model, is 52.05 GW, accounting for 6.5% of the wind energy input into the classical Ekman layer. The long-term variability of direct wind and Stokes drift-induced energy inputs into the Ekman layer within the ACC is also investigated, and the result shows that the Stokes drift hinders the decadal increasing trend of direct wind energy input. Meanwhile, there is a period of 4-5 a in the energy spectrums, as same as the Antarctic circumpolar wave.     

The role of mindanao dome in the variability of the Pacific North equatorial current bifurcation

The Mindanao Dome (MD) features prominent oceanic variability and is located geographically close to the bifurcation latitude Y _b of the Pacific North Equatorial Current. In this study, the role of the MD in the variability of Y _b is examined with 20 years of satellite altimetric sea surface height (SSH) data and a 1.5-layer linear Rossby wave model. It is shown that the seasonal variations of surface Y _b are related to not only the SSH fluctuations near the bifurcation point (bifurcation box; 125°–130°E, 12°–15°N) but also those outstanding in the MD region (MD box; 127°–132°E, 6°–9°N). The impact of the MD SSH changes is significant when the bifurcation point stays at southerly latitudes during February–September, which hinders (delays) the southward leap (northward retreat) of Y _b in April–May (July–August) and thus leads to the asymmetry of the mean Y _b seasonal cycle (with a positive skewness of γ = +0.64). Such asymmetry also shows year-to-year variations depending on yearly mean Y _b value. A southerly yearly mean Y _b involves larger contribution of the MD and thus causes larger asymmetry of Y _b seasonal cycle. At interannual and longer timescales, the MD acts to amplify the fluctuations of the bifurcation. It is responsible for about 20 % of the total low-frequency Y _b variances and plays an important role in the 0.12° year^?1 southward trend of Y _b in the past two decades. The impact of the MD on Y _b changes is becoming increasingly significant at various timescales such as the bifurcation point migrating southward in recent years.     

The Global Distribution of Diapycnal Mixing and Mixing Coefficient Tensor in the Upper 2000m Ocean from Argo Observations

Diapycnal Mixing (DM) within the upper 2000m of the global ocean is calculated by a fine-scale parameterization using the multiyear-mean density gridded product that created by employing all the Argo float observations to date through the recently published equation of seawater TEOS-10. The geographic distribution of Argo-derived DM derived in this study is spatial-dependent and varies with latitude and depth. The magnitude and pattern of DM is favorably validated by comparisons with previous studies. Furthermore, the mixing coefficient tensor K is calculated and analyzed. Components of the tensor fitting for the geopotential coordinate models are also presented. It is found that the tensor components in horizontal direction, K_xx and K_yy, have similar magnitude and distribution pattern. In the vertical, K_zz is enhanced over regions with rough topography and strong wind (e.g., Westerly region), suggesting agreement with previous estimates. This work presents a scheme to estimate the DM and mixing coefficient tensor using Argo observations, and offers a useful Argo-based mixing product for the purpose of promoting the study and modeling of ocean circulation and other processes.     

北极海冰与北半球大气环流及气温的相关性分析

利用NASA的北极海冰密集度资料(分辨率1.0°×0.25°,时间1979.10-2002.8)对冬季(12-2月)鄂霍次克海到白令海(42°-66°N、131°-158°W)的海冰场进行EOF分解,得到特征向量的空间分布及时间系数.利用NCEP再分析月资料(分辨率2.5°×2.5°,时间1979-2002年),采用合成分析的方法,分别对该区域海冰分布第一特征向量时间系数超过+0.5和低于-0.5年份做冬季500hPa高度、l000hPa高度、1000hPa气温的合成距平场.分析结果表明该区域的海冰分布与北半球中高纬度的大气环流和气温有显著的关系,同一模态下的海冰分布反位相时对应的大气状况也有明显的相反趋势.     

Research for length change of four seasons over China in recent 47 years

Using daily temperature data from 599 Chinese weather stations during 1961–2007, the length change trends of four seasons during the past 47 years were analyzed. Results show that throughout the region, four seasons’ lengths are: spring becomes shorter (-0.8 d/10yrs), summer becomes longer (3.2 d/10yrs), autumn (-0.5 d/10yrs) and winter (-1.6 d/10yrs) becomes shorter. This trend is different in spatial distribution, namely it is very obvious in northern than southern China, and also remarkable in eastern than western China. Summer change is most obvious, but autumn has little change comparatively. This trend is highly obvious in North, East, Central and South China. In the Southwest starting in the 21st century, summer becomes longer and winter shortens. The trend in the Plateau region since the 1980s is that spring becomes longer and winter shortens. The average annual temperature increased during the past 47 years, and the change of the average annual temperature precedes seasons’ length. Thus, the average annual temperature has a certain influence on the length change of seasons.     

三峡库区作辑托背斜和巴东断裂与滑坡类型的关系

三峡库区作为地质灾害的多发地区,有关构造特征与滑坡之间的因果关系及相同局部构造上多个滑坡个体之间的因果关系研究很少。在应用断层相关褶皱理论方法的基础上,结合工程地质研究现状,以作辑托背斜和巴东断裂为研究重点,对局部构造与滑坡类型之间的关系进行了深入研究。结果表明：大型滑坡发生与局部构造类型及河流切割局部构造的部位相关,不仅体现于对单个滑坡的控制,更体现在对整体岸坡演化规律、个体滑坡演化因果关系的控制上。对研究区而言,滑坡的形成与作辑托背斜构造样式和巴东断裂的反转活动相关,也与长江切割局部构造位置相联系,使滑坡类型在局部地段发生根本性转变,表现出岸坡破坏发展空间演化过程有很强的方向性。     

胶莱盆地莱阳凹陷莱阳组储层成岩作用及孔隙演化

以野外露头、岩心观察为基础,综合采用普通薄片、铸体薄片、阴极发光薄片、扫描电镜、物性分析、黏土矿物X衍射等多种测试手段对胶莱盆地莱阳组砂岩储层特征、成岩作用及孔隙演化进行了研究。研究结果表明：受物源差异影响,凹陷东部以长石砂岩为主,凹陷西部以岩屑砂岩为主,富含各种塑性岩屑,莱阳组砂岩总体以低成分成熟度、中等结构成熟度为特征。压实作用、压溶作用和胶结作用是造成砂岩储层致密的主要原因。凹陷东部以胶结作用减孔为主,压实程度较弱,碳酸盐胶结物是造成砂岩孔隙度降低的主要胶结物。凹陷西部以压实作用为主,但绿泥石薄膜胶结物的存在有利于保存部分原生孔隙。莱阳组砂岩储层原生孔隙残留较少,多以次生孔隙为主。溶蚀作用,尤其是长石的溶解作用,对改善储层物性有重要作用。次生孔隙发育带主要在K₁llw、K₁ls中,成岩演化达中成岩A期,溶蚀型次生孔隙成为这一阶段主要的孔隙类型,其发育带往往是有利储层发育区。     

基于竖直基线摄影测量的电力线测量方法

对电力线进行定期巡查测量是保障输电线路的稳定和安全的重要手段。针对当前巡线方式存在的可靠性差、灵活性低、成本高等问题,本文研究了一种基于竖直基线摄影测量的电力线测量方法：巡线人员利用便携式竖直基线双目立体相机在野外对电力线进行拍摄,在巡线中或事后对拍摄得到的立体像对中进行准确测量。本文描述了系统设计与技术方法、剖析了系统检校与测量中的关键技术,并利用几组实验证明了本方法的精确性和可行性。