清江隔河岩两级升船机中间渠道及下游引航道船舶牵引方式优化方案

清江隔河岩升船机系统,原设计规划配置4艘消拖船用于推(拖)无动力分节驳进出两级垂直升船机,由于原设计考虑的条件与实际情况差异极大,势必会造成设备利用率低,并且,消拖船投入运行后还要产生难以承受的维修费用和人员成本。为此,提出了一种岸边牵引方式,对无动力分节驳进出升船机是一种既经济、又有效的优化方案。     

A Late Cretaceous pole for the Pacific plate: implications for apparent and true polar wander and the drift of hotspots

We present a Late Cretaceous (81 Ma) pole position for the Pacific plate derived from paleomagnetic analyses of basalt samples from Detroit Seamount (of the Hawaiian–Emperor seamounts) that were oriented using Brunhes-age overprints. This pole is at much higher latitudes than the previously published Late Cretaceous pole positions based on the modeling of magnetic anomalies observed during marine surveys over seamounts. Our new pole suggests that the Pacific plate would have moved rapidly between 95 and 81 Ma at speeds as high as 19.8 (−10.8/+11.2) cm/year. The Pacific plate at this time was smaller than the present-day plate and had a substantial subducting boundary. The high-velocity estimates are comparable with those of other paleoplates having similar characteristics. Therefore, plate tectonic driving forces can explain the motion and there is no need to invoke true polar wander. Decreases in mantle drag associated with vigorous Late Cretaceous volcanism in the Pacific, however, may have contributed to the rapid plate speed. The new pole position, together with other reliable paleomagnetic indicators of Pacific apparent polar wander, further supports the notion of drift of the Hawaiian hotspot during the Late Cretaceous.     

川北旺苍-南江地区晚侏罗世古地磁学研究与真极移的探讨

本文对四川北部旺苍-南江地区晚侏罗世蓬莱镇组进行了较为详细的岩石磁学和古地磁学研究．逐步热退磁揭示出蓬莱镇组岩石所携带的剩磁由两个分量组成,其中低温组分（次生剩磁）的解阻温度低于420℃;高温组分（特征分量）可通过褶皱及倒转检验,由此求得磁偏角和磁倾角分别为18．4°和29．3°（构造校正后）,95％置信回（α95）为8．5°,对应的古地磁极经纬度分别为236．4°E和66．6°N．基于古地磁结果,并结合已有的地质证据,提出根据古地磁学确定的扬子地块晚侏罗世古纬度偏低的原因可能是由真极移造成的．     

A Bootstrap Test Using Maximum Likelihood Ratio Statistics to Check the Similarity of Two 3-Dimensionally Oriented Data Samples

Comparing three-dimensionally oriented datasets is a problem encountered in various branches of earth science. A simple statistical tool for the comparison of two 3-dimensionally oriented datasets using the bootstrap method in line with the usual nonparametric permutation test is described here. This bootstrap test involves the estimation of maximum likelihood ratio statistic for properly constructed joint frequency tables of the datasets to be compared. This test does not use asymptotic result and will work well even for small sample sizes. Also this test does not make any specific distributional assumptions.     

Imaging of structures in the high-latitude ionosphere: model comparisons

The tomographic reconstruction technique generates a two-dimensional latitude versus height electron density distribution from sets of slant total electron content measurements (TEC) along ray paths between beacon satellites and ground-based radio receivers. In this note, the technique is applied to TEC values obtained from data simulated by the Sheffield/UCL/SEL Coupled Thermosphere/Ionosphere/Model (CTIM). A comparison of the resulting reconstructed image with the input modelled data allows for verification of the reconstruction technique. All the features of the high-latitude ionosphere in the model data are reproduced well in the tomographic image. Reconstructed vertical TEC values follow closely the modelled values, with the F-layer maximum density (NmF2) agreeing generally within about 10%. The method has also been able successfully to reproduce underlying auroral-E ionisation over a restricted latitudinal range in part of the image. The height of the F2 peak is generally in agreement to within about the vertical image resolution (25 km).     

南海海温异常对华南气候影响的数值研究

采用NCEP／NCAR再分析的500hPa高度场、海温场(SST)、极冰资料，分析讨论了登陆广东省热带气旋活动异常与大气环流、极冰、SST、各种环流指数等影响因子之间的关系，得到登陆广东省热带气旋(TC)偏多、偏少年对应的大气环流、极冰、SST、各种环流指数的概念模型。分析结果表明：(1)亚欧大陆在秋、冬季中高纬度以经(纬)向环流为主，则次年登陆广东省的TC偏多(少)；(2)赤道东太平洋SST对热带气旋的影响最稳定和最明显，当1～4月赤道东太平洋SST偏暖(冷)时，当年登陆广东省的TC偏少(多)，次年登陆的TC偏多(少)；(3)夏、秋、冬季多(少)冰年，或者秋冬季连续多(少)冰年时，登陆热带气旋多为正常偏少(多)。     

Influence Of The Atmosphere On Earth Rotation: What New Can Be Learned From The Recent Atmospheric Angular Momentum Estimates?

The interaction between the atmosphere and the underlying solid mantle is oneof the most important sources of changes in all three components of theEarth's rotation vector on different time scales. In this paper the NCEP/NCARreanalysis time series of four times daily atmospheric effective angularmomentum (EAM) estimates is used to investigate some selected aspects of theatmospheric influence on Earth rotation. Emphasis is placed on thecontroversial features which were difficult or impossible to study using theoperational EAM data, such as excitation of the free oscillations in polarmotion, the Chandler wobble (CW) and the free core nutation (FCN), or theroles of diurnal and semidiurnal atmospheric tides and atmospheric normalmodes in the rotational dynamics of the Earth.     

OBSERVATIONAL STUDY OF MERIDIONAL VARIATION OF UV-B RADIATION DURING VOYAGES TO THE ARCTIC AND ANTARCTIC REGIONS*

Based on 1999-2000 observations made by the first Arctic and sixteenth Antactic scientific voyages,a study is undertaken about the meridional surface UV-B (B band ultraviolet rays) variations in 75°N-70°S.It is mitigated as a function of latitudes and marked by lower radiation averaged over the Northern Hemisphere (NH) than over the Southern Hemisphere (SH),with its daily course basically similar to that of total radiation.Around polar summer noon hours (localtime) and where ice albedo is maximum,the strongest UV-B irradiance on the surface perpendicular to sun's beams as found at equatorial latitudes is measured sometimes.In the areas near Zhongshan Station the increase of surface UV-B radiation shows a close relation to the decrease of ozone in the higher atmosphere but it has a less intimate relation with its concentration at ground.     

Earth Rotation Parameters 1899.7–:1992.0 After Reanalysis Within The Hipparcos Frame

Earth rotation parameters (ERP) in the interval 1899.7–1992.0 are obtained from re-analysis of the observed latitude/universal time variations by optical astrometry. Hipparcos Catalogue is used to define the celestial reference frame, within which the ERP are described, with special care devoted to 'problematic' double and/or multiple stars. The terrestrial reference frame is defined by the adopted latitudes/longitudes of participating instruments and their secular motions as given by the NUVEL-1 NNR model of plate motions, and it is chosen to be very close to the International Terrestrial Reference Frame (ITRF). More than four million observations made with 48 different instruments at 31 observatories, located all over the world, are utilized to determine polar motion, celestial pole offsets and (after 1956) universal time UT1, all at 5-day intervals. Along with these parameters, the combinations of Love and Shida numbers, governing the tidal variations of the local verticals at individual observatories, are also determined. The analysis of the results covering almost a century, namely the long-periodic polar motion and length-of-day changes, is presented.     

海洋测量船激光码头标校的论证与试验

本文简要介绍激光码头标校方案,采用电子全站仪的极坐标法测定激光束首尾两点的坐标,来解算惯性导航平面倾角(θ、ψ)和航向角κ。文中对DIOR 3002测距仪无反光镜合作时的测距精度、电子全站仪的定点精度、电子全站仪之间同步测量、数据自动传输等作了详细的试验,得出了适合于激光码头标校最佳测量条件,为激光码头标校部分代替船坞标校提供了论证基础。