统一监管 任重道远

最近,胡锦涛总书记对测绘工作做出了重要指示:“加强测绘统一监督管理和基础测绘工作”。这使广大测绘工作者很受鼓舞和振奋。领导同志的重视支持,新测绘法的颁布实施,可持续发展战略的深入推进,信息化进程的日益加快,都给测绘行业在更高层次更深领域更广范围的发展带来了前所未有的大好机遇。测绘业应当摆脱传统思想观念的羁绊,开阔视野,拓宽思路,勇于创新,迈开大步往前闯,呈现新的繁荣,为经济和社会发展做出更加实际更加突出的贡献。作为测绘管理工作,应站在全新的角度,既要从宏观着眼,加强测绘发展战略研究,制定好测绘发展规划和产业政策…     

东风盐场卤水中可溶性糖的研究Ⅱ、盐田卤水中可溶性糖的来源、消耗及其调控方法初探

本文研究了东风盐场不同盐度的卤水中可溶性糖的变化及其与微藻优势种的组成和细胞数量之间的关系，卤虫对可溶性糖的调节作用及嗜盐菌对可溶性糖的消耗。结果表明，可溶性糖在低卤区和硅藻、甲藻等微藻密切相关，在中、高卤区与蓝藻和盐藻等密切相关，卤水中的卤虫能通过滤食微藻而有效地控制卤水中可溶性糖的浓度，在结晶卤水中接种嗜盐菌能有效地降解卤水中的可溶性糖，从而达到提高盐质的目的。     

Ekman层风速随高度分布方程的数值解试验

根据大气水平运动方程推导出Ekman层风速随高度分布方程,该分布可用二阶线性微分方程表示,用有限差分法求解该二阶线性微分方程的边值问题的数值解,并给出计算程序,输出结果。将结果与经典解析解比较,讨论了经典解的正确性和适用范围。     

Grazing of Salpa thompsoni on phytoplankton in summer in the Prydz Bay region, Antarctica

During the CHINARE-Ⅺ cruise in austral summer of 1998/1999, the abundance and feeding activity of Salps thompsoni were investigated in the Prydz Bav region. Salps samples were collected by vertical tows from the depth of 200 m to the surface with a conical net of 330 μm mesh-size. At Ⅵ-3 station, the grazing rates were studied by the gut fluorescence method and culture experiments. S. Thompsoni was mainly distributed in the northern part of the survey area, and its maximum densities reached to 2795 ind. · 1000 m-3. A dramatic decrease in salp stock was observed at the Marginal Ice Zone. The results of the feeding experiments at the Ⅵ-3 show that the gut pigment contents of S. thompsoni ranged from (0. 14 - 1.27) μig ind. -1(average 0. 98 μg ind.-1). The individual ingestion rate is 7. 9 μg ind. -1 · day-1, and the filtration rate is 28 L ind. -1 · day-1 Through the daily grazing rate of S. thompsoni, which takes account of less than 1% of the phytoplankton standing stock, it shows arelatively higher grazing impress on the primary production (72. 2 % ).     

低纬子午环绝对测定仪器瞬时方位差方法的改进(Ⅱ)

在导出低纬子午环测定一颗星过卯酉、子午圈的记录时刻与瞬时方位差关系式的基础上，结合仪器在卯酉圈测定星对天顶距的方法［１］，提出了既可以绝对测定瞬时方位差，又可以绝对测定定位误差ε的新设想     

New confirmation of image-processing techniques for astrometry of Saturn and its satellites

The image-processing techniques used by Peng et al. are further improved to measure precisely the positions of Saturn and its satellites. 495 CCD images taken with the 1-m telescope at the Yunnan Observatory during the years 2002–2004 are processed with these techniques. These measured pixel positions are compared to their theoretical positions computed with the ephemerides of TASS1.7 for the satellites and JPL DE405 for Saturn itself. Analysis of the data for the intersatellite positions among four bright Saturnian satellites (S3–S6) and for Saturn–satellite (i.e. Saturn–Titan) positions shows that these measured positions have the same dispersions, i.e. about 0.05 and 0.06 arcsec in right ascension and declination, respectively. However, for the fainter satellites, Enceladus and Mimas, poorer residuals up to 0.1 and 0.2 arcsec, respectively, in both directions are found mainly due to their small separations from the primary planet and short exposure time in order to obtain useful images of Saturn.     

21cm波段太阳爆发中的精细结构

本文简要介绍了云南天文台新建立的21cm波段快速(不中断采样)记录系统,及使用该系统观测到的快速尖峰事件。系统得到的太阳分米波段爆发中不同时间尺度的精细结构与Stu-rroch等提出的太阳耀斑中能量释放的模式相一致。     

汉江丹江口水库下游河床演变

丹江口水库建库20多年来,下游河道由堆积性河道变成了冲刷性的河道,河床物质沿程粗化,比降得以调平。水深增加幅度大于河宽,流速并不随着水深增加而加快。深槽、浅滩分布明显化,宽深比不断在减少。整个库下游变化可分为三段:1)近库段,游荡河道向单一限制性曲流转化;2)大支流影响段,河道仍保持着游荡特性;3)下游段,游荡段游荡特性减弱,弯曲段则深蚀作用加强。     

Mantle plumes and their record in Earth history

In recent years, the study of mantle plumeshas become a “hot spot” in earth sciences;enormous papers and data have been published, and many mantle plume-related questions have arisen: Did mantle plumes in the Precambrian behave the same way as they do today? What are the roles of plumes in the evolution of the earth? What are the effects of mantle plumes on global changes and metallogenesis? These issues are frequently encountered and hotly debated in a wide range of earth science fields such as tectonics geochemistry, geophysics, metallogenesis,     

地形作用下有限振幅Rossby波的稳定性分析

本文用微分方程定性理论方法分析了地形对有限振幅Rossby波的稳定性影响。结果表明:地形北坡有利于波动出现不稳定,南坡使波动稳定;西坡使导式波动不稳定但使曳式波动稳定,东坡使导式波动稳定但使曳式波动不稳定。