Estimating the minimum in-stream flow requirements via wetted perimeter method based on curvature and slope techniques

Under the assumptions of triangular cross section channel and uniform stable flow, an analytical solution of the minimum ecological in-stream flow requirement (MEIFR) is deduced. Based on the analytical solution, the uncertainty of the wetted perimeter method is analyzed by comparing the two techniques for the determination of the critical point on the relationship curve between wetted perimeter, P and discharge, Q. It is clearly shown that the results of MEIFR based on curvature technique (corresponding to the maximum curvature) and slope technique (slope being 1) are significantly different. On the P-Q curve, the slope of the critical point with the maximum curvature is 0.39 and the MEIFR varied prominently with the change of the slope threshold. This indicates that if a certain value of the slope threshold is not available for slope technique, curvature technique may be a better choice. By applying the analytical solution of MEIFR in the losing rivers of the Western Route South-to-North Water Transfer Project in China, the MEIFR value via curvature technique is 2.5%-23.7% of the multi-year average annual discharge, while that for slope technique is 11%-105.7%. General conclusions would rely on the more detailed research for all kinds of cross-sections.     

Photopolarimetry of 3C 66A in 2003

The BL Lac-type object 3C 66A was observed at the Crimean Astrophysical Observatory during the international project OJ-94. Observations were made over 10 nights from February through December 2003 at the Cassegrain focus of the 125-cm AZT-11 telescope with a photopolarimeter capable of simultaneous measurements in the UBVRI bands. In the course of our measurements the brightness of the object increased by more than 1 magnitude in all these bands. Its color indices varied and the degree of polarization decreased from ∼16% in February to ∼3% at the end of our observations. In December 2003 a rapid change in the position angle from 15° to 40° was noticed. The spectral energy distribution F_n is well described by a power law with a spectral index a (F_ν ∝ ν ^−α . The increase in brightness was accompanied by a reduction in the spectral index. The most probable mechanism for the observed changes in the brightness, degree of polarization, and spectral index may be a decrease in the magnetic field strength or a change in its configuration owing to a increase in the chaotic component of the field. __________ Translated from Astrofizika, Vol. 49, No. 1, pp. 41–59 (February 2006).     

Chandra observations of the X-ray jet in 3C 66B

Our Chandra observation of the FR I radio galaxy 3C 66B has resulted in the first detection of an X-ray counterpart to the previously known radio, infrared and optical jet. The X-ray jet is detected up to 7 arcsec from the core and has a steep X-ray spectrum, α ≈1.3±0.1 . The overall X-ray flux density and spectrum of the jet are consistent with a synchrotron origin for the X-ray emission. However, the inner knot in the jet has a higher ratio of X-ray to radio emission than the others. This suggests that either two distinct emission processes are present or differences in the acceleration mechanism are required; there may be a contribution to the emission from the inner knot from an inverse Compton process or it may be the site of an early strong shock in the jet. The peak of the brightest radio and X-ray knot is significantly closer to the nucleus in the X-ray than in the radio, which may suggest that the knots are privileged sites for high-energy particle acceleration. 3C 66B's jet is similar both in overall spectral shape and in structural detail to those in more nearby sources such as M87 and Centaurus A.     

东风螺、弯竹蛏和斑节对虾的壳基质蛋白组学分析

从软体动物中的腹足纲、双壳纲以及节肢动物中的甲壳纲分别选取了3种中国沿海常见的品种——东风螺、弯竹蛏、斑节对虾,提取并分析它们的壳基质蛋白。利用液相色谱串联质谱（LC-MS/MS）技术对蛋白质组学进行分析发现特定的蛋白质具有明显的种属差异：①N66蛋白（一种碳酸酐酶）通常存在于弯竹蛏中,但不存在于东风螺和斑节对虾中,揭示N66蛋白质具有特异性,在未来的物种鉴定中可能具有重要的参考意义;②角质层蛋白AM1199和CP14.6存在于斑节对虾的表皮结构中,在东风螺和弯竹蛏中未检测到;③血蓝蛋白同时在3种动物外壳的基质蛋白中被鉴定出来,揭示了其在不同物种的外壳形成与发育过程中的重要作用。该研究为壳基质蛋白在软体动物或节肢动物外壳中的鉴定提供了基础,也为探索不同物种的生物矿化过程提供了重要参考。     

南水北调中线工程征地测量数据处理系统设计

针对南水北调中线工程征地测量内外业效率的不匹配状况,本文提出征地测量数据处理系统设计思路,给出了地块面积计算原理及主程序模块,结合工程实例对系统具有的地块自动分离、分类汇总、自由分割、边长方位量测、报表和宗地图输出等功能进行了介绍。     

Blazar天体3C 66A光学波段准周期光变分析

研究了Blazar天体3C 66A光学波段的准周期光变行为.收集了3C 66A光学V波段将近18 yr (2003—2021年)的测光数据,观测数据主要来源是:上海天文台(ShAO)、 AAVSO (The American Association of Variable Star Observers)数据库、Steward天文台.使用了Jurkevich和Lomb-Scargle两种方法分析了光变数据.Jurkevich方法得到了(850±90) d (～2.3 yr)和(1150±140) d (～3.2 yr)的光变周期,而Lomb-Scargle方法在充分考虑了“红噪声”效应之后同样得到了(869±70) d和(1111±90) d的光变周期,它们的置信水平分别为>99%和> 95%.通过与之前的研究结果比较,发现～2.3 yr的光变周期在3C 66A的历史光变数据中是一个稳定的周期,而～3.2 yr的周期则是不稳定的.     

铜陵地区晚古生代岩浆活动的发现：来自凤凰山岩体ZK66钻孔岩心辉绿岩锆石U–Pb定年的证据

凤凰山花岗闪长岩是铜陵地区出露面积最大的岩体,约10 km2,属高钾钙碱性系列.位于该岩体西北角的朱家山附近ZK66钻孔揭示,岩体超覆于三叠纪碳酸盐岩地层之上.除在浅部见到花岗闪长岩之外,深部主要见到晚泥盆世-二叠纪地层.特别是在石炭纪大理岩中见到辉绿岩和花岗斑岩,其锆石LA-ICP-MS U-Pb年龄分别为304 Ma和132 Ma,证明本区存在晚古生代岩浆活动,而中生代花岗质岩浆活动可能持续到132 Ma.晚石炭世辉绿岩的发现,说明该时期海底是一种拉张环境,海底喷流作用可能与岩浆活动有密切的成因关系,为该时期形成大型矿床奠定了基础.     

南水北调中线工程不同调水规模对汉江中下游影响分析

南水北调中线工程是解决我国北方地区水资源紧缺的重大战略措施。但调水将给汉江中下游的水文情势及用水带来一定的影响。文章分析了丹江口水库不同调水方案对汉江中下游水位、流量及灌溉和航运的影响,并提出补偿工程措施。调水６０×１０８ｍ３对汉江中下游的影响较小,可基本不予补偿;调水１５０×１０８ｍ３的影响稍重,但对航运和灌溉用水的影响不大,适当补偿可以解决;调水２３０×１０８ｍ３对汉江中下游水位流量及用水的影响十分严重,必须全部渠化并修建江汉运河。     

气候波动和人类活动对南水北调中线工程典型流域径流影响的定量评估

以南水北调中线工程典型流域汉江上游流域和滦河流域为研究对象,采用敏感性分析法、降水?径流双累积曲线法、累积量斜率变化率比较法定量评估了气候波动和人类活动对流域径流变化的影响。结果表明：汉江上游流域和滦河流域变异Ⅰ/Ⅱ期年均径流深相对于基准期分别减少了29.5% / 19.1%和49.8% / 70.0%;对于汉江上游流域,1991-1999年（变异Ⅰ期）气候波动是径流减少的主要影响因素,2000-2008年（变异Ⅱ期）人类活动则是径流减少的主要影响因素,且人类活动对汉江上游流域径流减少的影响逐步增加;对于滦河流域,1980-2010年（变异Ⅰ/Ⅱ期）人类活动一直是径流减少的主要影响因素,且气候波动和人类活动对径流减少的影响贡献率基本保持不变。