The Basin Water Resources Management System and Its Innovation in China

Water provides the origin of human survival and prosperity,and the basic resource for the maintenance of terrestrial eco-systems,their biodiversity,productivity and ecological services.With China’s recent,rapid growth both in population and economic development,the water shortage has become one of the most constraints on its ecological restoration and socio-economic development,especially in the arid inland regions of northwest China.At first glance,this water shortage in China appears to be a resource crisis.But second,an in-depth analysis reveals that the water shortage crisis arises mainly resulting from the poor water management system and operating mechanism that cannot facilitate fair allocation and efficient utilization of water resources both regionally and nationally and thus is viewed as a crisis of water manage-ment.The solution of China’s water shortage and low-efficient utilization problem will,in particular,require a fundamen-tal and substantial reform or innovation of the existing water management system and operating mechanism.In this paper,we address explicitly the problems existed in the current water management system,explore the basic theory of water re-sources management and provide some insights into the way how to establish a river basin based integrated water re-sources management system in China.     

几种垂直跳点网格计算频散性的比较研究

为证明两种新的垂直跳点网格--LZ网格和LY网格的有效性,从频率、群速和出现错误群速的垂直尺度范围等方面与现有的几种垂直跳点网格和时间--垂直跳点网格进行了比较.结果表明:LZ网格计算频散性与目前使用的最广泛的并且计算频散性也是最佳的CP网格相当,而LY网格次之,从而为模式设计者选取垂直网格提供了又一种选择.     

人工湿地植物研究

本文阐述了植物在人工湿地污水净化过程中作用及存在的若干问题,提出了研究人工湿地植物的一些设想,植物在人工湿地中起着非常重要的作用,不但直接摄取利用污水中的营养物质、吸收富集污水中的重金属等有毒有害物质;而且输送氧气到根区,提供根区微生物生长、繁殖和降解对氧的需求;还能维持和加强人工湿地系统内的水力学传输,但目前人工湿地植物的应用还存在着枯死衰退、杂草丛生和根系扩展较浅等问题,影响人工湿地的净化功能,通过对人工湿地植物生理生态特性如气体代谢、光合作用、逆境生理和相生相克等研究,筛选出优良植物种类,创造适宜人工生,将有利于发育发挥湿地植物功能,提高人工湿地污水处理能力。     

GRAPES双参数云微物理方案的改进和云降水个例模拟研究：GRAPES_SCM对热带对流云个例的模拟研究

应用全球-区域同化预报系统单柱模式(GRAPES_SCM),对热带暖池国际云试验(TWP-ICE)个例进行数值模拟。通过和实际观测资料进行对比,诊断并改进了Liuma云微物理方案对热带对流云微物理特征的模拟能力。结果显示在GRAPES_SCM框架下,Liuma原方案和WSM6(WRF single moment)方案均能呈现出TWP-ICE期间热带云系的发展特征,并能够明显区分试验期间的季风活跃期和季风抑制期。活跃期Liuma原始方案和WSM6方案模拟的冰云组成结构差异显著,在Liuma原始方案所模拟的冰相水凝物分布中,存在冰雪含量过少、霰过多的现象。改进后的Liuma方案对程序中各微物理过程计算顺序进行了优化,改进后霰质量混合比明显减少,冰雪质量混合比明显增加,冰相水凝物分布较合理。     

Structural Evidence for the in-situ Origin of the HP and UHP Eclogites in the Dabie-Sulu Orogenic Belt

Whether the HP and UHP metamorphic rocks of the Dabie-Sulu orogenic belt are of an "in-situ" or "foreign" origin is a long-standing dispute among geologists. Eclogites preserved today in the HP and UHP units constitute merely 5-10%, which are not isolated exotic bodies tectonically intruding into amphibolite facies gneiss, but remnants of once pervasive or widespread eclogite-facies terranes or slabs. The present spatial distribution and forms of the eclogites have resulted from polyphase and progressive deformation and strain partitioning of the HP and UHP slabs. From their formation in deep mantle to their exhumation to the surface, the eclogites have experienced long-term deformation with different strain regimes. The dominant regime responsible for the present spatial distribution and forms of the eclogites is the shear process. The deformation patterns of the eclogites and gneiss matrix also clearly show that the eclogites were metamorphosed in situ. The original distribution area of the eclogites     

太阳大气磁精细结构的射电探讨

太阳大气磁场的研究对于太阳大气物理及太阳活动研究是十分重要的。目前探测光球以外的日够以球，过渡区磁场的几乎唯一办法，是在紧密联系其他频说段取得的信息基础上使用射电观测。根据在微波，米波段有关辐射机制和传播过程，介绍了推导磁场讯息的基本射电方法。     

Comparative study of brine shrimp bioassay-based toxic activities of three harmful microalgal species that frequently blooming in aquaculture ponds

Journal of Oceanology and Limnology - Typical harmful micro-algal species constantly occurred in high density in marine aquaculture ponds in Xiangshan and Sanmen Bay, Zhejiang Province. Fates of...     

太阳spike辐射中的MHD振荡

我们在1981年5月16日所观测到的典型的微波大爆发的spike辐射中,发现存有～1.4—1.6秒的准周期振荡特征。本文依据MHD波理论,对观测进行了分析讨论,本文认为在日冕圈内外传播着的快磁声波(“腊肠”模)调制了源区的磁场以及电子束的投射角分布,从而影响了ECM不稳定性的增长率,因此而产生了spike辐射中的准周期振荡。另外,本文还对一些有关的物理参数作了定量的估算。     

Multi-Site Spectrographic and Heliographic Observations of Radio Fine Structure on April 10, 2001

We present results of the first simultaneous observations of zebra patterns (ZPs) with super-fine spiky structure in the microwave range made at two observatories ～1000 km apart (Beijing and Nanjing, China). The fine structure was recorded by a spectra polarimeter in the 5.2 – 7.6 and 2.8 – 3.6 GHz ranges at the Huairou station and by the spectrometer in the 4.5 – 7.5 GHz range at the Purple Mountain Observatory. Simultaneously, the locations of radio sources were observed by the Siberian Solar Radio Telescope (SSRT) at 5.7 GHz. For a general analysis of the April 10, 2001 event, the Solar and Heliospheric Observatory/Michelson Doppler Imager (SOHO/MDI) data and Transition Region and Coronal Explorer (TRACE) images in EUV 171 Å line were used. The circular polarization degree was very weak for the burst background radio emission and moderate to strong for the fine structure. The polarization sign in all the cases probably corresponds to the extraordinary wave mode. Estimations of the magnetic field values in the whistler model for fine structure agree well with the extrapolated values from magnetic maps. Given the possibility of wave transformation in the perpendicular magnetic field and the spiky structure of the ZP, the whistler wave model appears to be the most appropriate explanation for the zebra stripe phenomenon.     

微U型爆发及微波精细结构

我们用新的时间分辨率短至８ｍｓ 的２ ．６ ～３ ．８ＧＨｚ 微波动态频谱仪在１９９８ 年４ 月１５ 日爆发和１９９７ 年１１ 月３ 日爆发中发现了微Ｕ 型爆发。其顶部频率为３ ．２ ～３ ．４ＧＨｚ（ 相应的等离子体密度：基波：１ ．２ ×１０１１ － １ ．４ ×１０１１／ｃｍ ３ ,二次谐波：３ ．２ ×１０１０ － ３ ．５ ×１０１０／ｃｍ ３） ;根部频率为３ ．４ ～３ ．６ＧＨｚ;单个Ｕ 型爆发的频率范围为６０ ～２２０ ＭＨｚ ;上升段频漂率为７ ～２８ＧＨｚ／ｓ;上升段持续时间为８ ～２４ｍｓ;寿命为１６ ～４８ｍｓ;偏振度大于８０ ％ 。在活动区为偶极子磁场的假设下,估计源区高度约为１ ．３ ×１０４ 公里,单一环的高度为２５０ ～８００ 公里。由此得出结论：１ ．由于高频漂率和高偏振度,似乎发现的微Ｕ 型爆发不是Ⅲ型爆发形成,而是尖峰辐射（Ｓｐｉｋｅ） 形成。２ ．我们发现的是小尺度的微磁环,其尺度与Ｓｐｉｋｅ 辐射的寿命相当。我们在１９９７ 年１１ 月２ 日的爆发中发现平均周期为数十ｍｓ 的准周期振荡群。在高密度流管的磁声波ＭＨＤ 振荡条件下,可取得磁环半径约９０ 公里的结果。由此可以得到微磁环物理尺度的图象