Evaluation of Electro-Oxidation of Textile Effluent Using Response Surface Methods     

R. Saravanathamizhan  N. Mohan  N. Balasubramanian  V. Ramamurthi  C. Ahmed Basha 《洁净——土壤、空气、水》2007,35(4):355-361

In the present investigation, treatment of textile effluent using an electrochemical technique was designed and analyzed using the Box-Behnken method. The influence of individual parameters on electro-oxidation of textile effluent has been critically examined using the response surface method (RSM), and a quadratic model for chemical oxygen demand (COD) reduction has been developed. It has been observed from the present analysis that the predicted values are in good agreement with experimental data with a correlation coefficient of 0.945.  相似文献   

复杂地形下地面观测资料同化I. 模式地形与观测站地形高度差异对地面资料同化的影响研究   总被引：4，自引：0，他引：4       下载免费PDF全文

徐枝芳  龚建东  王建捷 《大气科学》2007,31(2):222-232

中国地形复杂，模式地形与实际观测地形存在一定高度差异，因此设计合理的复杂地形下地面观测资料的同化方案有利于使我国目前仅用作探测手段的地面观测资料（常规地面观测站和地面自动站）在中尺度数值模式中得到充分利用。作者在MM5_3DVAR同化系统中利用近地层相似理论将地面观测资料进行直接三维变分同化分析，并对地面资料同化方案设计中是否需要考虑模式与实际观测站地形高度差异进行探讨研究。研究结果表明：通过近地层相似理论将地面观测资料同化到数值模式能起到一定的作用，并且地面观测资料（温度、 湿度、 风场、 地面气压）中各物理量同化到数值模式都能影响24小时降水数值结果，但各物理量起的作用大小不一样，其中影响最大的是温度，其次为湿度；地面观测资料同化方案设计有必要考虑模式地形与实际观测站地形高度差异，适当考虑这种高度差异能取得较好的结果。  相似文献   

GPS高程测量在也门Block69中的应用分析     

张予杰  马素文  侯金根 《全球定位系统》2007,32(1):35-38

GPS高程测量代替常规水准测量的技术和方法已经成为这些年来许多大地测量学者们研究的热门课题之一，本文简单地介绍了GPS高程测量的模型及其适用范围，并通过在也门Block 69的应用分析，说明了在高程异常值变化平缓的平坦地区，只需测定少量（不少于3个）较均匀分布于测区的已知高程控制点，采用平面拟合法，拟合精度就能够达到测区测量精度的要求。  相似文献   

一种复杂轮廓线的真三维TIN算法     

朱庆  李逢春  张叶廷 《武汉大学学报(信息科学版)》2007,32(3):259-262

针对多层轮廓线三维重构问题，研究了真三维复杂轮廓线的空间分布特征，通过引入参考基准面概念，提出了一种顾及局部平展特性的真三维TIN生成算法。该方法在递增生成表面过程中，利用了加权最小三角化方法，动态建立参考基准面，将三角面片自身形态和局部邻接轮廓点的相对空间关系有机地结合起来，避免了面片的遮掩重叠和自相交，使得重建表面和原始表面的拓扑差异最小。选取三维地震量测的多层反射波剖面数据进行了实验，并对不同算法得到的实验结果进行了分析比较，得出实验结论：本文算法快速可靠，重建出来的三维表面过渡光滑、自然，更接近实际的表面形态。该方法对于石油、地质勘探三维地质构造形态辅助解译具有现实的应用意义。  相似文献   

基于k阶Voronoi多边形划分的k阶数据场拟合   总被引：2，自引：1，他引：2  

韩元利  胡鹏  黄雪莲  张立华 《武汉大学学报(信息科学版)》2007,32(4):353-357

讨论了k阶Voronoi图的离散点集的生成算法，挖掘了k阶Voronoi图的性质并加以证明；参照k阶Voronoi图的定义提出了k阶空间数据场的定义，并结合参考点利用其影响因子给出了低阶空间数据场的拟合函数通式；利用k阶Voronoi图对平面空间的平面区域最近邻近划分实现了对空间数据场的分割，从而将大量参考点集数据场化解为多个单元数据场的低阶拟舍，有效地降低了数据场拟舍的难度；提出了合并拟合和叠加拟合策略，实现了将单元数据场综合为完整的空间数据场。  相似文献   

基于数值模拟的汾河二库对晋祠泉岩溶水系统渗漏补给作用研究   总被引：1，自引：0，他引：1  

梁腾飞  成建梅  张乃俨  史文  开萨尔江·艾合买提 《中国岩溶》2020,39(2):147-153

汾河二库的下闸蓄水，改变了晋祠泉域汾河地表水对岩溶水的渗漏补给条件，对区域岩溶水流场变化有着长远的影响。本研究通过系统梳理库区水文地质条件，勾画地表水渗漏补给岩溶水范围，考虑地层岩性、蓄水高度等因素，确定二库不同蓄水水位下晋祠泉域获渗漏量占比；构建晋祠泉三维岩溶地下水流模型，研究二库渗漏对泉域岩溶地下水补给作用，并预测不同蓄水情景下晋祠泉口水位变化趋势。结果表明:晋祠泉域获渗漏量占比随二库蓄水位非线性变化，最低为92.8%，在二库蓄水位达902 m后稳定在93.7%，而渗漏量与二库蓄水高度呈正相关；泉域岩溶水径流区受渗漏补给作用最显著，其次为排泄区、北部补给区；渗漏补给作用下，地下水位回升值受二库水位和补水距离影响；维持设计水位（905.7 m）和2017年水位（895.9~902.4 m）时，预计晋祠泉口水位分别在2021年7月和2023年1月达到泉口高程。   相似文献   

On the Dynamics of Dust Grains in a Hierarchical Environment     

Marcos  C. De La Fuente  Marcos  R. De La Fuente 《Earth, Moon, and Planets》1998,81(2):145-173

Most main sequence stars are binaries or higher multiplicity Systems and it appears that at birth most stars have circumstellar disks. It is commonly accepted that planetary systems arise from the material of these disks; consequently, binary and multiple systems may have a main role in planet formation. In this paper, we study the stage of planetary formation during which the particulate material is still dispersed as centimetre-to-metre sized primordial aggregates. We investigate the response of the particles, in a protoplanetary disk with radius R_D = 100 AU around a solar-like star, to the gravitational field of bound perturbing companions in a moderately wide (300–1600 AU) orbit. For this purpose, we have carried out a series of simulations of coplanar hierarchical configurations using a direct integration code that models gravitational and viscous forces. The massive protoplanetary disk is around one of the components of the binary. The evolution in time of the dust sub-disk depends mainly on the nature (prograde or retrograde) of the relative revolution of the stellar companion, and on the temperature and mass of the circumstellar disk. Our results show that for binary companions near the limit of tidal truncation of the disk, the perturbation leads to an enhanced accretion rate onto the primary, decreasing the lifetime of the particles in the protoplanetary disk with respect to the case of a single star. As a consequence of an enhanced accretion rate the mass of the disk decreases faster, which leads to a longer resultant lifetime for particles in the disk. On the other hand, binary companions may induce tidal arms in the dust phase of protoplanetary disks. Spiral perturbations with m = 1 may increase in a factor 10 or more the dust surface density in the neighbourhood of the arm, facilitating the growth of the particles. Moreover, in a massive disk (0.01M⊙) the survival time of particles is significantly shorter than in a less massive nebula (0.001M⊙) and the temperature of the disk severely influences the spiral-in time of particles. The rapid evolution of the dust component found in post T Tauri stars can be explained as a result of their binary nature. Binarity may also influence the evolution of circumpulsar disks. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

太阳常数的变化与太阳软x射线辐射流量及低频天波时延的关系   总被引：1，自引：0，他引：1  

王素琴  潘炼德 《时间频率学报》1998,21(1):49-53

本文对1982年在陕西临潼接收的美国罗兰-C西北大平洋链Y台发射的100kHz低频一跳天波时延的实测资料及SMS－GOES测量的太阳1～8A软x射线的每日辐射流量与SMM／ACRIMI测量的太阳常数之间的关系进行了分析。结果表明：太阳1～8A软x射线辐射流量与太阳常数之间存在较强的负相关;低频一跳天波时延与太阳常数之间存在着较强的正相关。并对此进行了讨论。  相似文献   

Fine structure of the red giant clump from Hipparcos data, and distance determinations based on its mean magnitude     

Léo Girardi  Martin A. T. Groenewegen  Achim Weiss  & Maurizio Salaris 《Monthly notices of the Royal Astronomical Society》1998,301(1):149-160

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Non-stationary pair plasma in a pulsar magnetosphere and the two-stream Instability     

E. Asseo  & G. I. Melikidze 《Monthly notices of the Royal Astronomical Society》1998,301(1):59-71

We test a new emission mechanism in pulsar magnetospheres, eventually responsible in part for the high level of observed radio radiation. This is carried out by comparing the efficiency of the two-stream instability of Langmuir waves in a pulsar emission region, where the stationary and non-stationary characters of pair plasma outflows produced in the gap region are characterized by two different time-scales. On the shorter time-scale, the Ruderman &38; Sutherland 'sparking' phenomenon leads to the creation of pair plasma clouds, in motion along magnetic field lines, that contain particles with a large spectrum of momenta. The overlapping of particles with different energies produced in successive clouds results in an efficient 'two stream'-like instability. This effect is a consequence of the non-stationary character of the pair plasma produced in the gap region, just above the magnetic poles of the neutron star. On a long time-scale, resulting pair plasma outflows in pulsar magnetospheres can be treated as stationary. In this case, the instability which results from interaction between existing primary beam particles and the pair plasma is negligible, whereas the instability owing to interaction between electrons and positrons of the pair plasma itself, and more precisely to their relative drift motion along curved magnetic field lines, is effective. We derive characteristic features of the triggered instability, using specific distribution functions to describe either particles in the assembly of clouds or relative drifting of electrons and positrons in these same plasma clouds. Although linear and local, our treatment suggests that non-stationary effects may compete with, or even dominate over, drifting effects in parts of pulsar emission regions.  相似文献