A spatially and temporally adaptive solution of Richards’ equation     

Cass T. Miller  Chandra Abhishek  Matthew W. Farthing 《Advances in water resources》2006

Efficient, robust simulation of groundwater flow in the unsaturated zone remains computationally expensive, especially for problems characterized by sharp fronts in both space and time. Standard approaches that employ uniform spatial and temporal discretizations for the numerical solution of these problems lead to inefficient and expensive simulations. In this work, we solve Richards’ equation using adaptive methods in both space and time. Spatial adaption is based upon a coarse grid solve and a gradient error indicator using a fixed-order approximation. Temporal adaption is accomplished using variable order, variable step size approximations based upon the backward difference formulas up to fifth order. Since the advantages of similar adaptive methods in time are now established, we evaluate our method by comparison with a uniform spatial discretization that is adaptive in time for four different one-dimensional test problems. The numerical results demonstrate that the proposed method provides a robust and efficient alternative to standard approaches for simulating variably saturated flow in one spatial dimension.  相似文献   

多源异质遥感影像的分形特征分析   总被引：5，自引：0，他引：5  

邢帅  郭金华  徐青 《测绘科学技术学报》2006,23(4):254-257,264

分形理论已经在影像压缩、分割、去噪等方面表现出了较大的优势,其特点是能够准确地描述影像的空间结构信息和变化规律.分别采用分线法和三角棱柱法对同一实验地区的多种分辨率不同波段的遥感卫星影像进行分析,分别计算了图像中不同地形区域(如城区、湖泊、田地等)的分形维数,并根据两种算法的特性对图像进行了特征分析.多源遥感影像的实验结果证明,分形维数确实可以作为影像特征分析的一个重要工具,并可以指导分析遥感影像的应用情况.此外,在计算分形维数的过程中,采用三折线拟合法自适应地确定影像的无标度区间,提高了分形维数计算结果的可靠性.  相似文献   

核筒悬挂结构三道抗震防线时程分析设计方法   总被引：2，自引：0，他引：2  

周坚  伍孝波 《世界地震工程》2006,22(1):49-56

提出了高层建筑核筒式悬挂结构三道抗震防线的时程分析设计计算方法,并编制了相应的计算程序Hangsys。计算结果与核筒悬挂结构模拟地震振动台试验的结果符合较好。因此,核筒悬挂结构完全可以通过精心设计使该类结构具有多道抗震防线,使悬挂结构既具有安全性又具有适用性。  相似文献   

二维勘探新观点     

吴铁军 《中国煤田地质》2006,(Z1)

应用大容量、大道数地震仪,改变传统二维地震排列方式,由单线排列接收改为多线排列接收。根据勘探精度的要求、测线网度的不同分二种方式:一是适合于大网度概查普查的单条测线多线排列接收;二是适合于精查和采区二维地震的多条测线多线排列接收方式。  相似文献   

A sensitivity of squall-line intensity to environmental static stability under various shear and moisture conditions   总被引：2，自引：0，他引：2  

Tetsuya Takemi   《Atmospheric Research》2007,84(4):374-389

Squall lines develop in various climate regions having diverse environmental profiles of wind shear, moisture, and temperature. In order to explore the sensitivity of squall lines to these environmental profiles, we have performed an extensive set of numerical simulations under various shear and moisture conditions in midlatitude-continental and tropical–oceanic temperature environments. From the results of the sensitivity simulations and the analyses of the environmental parameters, it is found that the static stability in a convectively unstable layer is of primary importance in determining the strength of squall lines. Under temperature environments having the same static stability, convective available potential energy (CAPE) and precipitable water content (PWC) well describe the squall-line intensity. Vertical shear also plays an important role in determining the squall-line structure as well as the intensity through the interaction with surface cold pool. The combination of the static stability in a convectively unstable layer, CAPE, and PWC should be examined in diagnosing the intensity of squall lines that develop with an optimal shear for their environment.  相似文献   

伪三维地震勘探法在煤田勘查中的应用     

李金花  李建国 《中国煤田地质》2007,19(1):63-65

勘探区属郭庄煤矿的后备井田，勘探的目的是掌握井田主可采煤层的赋存形态与断层、陷落柱发育特征。根据勘探区的地质条件，地质任务，兼顾质量和成本，勘探设计方案最终确定为3线1炮制线束状观测系统，采用中间放炮，使勘探物理点由常规二维设计的3000个减至700个，勘探成本明显降低。勘探前后的资料对比分析表明，3#煤层的展布特征和断层构造有较大不同，其中3#煤层展布形态由NE向变化均匀，两翼对称的背斜构造修改为等高线变化扭曲相对剧烈，两翼对称的向斜构造；勘探后新解释断层5条，断点3处，另外3条已知断层的形态、位置、落差等相差各异。  相似文献   

基于地图代数的数字地表流线模拟研究          下载免费PDF全文

吴艳兰  胡鹏  刘永琼 《水科学进展》2007,18(3):356-361

降雨在地表上随地形流动自然形成沟谷线、汇流区、分水岭等流域形态,研究地表流水线的数字模拟对数字流域水文分析具有重要意义.提出数字地表流线模型的概念,只考虑地形因素,利用等高线图建立一个能获得区域内每滴雨水沿地表流动的轨迹模型.并运用地图代数的距离变换对等高线及所在空间进行全方位的距离度量,研究了数字地表流线模型的建立方法.实验表明,该模型利用距离变换信息而不是高程计算流向,可避免DEM高程误差对流向、流线的影响,且不需要在DEM上进行复杂的洼地、平地的识别与处理.该模型对原始数据要求不高,能有效应用于沟谷线的自动提取、汇流区自动分割和分水线网络的自动提取.  相似文献   

A review and analyses of plumb-line calibration     

José L.  Lerma  Miriam  Cabrelles 《The Photogrammetric Record》2007,22(118):135-150

  相似文献   

Studies of ultracompact H ii regions — II. High-resolution radio continuum and methanol maser survey     

A. J. Walsh    M. G. Burton    A. R. Hyland  & G. Robinson 《Monthly notices of the Royal Astronomical Society》1998,301(3):640-698

High spatial resolution radio continuum and 6.67-GHz methanol spectral line data are presented for methanol masers previously detected by Walsh et al. (1997). Methanol maser and/or radio continuum emission is found in 364 cases towards IRAS -selected regions. For those sources with methanol maser emission, relative positions have been obtained to an accuracy of typically 0.05 arcsec, with absolute positions accurate to around 1 arcsec. Maps of selected sources are provided. The intensity of the maser emission does not seem to depend on the presence of a continuum source. The coincidence of water and methanol maser positions in some regions suggests there is overlap in the requirements for methanol and water maser emission to be observable. However, there is a striking difference between the general proximity of methanol and water masers to both cometary and irregularly shaped ultracompact (UC) H  ii regions, indicating that, in other cases, there must be differing environments conducive to stimulating their emission. We show that the methanol maser is most likely present before an observable UC H  ii region is formed around a massive star and is quickly destroyed as the UC H  ii region evolves. There are 36 out of 97 maser sites that are linearly extended. The hypothesis that the maser emission is found in a circumstellar disc is not inconsistent with these 36 maser sites, but is unlikely. It cannot, however, account for all other maser sites. An alternative model which uses shocks to create the masing spots can more readily reproduce the maser spot distributions.  相似文献   

Damped Lyα absorbers from dwarf galaxy ejecta     

P. E. J. Nulsen  X. Barcons  & A. C. Fabian 《Monthly notices of the Royal Astronomical Society》1998,301(1):168-174

It is argued that the formation of a dwarf galaxy causes a massive burst of star formation, resulting in the ejection of most of the available gas from the galaxy as a weakly collimated wind. The ejected gas can give rise to a damped Lyα absorber (DLA). Weakly collimated outflows naturally explain the asymmetric profiles seen in low-ionization absorption lines caused by heavy elements associated with DLAs, where absorption is strongest at one edge of the absorption feature. The shape of the distribution of column densities in the model agrees reasonably well with observations. In particular, the break in slope is caused by external photoionization of the wind. A semi-analytical model for galaxy formation is used to show that, for currently acceptable cosmological parameters, dwarf galaxy outflows can account for the majority of DLA systems and their distribution with redshift. This model also predicts a correlation between velocity structure and metallicity of DLA systems, in qualitative agreement with observations. DLAs do not require many large, rapidly rotating disc galaxies to have formed early on, as in other models for their origin.  相似文献