应用沉降和水位数据计算上海地区弱透水层的参数   总被引：3，自引：0，他引：3  

叶淑君  薛禹群 《岩土力学》2005,26(2):256-260

弱透水层参数的确定是准三维或三维地下水流数学模型应用时的难点,而应力-应变图解法是一种估计弱透水层参数的有效方法。在介绍该法的基本原理之后,结合上海沉降和水位观测资料,求出了上海地区弱透水层的弹性贮水率、非弹性贮水率和垂向渗透系数,为上海地面沉降的数值模拟提供了较好的初始参数值。对于弱透水层,抽水试验的方法是不可取的,如果又没有条件取土样作室内试验时,若有沉降资料和相应的水位资料,则应力-应变图解法是确定近似参数值的一种比较好的方法。  相似文献   

大安山矿后槽构造应力场数值模拟研究     

司荣军  王春秋  程国强 《岩土力学》2006,27(Z1):167-170

应用ANSYS软件模拟了大安山矿后槽区域构造应力场,数值模拟结果显示,后槽区域最大主应力为水平应力;断层、煤层的变化对整个后槽区域的应力分布有较大影响。这为后槽区域的巷道布置和采煤方法的选择提供了理论依据。  相似文献   

Hydrogeochemical characteristics of groundwater from the two main aquifers in the Red River Delta,Vietnam     

《Journal of Asian Earth Sciences》2014

In the Red River Delta, situated in the northern part of Vietnam, nearly its entire population depends solely on groundwater for daily water consumptions. For this reason, groundwater quality assessments must be carefully carried out using hydrogeochemical properties, to ensure effective groundwater resource planning for the Delta’s present and future groundwater use. In this study, the spatial and seasonal changes in the hydrogeochemical characteristics of groundwater in the two main aquifers of the RRD were investigated by analyzing the physicochemical data obtained in 2011 from 31 conjunctive wells in the Delta’s Holocene unconfined aquifer (HUA) and Pleistocene confined aquifer (PCA) using the Piper diagram and the Gibbs diagram. Results of the data analysis show that the groundwater in both aquifers in the upstream area of the delta is dominated by the [Ca²⁺–HCO₃⁻] water-type, while the [Na⁺–Cl⁻] dominates along the middle-stream and downstream areas. Seasonal changes in the hydrogeochemical facies in both aquifers, comparing the results for the dry and the rainy seasons, were detected in about one third of the sampling wells, which were mainly located at the upstream portion of the Delta. The hydrogeochemical facies of HUA were different from that of PCA by about 45% of the sampling wells in both the dry and the rainy seasons, which were found mostly in the upstream and middle-stream areas.  相似文献   

Reactions leading to the formation and breakdown of stilpnomelane in the Otago Schist, New Zealand     

Li  Essene  Peacor  & Coombs 《Journal of Metamorphic Geology》2000,18(4):393-407

Semi‐pelitic rocks ranging in grade from the prehnite–pumpellyite to the greenschist facies from south‐eastern Otago, New Zealand, have been investigated in order to evaluate the reactions leading to formation and breakdown of stilpnomelane. Detrital grains of mica and chlorite along with fine‐grained authigenic illite and chlorite occur in lower‐grade rocks with compactional fabric parallel to bedding. At higher grades, detrital grains have undergone dissolution, and metamorphic phyllosilicates have crystallized with preferred orientation (sub)parallel to bedding, leading to slaty cleavage. Stilpnomelane is found in metapelites of the pumpellyite–actinolite facies and the chlorite zone of the greenschist facies, but only rarely in the biotite zone of the greenschist facies. Illite or phengite is ubiquitous, whereas chlorite occurs only rarely with stilpnomelane upgrade of the pumpellyite‐out isograd. Chemical and textural relationships suggest that stilpnomelane formed from chlorite, phengite, quartz, K‐feldspar and iron oxides. Stilpnomelane was produced by grain‐boundary replacement of chlorite and by precipitation from solution, overprinting earlier textures. Some relict 14 Å chlorite layers are observed by TEM to be in the process of transforming to 12 Å stilpnomelane layers. The AEM analyses show that Fe is strongly partitioned over Mg into stilpnomelane relative to chlorite (K_D≈2.5) and into chlorite relative to phengite (K_D≈1.9). Modified A′FM diagrams, projected from the measured phengite composition rather than from ideal KAl₃Si₃O₁₀(OH)₂, are used to elucidate reactions among chlorite, stilpnomelane, phengite and biotite. In addition to pressure, temperature and bulk rock composition, the stilpnomelane‐in isograd is controlled by variations in K, Fe³⁺/Fe²⁺, O/OH and H₂O contents, and the locus of the isograd is expected to vary in rocks of different oxidation states and permeabilities. Biotite, quartz and less phengitic muscovite form from stilpnomelane, chlorite and phengite in the biotite zone. Projection of bulk rock compositions from phengite, NaAlO₂, SiO₂ and H₂O reveals that they lie close to the polyhedra defined by the A′FM minerals and albite. Other extended A′FM diagrams, such as one projected from phengite, NaAlO₂, CaAl₂O₄, SiO₂ and H₂O, may prove useful in the evaluation of other low‐grade assemblages.  相似文献   

Instability regions in the upper HR diagram     

Cornelis de Jager  Alex Lobel  Hans Nieuwenhuijzen  Richard Stothers 《Monthly notices of the Royal Astronomical Society》2001,327(2):452-458

The following instability regions for blueward evolving-supergiants are outlined and compared. (1) Areas in the Hertzsprung–Russell (HR) diagram where stars are dynamically unstable. (2) Areas where the effective acceleration in the upper part of the photospheres is negative, hence directed outward. (3) Areas where the sonic points of the stellar winds (where     are situated inside the photospheres, at a level deeper than     . We compare the results with the positions of actual stars in the HR diagram and we find evidence that the recent strong contraction of the yellow hypergiant HR 8752 was initiated in a period during which     , whereupon the star became dynamically unstable. The instability and extreme shells around IRC+10420 are suggested to be related to three factors:     the sonic point is situated inside the photosphere; and the star is dynamically unstable.  相似文献   

Empirical isochrones and relative ages for young stars, and the radiative–convective gap     

N. J. Mayne  Tim Naylor  S. P. Littlefair  Eric S. Saunders  R. D. Jeffries 《Monthly notices of the Royal Astronomical Society》2007,375(4):1220-1240

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尕斯库勒盐湖卤水模拟自然蒸发试验研究   总被引：4，自引：3，他引：1       下载免费PDF全文

王丽娜  许建新  闵秀云  王亚静 《盐湖研究》2011,19(3):26-30

尕斯库勒湖是柴达木盆地众盐湖中较为典型的硫酸镁亚型盐湖。利用相图规律对该盐湖卤水自然蒸发的结晶路线进行了分析,并通过室内模拟自然蒸发试验进行了验证,最终获得了在自然条件下蒸发卤水分步结晶不同盐类的工艺路线,可为该盐湖资源综合利用提供依据。  相似文献   

The young open cluster NGC 2129     

Giovanni Carraro  Brian Chaboyer  James Perencevich 《Monthly notices of the Royal Astronomical Society》2006,365(3):867-873

The first charge-coupled device   UBV ( RI )_C  photometric study in the area of the doubtful open cluster NGC 2129 is presented. Photometry of a field offset 15 arcmin northwards is also provided, to probe the Galactic disc population towards the cluster. Using star counts, proper motions from the UCAC2 catalogue, colour–magnitude and colour–colour diagrams, we demonstrate that NGC 2129 is a young open cluster. The cluster radius is 2.5 arcmin, and across this region we find evidence of significant differential reddening, although the reddening law seems to be normal towards its direction. Updated estimates of the cluster fundamental parameters are provided. The mean reddening is found to be   E ( B − V ) = 0.80 ± 0.08  and the distance modulus is  ( m − M )₀= 11.70 ± 0.30  . Hence, NGC 2129 is located at 2.2 ± 0.2 kpc from the Sun inside the Local spiral arm. The age derived from 37 photometrically selected members is estimated to be approximately 10 Myr. These stars are used to provide new estimates of the cluster absolute proper-motion components.  相似文献   

The radio structure of S5 1803+784     

S. Britzen  A. Witzel  T. P. Krichbaum  T. Beckert  R. M. Campbell  C. Schalinski  J. Campbell 《Monthly notices of the Royal Astronomical Society》2005,362(3):966-974

We present deep CCD BVI photometry of the distant, old open cluster Berkeley 22, covering from the red giant branch (RGB) to about six magnitudes below the main-sequence (MS) turn-off. Using the synthetic colour–magnitude diagram method with three different types of stellar evolutionary tracks, we estimate values and theoretical uncertainties of the distance modulus ( m − M )₀, reddening E ( B − V ), age τ and approximate metallicity. The best fit to the data is obtained for  13.8 ≤ ( m − M )₀≤ 14.1,  0.64 ≤ E ( B − V ) ≤ 0.65,  2.0 ≤τ≤ 2.5 Gyr  (depending on the amount of overshooting from convective regions adopted in the stellar models) and solar metallicity.  相似文献   

Unveiling the nature of the highly obscured active galactic nucleus in NGC 5643 with XMM–Newton     

M. Guainazzi  P. Rodriguez-Pascual  A. C. Fabian  K. Iwasawa  G. Matt 《Monthly notices of the Royal Astronomical Society》2004,355(1):297-306

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