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1.
沉积盆地中未遭受热重置的碎屑颗粒裂变径迹(FT)热年代学正成为山前冲断带蚀源区抬升-剥露过程及其与相邻盆地沉积作用关系研究的重要方法.对于未热重置碎屑岩样品的磷灰石(或锆石)单矿物颗粒裂变径迹年龄(FTGA)数据,采用高斯或二项式拟合方法可以获得样品中不同组分碎屑颗粒矿物的FT峰值年龄或称蚀源区抬升一剥露事件的FT封闭(冷却)年龄.已有的统计分析结果表明,抬升冷却矿物的FT封闭年龄(tc)与其剥露搬运至相邻盆地的沉积年龄(td)之间具有较好的线性关系(tc=A+Btd),二者的滞后时间(△t=tc-td≈tc-te,te为抬升冷却的碎屑颗粒矿物剥露到近地表的剥露年龄)构筑了蚀源区抬升冷却矿物FT封闭深度(Zc)与抬升剥露速率(E)之间的定量关系(E=Zc/△t)和不同碎屑颗粒的滞后时间与其沉积年龄之间相关变化的统计预测模型△t=A+(B-1)td.显然,滞后时间越短,造山带蚀源区的抬升剥露速率越大、物源供应越充分,山前带沉积一沉降作用趋于增强,反之亦然. 相似文献
2.
Numerical evaluation of multicomponent cation exchange reactive transport in physically and geochemically heterogeneous porous media 总被引：1，自引：0，他引：1
Experimental evidence and stochastic studies strongly show that the transport of reactive solutes in porous media is significantly
influenced by heterogeneities in hydraulic conductivity, porosity, and sorption parameters. In this paper, we present Monte
Carlo numerical simulations of multicomponent reactive transport involving competitive cation exchange reactions in a two-dimensional
vertical physically and geochemically heterogeneous medium. Log hydraulic conductivity, log K, and log cation exchange capacity (log CEC) are assumed to be random Gaussian functions with spherical semivariograms. Random
realizations of log K and log CEC are used as input data for the numerical simulation of multicomponent reactive transport with CORE2D, a general purpose reactive transport code. Longitudinal features of the fronts of reactive and conservative species are
computed from the temporal and spatial moments of depth-averaged concentrations. Monte Carlo simulations show that: (1) the
displacement of reactive fronts increases with increasing variance of log K, while it decreases with the variance of log CEC; (2) second-order spatial moments increase with increasing variances of
log K and log CEC; (3) uncertainties in the mean arrival time are largest (smallest) for negatively (positively) correlated log
K and Log CEC; (4) cations undergoing competitive cation exchange exhibit different apparent velocities and retardation factors
due to both physical and geochemical heterogeneities; and (5) the correlation between log K and log CEC affects significantly apparent cation retardation factors in heterogeneous aquifers. 相似文献
3.
The occurrence of talc and tremolite in a temperature gradient was investigated in siliceous calcite-dolomite sediments exposed along a strip in the southeastern part of the Damara Orogen. Five bivariant reactions may lead to the formation of talc and tremolite:
- 3 dolomite+4 quartz+1 H2O ? 1 talc+3 calcite+3 CO2
- 5 talc+6 calcite+4 quartz ? 1 tremolite+6 CO2+2 H2O
- 2 talc+3 calcite ? 1 tremolite+1 dolomite+1 CO2+1 H2O
- 5 dolomite+8 quartz+1 H2O ? 1 tremolite+3 calcite+7 CO2
- 2 dolomite+1 talc+4 quartz ? 1 tremolite+4 CO2.
4.
T. M. Rachkovskaya 《Astronomy Reports》2003,47(10):865-872
We have studied the star 30 LMi using high-dispersion CCD spectra and photographic observations. We estimate the star's effective temperature Teff=7210 K, gravity log g=3.34, and microturbulence velocity ξt=5.8 km/s. The carbon abundance, log ?(C)=8.57, is close to the solar value. Nitrogen (log ?(N)=7.81), oxygen (log ?(O)=8.76), and sulfur (log ?(S)=7.20) are slightly underabundant compared to the Sun, by ?0.16 dex, ?0.11 dex, and ?0.13 dex, respectively. A relatively large underabundance of ?0.27 dex was found for titanium (log ?(Ti)=4.75), whereas zinc shows an over-abundance by +0.21 dex (log ?(Zn)=4.81). Sodium (log ?(Na)=6.26), silicon (log ?(Si)=7.57), calcium (log ?(Ca)=6.38), chromium (log ?(Cr)=5.62), iron (log ?(Fe)=7.51), nickel (log ?(Ni)=6.34), and yttrium (log ?(Y)=2.34) exhibited abundances close to the solar values. We find no chemical anomalies characteristic of Am stars or δ Scuti stars in the spectrum of 30 LMi. 相似文献
5.
Among hygric properties of stone material, the sorption behaviour is of essential importance because of the permanence of the processes involved. New results from static sorption experiments performed by standard techniques and by a new tool are reported for six different building stones. Furthermore, an example of dynamic sorption behaviour under continuously changing humidity is presented. For the static equilibrium sorption measurements a close relation to the stone type, its pore properties, such as specific inner surface, pore volume, pore size distribution as well as capillary water uptake and water saturation, is drawn. The comparison of the different data allows us to retrieve correlations between material features that are crucial for weathering processes. The sorption–desorption processes respond spontaneously on even small humidity changes as shown by the dynamic sorption experiment. A permanent breathing-process of the material is imposed. 相似文献
6.
T. M. Rachkovskaya 《Astronomy Reports》2002,46(9):760-764
We have studied the giant 20 Peg using high-resolution spectra. We derive the star’s effective temperature, T eff=6970 K, gravity, logg=3.35, and microturbulence velocity from FeI lines, ξt=2.70 km/s, and from NiI lines, ξt=2.45 km/s. The abundances of carbon, log?(C)=8.78, nitrogen, log?(N)=8.28, and silicon, log?(Si)=7.85, are enhanced compared to the solar values by 0.23, 0.31, and 0.30 dex, respectively. The abundances of oxygen, log?(O)=8.83, sodium, log?(Na)=6.37, and sulfur, log?(S)=7.33, are nearly solar. Calcium and nickel show normal abundances, log?(Ca)=6.44 and log?(Ni)=6.32. Iron log?(Fe)=7.63 and yttrium log?(Y)=2.41 are only slightly overabundant compared to the solar values (by 0.13 and 0.17 dex). We find a rather large (0.95 dex) overabundance of barium log?(Ba)=3.08. 相似文献
7.
Sixteen soil samples were collected from the vicinity of an abandoned lead–zinc mine in Shangyu City, eastern China, and the
heavy-metal speciation and wheat phytotoxicity in the soils were studied. The results showed that the concentrations of free
Cu2+, Zn2+, Cd2+ and Pb2+ were highly variable and ranged from <0.01 to 0.32, 0.06 to 10.62, <0.01 to 1.40 and 0.02 to 37.10 μmol l−1, respectively. The concentrations of soluble Cu, Zn, Cd and Pb ranged from 0.38 to 3.24, 0.72 to 78.74, <0.01 to 1.95 and
0.15 to 639.34 μmol l−1, respectively. The general trend of mean solid/liquid partition coefficient and percentage of free metal ion to total soluble
metal concentration were Cu > Pb > Zn > Cd and Cd > Zn > Cu > Pb, respectively. Stepwise multiple linear regression with pH,
log(total metal) and log(organic matter) showed that log(total metal) was an important factor that controlled log(free metal
ion) and log(soluble metal). Of the variability in log(free Cu2+), log(free Cd2+) and log(free Pb2+), 55.2, 58.6 and 64.3% could be explained by log(total Cu), log(total Cd) and log(total Pb) alone, respectively. Of the variability
in log(soluble Cu) and log(soluble Cd), 77.1 and 72.5% could be explained by log(total Cu) and log(total Cd) alone, respectively.
Wheat root length was controlled by the various metals with different free and soluble concentrations, and 99.2% of the variability
in root length could be explained by concentrations of free and soluble Pb, soluble Cu and total Zn in the soils. 相似文献
8.
构造动力变质作用初论 总被引：3，自引：1，他引：2
本文提出了构造动力变质作用的基本概念。即在构造动力及其引发的动力热流共同作用下,岩石、矿物在构造运动中发生的形变、相变而呈现的变质作用。按构造动力变质作用的物理化学条件,动力变质岩的结构构造、动态重结晶和混合岩化作用、应力矿物共生组合关系及其空间分布等特征,将构造动力变质作用由弱到强划分为4个发展阶段和相应的4种基本变质类型——脆性、脆-塑性、塑性和动力热流变形变质,并论述了它们各自的基本特征。 相似文献
9.
Characteristics of geochemical evolution of trace elements and REE in Gejiu granites,Yunnan Province
Jie Lu 《中国地球化学学报》1988,7(2):155-169
The evolution characteristics of Gejiu granites, Yunnan Province are described in terms of their petrology, especially their
trace elements and REE geochemistry. The three major types of Gejiu granites: porphyritic biotite monzonitic granite (stage
I), medium-coarse-grained biotite-K-feldspar granite (stage II) and two-mica alkali-feldspar granite (stage III) are thought
to have been formed successively from the same granite magma source through fractional crystallization (Rayliegh fractionation),
because linear correlations are found between log(Rb/Sr)-log Sn, log(Rb/Ba)-log Sn, log(Rb/Ba)-log(Rb/Sr), log La-log Sr,
log Ce-log Sr, log Eu-log Sr, etc. In addition, the characteristics of REE distribution patterns in these three major types
of granites also reflect the magmatic differentiation features of Gejiu granites. Of the three major types, the two-mica alkali-feldspar
granite of stage III underwent the strongest differentiation, and thus has the closest genetic relationship with the Gejiu
tin-polymetallic ore deposit. Such tin-polymetal mineralized granites are characterized by high Rb/Sr and Rb/Ba ratios, low
K/Rb and ΣCe/ΣY ratios and remarkable Eu depletion. 相似文献
10.
Experiments have been carried out to determine the temperature, oxygen fugacity (fO2) and compositional dependence of the tracer diffusion coefficient (D) of calcium in olivine. These data constrain the diffusion coefficient over the temperature range 900 to 1500°C for the three principal crystallographic axes. Well constrained linear relationships between the reciprocal of the absolute temperature and log(D) exist at any given oxygen fugacity. There is a strong dependence of the diffusion coefficient on oxygen fugacity with D ∝ fO2(1/3). This makes a knowledge of the T-fO2 path followed by geological samples a prerequisite for modelling Ca diffusion in olivine. The best fitting preexponential factor (Do) and activation energy (E) to the Arrhenius equation log (D) = log [Do exp(−E/RT)] + 0.31Δ log fO2 for Ca diffusion in olivine at a given oxygen fugacity (fO2*) are given by:diffusion along [100]: log [Do (m2/s)] = −10.78 ± 0.43; E = 193 ± 11 kJ/moldiffusion along [010]: log [Do (m2/s)] = −10.46 ± 0.37; E = 201 ± 10 kJ/moldiffusion along [001]: log [Do (m2/s)] = −10.02 ± 0.29; E = 207 ± 8 kJ/molwhere Δ log fO2 = log[fO2*] − log[10−12] with fO2* in units of bars. There is no measurable compositional dependence of the diffusion coefficient between Fo83 and Fo92. Diffusion in Fo100 has a much higher activation energy than in Fe-bearing olivine and has a weaker fO2 dependence. 相似文献
11.
三露天天然气水合物钻探结果揭示,水合物主要赋存于裂隙型和孔隙型储层中。基于钻探结果,在测井岩性识别的基础上,综合利用常规测井和超声波成像测井等资料,总结两类天然气水合物储层的测井响应特征,形成了基于测井资料的水合物储层识别方法,并对该区储层进行划分。结果表明：(1)裂隙型水合物储层比纯泥岩层段的裂隙发育;声波速度较高,范围为1.5~4.5 km/s ;电阻率最高可达90 Ω·m。孔隙型水合物储层比砂岩水层的声波速度高,范围为2.0~4.0 km/s;电阻率亦为高值,范围为90~180 Ω·m。(2)研究区14个钻孔共识别出裂隙型储层12层,孔 隙型储层15层,总厚度为217.2 m。钻遇水合物的厚层均能识别,但少量钻遇的薄层未能识别,原因可能为薄层水合物含量少,导致测井响应不明显。总体上,测井方法在三露天天然气水合 物储层识别方面应用效果良好。 相似文献
12.
A very fast and efficient approach to self-potential (SP) data inversion for ore exploration has been developed. This approach is based on Tikhonov regularization and the conjugate gradient method, and simultaneously inverts for the depth (z), electric dipole moment (k), and angle of polarization (θ) of a buried anomalous body from SP data measured along a profile. This inversion algorithm works iteratively, and solves for z and k in the logarithmic-space (log(z) and log(k)), and solves for θ in the linear-space (non-logarithmic). It is found that the original inversion formulation that uses the model parameters themselves (z, k and θ) is unstable and divergent. It is also found that the inversion formulation that uses the logarithm of the model parameters (log(z), log(k) and log(θ)) is unstable and divergent. Rather, the new inversion scheme that is based on the aforementioned mixed log-linear combination of the model parameters (log(z), log(k), and θ) overcomes and eliminates the mentioned instability and divergence problems. The sensitivity analysis and numerical experiments investigated have indicated that the new approach has a far better and far more optimized minimization search direction. This proposed technique fits the observed data by some geometrically simple body in the restricted class of vertical cylinder, horizontal cylinder, and sphere models. The applicability of the algorithm has been demonstrated on various reliable synthetic data sets with and without noise. The algorithm has been carefully and successfully applied to six real data examples, with ore bodies buried in different complex geologic settings and at various depths in the subsurface. The method is shown to be highly applicable for mineral exploration, and is of particular value in cases where the SP observed data is due to ore body embedded in the subsurface. On average, it took about 40 s of computation (not CPU) time on a 1 GHz PC. 相似文献
13.
辽河油田兴隆台太古界古潜山储层评价标准研究 总被引：1，自引：0，他引：1
兴隆台古潜山是辽河坳陷中重要的深层潜山油藏,对提高辽河油田原油产量具有重要意义。兴隆台太古界潜山主要
储层由变质岩和岩浆岩组成,其中变质岩储层包括黑云斜长片麻岩、黑云母变粒岩、斜长角闪岩、角闪岩和混合岩。储集
空间以构造裂缝为主,储层渗透性好。在测井曲线对储层敏感因素分析的基础上,选用现有测井资料中带有裂缝信息的电
阻率、声波时差、密度、自然电位幅度差和双侧向等测井数据,应用测井交会图方法,结合试油工作的结果,寻找规律,
得出了针对兴隆台古潜山储层进行定量及定性识别和评价的标准,即：岩石密度＜2.75 g/cm3
,自然电位幅度差≥7 Ω·m,
双侧向幅度差20~1 500 Ω·m,深侧向电阻率20~2 000 Ω·m,声波时差170~230 μs/m。通过生产测井解释数据进行了验证,
证明上述储层评价标准基本适用,为兴隆台古潜山油井调层提供了理论基础。 相似文献
14.
We perform a statistical analysis of the properties of 170 rich clusters of galaxies. We confirm the existence of correlations
between the X-ray luminosity and temperature of the cluster intergalactic medium (IGM) and between the velocity dispersion
of the galaxies and the X-ray luminosity of the IGM. In addition, we have found a new anti-correlation between the optical
luminosity in Hα and the X-ray luminosity of the cluster IGM: log $
\left( {\frac{{L_{H\alpha } }}
{{L_ \odot }}} \right) = a - b\log \left( {\frac{{L_x }}
{{L_ \odot }}} \right)
$
\left( {\frac{{L_{H\alpha } }}
{{L_ \odot }}} \right) = a - b\log \left( {\frac{{L_x }}
{{L_ \odot }}} \right)
. Clusters form sequences with different values of a but similar values of b. 相似文献
15.
T. M. Rachkovskaya 《Astronomy Reports》2000,44(4):227-234
Using high-resolution spectra, we have determined the abundances of carbon (logε(C)), nitrogen (logε(N)), oxygen (logε(O)), silicon (logε(Si)), sulphur (logε(S)), and some other elements for three δ Scuti stars. Logε(C) for all three stars and logε(N) for δ Sct and HD 127986 are close to the solar values, while there appears to be a slight (0.15 dex) nitrogen deficiency for 14 Aur. The logε(O) values correspond to a 0.30-dex deficiency for 14 Aur and δ Sct and a 0.20-dex deficiency for HD 127986. The values of logε(Si) for the three stars are close to solar, and the logε(S) values indicate a slight deficiency (0.10 dex) for 14 Aur and HD 127986 and a 0.20-dex excess for δ Sct. Comparison of the elemental abundances for seven δ Scuti stars with those for Am stars shows that the mean deficiencies of C, N, and O are smaller for pulsating δ Scuti stars than for Am stars with similar effective temperatures. The sulphur abundances are virtually the same for both types of stars. 相似文献
16.
As part of our study of the components of the hierarchic quadruple system ADS 11061, we acquired spectroscopic observations of the binary 40 Dra. Echelle spectra showing the separation of the components’ lines were obtained in the spectral range 3700–9200 Å. Effective temperatures and surface gravities were derived for the components from BV photometry and the hydrogen-line profiles. The components of the 40 Dra system have parameters close to T eff a = 6420 K, log g a = 4.17, T eff b = 6300 K, and log g b = 4.20. We find the microturbulence velocity in the component atmospheres to be V t = 2.6 km/s. The abundances of iron, carbon, nitrogen, and oxygen in the atmospheres of both components are estimated to be log N(Fe)a = 7.50, log N(Fe)b = 7.46, log N(C)a = 8.39, log N(C)b = 8.45, log N(N)a = 8.12, log(N)b = 8.15, log N(O)a = 8.77, log N(O)b = 8.74. 相似文献
17.
利用标准偏差法和固定质量法，研究了新疆天山地区3种不同构造地貌单元地形剖线的自仿射分形和多重分形特征。结果表明，在所研究的标度范围内，不同构造地貌单元剖线分维值总体上呈现出高山区大于中低山区大于盆地区特点，同一个地貌研究区不同方向的剖线呈现不同程度的各向异性。多重分形谱Dq的形态和值域范围也呈现出不同特征。研究认为，地貌表面形态并不是完全随机的，而是一种各向异性的分形布朗运动，分维值表征了内外营力作用的方向和强度，渡越长度是自仿射分形研究中的另一个重要参量。利用上述分形特征可定量研究地貌的发展阶段和地貌动力学。 相似文献
18.
Ya. V. Pavlenko 《Astronomy Reports》2008,52(9):749-759
We have modeled absorption lines of the 12CO and 13CO (Δυ = 2) molecular bands at λλ 2.29–2.45 µm in the spectrum of Arcturus (K2III). A grid of model atmospheres and synthetic spectra were computed for the red giant using T eff = 4300, log g = 1.5, and the elemental abundances of Peterson et al. (1993), with the exception of the abundances of carbon, log N(C), and oxygen, log N(O) and the carbon isotopic ratio, 12C/13C, which were varied in our computations. The computed spectra were compared to the observed spectrum of Arcturus from the atlas of Hinkle et al. (1976). The best fit between the synthetic and observed spectra is achieved for log N(C) = ?3.78, 12C/13C = 8 ± 0.5. We discuss the dependence of 12C/13C on log N(C) and log N(O) in the atmosphere of the red giant. 相似文献
19.
T. M. Rachkovskaya 《Astronomy Reports》2005,49(9):714-723
An analysis of high-resolution CCD spectra of the giant 25 Mon, which shows signs of metallicity, and the normal giant HR 7389 is presented. The derived effective temperatures, gravitational accelerations, and microturbulence velocities are Teff = 6700 K, log g = 3.24, and ξ t = 3.1 km/s for 25 Mon and Teff = 6630 K, log g = 3.71, and ξ t = 2.6 km/s for HR 7389. The abundances (log ε) of nine elements are determined: carbon, nitrogen, oxygen, sodium, silicon, calcium, iron, nickel, and barium. The derived excess carbon abundances are 0.23 dex for 25 Mon and 0.16 dex for HR 7389. 25 Mon displays a modest (0.08 dex) oxygen excess, with the oxygen excess for HR 7389 being somewhat higher (0.15 dex). The nitrogen abundance is probably no lower than the solar value for both stars. The abundances of iron, sodium, calcium (for HR 7389), barium, and nickel exceed the solar values by 0.22–0.40 dex for both stars. The highest excess (0.62 dex) is exhibited by the calcium abundance for 25 Mon. Silicon displays a nearly solar abundance in both stars—small deficits of ?0.03 dex and ?0.07 dex for 25 Mon and HR 7389, respectively. No fundamental differences in the elemental abundances were found in the atmospheres of 25 Mon and HR 7389. Based on their Teff and log g values, as well as theoretical calculations, A. Claret estimated the masses, radii, luminosities, and ages of 25 Mon (M/M⊙ = 2.45, log(R/R⊙) = 0.79, log(L/L⊙) = 1.85, t = 5.3 × 108 yr) and HR 7389 (M/M⊙ = 2.36, log(R/R⊙) = 0.50, log(L/L⊙) = 1.24, t = 4.6 × 108 yr), and also of the stars 20 Peg (M/M⊙ = 2.36, log(R/R⊙) = 0.73, log(L/L⊙) = 1.79, t = 4.9 × 108 yr) and 30 LMi (M/M⊙ = 2.47, log(R/R⊙) = 0.73, log(L/L⊙) = 1.88, t = 4.8 × 108 yr) studied by the author earlier. 相似文献
20.
An examination of the relation between runoff rate, R, and concentration, C, of twelve major constituents in four small watersheds in eastern Puerto Rico demonstrates a consistent pattern of responses. For solutes that are not substantially bioactive (alkalinity, silica, calcium, magnesium, sodium, and chloride), the log(R)–log(C) relation is almost linear and can be described as a weighted average of two sources, bedrock weathering and atmospheric deposition. The slope of the relation for each solute depends on the respective source contributions to the total river load. If a solute were strictly derived from bedrock weathering, the slope would be ?0.3 to ?0.4, whereas if strictly derived from atmospheric deposition, the slope would be approximately ?0.1. The bioactive constituents (dissolved organic carbon, nitrate, sulfate, and potassium), which are recycled by plants and concentrated in shallow soil, demonstrate nearly flat or downward-arched log(R)–log(C) relations. The peak of the arch represents a transition from dominantly soil-matrix flow to near-surface macropore flow, and finally to overland flow. At highest observed R (80 to >90 mm/h), essentially all reactive surfaces have become wetted, and the input rate of C becomes independent of R (log(R)–log(C) slope of –1). The highest R are tenfold greater than any previous study. Slight clockwise hysteresis for many solutes in the rivers with riparian zones or substantial hyporheic flows indicates that these settings may act as mixing end-members. Particulate constituents (suspended sediment and particulate organic carbon) show slight clockwise hysteresis, indicating mobilization of stored sediment during rising stage. 相似文献