Accounting for site effect in probabilistic assessment of seismic hazard for Romania and Bucharest: a case of deep seismicity in Vrancea zone     

Vladimir Sokolov  Klaus-Peter Bonjer  Friedemann Wenzel 《Soil Dynamics and Earthquake Engineering》2004,24(12):929-947

The paper presents recent achievements in evaluations of site-dependent seismic hazard in Romania and the capital city of Bucharest caused by the Vrancea focal zone (SE-Carpathians). The zone is characterized by a high rate of occurrence of large earthquakes in a narrow focal volume at depths 60–170 km. The database that was used for the hazard evaluation includes parameters of seismicity, ground-motion source scaling and attenuation models (Fourier amplitude spectra), and site-dependent spectral amplification functions. Ground-motion characteristics were evaluated on the basis of several hundred records from more than 120 small magnitude (M 3.5–5) earthquakes occurred in 1996–2001 and a few tens of acceleration records obtained during four large (M 7.4, 7.2, 6.9 and 6.3) earthquakes. The data provide a basis for probabilistic seismic hazard assessment in terms of peak ground acceleration, peak spectral acceleration and MSK intensity using Fourier amplitude spectra for various exceedance probabilities or average return periods. It has been shown that the influence of geological factors plays very important role in distribution of earthquake ground-motion parameters along the territory of Romania.  相似文献   

Seismic characterization of vertical fractures described as general linear-slip interfaces     

Vladimir Grechka  rey Bakulin  Ilya Tsvankin 《Geophysical Prospecting》2003,51(2):117-130

Fluid flow in many hydrocarbon reservoirs is controlled by aligned fractures which make the medium anisotropic on the scale of seismic wavelength. Applying the linear‐slip theory, we investigate seismic signatures of the effective medium produced by a single set of ‘general’ vertical fractures embedded in a purely isotropic host rock. The generality of our fracture model means the allowance for coupling between the normal (to the fracture plane) stress and the tangential jump in displacement (and vice versa). Despite its low (triclinic) symmetry, the medium is described by just nine independent effective parameters and possesses several distinct features which help to identify the physical model and estimate the fracture compliances and background velocities. For example, the polarization vector of the vertically propagating fast shear wave S₁ and the semi‐major axis of the S₁‐wave normal‐moveout (NMO) ellipse from a horizontal reflector always point in the direction of the fracture strike. Moreover, for the S₁‐wave both the vertical velocity and the NMO velocity along the fractures are equal to the shear‐wave velocity in the host rock. Analysis of seismic signatures in the limit of small fracture weaknesses allows us to select the input data needed for unambiguous fracture characterization. The fracture and background parameters can be estimated using the NMO ellipses from horizontal reflectors and vertical velocities of P‐waves and two split S‐waves, combined with a portion of the P‐wave slowness surface reconstructed from multi‐azimuth walkaway vertical seismic profiling (VSP) data. The stability of the parameter‐estimation procedure is verified by performing non‐linear inversion based on the exact equations.  相似文献   

Reconnaissance paleomagnetism of Late Triassic blocks, Kuyul region, Northern Kamchatka Peninsula, Russia     

William Harbert  Sergei Sokolov  Maxim Alexutin  Kirill Krylov  Vladimir Grigoriev  Alexander Heiphetz   《Tectonophysics》2003,361(3-4):215-227

The northernmost Kamchatka Peninsula is located along the northwestern margin of the Bering Sea and consists of complexly deformed accreted terranes. Progressing inland from the northwestern Bering Sea, the Olyutorskiy, Ukelayat and Koryak superterranes (OLY, UKL and KOR) are crossed. These terranes were accreted to the backstop Okhotsk-Chukotsk volcanic-plutonic belt (OChVB) in northernmost Kamchatka. A sedimentary sequence of Albian to Maastrichtian age overlaps the terranes and units of the Koryak superterrane, and constrains their accretion time. A paleomagnetic study of blocks within the Kuyul (KUY) terrane of the Koryak superterrane was completed at two localities (Camp 2: λ=61.83°N, φ=165.83°E and Camp 3: λ=61.67°N, φ=164.75°E). At both localities, paleomagnetic samples were collected from Late Triassic (225–208 Ma) limestone blocks (2–10 m in outcrop height) within a melange zone. Although weak in remanent magnetization, two components of remanent magnetization were observed during stepwise thermal demagnetization at 32 sites. The A component of magnetization was observed between room temperature and approximately 250 °C. This magnetic component is always of downward directed inclination and shows the best grouping at relatively low degrees of unfolding. Using McFadden–Reid inclination-only statistics and averaging all site means, the resulting A component mean is I_opt=60.3°, I₉₅=5.0° and n=36 (sites). The B magnetic component is observed up to 565 °C, at which temperature, most samples have no measurable remanent magnetization, or growth of magnetic minerals has disrupted the thermal demagnetization process. Combining sites with Fisher estimates of kappa (k-value)≥13 and n (sites)≥3, where bedding orientation differs within a block, most of these sites show the best grouping of B component directions at 100% unfolding, and two of the blocks display remanent magnetizations of both upward and downward directed magnetic inclination. Combining sites with Fisher estimates of kappa (k-value)≥13 and n (sites)≥3, the resulting overall B component paleolatitude and associated uncertainty are λ_obs=30.4°N or S, λ₉₅=8.9° and n=19 (sites). When compared with the expected North America paleolatitude of λ_{APWP expected}=57.9°N, our data support a model in which blocks within the Koryak superterrane are allochthonous and far travelled.  相似文献   

Evaluation of models for Fourier amplitude spectra for the Taiwan region     

Vladimir Sokolov  Chin-Hsiung Loh  Kuo-Liang Wen 《Soil Dynamics and Earthquake Engineering》2002,22(8)

In the Taiwan region, the empirical spectral models for estimating ground-motion parameters were obtained recently on the basis of recordings of small to moderate (5.0≤M_L≤6.5) earthquakes. A large collection of acceleration records from the M_L=7.3 Chi-Chi earthquake (21 September, 1999) makes it possible to test the applicability of the established relationships in the case of larger events. The comparison of ground-motion parameters (Fourier amplitude spectra, peak accelerations and response spectra), which were calculated using the models, and the observed data demonstrates that the models could provide an accurate prediction for the case of the Chi-Chi earthquake and the largest aftershocks. However, there are some peculiarities in the ground-motion frequency content and attenuation that, most probably, are caused by the features of the rupture process of the large shallow earthquake source.  相似文献   

Chironomid responses to long-term metal contamination: a paleolimnological study in two bays of Lake Imandra, Kola Peninsula, northern Russia     

Boris Ilyashuk  Elena Ilyashuk  Vladimir Dauvalter 《Journal of Paleolimnology》2003,30(2):217-230

Short sediment cores from two gulfs, Monche Bay and Kunchast Bay, of Lake Imandra (Kola Peninsula, northern Russia) were analysed for sediment chemistry and chironomid head capsule remains. Monche Bay has been receiving metals from the Severonikel copper-nickel smelter since the late 1930's. Kunchast Bay was selected in the remotest lake basin as an internal reference site. There were no pronounced changes in the chironomid assemblages with the beginning of slight metal contamination of Kunchast Bay. Based on the reconstructed environmental variables and chironomid assemblages, three developmental stages were distinguished from the chironomid fauna history of Monche Bay: (1) A natural development stage; (2) the early warning stage; and (3) the developing crises stage. During the first period, the changes in the chironomid fauna reflect an anthropogenically undisturbed assemblage, with Micropsectra insignilobus dominating (17–23%). The changes during the second period reflect the initial phase of anthropogenic succession associated with the beginning of metal pollution. The main species showed opposite distributional patterns in this period: the abundance of M. insignilobus decreased, whereas the abundance of Chironomus, Procladius and Sergentia coracina increased. At the same time, maximal numbers were attained for species richness (45) and Shannon-Weaver diversity (4.85) of chironomid assemblages, and the highest head capsule concentration (75 head capsules · g^–1 of dry sediment). The third period was characterized by a major shift in the faunal assemblages, from M. insignilobus to other dominant species, including Chironomus (22–44%), Procladius (10–30 %) and S. coracina (15–18%). Besides fauna changes, assemblages of the third period are distinguished by the occurrence of mouthpart deformities in Chironomus head capsules.  相似文献   

Carbon in Russian Soils     

Vladimir Stolbovoi 《Climatic change》2002,55(1-2):131-156

Soil carbon densities and pools have been estimated for Russia. The estimate was derived from the generalized version of the soil map of the country at the scale 1:2.5 million (Fridland, 1988), which has been designated a countrywide standard. At the pre-developed stage, the soils in Russia captured about 373 Pg of organic and 75 Pg of inorganic C in the 0–2.0 m layer. Organic C is intensively accumulated in the topsoil. Inorganic C tends to concentrate in deep soils and is of non-pedogenic origin. The mass of organic matter is captured in the tundra, pre-tundra, and the northern and middle taiga of Russia. Anthropogenic impacts have led to a loss of about 5 Pg of C in the 0–1.0 m layer, which is some 2% of the total C content in Russian soils. From this amount, the topsoil of cropland has lost 2.6 Pg (20% of the initial C content in soils), including 0.4 Pg caused by erosion. The deep soil (0.3–1.0 m) of cropland has lost 1 Pg. Some 0.5 Pg of C are removed from the topsoil (7%) and 0.6 Pg by the deep soil from pastures. Forest soils have roughly lost about 0.3 Pg of C due to the decline of C input into soils caused by various disturbances. The predicted climate warming is expected to enhance the C sequestration by soil in Russia.  相似文献   

The use of uniaxial recordings in moment tensor inversions for induced seismic sources     

Cezar I. Trifu  Vladimir Shumila 《Tectonophysics》2002,356(1-3)

This study shows that the use of uniaxial recordings maintains the linear dependence of the low frequency displacements, with first polarities included, on the moment tensor components, and thus can be easily incorporated in the evaluation of failure mechanism using a moment tensor approach. Synthetic data analysis demonstrates that the errors in the orientation of the principal strain axes of the mechanism solution can be reliably evaluated using a linear error propagation approximation for up to 30% variance in the amplitude data. Case studies at the Kidd Mine indicate that the general characteristics of the mechanism solution are well retrieved, regardless of the type of data used, as relatively small disorientation angles of 15–20° are found between the solutions derived from rotated triaxial data and those from unrotated triaxial data used as uniaxial data, and of 25–30° between the solutions based on rotated triaxial data and those on independent uniaxial data.  相似文献   

阿穆尔板块相对欧亚板块的欧拉运动   总被引：3，自引：2，他引：1  

孟国杰  申旭辉  伍吉仓  任金卫 《大地测量与地球动力学》2006,26(3):23-28

利用中国东北地区1998～2005年的GPS数据,结合俄罗斯、韩国和蒙古的部分GPS观测资料,用加权最小二乘方法以迭代的方式解算了阿穆尔板块相对欧亚板块的欧拉运动矢量。最终的33个测站的位移速率加权均方根残差(WRMS)为0.98mm/a。计算结果表明阿穆尔相对欧亚板块运动的欧拉极位于阿穆尔板块的北部边界外兴安岭东端(54.06±1.13°N,135.87±7.16°E),欧拉旋转量为0.099±0.00735°/Ma。  相似文献   

Role of the Rossiter-McLaughlin effect in the study of close binaries     

Galina N.Dryomova  Vladimir V.Dryomov 《天文和天体物理学研究(英文版)》2019,(3):21-30

This paper is devoted to binary stars belonging to the class of eclipsing-variable systems.Photometric and spectroscopic analysis of eclipses allows us to determine geometric parameters of the orbit and physical characteristics of stellar components as well as inclinations of stellar equators to the orbital plane. Estimations of inclinations can be obtained from measurement of the Rossiter-McLaughlin effect, which is discussed using examples of some eccentric binaries with an anomalous apsidal effect. Our task is to find the complete spectrum of solutions of the equation of apsidal motion, depending on the inclinations of the polar axes of the components to the orbital one for these systems, based on their individual spectroscopic and photometric observational data. The matrix of solutions allows us to select those pairs of polar inclinations that provide agreement with the observational apsidal period.  相似文献   

On the radiative and thermodynamic properties of the cosmic radiations using COBE FIRAS instrument data: IV. Sunyaev-Zel’dovich ($\mu$-type) distortion effect     

Anatoliy I. Fisenko  Vladimir F. Lemberg 《Astrophysics and Space Science》2018,363(11):224

The Sunyaev-Zel’dovich (SZ) effect represents a small spectral distortion to the cosmic microwave background (CMB) radiation, caused by the Compton scattering of CMB photons by the hot gas of galaxy clusters. In an early stage of universe, the SZ effect generates \(\mu\)-type of distortions for the CMB spectrum. A \(\mu\)-type distortion is created between the double Compton scattering decoupling (\(z \sim 10^{6}\)) and the thermalization decoupling by the Compton scattering (\(z \sim 10^{5}\)). In this case, to describe the small spectral distortion of the CMB spectrum, we use the Bose-Einstein (\(\mu\)-type) distribution with a non-zero chemical potential. At present, it is interesting to investigate the effect of this spectral distortion on the integral characteristics of the Bose-Einstein (\(\mu\)-type) spectrum. The thermal radiative and thermodynamic functions are such integral characteristics. These functions are as follows: a) the total radiation power per unit area; b) total energy density; c) number density of photons; d) grand potential density; e) Helmholtz free energy density; f) entropy density; g) heat capacity at constant volume; h) enthalpy density; and i) pressure. Precise analytical expressions are obtained for the temperature dependences of these functions. Using the observational data obtained by the COBE FIRAS, PIXIE, PRISM, and Planck missions, the thermal radiative and thermodynamic functions are calculated. A comparative analysis of the results obtained with the results for the same functions of the CMB spectrum at \(T = 2.72548~\mbox{K}\) is carried out. Very small distortions are observed for the thermal radiative and thermodynamic functions. In the redshift range \(10^{5} < z < 3 \times10^{6}\), these functions are calculated. The expressions are obtained for new astrophysical parameters, such as the entropy density/Boltzmann constant and number density, created by the Bose-Einstein (\(\mu\)-type) spectrum.  相似文献