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301.
Unequal illumination of the subsurface highly impacts the quality of seismic imaging. Different image points receive different folds of reflection‐angle illumination, which can be caused by irregular acquisition or by wave propagation in complex media. Illumination problems can deteriorate amplitudes in migrated images. To address this problem, we present a method of stacking angle‐domain common‐image gathers, in which we use local similarity with soft thresholding to determine the folds of local illumination. Normalization by local similarity regularizes local illumination of reflection angles for each image point of the subsurface model. This approach compensates for irregular illumination by selective stacking in the image space, regardless of the cause of acquisition or propagation irregularities. Additional migration is not required because the methodology is implemented in the reflection angle domain after migration. We use two synthetic examples to demonstrate that our method can normalize migration amplitudes and effectively suppress migration artefacts. 相似文献
302.
Numerical simulation of seismotectonic tsunamis usually starts with specification of the initial elevation of the water surface in the tsunami source. The initial elevation is traditionally set equal to the vertical residual bottom deformation resulting from earthquakes. We discuss the imperfectness of the traditional approach and suggest an improved practical method of calculating the initial elevation from the solution of the 3D problem in the framework of potential theory. The method takes into account horizontal and vertical components of bottom deformation and bathymetry in the source area. Within the assumption of instant tsunami generation the suggested method represents the optimal way to specify the initial condition in the tsunami propagation problem. The tsunamis in the Central Kuril Islands on 15 November 2006 and 13 January 2007 are taken as examples to demonstrate the efficiency of the new method. 相似文献
303.
Sergey A. Arsen’yev 《地学前缘(英文版)》2011,2(2):215-221
Recent advances in modeling of tornadoes and twisters consist of significant achievements in mathematical calculation of occurrence and evolution of a violent F5-class tornado on the Fujita scale, and four-dimensional mathematical modeling of a tornado with the fourth coordinate time multiplied by its characteristic velocity.Such a tornado can arise in a thunderstorm supercell filled with turbulent whirlwinds.A theory of the squall storms is proposed.The squall storm is modeled by running perturbation of... 相似文献
304.
Sergey V. Pribavkin Irina S. Avdonina Dmitry A. Zamyatin 《Mineralogy and Petrology》2013,107(1):125-147
Epidote-bearing porphyritic dikes (whole rock analysis: SiO2?=?55–65 wt. %, MgO <2.1 wt. %, K2O <2.5 wt. %, Al2O3 >17 wt. %, Na2O + K2O?=?5.7–9.4 wt. %) situated in the continental margin zone, the Middle Urals, Russian Federation have been dated using SHRIMP U-Pb zircon techniques and give a Middle Devonian age of 388?±?2 Ma and 389?±?6 Ma. The porphyries contain phenocrysts of magmatic epidote (Ps?=?17–25 %), Ca- and Mn-rich (CaO >9 wt. %; MnO >6 wt. %) almandine garnet, Al-rich (Al2O3?=?12–16 wt. %) amphibole, titanite, plagioclase, biotite, muscovite, apatite, and quartz. 60 to 70 % groundmass of the porphyritic dikes consists of fine-grained albite, quartz, and K-feldspar. A variety of thermobarometric estimations, plus comparison with published experimental data indicate that the phenocryst assemblage was stable between 5 and 11 kbar and 690 to 800 °C. Oxygen fugacity was close to or greater than logfo2 = Ni-NiO + 1. Later stage formation of the quartz-feldspar groundmass took place at hypabyssal conditions, corresponding to 1 to 2 kbar and 660 to 690 °C. The porphyritic dikes are metaluminous to slightly peraluminous (ACNK?=?0.7–1.17). They are enriched in REE and depleted Nb and Ti. They show features typical of subduction-related magmas. Chemical composition and isotopic ratios of 86Sr/87Sri?=?0.709–0.720 suggest that both mantle- and deep crustal-derived materials were involved in their petrogenesis. 相似文献
305.
Nadezhda Alexandrovna Krivolutskaya Alexandr Vladimirovich Sobolev Sergey Grigor’evich Snisar Bronislav Iosiphovich Gongalskiy Dmitry Vladimirovich Kuzmin Folkmar Hauff Irina Nikolaevna Tushentsova Natalya Mikhailovna Svirskaya Natalya Nikolaevna Kononkova Tatyana B. Schlychkova 《Mineralium Deposita》2012,47(1-2):69-88
We report new data on the stratigraphy, mineralogy and geochemistry of the rocks and ores of the Maslovsky Pt–Cu–Ni sulfide deposit which is thought to be the southwestern extension of the Noril’sk 1 intrusion. Variations in the Ta/Nb ratio of the gabbro-dolerites hosting the sulfide mineralization and the compositions of their pyroxene and olivine indicate that these rocks were produced by two discrete magmatic pulses, which gave rise to the Northern and Southern Maslovsky intrusions that together host the Maslovsky deposit. The Northern intrusion is located inside the Tungusska sandstones and basalt of the Ivakinsky Formation. The Southern intrusion cuts through all of the lower units of the Siberian Trap tuff-lavas, including the Lower Nadezhdinsky Formation; demonstrating that the ore-bearing intrusions of the Noril’sk Complex post-date that unit. Rocks in both intrusions have low TiO2 and elevated MgO contents (average mean TiO2 <1 and MgO?=?12?wt.%) that are more primitive than the lavas of the Upper Formations of the Siberian Traps which suggests that the ore-bearing intrusions result from a separate magmatic event. Unusually high concentrations of both HREE (Dy+Yb+Er+Lu) and Y (up to 1.2 and 2.1?ppm, respectively) occur in olivines (Fo79.5 and 0.25% NiO) from picritic and taxitic gabbro-dolerites with disseminated sulfide mineralization. Thus accumulation of HREE, Y and Ni in the melts is correlated with the mineral potential of the intrusions. The TiO2 concentration in pyroxene has a strong negative correlation with the Mg# of both host mineral and Mg# of host rock. Sulfides from the Northern Maslovsky intrusion are predominantly chalcopyrite–pyrrhotite–pentlandite with subordinate and minor amounts of cubanite, bornite and millerite and a diverse assemblage of rare precious metal minerals including native metals (Au, Ag and Pd), Sn–Pd–Pt–Bi–Pb compounds and Fe–Pt alloys. Sulfides from the Southern Maslovsky intrusion have δ 34S?=?5–6‰ up to 10.8‰ in two samples whereas the country rock basalt have δ 34S?=?3–4‰, implying there was no in situ assimilation of surrounding rocks by magmas. 相似文献
306.
In this paper, we propose a method of cost distribution analysis of new consumer connections to a city power grid by accounting for spatial restrictions and characteristics of existing networks. In practice, the calculation of connection costs for each new consumer includes the network design and financial expenditure. We suggest that connection costs should be calculated for the whole city based on the normative parameters at the stage when the object location is selected by investors and when power grid development is planned by power companies. The proposed method enables the modeling of new power line connection routes from every parcel of city land to possible points of connection to the operating networks based on the raster design of the area. The optimal path is chosen by one criterion consisting of two components: the costs of both laying new power lines and providing sufficient power reserve in the chosen network connection point. Realized as a computer program, the method has been used to calculate the costs of connections to low-voltage power lines. 相似文献
307.
Mark R. Yoder Jordan Van Aalsburg Donald L. Turcotte Sergey G. Abaimov John B. Rundle 《Pure and Applied Geophysics》2013,170(1-2):155-171
Aftershock statistics provide a wealth of data that can be used to better understand earthquake physics. Aftershocks satisfy scale-invariant Gutenberg–Richter (GR) frequency–magnitude statistics. They also satisfy Omori’s law for power-law seismicity rate decay and Båth’s law for maximum-magnitude scaling. The branching aftershock sequence (BASS) model, which is the scale-invariant limit of the epidemic-type aftershock sequence model (ETAS), uses these scaling laws to generate synthetic aftershock sequences. One objective of this paper is to show that the branching process in these models satisfies Tokunaga branching statistics. Tokunaga branching statistics were originally developed for drainage networks and have been subsequently shown to be valid in many other applications associated with complex phenomena. Specifically, these are characteristic of a universality class in statistical physics associated with diffusion-limited aggregation. We first present a deterministic version of the BASS model and show that it satisfies the Tokunaga side-branching statistics. We then show that a fully stochastic BASS simulation gives similar results. We also study foreshock statistics using our BASS simulations. We show that the frequency–magnitude statistics in BASS simulations scale as the exponential of the magnitude difference between the mainshock and the foreshock, inverse GR scaling. We also show that the rate of foreshock occurrence in BASS simulations decays inversely with the time difference between foreshock and mainshock, an inverse Omori scaling. Both inverse scaling laws have been previously introduced empirically to explain observed foreshock statistics. Observations have demonstrated both of these scaling relations to be valid, consistent with our simulations. ETAS simulations, in general, do not generate Båth’s law and do not generate inverse GR scaling. 相似文献
308.
309.
Sergey A. Silich † Guillermo Tenorio-Tagle ‡ Roberto Terlevich § Elena Terlevich †¶ Hagai Netzer 《Monthly notices of the Royal Astronomical Society》2001,324(1):191-200
We have modelled the evolution of hot superbubbles in starbursts, taking into account the rapid changes in the chemical composition of the interior of the superbubbles resulting from the large stellar mass loss, i.e. stellar winds from massive young stars and type II supernovae. We have followed in detail the time-dependent production and mixing of oxygen and iron in the interior of the hot superbubbles and showed that while the oxygen abundance rapidly climbs to over solar values in less than 10 Myr, iron abundance remains always under solar. This highly enhanced oxygen metallicity boosts the early X-ray luminosity of superbubbles while keeping the iron abundance subsolar. This brings theory and X-ray observations of the luminosity and metal content of young starbursts closer together. 相似文献
310.
This work concerns possible connection between variations of δ18O in Greenland ice, temperature, precipitation amount, NAO indices and relative sunspot numbers. The relationships between
10-year averaged values of this data were derived making use of regression analysis methods. It was discovered that February
temperature yields the main contribution in variability of δ18O. The multiple correlation coefficient between weighted night temperature of the most important months and δ18O equals 0.95±0.01. Besides the local source of δ18O changes, defined by the amount of precipitation and temperature, an additional source correlated with the level of solar
activity has been revealed. The relative contribution of this source in the δ18O variance is about 0.1. It has been shown that the multiple correlation coefficient between δ18O and NAO indices is equal to 0.85. Therefore the NAO yields more than 2/3 of the variances of climatic change in Greenland.
An independent contribution of solar activity in climatic changes is about 1/3. 相似文献