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251.
Seismic and field evidence for selective inversion of Cretaceous normal faults, Salta rift, northwest Argentina 总被引:1,自引:0,他引:1
Northwestern Argentina was the site of the continental Salta rift in Cretaceous to Paleogene time. The Salta rift had a complex geometry with several subbasins of different trends and subsidence patterns surrounding a central high. Fault trends in the rift were extremely variable. There is evidence of normal and/or transfer faults trending N, NE, E and SE. It is not clear if all these faults were active at the same time, indicating a poorly defined extension direction, or if they formed in different, non-coaxial extension phases. In either case, their trends were very likely influenced by preexisting fault systems. Beginning in early Eocene time, the rift basins were superseded by Andean foreland basins and later became caught in the Andean thrust deformation propagating eastward, resulting in the inversion of rift faults. Due to their different orientations, not all faults were equally prone to reactivation as thrusts. N to NNE trending faults were apparently most strongly inverted, probably often to a degree where the traces of their normal fault origin have become obliterated. We present seismic evidence of moderately inverted N trending faults in the Tres Cruces basin and field examples of preserved E trending normal faults. However, reactivation sometimes also affects faults trending approximately parallel to the main Neogene shortening direction, indicating short-term deviations from the general pattern of Neogene thrust deformation. These pulses of orogen-parallel contraction may be linked to the intermittent activity of oblique transfer zones. 相似文献
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在X射线荧光光谱(XRF)分析中,粉末压片制样是被广泛应用的一种制样方法,但由于存在样品粒度、矿物和基体效应对其测量条件进行优化。本文应用XRF法测量地球化学调查样品中24种主次量元素,综合优化了制样压力、仪器工作电压和工作电流、待测元素分析谱线、探测器的调节和探测效率等实验条件。在最优测量条件下,用土壤和水系沉积物国家标准物质GBW07402、GBW07404、GBW07424、GBW07426、GBW07429验证方法的准确度,结果表明个别元素如GBW07402中的Na2O、GBW07404中的Pb相对误差大于10%,其余元素的相对误差小于10%,但均达到了地球化学调查样品的质量监控要求。经优化的仪器测量条件为我国地球化学调查样品提供了可靠的基础数据。 相似文献
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Saleem Zaroubi Rajat M. Thomas Naoshi Sugiyama Joseph Silk 《Monthly notices of the Royal Astronomical Society》2007,375(4):1269-1279
A simple analytical model is used to calculate the X-ray heating of the intergalactic medium (IGM) for a range of black hole masses. This process is efficient enough to decouple the spin temperature of the IGM from the cosmic microwave background (CMB) temperature and produce a differential brightness temperature of the order of ∼ 5–20 mK out to distances as large as a few comoving Mpc, depending on the redshift, black hole mass and lifetime. We explore the influence of two types of black holes, those with and without ionizing ultraviolet radiation. The results of the simple analytical model are compared to those of a full spherically symmetric radiative transfer code. Two simple scenarios are proposed for the formation and evolution of black hole mass density in the Universe. The first considers an intermediate mass black hole that form as an end-product of pop III stars, whereas the second considers supermassive black holes that form directly through the collapse of massive haloes with low spin parameter. These scenarios are shown not to violate any of the observational constraints, yet produce enough X-ray photons to decouple the spin temperature from that of the CMB. This is an important issue for future high-redshift 21-cm observations. 相似文献
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