Spectral index determination between 408 MHz and 5 GHz in the northern sky

We present the joint analysis of two 5-GHz interferometric surveys of the northern sky, taken with different baselines. The two surveys were carried out on the Jodrell Bank 5-GHz interferometer based at Manchester. The Maximum Entropy Method is used to check the consistency of the two surveys and the final two-dimensional maps are used, together with low-frequency full sky surveys, to put constraints on the Galactic spectral index. It is found that synchrotron emission is the dominant process at high Galactic latitudes below 5 GHz.     

对胶南群的异议

对苏北～胶南一带胶南群的变质岩系进行研究，其边界特征、横向不连续性、岩石类型及相互关系、同位素年龄等资料表明，胶南群不具有单一地层单元的含义，而是挟于五莲－荣成断裂与海州－泗阳断裂之间的构造岩石组合体，它由上壳岩类和深源岩类组成，前者包括了３个构造位。其形成可能与边界深大断裂的开合作用有关     

青海日月山断裂德州段断错地貌的高分辨率遥感影像解译

青海日月山断裂带是青藏高原东北缘柴达木—祁连活动地块内部的一条NNW走向的右旋走滑兼逆冲断裂。 本文基于ENVI 5.1遥感图像处理平台对研究区高分一号多光谱(分辨率8 m)和全色(分辨率2 m)影像进行融合, 获取了高保真、 高分辨率的卫星遥感影像。 通过多尺度、 多角度、 多层次的构造解译以及对比, 将日月山西支断裂的海晏段划分为德州段(F_1-3)和海晏段(F_1-4)两个次级段, 同时利用高分辨率Google Earth影像对德州段断错微地貌进行了解译、 分析, 结合对德州段野外地质考察, 进一步验证了影像解译结果。 研究表明: 日月山断裂的德州段由5条次级段落组成(f₁, f₂, f₃, f₄, f₅), 并且该段断裂晚更新世以来活动性明显, 以右旋走滑为主兼有逆倾滑分量; 断裂在晚更新世以来发生过多期断层活动, 其中全新世断层活动可划分为两期, 最新一期水平位错量为6.5~8.7 m, 第二期水平位错量为12.3~14 m; 晚更新世也可划分出两期活动, 第一期水平位错量为16~20 m, 第二期水平位错量为28.5~47 m。     

Exploration and Study on Deep Crust Structural Characteristics in the Jiashi-Artux Seismic Region

The data from two deep seismic sounding profiles was processed and studied comprehensively. The results show that crnst-mantle structures in the investigated region obviously display layered characteristics and velocity structures and tectonic features have larger distinction in different geological structure blocks. The boundary interface C between the upper and lower crust and Moho fluctuate greatly. The shallowest depths of C (30.0km) and Moho (45.5km) under Jiashi deepen sharply from Jiashi to the western Kunlun mountain areas, where the depths of C and Moho are 44.0km and 70.0km, respectively. The higher velocity structures in the Tarim massif determine its relatively “stable“ characteristics in crust tectonics. The phenomenon in the Jiashi region, where the distribution of earthquake foci mostly range from 20kin to 40kin in depth, may infer that the local uplift of C and Moho interface, anomalonsly lower velocity bodies and deep large faults control earthquake occurrence and seismogenic processes in the Jiashi strong earthquake swarm.     

No Higher Criticism of the Bianchi-corrected Wilkinson Microwave Anisotropy Probe data

Higher Criticism (HC) has been proposed by Donoho & Jin as an effective statistic to detect deviations from Gaussianity. Motivated by the success of the Bianchi VII_h model in addressing many of the anomalies observed in the Wilkinson Microwave Anisotropy Probe ( WMAP ) data (Jaffe et al.), we present calculations in real and in wavelet space of the HC statistic of the Bianchi-corrected WMAP first-year data. At the wavelet scale of 5°, the HC of the WMAP map drops from a value above the 99 per cent confidence level (c.l.) to a value below the 68 per cent CL when corrected by the Bianchi template. An important property of the HC statistic is its ability to locate the pixels that account for the deviation from Gaussianity. The analysis of the uncorrected WMAP data pointed to a cold spot in the Southern hemisphere, centred at   l ∼ 209°, b ∼−57°  . The HC of the Bianchi-corrected map indicates that this spot remains prominent, albeit at a level completely consistent with Gaussian statistics. Consequently, it is debatable how much emphasis should be placed on this residual feature, but we consider the effect of modestly increasing the scaling of the template. A factor of only 1.2 renders the spot indistinguishable from the background level, with no noticeable impact on the results published in Jaffe et al. for the low- l anomalies, large-scale power asymmetry or wavelet kurtosis. A trivial interpretation would be that the Bianchi template may require a small enhancement of power on scales corresponding to the wavelet scale of 5°.     

中上扬子海相层系埋藏史与构造运动的关系

依据复杂岩性条件下孔隙度—深度关系模型,采用回剥法重建埋藏史。结果表明,中上扬子地区的埋藏史可分为3种主要类型：早抬持续型、早抬再降型和晚抬持续型。埋藏史的类型受区域构造运动控制,具有明显的分带性。齐岳山断裂以西为晚抬持续型,齐岳山断裂与黄陵隆起之间为早抬持续型,黄陵隆起以东为早抬再降型。印支运动在中上扬子地区只对海相层系有一次短暂抬升剥蚀,剥蚀量小,对埋藏史特征影响不大。燕山运动表现形式、作用强度、对海相层系的改造程度均存在明显的地区差异性,导致海相层系埋藏史类型也有地区差异性。喜马拉雅运动波及整个中国南方,但岩石圈受力性质不同,表现为西挤东张,导致K2—E期间黄陵隆起以西持续抬升,形成“持续抬升型”埋藏史类型,以东则发生拉张断陷,形成“再降型”埋藏史类型。     

云南地区的背景弹性波场分析

利用云南省地震台网44个台站记录的2008年1-9月连续波形数据进行互相关计算,得到了台站间的格林函数,并获取对应的频散曲线,据此分析了该地区的区域背景弹性波场的来源及分布.研究发现,该地区的区域背景弹性波场有着明显的方向性,15s信号的总体传播方向是从东南向西北,也就是说主要来自云南省的东南方向,据此推测区域背景弹性...     

我国重晶石矿床成因及成矿远景综述

我国重晶石矿床的形成受大陆裂谷系、弧-盆系和陆内挤隆系三种大地构造环境控制,多数矿床形成于大构造旋回的早期阶段,并与一定的岩相古地理环境及岩浆活动有关。矿床可划分为外生成因[沉积型、风化（残积坡积）型]和内生成因（火山-沉积型、层控型、热液型）等不同类型。成矿之钡源主要来自深部的火山-气液。矿床多在中、低温,弱酸性向弱碱性过渡的氧化环境的硫酸盐型成矿溶液中形成。中国重晶石矿具有较好的找矿前景,在一些工业需求地区,有发现新矿床的可能。     

The effect of reionization on the cosmic microwave background–density correlation

In this paper, we show how the rescattering of cosmic microwave background photons after cosmic reionization can give a significant linear contribution to the temperature–matter cross-correlation measurements. These anisotropies, which arise via a late-time Doppler effect, are on scales much larger than the typical scale of non-linear effects at reionization; they can contribute to degree scale cross-correlations and could affect the interpretation of similar correlations resulting from the integrated Sachs–Wolfe effect. While expected to be small at low redshifts, these correlations can be large given a probe of the density at high redshift, and so could be a useful probe of the cosmic reionization history.