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1.
A nearly 160-km long Wollaston Lake Reflector (WLR) observed in seismic reflection profile S2b of the 1994 Lithoprobe Trans-Hudson Orogen transect (THOT) in northern Saskatchewan (Canada) is among the most spectacular and well-recorded features imaged within the crystalline crust. Based on modeling of its normal-incidence reflectivity, the observed bright spot reflector was originally interpreted as a series of tabular diabase intrusions. In order to further elucidate its structure, we reprocessed line S2b and analysed the WLR for the Amplitude Variations with Offset (AVO). By contrast to conventional (approximate) AVO analysis, we used the exact Zoeppritz equations and considered a thin-layer (mixed positive and negative polarities) reflectivity. The results suggest two possible interpretations of the WLR: 1) the reflector caused by a massive mafic intrusion as suggested earlier, in which case the intruded rocks should have anomalous Poisson's ratios of σ ≥ 0.33, and 2) the WLR represents a silicified shear zone, with only moderate (e.g., 5–10%) alteration of the host rock and σ ≈ 0.2. Although both of these models may to some extent co-exist within the WLR, its brightness, sharpness, great lateral extent and smooth shape favour the second interpretation.In both models, a fractured fluid-filled zone within a major crustal detachment should have played a key role in the formation of the WLR. The association of the reflector with laterally- and depth-migrating fluids is also supported by magneto-telluric measurements of crustal conductivity beneath the WLR. Analogies from the studies of the Kola Superdeep Borehole (Russia), where free or metamorphic fluids were found at comparable depths, also suggest that fluids may contribute to WLR structure and formation. 相似文献
2.
2007年中国在南海北部神狐海域通过钻探首次获得天然气水合物样品,证实了珠江口盆地深水区是水合物富集区。通过对珠江口盆地深水区构造沉降史的定量模拟研究,发现晚中新世以来区内构造沉降总体上具有由北向南、自西向东逐渐变快的演化趋势;从晚中新世到更新世,盆地深水区经历了构造沉降作用由弱到强的变化过程：晚中新世(11.6～5.3 Ma),平均构造沉降速率为67 m/Ma;上新世(5.3～1.8 Ma),平均构造沉降速率为68 m/Ma;至更新世(1.8～0 Ma),平均构造沉降速率为73 m/Ma。而造成这些变化的主因是发生在中中新世末-晚中新世末的东沙运动和发生在上新世-更新世早期的台湾运动。东沙运动（10～5 Ma）使盆地在升降过程中发生块断升降,隆起剥蚀,自东向西运动强度和构造变形逐渐减弱,使得盆地深水区持续稳定沉降;台湾运动（3 Ma）彻底改变了盆地深水区的构造格局,因重力均衡调整盆地深水区继续沉降,越往南沉降越大。将似海底反射（BSR）发育区与沉降速率平面图进行叠合分析,发现80％以上的BSR分布趋于构造沉降速率值主要在75～125 m/Ma之间、沉降速率变化迅速的隆坳接合带区域。 相似文献
3.
张毅 《中国海洋湖沼学报》2011,29(5):1128-1130
Herein we would like to comment on the paper "Estimation of potential distribution of gas hydrate in the northern South China Sea" by Wang et al. 2010 in Chinese Journal of Oceanology and Limnology, 28(3): 693-699. The purpose of this comment is to point out that the given probabilities of gas hydrate occurrence in the northern Zhujiang Mouth Basin and the Yinggehai Basin in the figure of Wang et al. (2010) are improper. After introducing our work of estimation of gas hydrate stability distribution in the northern South China Sea, we suggest that Wang et al. (2010) dismissed the basic P-T rule for the existence of gas hydrate. They should consider more the variables of water depth, seabed temperature and geothermal gradient in their gas hydrate distribution model in future studies. 相似文献
4.
针对永久散射体差分干涉测量(PSIn SAR)算法流程,发展了基于周期函数模型的空间维解缠方法,并将其应用于矿区时间序列地表变形反演。通过在研究区域内安装人工角反射器(CR),将CR点上计算所得的周期模型参数分量作为整个网络的约束,通过空间约束平差以实现空间维解缠。选取了河南省境内白沙水库附近的煤矿密集区为主要研究区域,采用周期函数模型对矿区线性及非线性形变分量进行模拟,反演了2007年2月—2010年2月的时间序列形变场,并采用研究区域内的水准实测数据作为外部验证数据。实验结果表明:白沙水库周围区域存在着较为明显的沉降,在煤矿分布区域内累积最大沉降量超过了10 cm。沉降区域内以线性沉降趋势为主,非线性沉降较为缓慢,仅在水库的西南方向较为明显。应用已有的水准点实测形变值对实验结果进行验证分析,结果表明该方法精度可达约±2.1 mm,证实了本文采用的方法在矿区地表时序形变反演中的可行性和可靠性,对预防过度采矿导致的矿区塌陷具重要现实意义。 相似文献
5.
Complementary to previous work mainly based on seismic interpretation, our compilation of geophysical data (multibeam bathymetry,
gravity, magnetic and seismic) acquired within the framework of the ZoNéCo (ongoing since 1993) and FAUST (1998–2001) programs
enables us to improve the knowledge of the New Caledonia Basin, Fairway Basin and Fairway Ridge, located within the Southwest
Pacific region. The structural synthesis map obtained from geophysical data interpretation allows definition of the deep structure,
nature and formation of the Fairway and New Caledonia Basins. Development of the Fairway Basin took place during the Late
Cretaceous (95–65 Ma) by continental stretching. This perched basin forms the western margin of the New Caledonia Basin. A
newly identified major SW–NE boundary fault zone separates northern NW–SE trending segments of the two basins from southern
N–S trending segments. This crustal-scale fault lineament, that we interpret to be related to Cretaceous-early Cainozoic Tasman
Sea spreading, separates the NW–SE thinned-continental and N–S oceanic segments of the New Caledonia Basin. We can thus propose
the following pattern for the formation of the study area. The end of continental stretching within the Fairway and West Caledonia
Basins (
65–62 Ma) is interpreted as contemporaneous with the onset of emplacement of oceanic crust within the New Caledonia Basin’s
central segment. Spreading occurred during the Paleocene (62–56 Ma), and isolated the Gondwanaland block to the west from
the Norfolk block to the east. Finally, our geophysical synthesis enables us to extend the structural Fairway Basin down to
the structural Taranaki Basin, with the structural New Caledonia Basin lying east of the Fairway Basin and ending further
north than previously thought, within the Reinga Basin northwest of New Zealand. 相似文献
6.
MEI Geng-jun XIANG Bin-bin WANG Na WANG Zhao-jun 《Chinese Astronomy and Astrophysics》2021,45(2):236-251
The pointing accuracy of a radio telescope is usually less than one-tenth of its antenna beam width. For large-aperture antennas at the short-centimeter band or millimeter-wave band, the pointing accuracy must be as high as several arc seconds. Therefore, for large-diameter and high-frequency reflector antennas, the pointing problem has become an important focal point to realize the antenna performance. Among many structural subsystem factors that affect the antenna pointing accuracy, there has been only less study on the factor of main reflector deformation. Based on the structural characteristics of the antenna, a reflector space coordinate system is established in this paper. And based on the space coordinates of the main reflector surface points after deformation, a non-linear least squares fitting method with 3 degrees of freedom is proposed to accurately predict the antenna pointing. Finally, the space geometric relationship is used to strictly derive the precise adjustments on the elevation and azimuth in order for correcting the antenna pointing error, and the indirect relationship between the main reflector deformation and the pointing error is constructed. This has certain guiding significance for improving the pointing accuracy of large radio antennas. 相似文献
7.
南海北部陆缘天然气水合物初探 总被引：89，自引：8，他引：89
姚伯初 《海洋地质与第四纪地质》1998,18(4):11-18
根据天然气水合物存在的温度－压力条件,研究了南海北部的地球物理资料,发现有些地方在地震剖面上出现的海底反射ＢＳＲ,而在另一些地方海底第一沉积的层速度偏高,比一般海洋沉积高０．２－０．６４ｋｍ／ｓ。将这些地方海底第一层沉积界面处的温度－压力参数投于甲烷形成天然气水合物的温度－压力图上,发现它们的出现于水合物存在之区域中。 相似文献
8.
A. Kawachi Y. Hayami J. Jimbo S. Kamei T. Kifune H. Kubo J. Kushida S. LeBohec K. Miyawaki M. Mori K. Nishijima J. R. Patterson R. Suzuki T. Tanimori S. Yanagita T. Yoshikoshi A. Yuki 《Astroparticle Physics》2001,14(4):1492-269
A new imaging atmospheric Cherenkov telescope with a light-weight reflector has been constructed. Light, robust, and durable mirror facets of containing carbon fiber reinforced plastic laminates were developed for the telescope. The reflector has a parabolic shape (f/1.1) with a 30 m2 surface area, which consists of 60 spherical mirror facets. The image size of each mirror facet is 0°.08 (FWHM) on average. The attitude of each facet can be adjusted by stepping motors. After the first in situ adjustment, a point image of about 0°.14 (FWHM) over 3° field of view was obtained. The effect of gravitational load on the optical system was confirmed to be negligible at the focal plane. The telescope has been in operation with an energy threshold for γ-rays of 300 GeV since May 1999. 相似文献
9.
Regional seismic reflection and potential field data document the South Atlantic's break-up history, between 39°S and 19°S, from the Early Cretaceous onwards. Previous maps of distribution of volcanics along the margin showed volcanics along the whole African margin based on extrapolation of data. Based on previously unpublished marine geophysical data, we found the southernmost 460 km long margin segment to be lacking huge volumes of break-up related volcanic effusives. Northwards, break-up was accompanied by the emplacement of huge volumes of volcanic material, prominently featured in seismic sections as huge wedge-shaped seaward dipping reflectors (SDRs). Detailed mapping of offsets (left- and right-stepping) and variations in structural character of the volcanics reveal the segmentation along and the break-up history of the margin. Several superimposed SDR sequences, suggesting episodicity of volcanic emplacement (divided by periods of erosion and sedimentation), are distinct along southerly lines, losing prominence northwards.A main outcome of our study is that this passive margin is not continuously of the volcanic type and that the change from a non-volcanic to a volcanic margin occurs abruptly.We define four distinct First-order Segments along the 2400 km section of the southwestern African margin covered by our seismic data. From south to north these First-order Segments are: Magma-poor Segment I; Segment II with enormous SDRs volumes; decreasing SDRs volumes in Segment III; Segment IV again with enormous volcanic output, likely influenced by Walvis Ridge volcanism.Most important is that there is no systematic increase in the volumes of the effusives towards the Tristan da Cunha hot-spot. Rather there is an alternating pattern in the SDRs' volumes and widths.The boundary between the volcanic and magma-poor margin segments in the southernmost study area is sharp (10s of km), which we propose is reflected in magnetic anomaly data as well. We suggest that this variability along the margin is mainly due to a change in stretching/rifting character from oblique during the early stages of breakup to conventional seafloor spreading from Chron M4 (∼130 Ma) onwards. 相似文献
10.
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