南海东南部陆缘地壳结构特征及其构造意义

南海东南部海域沉积厚度较大,礁体发育,构造演化复杂,导致深部结构探测不清楚,制约了对南部陆缘地壳结构的认识.本文通过对新采集和重新处理的多道地震剖面解释,结合钻井、拖网资料,对浅部地层和构造进行约束,同时利用附近海底地震(OBS)测线的速度结构,对深部结构和界面解释约束;在此基础上,开展了重震联合反演,分析地壳密度空间分布特征,结合重力梯度特征对构造单元进行识别.通过对东西两条测线的上下和全地壳厚度、拉伸因子比较,发现南海东南部的东西部深部结构存在差异性;礼乐断裂可能是礼乐和郑和地块的分界,并控制了两个地块在南海扩张时期的相对运动.     

南海西南次海盆岩石圈结构及其地质意义

南海地区岩石圈资料稀少,阻碍了其形成演化过程的研究.为此,本次研究结合大地热流、空间重力异常、高程、大地水准面和地震数据,在南海西南次海盆反演了两条2.5维岩石圈剖面.本次计算基于三种假设：岩石圈地幔的密度取决于岩石温度;研究区岩石圈处于热稳定状态;研究区处于重力均衡状态.在剖面A-E中,岩石圈底界面从珠江口盆地的105 km迅速抬升到西沙海槽处的50 km,在西沙海槽、西沙-中沙群岛和西南次海盆变化不大,为50~60 km.在剖面F-I中,岩石圈底界面从西沙群岛-中建地块处的88 km向海盆逐渐抬升,在西南次海盆处为46~50 km,到郑和隆起再逐渐变深至64 km.我们比较了西南次海盆岩石圈的冷却模型和热稳定模型,根据冷却模型由水深和热流数据所推断的西南次海盆年龄比实际年龄差很多,说明冷却模型不适用于西南次海盆.通过对比剖面A-E和剖面F-I,说明了剖面A-E经历了更长时间的拉伸,证明南海西南次海盆在形成演化过程中是从北东向南西逐步打开的渐进式扩张.最后,我们综合分析西南次海盆及其大陆边缘的岩石圈结构、减薄陆壳区范围、碳酸盐台地的分布、下地壳韧性流动、流变结构和沉积层特征等多方面资料,认为西南次海盆在形成演化过程中岩石圈地幔首先破裂而地壳后破裂,属于type Ⅱ型非火山型大陆边缘.     

A response spectrum approach for seismic performance evaluation of actively controlled structures

To evaluate and measure the effectiveness of active control schemes in reducing the response of structures subjected to earthquake excitations, it is common to use recorded or artificially generated earthquakes as input motions. This paper introduces the response spectrum analysis to evaluate linear control systems for seismic inputs defined by code‐prescribed or site‐specific ground response spectra. Using such a method one can evaluate a control system in a single analysis for the ensemble of time histories that are represented by the input response spectra. The response spectrum analysis can also facilitate the implementation of comprehensive parametric studies. A generalized response spectrum method is used to analyse systems with non‐symmetrical matrices that are caused by the general nature of the control actions imposed on the structure. The application of the method is demonstrated on several numerical examples of a building structure where the control force is applied through an active tuned‐mass damper. Copyright © 2000 John Wiley & Sons, Ltd.     

Modeling of an actively braced full‐scale building considering control–structure interaction

Recently, the application of active control to seismic‐excited buildings has attracted international attention. To demonstrate the practical applicability of active control, we have conducted experimental tests using a full‐scale three‐storey building equipped with active bracing systems on the shake table at the National Center for Research on Earthquake Engineering (NCREE), Taiwan. Experimental results indicate that the control–structure interaction (CSI) effect is significant. A state‐space analytical model of this actively controlled building taking into account the CSI effect is established in this paper using a system identification technique based on curve‐fitting of transfer functions. To verify the accuracy of the analytical model for simulating the controlled response, four sets of linear quadratic Gaussian (LQG) controllers using acceleration feedback are designed and further experimental tests are conducted for comparison. It is demonstrated that the correlations between the simulation and experimental results are remarkable. The construction of an accurate analytical model is important for active control, and such an analytical model can be used for future benchmark studies of different control algorithms based on numerical simulations. Copyright © 2000 John Wiley & Sons, Ltd.     

Sliding mode fuzzy control: Theory and verification on a benchmark structure

A sliding mode fuzzy control (SMFC) algorithm is presented for vibration reduction of large structures. The rule base of the fuzzy inference engine is constructed based on the sliding mode control, which is one of the non‐linear control algorithms. In general, fuzziness of the controller makes the control system robust against the uncertainties in the system parameters and the input excitation, and the non‐linearity of the control rule makes the controller more effective than linear controllers. For verification of the present algorithm, a numerical study is carried out on the benchmark problem initiated by the ASCE Committee on Structural Control. To achieve a high level of realism, various aspects are considered such as actuator–structure interaction, sensor noise, actuator time delay, precision of the A/D and D/A converters, magnitude of control force, and order of control model. Performance of the SMFC is examined in comparison with those of other control algorithms such as H_{mixed 2/∞}, optimal polynomial control, neural networks control, and SMC, which were reported by other researchers. The results indicate that the present SMFC is efficient and attractive, since the vibration responses of the structure can be reduced very effectively and the design procedure is simple and convenient. Copyright © 2000 John Wiley & Sons, Ltd.     

Galaxy activity and interaction: the optical view

The relevance of interaction to the presence of Seyfert or starburst activity in the nuclei of galaxies is examined. We focus the attention on the close environments of spectroscopically selected samples of Seyfert-1, Seyfert-2 and starburst galaxies. In particular the results of a statistical procedure aimed at finding physical pairs are tested with redshift measurements of the identified pairs. Seyfert and starburts galaxies show an excess of physical companions compared to normal galaxies. This excess tends to increase as one moves from Seyfert to starburst galaxies.     

Narrow-line Seyfert 1 galaxies

This paper summarizes the soft X-ray properties of narrow-line Seyfert 1 galaxies (NLS1). NLS1 have generally steeper soft X-ray continuum slopes than Seyfert 1s with broader lines, and there exists an anticorrelation between 0.1–2.4 keV continuum slope and the FWHM of the Hβ line. Objects with steep 0.1–2.4 keV continuum slopes and Hβ FWHM > 3000 km s⁻¹ are clearly discriminated against by nature. When simple power-law models are fit to the data, photon indices reach values up to about 5, much higher than is usually seen in Seyfert 1s. Models with smaller mass black holes and/or higher Eddington fractions show some promise to explain the relation between the FWHM of the Hβ line and the X-ray continuum slope. We further report evidence for persistent gaint and rapid variability in the ultrasoft narrow-line Seyfert 1 galaxy IRAS 13224–3809. We have examined possible explanations for the gaint variability. Unusually strong relativistic effects provide a plausible explanation of the X-ray data. Relativistic boosting effects may be relevant to understanding the strong X-ray variability of some steep spectrum Seyferts more generally.     

Ultrasoft narrow-line Seyfert 1 galaxies and X-ray surveys

Note from the editor: This article is a re-print of the original, which appeared in Astron. Nachr. 319 (1/2), 7 (1998). In the original version the figure was ruined in the process of paper production and the scientific content of the paper considerably degraded. Instead of printing only the correct figure, thus loosing the scientific context, we decided to re-print the whole article. We describe how recent X-ray surveys have led to advances in the understanding of ultrasoft narrow-line Seyfert 1 galaxies. The number of known ultrasoft narrow-line Seyfert 1s has increased greatly in recent years due to X-ray surveys, and it is now possible to obtian high quality 0.1–10 keV spectral and variability measurements for a large number of these galaxies. We generalize some of the correlations between X-ray properties and optical emission line properties,focusing on how the ROSAT band spectral slope appears to be directly connected to the Boroson & Green (1992) primary eigenvector. We discuss how ultrasoft narrow-line Seyfert 1s may well have extremal values of a primary physical parameter, and we describe new projects that should further improve our understanding of these extreme representatives of Seyfert activity.     

面向服务架构下主动地理信息服务模型研究

通过引入服务的主动发现、定制、加载与使用机制,支持新服务、新应用的按需创建,为用户发现、定制和运行能够满足用户需求的服务,从而改变当前用户只能被动地使用现有服务的应用模式,以应对信息化需求的不断发展和变化。主动型的地理信息服务在Web服务框架模型、基础协议的基础之上,增加识别用户需求和处理的能力,使用户能够根据特定需要选择合适的服务,使服务能够自动适应用户的需求。本文讨论了面向服务架构下的主动地理信息服务模型,该模型以Web服务技术为支撑,以扩展的UDDI等协议为规范,并对该模型进行测试,实验证明该模型可以有效地主动式的地理信息服务。