用对合图件和密封带图件帮助分析油气储层内断层密封性

有一套新的图件能够帮助分析断层对合情况和密封作用。这套图件依据岩性和断层位移大小间的相互影响确定断层的对合和密封类型，其优点是无需作出地层面和断层面的详细三维图件即可评价断层封闭性，并可用于绘制断层带的渗透率、封闭性和传导能力值图件，用这些图件可以快捷地确定临界断层的断距和对合情况，这种对合需要作出相关的图件以确定油气储层内的不同区块。     

应力驱动的大陆碰撞作用：综合齿状构造作用和地幔俯冲构造作用

利用一种模式可能综合两种端员模式种类。这两种端员模式已经用于解释大陆碰撞期间地壳变形作用的模型，这种模式包括了来自侧翼的锯齿模式以及来自于下伏的俯冲层段的底部力作用。     

灾害的评估与管理

本文根据灾害威胁的范围不同,提出了自然灾害与技术灾害在不同的社会时期和不同性质的国家的分布与造成的影响不同的观点,进而从灾害研究的历史中分析自然灾害与技术灾害的内在联系以及人们对灾害研究的观念与方法的历史变革。在上述基础上,重点阐述了灾害评估的基本概念、灾害评估的内容和程序以及灾害管理的过程与方法。     

A High-Eccentricity Low-Mass Companion to HD 89744

We present deep Hubble Space Telescope (HST) imaging, as well as ground-based imaging and spectroscopy, of the optical afterglow associated with the long-duration gamma-ray burst GRB 990712 and its host galaxy. The data were obtained 48-123 days after the burst occurred. The magnitudes of the host (R=21.9, V=22.5) and optical afterglow (R=25.4, V=25.8, 47.7 days after the burst) favor a scenario in which the optical light follows a pure power-law decay with an index of alpha approximately -1.0. We find no evidence for a contribution from a supernova like SN 1998bw. This suggests that either there are multiple classes of long-duration gamma-ray bursts or that the peak luminosity of the supernova was more than 1.5 mag fainter than SN 1998bw. The HST images and EFOSC2 spectra indicate that the gamma-ray burst was located in a bright, extended feature (possibly a star-forming region) 1.4 kpc from the nucleus of a 0.2L*B galaxy at z=0.434, possibly a Seyfert 2 galaxy. The late-time afterglow and host galaxy of GRB 990712 bear some resemblance to those of GRB 970508.