基于三差解检测与修复GPS载波相位周跳新方法

对飞行中初始化载波相位整周模糊度ＧＰＳ的动态差分定位而言,如果在整周模糊度初始化过程中发生载波相位周跳,将严重影响整周模糊度的确定,本文对已有的ＧＰＳ静态差分定位中通过三差解检测与修复周跳的方法进行了推广,提出了一种适合于解决Ｏｎ－Ｔｈｅ－Ｆｌｙ整周模糊度初始化过程中周跳问题的新方法。新方法保持了静态情况下原有方法的特点,分析和利用实采数据进行的检验表明,新方法是有效和实用的。     

湘赣边区NNE向走滑断裂-流体-铀成矿动力学分析

以湘赣边区ＮＮＥ向走滑断裂系统构造解析及其演化和动力学分析为主线,结合含矿流体的运动学过程研究,进行热液铀成矿动力学分析,以探讨成矿作用的动力来源、作用机制和演化过程。     

1976年唐山地震发震断裂的活动性研究

震后野外考察及航空摄影发现的地裂缝带,说明唐山断裂与１９７６年唐山７．８级大地震的发震构造有密切关系。用卫星遥感信息和浅层地震勘探结果对唐山断裂的活动性做了新的研究。卫星图像解释结果表明：震前一年多时间内,ＮＥ向的唐山断裂被ＮＮＷ向断裂截切而ＮＷＷ向断裂受到牵引,因而显示出右旋走滑的活动形迹。浅层地震勘探结果则证明,唐山断裂是倾向ＮＷ,高倾角的右旋走滑正断层,它断错了全新统（Ｑ４）、晚更新统（Ｑ３）、中更新统（Ｑ２）和早更新统（Ｑ１）地层     

走滑断裂带中挤压阶区内部剪切构造初探

野外地质调查和航片立体镜下解译发现,小江断裂带北段蒙姑和东支大营盘两个挤压阶区内部发育有剪切构造,它们在地表主要表现为断裂槽地、断层陡坎、地裂缝等。挤压阶区内部剪切构造和拉张阶区内部剪切构造一样,是阶区形成后,随着走滑断裂的进一步活动而形成的新生性构造     

走滑拉分断块对沉积的控制作用——准噶尔盆地东部侏罗系中下统沉积主控因素新认识

通过在南缘露头剖面相构型识别,北部地震剖面解释的沉积体侧向迁移特征,建立了走滑拉分构筑的可容空间变化型式。此沉积对构造的响应模式,不仅可以很好的解释拼合砂体的分布,古流向偏转等问题,而且对于预测盆内沉积体走向也是一个很有用的工具。     

Diffuse interstellar bands in low E (B – V) objects

We analyse spectra of slightly reddened, early-type stars in which the major diffuse interstellar bands at 5870 and 5797 Å are either strong or weak in relation to E(B – V) . It is demonstrated that among the low E(B – V) objects one can find stars obscured by 'sigma' as well as 'zeta' type clouds. The profiles of the diffuse bands seem not to be dependent on the total opacities of the interstellar clouds. We also discuss the physical conditions leading to the formation of the diffuse band carriers in low-opacity interstellar clouds; the carriers are apparently formed in media in which one can observe complex velocity fields.     

B0712+472: a new radio four-image gravitational lens

A new four-image gravitational lens system, B0712+472, has been discovered during the Cosmic Lens All-Sky Survey. This system consists of four flat-spectrum radio images that are also seen on a Hubble Space Telescope ( HST ) image, together with the lensing galaxy. We present MERLIN, VLA and VLBA maps and WHT spectra of the system as well as the HST images. The light distribution of the lensing galaxy is highly elongated and so too is the mass distribution deduced from modelling. We suggest a redshift of ∼1.33 for the lensed object; the lens redshift will require further investigation. The discovery of this new system further increases the ratio of four-image to two-image lens systems currently known, exacerbating problems of required ellipticity of matter distributions in lensing galaxies.     

Microlensing of broad absorption line quasars

The physical nature of the material responsible for the high-velocity broad absorption line (BAL) features seen in a small fraction of quasar spectra has been the subject of debate since their discovery. This has been especially compounded by the lack of observational probes of the absorbing region. In this paper we examine the role of 'microlenses' in external galaxies in the observed variability in the profiles of BALs in multiply imaged quasars. Utilizing realistic models for both the BAL region and the action of an ensemble of microlensing masses, we demonstrate that stars at cosmological distances can provide an important probe of the physical state and structure of material at the heart of these complex systems. Applying these results to the macrolensed BAL quasar system H1413+117, the observed spectral variations are readily reproduced, but without the fine-tuning requirements of earlier studies which employ more simplistic models.