用于GNSS的SpT星载原子钟及时间系统介绍

研究了空间铷钟和被动型氢钟的地面批量和寿命试验测试结果,以及卫星在轨试验所达到的最新性能结果。基于这些星载钟的试验结果,对全球卫星导航系统的地面时间站的关键设备及其相关算法作了简要描述,并介绍了一种新颖的在轨技术,即从星载原子钟组（ONCLE）直接产生高度稳健的时间频率信号。     

广域差分的全矢量法

针对广域差分改正矢量的组成元素集之一的电离层模型参数集,分别用Klobuchar模型和Georgiadou模型进行了分析和比较,详细推演了广域差分改正矢量估计的全矢量法.在统一的数学模型中给出了统一解算卫星星历误差、卫星钟差和广域差分基准站时钟误差的计算公式;对理想状态下的模型参数、基准站和跟踪的卫星的数量关系进行了探讨.     

基于GPS的人工地震测深零时仪研制

在人工地震测深野外数据观测系统中,通过人工爆破激发地震波,利用布设在测线观测点位上的地震仪采集来自地壳上地幔的地震波震相信息来进行地震成像,获得研究区地壳上地幔精细结构、深浅部构造关系和发震构造的空间展布特征,进而研究岩石圈演化和动力学过程。为进行后期地震波资料信息的精确处理,需获得人工爆破地震波激发时刻的高精度时间和地理坐标信息。设计一种基于AT89C5115微处理器的GPS同步零时仪装置,介绍其硬件结构设计和固件程序实现方法,授时精度达微秒级,具有人机交互控制和信息数据通信功能。经室内测试和野外实验,零时仪装置运行稳定可靠,能完全满足野外测深工作的需要。     

汶川Mw7.9地震余震序列触发机制研究

余震触发机制的Dieterich解析模型被广泛应用于区域地震活动性的定量分析以及依赖时间的概率地震预测模型的建立等方面.基于滑移速率和状态相依赖的摩擦定律和弹簧-滑块模型,从Dieterich断层滑移速率方程出发,给出了静态应力扰动下触发地震的时钟提前或推后的近似解,从而明确地阐明了触发地震的产生机制与断层的演化过程密切相关,并与传统位错模型下库仑应力扰动时间提前或推后量作了比较.采用对数线性拟合方法求得了汶川Mw7.9主震后余震序列持续时间,符合Dieterich理论结果.以汶川余震序列为例,给出了两种不同的应力扰动模式在该余震序列中的应用.结果表明,经典Dieterich扰动解无法给出主震发生后即时余震数量的异常增加,而考虑主震前后剪应力速率变化的Dieterich分段解则可反映出余震发生率及个数随时间的演化特征.     

海底大地电磁数据采集器高精度应急时钟源的设计

为了实现海底大地电磁探测的远参考道测量,各台仪器需同步采集数据,为此,设计了1个具有微秒级误差的高精度应急时钟源.该时钟源的设计采用单片机(MCU)为主控单元,应用了串行通讯、I2C等技术手段.文中概要介绍了其硬件组成和软件程序的设计.     

考虑双向碰撞效应的连续斜交桥地震响应研究

为研究双向碰撞效应对连续斜交桥地震响应的影响,采用Kelvin-Voigt模型模拟桥台伸缩缝处的纵向碰撞现象,采用简化滞回模型模拟挡块与主梁的横向碰撞过程,针对某三跨连续斜交桥进行参数对比研究。研究表明,双向碰撞对主梁横向位移的影响远比纵向位移大,其中桥台间隙对主梁平面转角的影响最大,且平面转角随桥台间隙的增大而减小;横向碰撞对墩柱曲率变形的影响远比纵向碰撞大,其中挡块强度的影响特别大,当挡块强度由0%增至50%时,墩柱纵、横向曲率均值分别增大13.43倍、7.21倍。随着斜交角的增大,梁端纵向位移不断增大,横向位移和平面转角则先增后减;墩底纵向曲率不断增大,横向曲率经历先增后减\,再增的过程;纵向碰撞效应先减弱后增强,而横向碰撞效应则先增强后减弱。由于横向碰撞对墩柱的影响远大于纵向碰撞,因此在斜交角为15°～45°时,宜设法降低横向碰撞效应。     

强震作用下桥台对斜交连续梁桥抗震性能的影响研究

为研究强地震作用下,桥台及台后土体对斜交连续梁桥抗震作用的影响。以一座三跨连续斜交箱梁桥为依托,应用sap2000建立不同斜度的模型,针对有、无桥台两种工况,采用非线性时程分析方法,研究了纵向不同地震动强度输入下,桥台及台后土体作用对不同斜度的连续梁桥主梁和桥墩位移的影响规律,并对桥墩的延性性能进行分析。研究结果表明:桥台及台后土体的存在会抑制主梁的纵向位移,大大增加主梁梁端的横向位移,地震动幅值越大,这种作用越明显;桥台及台后土体作用会减小墩顶纵向位移和墩底纵向弯矩,降低桥墩纵向位移延性需求,提高桥墩纵向安全性,斜交角越大,该影响效果越小;桥台作用对桥墩的横向反应几乎无影响。建议在桥梁抗震设计时应考虑桥台以及台后土体的作用,并针对不同斜度的连续梁桥采取相应的抗震措施,以提高其抗震性能。     

TJ—90调速晶控钟

T—90调速晶控是比JK—79型晶控钟推功器及87型晶控推动钟更为完美的记录器动力源,它既保持了原晶控推动动力晶体稳速的特点又具备能在大范围内任意调速的功能,使得地震记录图纸时分号角度线能简便地满足台站记录规范的要求,它可以替代JK—79型及87型晶控钟,又可改进DD—1、DK—1及传输台网多笔记录器的动力源。     

The use of grain‐size distribution patterns to elucidate aeolian processes on a transverse dune of Thar Desert,India

The grain‐size distribution of aeolian dune sands in the Thar Desert, India was analyzed and compared with three model distributions – log‐normal, log‐hyberbolic and log‐skew‐Laplace – to determine the best‐fit statistical model. In total, 51 samples were collected along a single transect over a transverse dune, of which 15 were from the stoss side, 12 from the crest and 24 from the lee side. Samples were collected during a calm period in the afternoon of a winter's day. It was observed that of these 51 samples, 33 fit best to a log‐hyperbolic distribution, 14 fit best to a normal distribution and only four fit best to a Laplace distribution. However, it was further observed that of 24 samples from the lee side, 13 fit best to a normal distribution, eight fit best to a hyperbolic distribution, and three fit best to a Laplace distribution. Of 12 samples from the crest of the dune, 11 fit best to the log‐hyperbolic distribution, only one to the Laplace distribution but none to a normal distribution. Of 15 samples from the stoss side of the dune, only one sample best‐fits a normal distribution, 14 fit best to a log‐hyperbolic distribution, and none best fit to a Laplace distribution. During sample collection a calm period prevailed and there was no dusty wind. It was therefore assumed that in the initial stage a mixture of coarse, medium and fine sands was laid down on the stoss side of the dune. As wind speeds increased and saltation started, the coarser fractions were segregated and lagged behind on the stoss slope. In the final stage when the remaining intermediate and finer fractions reached the dune crest, the finer fractions were winnowed away to suspension from the crest of the dune. As a result, a narrow range of intermediate sized sediments was deposited by rolling down the lee side to explain the development of log‐normality. In such a situation, both the coarser and finer fractions, to which the skewed distributions can be attributed, are separated from the initial mixture of coarse, intermediate and fine fractions. Hence the main criteria for the development of a normal distribution is the lack of skewed fractions and the concentration of the narrow, intermediate size fractions in the final grain size distribution. This is also corroborated with the index of symmetry, which is a measure of the difference between the angle of two slopes of the hyperbolic distribution as represented by the coarser and finer fractions. Copyright © 2010 John Wiley & Sons, Ltd.     

Assessing the Clock of Gaia: Design and Implementation of A Clock Framework Simulator

A powerful and highly configurable simulator of generic clock frameworks is presented and evaluated. This software tool was initially designed to test the reliability of clock data for the Gaia space mission. However, our application has been developed as much parameterized as possible in order to easily adapt it to any other space mission. The main goals of our software tool are to simulate the real performance of an atomic master clock, including the typical noises present in this kind of devices, and to check the reliability of the generation and distribution of clock sub-products. The latter, which are generated by other devices such as frequency multipliers and dividers, are also implemented in the simulator, as well as the corresponding transmission lines. In our simulator the clock outputs obtained from the several nodes of the framework can be displayed with the appropriate graphical tools, therefore easing the task of validating several design issues. Also, the parameters of the master clock and of all the framework devices, as well as the whole clock framework structure are entered using XML files, which can also be graphically verified. Finally, the accuracy and stability of the atomic clock which is expected to fly on-board of Gaia is assessed. We also discuss in depth the several issues regarding the time data products that Gaia will require and we characterize the most important elements.