流数据复杂聚类查询处理算法

流数据上的连续查询,尤其连续聚类查询是流数据处理研究的难点.草图算法能够计算流数据上等值连接大小的高精度近似值,而直方图算法能够较精确地统计流数据的分布.本文结合这两种算法的优势,提出了一种能够高效处理流数据上复杂聚类查询的算法.理论和实验结果表明,该算法具有较高的精度和较小的空间复杂度.     

新三态故障分类模型及其阈值确定

将设备运行状态划分为三种状态,比以往的两态模型对于设备的故障分类具有更高的准确性.在设备运行状态三态划分的基础上,提出了新的三态模型,将设备运行状态定义为故障态、准故障态、健康态三种状态,其中准故障态包括间歇性故障和瞬态故障.对新三态模型与两态马尔可夫模型进行了分析比较.论文提出影响故障阈值设定的多方面因素,对新三态模型的高、低阈值进行了定义和分析,给出了求取阈值的目标函数.利用新三态的双阈值目标函数,进行了仿真计算分析,得到了传统的两态模型所达不到的总故障高检出率和低虚警率,取得了满意的结果.     

自治式水下机器人推进器故障检测、分离与重构

研究自治式水下机器人推进器故障检测、分离与重构问题。针对水下机器人故障诊断残差法中残差阈值不易选取的问题,提出了一种基于观测器的水下机器人推进器故障检测与分离方法,通过构建故障检测观测器对推进器故障与残差信号进行解耦,使推进器出现故障后仅引起与其相关的残差呈单调变化,从而可选择较大的阈值进行故障检测以提高诊断系统的可靠性,该方法在故障检测的同时可进行故障分离。针对系统不确定性导致的推进器故障重构精度低的问题,提出了一种RBF神经网络与等效输出注入相结合的故障重构方法,采用等效输出注入方法估计不确定性项,从神经网络输出中重构推进器故障。     

A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements

With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements.     

天基强银河背景下的空间碎片探测试验及分析

本文设计并完成了银河背景下碎片探测试验,数据分析表明,强的银河背景会降低探测器对暗弱碎片的探测能力,但对碎片的天文定位精度影响不大。本文验证了采用基于探测概率的极限探测星等方法表征探测器极限探测能力的合理性,以及基于仿真的方法增加数据完备度的可行性。本文的工作将为后续天基探测器的设计及探测试验的开展提供依据。     

A Nominator-Selector Two-Stage Signal Detection Scheme

A two-stage approach to computationally efficient signal detection is to nominate candidate signal vectors using a suboptimal, but computationally cheap, detection scheme, and subsequently perform optimal detection on the candidates. Bounds on the detection performance of this approach are presented along with sufficient conditions for optimality. Examples are presented of an optimal and nearly optimal two-stage detection scheme where computational costs are drastically reduced relative to the singli-stage optimal detector.     

Self-similar solutions to stellar winds with cosmic rays

A two-fluid model is used to study the time evolution of stellar winds including the dynamical effect of cosmic rays. Neglecting the diffusion of cosmic rays, we seek self-similar solutions to spherically symmetric winds with a termination shock. The velocity upstream of the shock is taken to be zero. Physical solutions are those that can connect the shock to the star with the velocity approaching zero at the star. Two parameters govern the behaviour of the solutions, namely, the ratio of the upstream sound speed to the shock speed (in an inertial frame) and the gravitation potential of the central star. In some parameter regimes, no physical solution is possible.     

RN-FD型固体氡气源的稳定性及应用分析

对测氡仪器进行精确校准是氡测量工作中的重要环节,固体氡气源的稳定性、可靠性在校准中则显得至关重要。本文通过分析RN-FD型固体氡气源对闪烁室K值的稳定性实验结果,认为:RN-FD型固体氡气源标称的浓度值与实际浓度值不一致,标称浓度值只是理论浓度值而不是实际浓度值,需重新刻度才能使用;RN-FD型固体氡气源抽气循环时间不同则浓度不同,但抽气循环时间固定,观测结果比较稳定;对于没有α检查源的台站,RN-FD型固体氡气源可用于氡观测仪器坪区检查。     

基于Web技术的产品数据管理研究

将Web技术引入产品数据管理系统(PDM)的研究和设计,分析了PDM系统中原有构架的特点与存在的不足,利用Web技术所提供独到的网络、数据库和分布式处理技术,结合开发实例提出了在Internet/Intranet解决方案下开发和研究产品数据管理系统的基本构想,并给出产品数据管理应用的组织和底层数据模式,研究了其对产品数据管理技术应用前景的影响.研究表明,Web技术的引入,将有力地推进产品数据管理技术的发展和应用.