The ultraviolet sky: An overview from the GALEX surveys

The Galaxy Evolution Explorer (GALEX) has performed the first surveys of the sky in the ultraviolet (UV). Its legacy is an unprecedented database with more than 200 million source measurements in far-UV (FUV) and near-UV (NUV), as well as wide-field imaging of extended objects, filling an important gap in our view of the sky across the electromagnetic spectrum. The UV surveys offer unique sensitivity for identifying and studying selected classes of astrophysical objects, both stellar and extra-galactic. We examine the overall content and distribution of UV sources over the sky, and with magnitude and color. For this purpose, we have constructed final catalogs of UV sources with homogeneous quality, eliminating duplicate measurements of the same source. Such catalogs can facilitate a variety of investigations on UV-selected samples, as well as planning of observations with future missions. We describe the criteria used to build the catalogs, their coverage and completeness. We included observations in which both the far-UV and near-UV detectors were exposed; 28,707 fields from the All-Sky Imaging survey (AIS) cover a unique area of 22,080 square degrees (after we restrict the catalogues to the central 1° diameter of the field), with a typical depth of ∼20/21mag (FUV/NUV, in the AB mag system), and 3008 fields from the Medium-depth Imaging Survey (MIS) cover a total of 2251 square degrees at a depth of ∼22.7mag. The catalogs contain ∼71 and ∼16.6 million sources, respectively. The density of hot stars reflects the Galactic structure, and the number counts of both Galactic and extra-galactic sources are modulated by the Milky Way dust extinction, to which the UV data are very sensitive.     

火星地形测绘研究综述

火星地形测绘是开展火星科学研究的基础。介绍了与地形测绘相关的火星探测任务,并对地形测绘传感器进行了分析。阐述了火星地形测绘摄影测量数据处理的基本原理,研究了基于SPICE库建立火星表面线阵影像严密几何模型的方法。讨论了火星地形测绘摄影测量数据处理中的光束法平差、密集匹配以及多线阵拼接等关键技术。在总结现有火星地形测绘任务特点的基础上,针对我国开展火星地形测绘研究提出了建议。     

基于CELMS数据的月球东海微波辐射特性研究

根据月壤(FeO+TiO2)含量数据和"嫦娥2号"卫星CELMS数据,对月球东海地区微波辐射特性进行了研究。结果表明,在东海内部(FeO+TiO2)含量较高的地区,其正午和午夜时刻的亮温值都比较高,亮温差值也比较大,但亮温及亮温差值的分布随频率变化呈现不均匀性;Maunder撞击坑的(FeO+TiO2)含量较低,但其低频和高频亮温及亮温差值的表现正好相反;区域F(约10°S/106°W)、G(约5°S/104°W)和以(13°S/103°W)为中心的区域的微波辐射存在明显异常。这些区域的微波辐射特性对研究东海地区的形成演化过程具有重要意义。     

非线性回归支持向量机的SMO算法改进

为了解决非线性数据和非线性函数的回归问题,采用了支持向量机序列最小优化算法.原始序列最小优化（SMO,Sequential Minimal Optimization）算法存在训练速度慢和训练结果不稳定的缺点,为了能加快SMO算法的训练速度和提高训练结果稳定性,通过改进优化乘子更新方法、采用双阈值法、预存核函数、增加停机准则等方法对SMO算法做了改进.仿真实验表明,改进的算法能很好地对非线性数据和非线性函数进行回归,具有比原始SMO算法更快的训练速度和稳定的训练结果.      

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

Study of the ionosphere during a magnetospheric storm using data on the ground and in space

For the magnetospheric storm of May 14–16, 1997 geophysical data of satellites DMSP and IMP-8 are compared with data of radio propagation on the high-latitude HF radio path of Heiss Island – St. Petersburg and data from European ionosondes. Peculiarities of variations of the operational frequencies range MOF–LOF (maximum and lowest observed frequencies) on the path were considered. The range has been determined by the method of oblique ionospheric sounding (OIS). The latter is more informative for observations during a magnetic storm compared to the vertical sounding method. Nevertheless, an analysis of variations of the critical frequency of the ionospheric F2 layer from the chain of European ionosondes was carried out. For interpretation of results, data of magnetospheric parameters, AE-indexes and riometer data were used. The variations of both frequency range on the path and critical frequencies of the F2 layer through the ionosondes chain during the disturbed period had certain regularities of behaviour. These regularities are being explained from the physical point of view. The analysis of the satellite DMSP data has showed that a magnetospheric disturbance causes displacement equatorward of precipitation and some growth of its width and energy.     

开关磁阻电机非线性磁参数建模方法

建立了一种基于MATLAB/SIMULINK的非线性磁参数法的开关磁阻电机数学模型,在电磁场有限元(FEM)数值计算结果的基础上,解算出电机磁特性函数矩阵ψ(i,θ),把ψ(i,θ)函数矩阵三次样条插值变换成电机电流特性矩阵i(ψ,θ),再利用MATLAB/SIMULINK中的查表模块建立了开关磁阻电机系统的非线性模型。该模型中的电机本体模块、功率变换器模块、控制模块等都是通过SIMULINK中PSB通用功能模块搭建起来的,修改容易且直观性强,试验结果验证了该模型的准确性。     

测量数据部分丢失的非线性系统迭代学习控制

研究非线性离散系统的迭代学习控制．利用并行分配补偿方法(PDC)确定非线性系统的T-S模型,把非线性模型特换为局部线性模型。假定数据丢失的概率已知,采用满足Bernoulli分布的序列来描述测量数据的丢失,研究具有测量数据部分丢失的线性离散系统的迭代学习控制器的设计。结合T-S模型设计了数据丢失的迭代学习控制器,所设计的迭代学习控制器具有期望收敛特性和二次型性能指标。仿真结果表明了该设计方法的有效性。     

基于时间序列数据挖掘的旋转机械故障预报

提出一种基于时间序列数据挖掘的故障预报新方法。把故障前兆因子作为一种暂态,根据旋转机械轴承振动的实验数据建立时间序列．利用时延嵌入的方法重构状态空间,在状态空间中使用遗传算法搜寻最优暂态束．组成暂态集。用暂态集对旋转机械轴承振动的测试数据进行分析．判断是否为故障前兆因子．从而实现故障预报。     

基于数据库的柔性MIS系统初探

本文针对传统MIS系统的局限,介绍了柔性MIS系统的概念和定义,着重讨论了柔性MIS系统的总体结构和各组成模块的功能及设计要点。主要阐述了库文件结构的定义及自动维护的原理和方法。给出了通过功能模块语句中条件成分的表达及处理方法、相关性的描述方法、屏幕记录界面和格式报表的生成原理、字段的属性分类以及关键字段、公共字段、代码字段的描述及处理。还简要涉及了各模块间的信息传输。