基于Gibbs-Markov随机场与连通聚类的SAR图像恢复

在传统的马尔可夫随机场(MRF)的图像建模方法基础上利用合成孔径雷达(SAR)图像的固有特性对Gibbs-MRF模型进行改进复原SAR图像,并进一步提出用数字形态学中连通性理论进行图像分割。在SAR图像像素空间的邻域内,估计最大后验概率(MAP)时引用Gamma分布代替传统的瑞利分布恢复数据,同时利用像素强度值相关性的连通模型将目标较好地提取出来。充分利用了SAR图像的数字形态信息和像素强度之间的相关性,得到了更好的分割效果。仿真实验说明本文方法是有效的。     

原子氧对红外干扰材料消光性能的影响研究

为探索大气中的红外干扰材料可否应用于外层空间, 利用原子氧效应地面模拟装置对铜粉和石墨粉两种红外干扰材料样品进行了原子氧暴露实验, 并对样品进行了质量分析、XRD分析和红外透过率测试. 结果表明, 原子氧累积通量达到5.0×1019cm-2时, 铜粉样品质量增加0.004mg•cm-2,石墨粉样品质量损失0.117mg•cm-2; 原子氧暴露后, 铜粉对3~5μm与8~12μm红外质量消光系数由3.64 m2•g-1与2.74 m2•g-1变为3.14 m2•g-1与2.65 m2•g-1, 消光能力降低; 石墨粉对3~5μm和8~12μm红外的质量消光系数由6.54 m2•g-1和5.78 m2•g-1减小为2.38 m2•g-1和2.27 m2•g-1, 消光能力明显减弱.      

Particle acceleration and gamma rays in solar flares: Recent observations and new modeling

Experiments on SMM, GAMMA, Yohkoh, GRANAT, Compton GRO, INTEGRAL, RHESSI and CORONAS-F satellites over the past three decades have provided copious data for fundamental research relating to particle acceleration, transport and energetics of flares and to the ambient abundance of the solar corona, chromosphere and photosphere. We summarize main results of solar gamma-astronomy (including some results of several joint Russian–Chinese projects) and try to appraise critically a real contribution of those results into modern understanding of solar flares, particle acceleration at the Sun and some properties of the solar atmosphere. Recent findings based on the RHESSI, INTEGRAL and CORONAS-F measurements (source locations, spectrum peculiarities, ³He abundance etc.) are especially discussed. Some unusual features of extreme solar events (e.g., 28 October 2003 and 20 January 2005) have been found in gamma-ray production and generation of relativistic particles (solar cosmic rays, or SCR). A number of different plausible assumptions are considered concerning the details of underlying physical processes during large flares: (1) existence of a steeper distribution of surrounding medium density as compared to a standard astrophysical model (HSRA) for the solar atmosphere; (2) enhanced content of the ³He isotope; (3) formation of magnetic trap with specific properties; (4) prevailing non-uniform (e.g., fan-like) velocity (angular) distributions of secondary neutrons, etc. It is emphasized that real progress in this field may be achieved only by combination of gamma-ray data in different energy ranges with multi-wave and energetic particle observations during the same event. We especially note several promising lines for the further studies: (1) resonant acceleration of the ³He ions in the corona; (2) timing of the flare evolution by gamma-ray fluxes in energy range above 90 MeV; (3) separation of gamma-ray fluxes from different sources at/near the Sun (e.g., different acceleration sources/episodes during the same flare, contribution of energetic particles accelerated by the CME-driven shocks etc.); (4) asymmetric magnetic geometry and new magnetic topology models of the near-limb flares; (5) modeling of self-consistent time scenario of the event.     

Lifetime prediction based on Gamma processes from accelerated degradation data

Accelerated degradation test is a useful approach to predict the product lifetime at the normal use stress level, especially for highly reliable products. Two kinds of the lifetime prediction based on Gamma processes were studied. One was to predict the lifetime of the population from accelerated degradation data, and the other was to predict the lifetime of an individual by taking the accelerated degradation data as prior information. For an extensive application, the Gamma process with a time transformation and random effects was considered. A novel contribution is that a deducing method for determining the relationships between the shape and scale parameters of Gamma processes and accelerated stresses was presented. When predicting the lifetime of an individual, Bayesian inference methods were adopted to improve the prediction accuracy, in which the conjugate prior distribution and the non-conjugate prior distribution of random parameters were studied. The conjugate prior distribution only considers the random effect of the scale parameter while the non-conjugate prior distribution considers the random effects of both the scale and shape parameter. The application and usefulness of the proposed method was demonstrated by the accelerated degradation data of carbon-film resistors.     

时延-角度特性研究

本文在球不对称局域准抛物电离层模型下,设计了一套射线追踪算法的计算机程序。研究了时延随角度变化特性。指出了最小时延的传统求解方法的适应范围,讨论了时延-角度特性曲线与返回散射电离图的关系及其能量分布特点。      

Radio-faint BL Lac objects and their impact on the radio/gamma-ray connection

Radio and gamma-ray emissions in Active Galactic Nuclei (AGNs) are both related to the presence of relativistic particles in jets. With the advent of the Fermi Large Area Telescope (LAT), and thanks to its large sensitivity up to several GeV, many observational results are changing our understanding of these phenomena. BL Lac objects, which made up only a fraction of the known extragalactic gamma-ray source population before Fermi, have now become the most abundant class. However, since they are relatively weak radio sources, most of them are poorly known as far as their parsec scale structure and multi-wavelength properties are concerned. For this reason, we have selected a complete sample of 42 low redshift BL Lacs (independently of their gamma-ray properties) to study with a multi-wavelength (radio, optical, X-ray, gamma-ray) approach. Here, we present results and images of sources in the sample (most of which have never been observed before), using new VLBA observations at 8 and 15 GHz. Beyond this sample of BL Lacs, the population of gamma-ray AGNs has also dramatically enlarged in the Fermi era, permitting us to discuss the presence of a correlation between radio and gamma-ray properties with improved statistical significance. We explore the radio-gamma relation with several hundreds sources and using both simultaneous and archival radio data, thus tackling the impact of time variability.     

基于 Gamma模型和加速退化数据的可靠性分析方法

为了对导弹连接器进行可靠性评估,提出了基于Gamma模型的可靠性分析方法。首先,以电连接器的接触电阻作为性能参量,通过温度、湿度双应力加速退化试验获取其性能退化数据;然后,利用Gamma模型描述样品的退化过程,使用广义艾林模型,描述了样品退化量与温度、湿度之间的关系;最后,使用极大似然估计的方法,估计出了样品在正常工作条件下的模型参数,并对该型电连接器的平均寿命进行了预测。     

电离层短波射线追踪

本文以电离层等离子体参量的平均背景模式计算为基础, 给出一种电离层短波射线轨迹计算方法。供短波通信系统、工作于短波段的其它系统(如HF雷达的目标定位系统)及有关研究工作使用参考。      

耗散大气中风场对内重力波传播的影响

使用考虑大气耗散的射线跟踪算法,计算了风场作用下重力波的传播情况.结果表明,风场对快速重力波分量影响较小,但对反射和传播区域的慢速波的影响较大,表现在顺风时使反射区范围缩小,逆风时使反射区范围扩大.在传播区,顺风场使慢速波分量的传播距离变小,传播高度降低,而逆风则使慢速重力波分量的传播距离明显增大,传播高度上升.分析表明,重力波传播的丰富多样性是由风场对波的衰减和反射等滤波作用引起的.      

基于混合Gamma分布的通用可靠性寿命数据拟合方法

 可靠性寿命数据分析是可靠性工程研究的重要基础。目前对于可靠性寿命数据分析的研究存在两个主要问题:一是凭经验选择的概率分布严重依赖于人的主观判断,不能保证所选分布的适用性;二是常用分布拟合能力有限,在很多情况下不能满足寿命数据处理的需要。针对这两个问题,在混合Gamma分布稠密性的基础上,提出了一种通用的可靠性寿命数据拟合方法,给出了基于期望极大化(EM)算法的混合Gamma分布的参数估计方法,并通过6个拟合实例验证了该方法的有效性。最后,结合WP-7乙型航空发动机I级导叶片故障数据分析问题,开展了应用研究,并且与目前常用的方法进行了对比。