基于小波包分解和FCM聚类的纹理图像分割方法

提出了一种新的图像特征提取中选取最优小波分解树的方法.塔式小波分解对信号解不够全面,而小波包全分解又引入庞大的计算量,因此小波分解最优树的选取尤为重要.结合模糊c均值(FCM,Fuzzy C-Mean)聚类,提出了一种能同时进行小波自适应分解和纹理特征分类的纹理图像分割方法,该方法将无监督聚类中的聚类有效性参数引入到自适应小波分解的判决中,能根据无监督聚类分割的需要,自适应地选取小波包分解的树形结构和分解层数.相对于小波包全分解,节省了大量的运算,并能取得良好的分割效果.      

基于支撑域的单分类器和密度估计的本质关系

单类支持向量机和支持向量数据描述是两种流行的基于支撑域的单分类器。为揭示采用高斯核后他们与密度估计之间的关系,首先将基于支撑域的单分类器统一到密度估计的框架下;其次证明了基于支撑域的单分类器诱导的密度估计和真实密度一致,同时也能减小积分平方误差。最后通过人工数据集实验验证了上述关系。     

飞机结构的随机振动疲劳分析方法

飞机使用中经常会遇到因为结构振动而产生的疲劳破坏现象。飞机结构的振动疲劳分析是进行飞机结构动力学设计的重要设计分析手段。本文通过对国内外几十年来形成的主要的振动疲劳分析方法进行了归纳整理,为飞机设计和维修提供振动疲劳的设计与分析技术支持。     

一种基于随机集的模糊观测的多目标跟踪算法

为解决目标数未知或随时间变化时模糊观测的多目标跟踪问题,将多目标状态和模糊 观测数据表示为随机集形式,利用模糊观测的似然函数融合模糊数据,建立了模糊观测的概 率假设密度(probability hypothesis density,PHD)粒子滤波方法。这种方法首先利用 粒子滤波预测和更新随机集的PHD,然后估计目标数N,最后找出N个PHD最大的点就 是多目标的状态估计。在相同的仿真环境中,用这种方法与用重心去模糊器进行去模糊处理 后的观测数据同时跟踪目标数变化情况下的多目标,并进行了比较,结果表明,模糊观测多 目标跟踪的PHD粒子滤波能稳健跟踪目标数未知或随时间变化时的目标状态和目标数,性能 好于去模糊情况。     

Bioinspired polarized light compass in moonlit sky for heading determination based on probability density estimation

Bioinspired polarized skylight navigation, which can be used in unfamiliar territories, is an important alternative autonomous navigation technique in the absence of Global Navigation Satellite System(GNSS). However, the polarization pattern in night environment with noise effects and model uncertainties is a less explored area. Although several decades have passed since the first publication about the polarization of the moonlit night sky, the usefulness of nocturnal polarization navigation is ...     

基于隶属度和LMK-ELM的航空电子部件诊断方法

为提高航空电子部件模块级故障诊断精度，提出一种新的面向"软聚类"的局部多核学习（LMKL）-超限学习机（ELM）离线诊断方法。通过引入模糊C均值聚类对样本空间进行模糊划分，挖掘聚类内部多样性的同时，实现了对过学习的抑制；将模糊划分产生的隶属度信息融入LMKL-ELM的优化过程，运用基于初始-对偶混合优化问题的三步优化策略克服了局部核权重二次非凸的问题，在l₁-范数与l₂-范数约束下分别给出了相应的更新方法。将所提方法应用于某型机前端接收机，结果表明：与4种流行的多核诊断方法相比，该方法可有效避免漏警、抑制虚警，在l₁-范数和l₂-范数约束下，其诊断精度比其他方法的平均值分别提升了4.09%和5.13%。     

Ionospheric parameters in the European sector during the magnetic storm of August 25–26, 2018

Variations of ionospheric parameters Total Electron Content (TEC) by GNSS, critical frequency (foF2) by vertical sounding and electron density (Ne) by low-altitude satellite were studied at high, mid and low latitudes of the European sector during the magnetic storm of August 25–26, 2018. During the main phase of the storm the ionospheric F2-layer was under the positive disturbance at mid and low latitudes. Then the transition from the positive to negative ΔfoF2 values occurred at all latitudes. The recovery phase was characterized by negative ionospheric disturbance at all latitudes. This is due to the decrease of thermospheric O/N2 ratio during the recovery phase of the storm. The intense Es layers screened the reflections from the F2-layer on August 26th at high and at low latitudes but at different times. Some blackouts occurred due to the high absorption level at high latitudes. In general, foF2 and TEC data were highly correlated. The major Ne changes were at the low latitudes. In general, Ne data confirmed the ionospheric dynamics revealed with foF2 and TEC.     

Post-midnight equatorial irregularity distributions and vertical drift velocity variations during solstices

Longitudinal distributions of post-midnight equatorial ionospheric irregularity occurrences observed by ROCSAT-1 (1st satellite of the Republic of China) during moderate to high solar activity years in two solstices are studied with respect to the vertical drift velocity and density variations. The post-midnight irregularity distributions are found to be similar to the well-documented pre-midnight ones, but are different from some published distributions taken during solar minimum years. Even though the post-midnight ionosphere is sinking in general, longitudes of frequent positive vertical drift and high density seems to coincide with the longitudes of high irregularity occurrences. Large scatters found in the vertical drift velocity and density around the dip equator in different ROCSAT-1 orbits indicate the existence of large and frequent variations in the vertical drift velocity and density that seem to be able to provide sufficient perturbations for the Rayleigh-Taylor (RT) instability to cause the irregularity occurrences. The need of seeding agents such as gravity waves from atmospheric convective clouds to initiate the Rayleigh-Taylor instability may not be necessary.     

基于磁致伸缩传感器的液体密度测量的研究

简要介绍了利用磁致伸缩传感器测量液体密度的原理以及测量系统的组成和应用。利用脉冲回波法测量了声速从而算出液体密度。验证了扭转波在液体中传播速度与液体密度的关系。     

Local clouds: Distribution, density and kinematics through ground-based and HST spectroscopy

The distribution, kinematics and physical properties of the interstellar matter surrounding the Sun can be inferred from ground-based and UV spectroscopic observations. On a 200 pc scale the local interstellar matter appears inhomogeneous and asymmetric. Although it generally flows towards the lower density region, it is composed of numerous small components a few parsecs in size with slightly different velocities. On a smaller scale the extent and the nature of the Local Cloud which flows over the Sun are discussed based on HST-GHRS observations of nearby stars.