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。     

Solar signals in the minimum extreme temperature records in the southern region of the Gulf of Mexico

Minimum extreme temperature series from several meteorological stations of the Gulf of Mexico are spectrally analyzed using the Maximum Entropy Method.We obtained significant periodicities similar to those found in meteorological and solar activity phenomena. This indicates that probably the solar activity signals are present in the minimum extreme temperature records of this Mexican region.     

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 ...     

铁电阴极用于小功率电推力器

分析了当前小功率电推力器对零流动无推进剂阴极的需求现状。提出铁电阴极用于小功率电推进中和器的可能性。研究了厚度为0．5mm的PLZT（锆钛镧酸铅）铁电陶瓷在低电压（1．0～1．2kV）条件下的电子发射性能。实验采用脉宽为1μs的单极性正高压脉冲作为激励源。在收集极获得了脉宽为320ns～3000ns,最高峰值为34A的发射电流。在10^-4乇的真空环境中得到了非常可靠的电子发射。     

诱发卫星深层充电的高能电子环境模式研究

文章介绍了与卫星介质深层充电相关的辐射带高能电子环境的主要特征和规律,建立了相应的高能电子环境模式及软件,并运用该模式针对某飞行器的深层充放电危险性进行了分析和评估。结果表明该模式相对于AE8模式更好地反映了高能电子环境的动态特征,与欧空局建立的FLUMIC模式符合较好。该模式与深层充电分析模型相结合,可用于对航天器的充放电异常进行在轨诊断,以及在工程上针对深层充电进行防护设计。     

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.     

Guidepost-based autonomous orbit determination method for GEO satellite

Guidepost-based navigation system is a novel autonomous orbit determination method for the GEO satellite. The system is achieved by using the camera imaging function to obtain the guidepost images and the GNSS signal receiver to obtain the pseudoranges between the GEO and the navigation satellites. Due to the high altitude of GEO satellite and the time-varying sunlight condition in the space environment, it may be difficult to obtain object image points and the distance measurements of GNSS because of the weak visibility of the guideposts. To deal with the problem, a novel integrated orbit determination system is presented. The Earth landmarks, the in-orbit spacecraft and GNSS navigation satellites whose line-of-sights and the distance can be easily obtained are used at the same time as information for the GEO satellite navigation based on the observability conditions analysis. The observability of the GEO satellite navigation system is analyzed through the physical observability, the mathematical observability and the engineering observability through the observing geometry, the rank of observability matrix and the Cramer-Rao lower bound (CRLB) respectively. Besides, the maximum correntropy unscented Kalman filter (MCUKF) algorithm is applied to improve the estimation stability of the system in the presence of non-Gaussian noises. The simulation indicates the feasibility of the proposed scheme.     

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.