基于CPHD的双层粒子滤波目标跟踪算法

常规基于势概率假设密度滤波(Cardinalized Probability Hypothesis Density,CPHD)的粒子滤波(Particle Fil? ter,PF)跟踪算法应用于多目标跟踪时,容易遇到因粒子数量增加而带来的运算效率下降、目标数目估计不准的问题。文章基于常规粒子滤波 CPHD跟踪算法,通过部署双层粒子,提出基于势概率假设密度滤波的双层粒子滤波 (Two-Layer Particle Filter-CPHD,TLPF-CPHD)算法,以便提高目标数目及状态估计精度。仿真实验结果证明,相比于常规 PF-CPHD算法,新算法具有更好的目标数目和状态估计准确性。     

激波风洞流场密度测量的聚焦纹影技术

在激波风洞试验中发展了聚焦纹影显示技术,对流场的密度进行了定量测量。聚焦纹影显示具有对流场区域聚焦显示的特点,可获得流场某个聚焦测试区域的密度变化信息。依据聚焦纹影成像原理建立了密度计算数学模型,对试验中获得的带窗口模型流场聚焦纹影图像与试验前获得的流场图像灰度变化处理后,得到了流场聚焦区域的密度定量值。试验测量密度值与数值计算结果进行了比较,结果表明试验获得的密度值变化规律与数值模拟吻合较好,证实了利用聚焦纹影技术开展流场密度测量是可行的。     

An improved multiple model GM-PHD filter for maneuvering target tracking

In this paper, an improved implementation of multiple model Gaussian mixture probability hypothesis density (MM-GM-PHD) filter is proposed. For maneuvering target tracking, based on joint distribution, the existing MM-GM-PHD filter is relatively complex. To simplify the filter, model conditioned distribution and model probability are used in the improved MM-GM-PHD filter. In the algorithm, every Gaussian components describing existing, birth and spawned targets are estimated by multiple model method. The final results of the Gaussian components are the fusion of multiple model estimations. The algorithm does not need to compute the joint PHD distribution and has a simpler computation procedure. Compared with single model GM-PHD, the algorithm gives more accurate estimation on the number and state of the targets. Compared with the existing MM-GM-PHD algorithm, it saves computation time by more than 30%. Moreover, it also outperforms the interacting multiple model joint probabilistic data association (IMMJPDA) filter in a relatively dense clutter environment.     

自相关回归法在地震地面运动功率谱分析中的应用

本文通过数值分析，对几个著名的地震记录的功率谱ARM解的特性作了讨论，并与高速富里衰变换（FFT）法的解进行了比较，讨论了ARM应用于各类地震记录的谱分析的适用性。比较结果表明：对于不同的地震记录，其功率谱的ARM解等价于按一定谱窗宽度平滑化的FFT法解。本研究还对赤池氏推荐的自相关回归次数的经验公式提出了修正意见。本研究的成果对于高层建筑抗震设计有一定的参考价值。     

Solar wind electron density and temperature over solar cycle 23: Thermal noise measurements on Wind

We present the solar wind plasma parameters obtained from the Wind spacecraft during more than nine years, encompassing almost the whole solar cycle 23. Since its launch in November 1994 Wind has frequently observed the in-ecliptic solar wind upstream of the Earth’s bow shock. The WIND/WAVES thermal noise receiver was specially designed to measure the in situ plasma thermal noise spectra, from which the electron density and temperature can be accurately determined. We present and discuss histograms of such measurements performed from 1994 to 2003. Using these large data sets, we study the density and core temperature variations with solar activity cycle and with different regimes of the solar wind. We confirm the anticorrelation of the electron density with the sunspot number, and obtain a positive correlation of the core temperature, with the sunspot number.     

利用电离层参量推断电子浓度剖面的一种简单方法

由武汉电离层观象台实测的电离层F2层临界频率foF2、3000km传播因子M(3000)F2的月中值资料，统计分析分别得出它们的经验模式，模式结果能够较好地再现这些参数的观测值．利用foF2、M(3000)F2以及TEC的经验模式，获得F2层的峰值参数，输入到电子浓度的Chapman α函数中，推断出了电子浓度的高度剖面；将剖面在一定的高度范围内积分，得到该区域内的电子含量并与实际观测TEC相比较，结果表明，在100-1000km高度范围内积分的电子含量与观测结果能够较好的符合．     

Thermospheric neutral density response to solar forcing

Recent measurements by the Solar EUV (Extreme Ultra Violet) Experiment (SEE) aboard the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics satellite (TIMED) provide solar EUV spectral irradiance with adequate spectral and temporal resolution, and thus the opportunity to use solar measurements directly in upper atmospheric general circulation models. Thermospheric neutral density is simulated with the NCAR Thermosphere–Ionosphere–Electrodynamic General Circulation Model (TIEGCM) using TIMED/SEE measurements and using the EUVAC solar proxy model. Neutral density is also calculated using the NRLMSISE-00 empirical model. These modeled densities are then compared to density measurements derived from satellite drag data. It is found that using measured solar irradiance in the general circulation model can improve density calculations compared to using the solar proxy model. It is also found that the general circulation model can improve upon the empirical model in simulating geomagnetic storm effects and the solar cycle variation of neutral density.     

碘工质电推进系统的储供设计及实验研究

碘工质以其低成本、低压且高密度贮存等特点越来越受到重视,承担固气相变和流量供给功能的储供系统是碘工质电推进系统的关键组件。为了提高直接影响阴极和推力器性能的流量供给准确性和稳定性,设计了可采用多种加热方式的碘工质储供系统,结合用于真空舱内的高精度质量传感器,实现了流量的动态监测及mg/s级别的碘蒸气流量控制。针对储罐外部加热、内部辐射加热以及二者复合加热三种加热方式开展实验测量,探究其对流量大小和稳定性的影响规律。结果表明,三种加热方式在满足实验所需条件下均可长期供给稳定流量,辐射加热式的响应时间最快,仅需要10min左右,而外部加热则超过1h;复合加热的方式热控调节虽更为复杂,但可以进一步降低功耗。     

一种氧杂蒽酮类海洋抗污损天然产物振动光谱的理论研究

基于 Gaussian 09W软件包,采用 DFT-B3LYP方法,研究了 1种来源于红树林未知真菌的海洋抗污损天然产物——6,8-di-O-methyl versiconol。先用 3-21G基组,再用 6-311G基组计算了分子的最稳定构型及其前线分子轨道分布。分析稳定构型发现,以蒽二酮为主体的分子是 1个三维非平面的结构,并且分子内部形成了 1个大的 π共轭体系。在最稳定构型的基础上,用同样的理论方法和 6-311G基组计算了该分子的红外振动频率及拉曼光谱频率,根据红外和拉曼光谱的振动频率特点,将红外光谱和拉曼光谱分成 3个区域,讨论了 2种光谱在各区域的特征峰的位置、振动特点、振动模式等,为氧杂蒽酮类海洋抗污损天然产物分子的振动光谱检测和分子结构的鉴定,提供了光谱解析方面的理论依据。     

ULF/ELF ionospheric electric field and plasma perturbations related to Chile earthquakes

ULF/ELF electric field perturbations in the ionosphere have been widely observed by the satellites. In this paper, we develop a method of Logarithm Electric Field Intensity (LEFI) to automatically distinguish this kind of disturbances based on the spectrum intensity and its damping exponent with frequency in electromagnetic signals. This method is applied to DEMETER data processing around Chile earthquakes with magnitude larger than 6.0. It is found that 2/3 earthquakes have shown obvious ULF/ELF electric field perturbations in this region. The temporal and spatial distributions of electron density and temperature were compared with that of electric field, which proved the existence of irregularities above epicentral area. Finally, the coupling mechanism of earthquake-ionosphere is discussed based on multi-parameter analysis.