强场脉冲充磁退磁装置

介绍了充电电容器通过磁路瞬时放电产生强磁场的原理 ,选择回路参数可实现高矫顽力类永磁材料的充磁或者退磁 ,介绍了所研制的脉冲充磁退磁装置的性能。     

基于强跟踪EKF的组合导航系统故障检测方法

针对大方位失准角的机载SINS/GPS组合导航系统,为保证在高动态环境下实现高精度、高可靠的导航,利用强跟踪EKF滤波残差设计了一种基于残差统计特性的坏值检测算法,对导航信息进行估计和跟踪.仿真结果表明,该算法能够实时检测出GPS量测信息中的坏值信息,隔离后可显著提高组合导航精度,具有较高的可靠性、出色的容错能力和重要的工程应用价值.     

Signatures of strong geomagnetic storms in the equatorial latitude

Ionosonde data from two equatorial stations in the African sector have been used to study the signatures of four strong geomagnetic storms on the height – electron density profiles of the equatorial ionosphere with the objective of investigating the effects and extent of the effects on the three layers of the equatorial ionosphere. The results showed that strong geomagnetic storms produced effects of varying degrees on the three layers of the ionosphere. Effect of strong geomagnetic storms on the lower layers of the equatorial ionosphere can be significant when compared with effect at the F2-layer. Fluctuations in the height of ionization within the E-layer were as much as 0% to +20.7% compared to −12.5% to +8.3% for the F2-layer. The 2007 version of the International Reference Ionosphere, IRI-07 storm-time model reproduced responses at the E-layer but overestimated the observed storm profiles for the F1- and F2-layers.     

Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

Physical processes in the strong magnetic fields of accreting neutron stars

The key radiative processes are discussed, numerical methods of magnetized radiative transfer are presented, and these are considered in their application to X-ray pulsar models.     

基于STF的Jerk模型自适应机动目标跟踪算法

在Jerk模型的基础上,提出了一种新的机动目标自适应跟踪算法STF-Jerk。该算法通过引入强跟踪滤波器(STF)的渐消因子,实时调节滤波器增益,增强了系统对突发机动的自适应跟踪能力,从而很好地改善了Jerk模型在跟踪机动目标时的跟踪精度。仿真结果表明,提出的STF-Jerk自适应跟踪算法显著提高了Jerk模型自适应算法的机动目标跟踪性能。     

强噪声环境下声波信号时延估计方法的比较

声波信号时延的准确估计是实现强噪声环境下声学法高精度测温的关键。介绍了声学测温中基于互相关函数、人工神经网络和小波变换等几种典型的信号时延估计方法．对这3种时延估计方法的实现原理分别进行了论述，分析比较了它们的优缺点，相比于其他两种方法，小波变换技术更适合于强噪声环境下的声波信号的时延估计。     

根据"大震不倒"要求反演优化设计工程结构

工程结构系统在地震作用下的设计要求是“小震不坏,大震不倒”,现行的概念设计加抗震验算设计方法给出的只能是一个可用解,而不是满足“大震不倒”要求的最优解。本文结合钢筋混凝土框架结构,讨论了根据工程结构“大震不倒”的要求反演优化设计工程结构的有关参数(如钢筋混凝土框架的配筋率、混凝土标号、截面尺寸等)的概念、方法并给出了算例,说明这种不同于传统结构设计的新的设计理念是可行的,有关方法是有效的。     

Strong perturbations on the Sun and in the heliosphere leading to large geomagnetic storms: Similar and individual characteristics

We briefly present the selected results obtained up to now by the Russian scientific groups regarding powerful solar ejections as main causes of large geomagnetic storms in the near-Earth space. Strongest perturbations on the Sun and in the near-Earth space responsible for large geomagnetic storms were well registered and analyzed during the 23rd solar cycle. Open issues and perspectives are discussed.     

基于强跟踪UPF的重力梯度辅助定位方法

针对重力梯度辅助定位中,存在重力梯度的强非线性分布及系统模型偏差等问题,将STUPF引入匹配定位过程。该方法根据残差信息实时调节系统状态跟踪能力,有效应对模型偏差对定位的影响。基于真实INS数据的仿真实验结果表明,STUPF可达到较好的定位效果,且与标准PF、GPF算法相比,其在定位的精度、稳定性及运算量上具有一定优势。