某陀螺仪二次项测试方法研究

本文通过对某陀螺仪二次项DSO产生原理的分析,发现陀螺仪二次项DSO与过载a0有关.通过对陀螺仪进行低过载测试试验和高过载测试试验,测试出了二次项DSO与过载a0的趋势性关系.即低过载下,陀螺仪二次项DSO与过载近似无关;高过载下,陀螺仪二次项DSO与过载之间成一定函数关系.     

干涉型光纤陀螺温度漂移建模与实时补偿

 分析了干涉型光纤陀螺(IFOG)温度漂移的影响因素,通过建立温度与陀螺模型参数之间的线性相关关系,推导出了光纤陀螺温度漂移的分布模型。为了提高陀螺温度漂移模型的适应性,设计了0.25,0.75,1.00 ℃/min三种变温速率的温度试验,并利用小波变换的方法分离数据中的噪声和趋势项。基于温度漂移的分布模型和最小二乘误差（LSE）准则,建立了多参量联合线性模型来估计陀螺温度漂移。采用升温过程和降温过程分段建模的方法将多参量联合线性模型算法进行了简化,并在现场可编程逻辑阵列（FPGA）中分时复用一个全串行有限冲激响应（FIR）滤波器实现了陀螺温度漂移的实时估计。仿真的温度补偿结果及实时的温度补偿结果显示,该方法可以使陀螺温度漂移减小到1/10~2/10。     

Matlab在光纤陀螺随机漂移建模中的应用

光纤陀螺随机漂移是捷联惯导系统的主要误差源,对其建立一个精确的、适用的模型有利于减小光纤陀螺漂移,提高系统精度。本文根据时序建模理论,利用Matlab中的自带函数,建立了光纤陀螺随机漂移模型。Matlab在光纤陀螺漂移建模中的应用,避免了传统编程建模的繁琐,简化了建模的计算过程,大大减小了工作量,提高了建模效率。     

Characteristics of the equatorial F-region vertical plasma drift observed during post-sunset and pre-sunrise hours

Post-sunset and pre-sunrise vertical plasma drifts at the equatorial F-region have been investigated using the HF Doppler radar and ionosonde observations. Observed vertical plasma drift features during the sunrise are found to complement that observed during the evening. The post-sunset vertical plasma drift is characterized by an upward enhancement, a pre-reversal enhancement and a reversal in the drift direction. Similarly, the pre-sunrise plasma drift is characterized by a sudden downward excursion followed by an upward turning. The wavelet analysis of the plasma drift shows the presence of fluctuations in the period range 4–32 min and the short period fluctuations are attributed to the atmospheric gravity waves.     

Dynamics of the convection in the inner magnetosphere by observations of the diffuse aurora,SAR arc and ionospheric drift

The first results of the comparison of subauroral luminosity dynamics in 557,7 and 630,0 nm emission with simultaneous measurements of the ionospheric drift in the F2 region with a digisonde DPS-4 at the Yakutsk meridian (CGMC: 55–60N, 200°E) at Kp = 2–6 are presented. It is shown from the analysis of individual events that during the magnetospheric convection intensification after the turn of the IMF B_z – component to the south the equatorward extension of diffuse aurora takes place. At the same time the westward ionospheric drift velocity increases both in the diffuse aurora region and much equatorward of it due to the occurrence of the northward polarization electric field. We suppose that the generation of polarization field can be associated with the development of the region 2 FAC during the intensification of magnetospheric convection. The comparison of ground-based observations with measurements of the plasma drift aboard the DMSP-F15 satellite has been carried out.     

天基空间碎片光学探测影响因素分析及仿真

光学手段在天基空间碎片探测中被广泛应用,但容易受到杂光等因素影响。结合在轨试验数据,从探测器和碎片两方面分析了影响天基空间碎片光学探测的因素。影响探测器探测效果的因素包括太阳光、月光、地气光、大气辉光等杂光及南大西洋异常区辐射等;影响碎片可见性的因素包括地球遮挡、地影及反射的太阳光等。分别给出了上述影响因素涉及的特征量及规避影响的计算方法。基于某天基探测设备的仿真结果表明,上述影响在自然交会及姿态机动模式下均可能发生,在试验设计时需被充分考虑。最后,针对某天基空间碎片探测任务进行了规划。文章对天基光学探测试验设计具有一定的指导意义。     

基于小波神经网络的陀螺漂移预测研究

实时识别陀螺漂移,并且预测漂移性能的变化趋势,对提高整个导航系统的精度有着十分重要的意义。本文结合小波分析理论和小波神经网络的非线性预测算法,对陀螺信号进行趋势提取与漂移预测。采用小波神经网络避免了其它神经网络存在的局部最小化的缺陷,小波分析的引入可以有效提取出原信号的趋势,大大降低了环境因素的影响。将小波神经网络非线性预测算法与小波趋势提取算法结合,建立陀螺仪漂移趋势的预测模型,对某光纤陀螺实测信号仿真预测其漂移趋势,仿真结果证实该预测模型与实际情况相符,具有较好的预测精度,为预测一般陀螺的随机漂移提供了一种新的有效途径,同时还对一般陀螺仪表的漂移模型建立方法提供借鉴。     

Probing afternoon detached aurora and high-latitude trough based on DMSP observations

The present work displays the observations of an afternoon detached aurora along with ionospheric high-latitude trough. The event was observed by DMSP F17 on 19 September 2014. The afternoon detached aurora was isolated from the auroral oval and was located between 12:00–18:00 magnetic local time (MLT) and 65–70° geomagnetic latitude (MLAT). Particle observations indicate that the afternoon detached aurora was produced by energetic ring current ions with energies above ~10 keV where the main ion energy was likely to be above the upper limit of DMSP measurement (~30 keV). Magnetometer observation from the ground implies that the energetic ions were likely scattered by EMIC waves. Both the detached aurora and the auroral oval are found to be well inside the high-latitude trough with MLAT between ~64° and ~76° (68–80° GLAT). The auroral oval corresponds to a westward (sunward) plasma drift. It is expected that the westward drift transports the low-density plasma in the nightside toward the dayside, leading to the high-latitude trough formation. The afternoon detached aurora was well equatorward of the high-latitude trough, and the corresponding plasma drift was nearly zero. The plasma associated with the detached aurora is expected to be stagnant, and broaden the high-latitude trough equatorward.     

The post sunset equatorial F- region zonal drift variability and its linkage with equatorial spread F onset and duration over Indian longitudes

The seasonal and solar activity variation of the post sunset F- region zonal plasma drift, at the magnetic equatorial region over Indian longitudes is analyzed using the Republic of China Satellite-1 data from January 2000 to April 2004. The post sunset F- region zonal drifts are observed to be higher in the years of high solar activity in comparison with low solar activity, while seasonally the drifts are minimum in summer with much higher values in other seasons. The seasonal and solar activity variations of zonal plasma drift are attributed to the corresponding variations in the neutral winds. The dependences of the F region peak vertical drift on the zonal plasma drift at 18.5 IST (Indian Standard Time) and the time difference of the conjugate points sunset times, are quantitatively analyzed. Further an integrated parameter (incorporating the above mentioned two independent factors), which is able to predict the peak vertical drift and growth rate of Rayleigh Taylor instability is proposed. The other major outcome of the study is the successful prediction of the Equatorial Spread F (ESF) onset time and duration using the new integrated parameter at 18.5 IST. ESF irregularities and associated scintillations adversely affect communication and navigation systems. Hence, the present methodology for the prediction of the characteristics of these nocturnal irregularities becomes relevant.     

压阻式加速度传感器封装应力隔离结构分析

测试特性的温度漂移是压阻式加速度传感器研发中的固有问题，与器件制造的多个环节相关，是多因素共同作用的结果。封装应力的隔离是消减传感器特性温度漂移的重要手段之一。为详细分析封装应力隔离结构的引入效果及其对传感器测试特性的影响，以传统双桥式敏感结构为基础，采用有限元方法分析了封装应力隔离结构对传感器附加干扰载荷抵抗力的提升作用，并分析了从其引入后对传感器敏感应力和结构固有频率的影响。分析结果表明，引入封装应力隔离结构可有效降低外部干扰应力对传感器敏感结构的影响，同时也会改变结构固有频率在内的传感器测试特性。因而，当封装应力隔离结构应用于高频型加速度传感器时，需通过优化结构质量分布、采用横向敏感结构等方法对提升结构自身固有频率及实现敏感方向与隔离变形方向解耦等问题进行进一步优化。