谐振式加速度计自激振荡电路性能评价方法的研究

针对谐振式加速度计成品率不高、精度低等问题,以石英振梁加速度计为例,采用引进标准信号,将谐振电路作为"黑盒子",对其开展独立的评价.通过评价电路的驱动电压幅值稳定性、移相稳定性、全温幅值/相位对称性等指标,与加速度计实际指标建立了一一对应的关系,为加速度计研制与性能提升提供了有效依据.实际运用表明,电路噪声性能、温度性...     

递推的TLS参数估计方法及其在飞轮FDD中的应用

飞轮是很多卫星姿态控制系统中的重要执行部件，其星上自主故障诊断是一个很有意义的研究课题。本文根据飞轮系统的特点，在最小二乘（ＬＳ）参数估计方法的基础上提出了全最小二乘（ＴＬＳ）参数估计的递推形式，证明了它对飞轮参数估计的收敛性，并用于飞轮缓变故障的检测和诊断，取得了较好结果。     

多传感器目标识别的优化融合

对于工作在复杂环境下的多传感器目标识别系统,确保其稳健性和准确性的关键是有效处理被融合信息的不确定性。根据影响信息不确定性的因素,文章把传感器本地识别信息的可信度分为了统计可信度和环境可信度;采用最小二乘法和神经网络实现统计可信度的估计,自适应神经模糊推理实现环境可信度估计;并利用这两种可信度实现以一致理论为基础的多传感器目标识别的优化融合。经实验仿真证明,该融合方案是有效的。     

预报误差法在伺服系统时域辨识中的应用与实现

介绍了系统辨识中的预报误差法的基本原理,设计了一种简洁通用的软硬件辨识平台。成功地应用预报误差的辨识方法对一个实际的中功率雷达伺服系统实现了时域辨识,得到了该伺服系统比较准确的模型。将辨识结果与一般最小二乘法的辨识结果进行了比较,发现此辨识方法在抑制噪声方面有很大的改进。     

用最小二乘法评定圆柱度误差的理论与算法

建立了用最小二乘法评定圆柱度误差的理论与算法,并对圆柱度误差进行了定量分析和定性分析,给出了误差分离的定量计算公式,将其分离成形状误差、参数误差和方向误差,并指出了每种误差的补偿原则。所推导的数学模型简单、明了,具有推广价值。     

GPS total electron content and surface latent heat flux variations before the 11 March 2011 M9.0 Sendai earthquake

The present paper describes the variations of the GPS total electron content (TEC) from the International GNSS service network and surface latent heat flux (SLHF) from the Scientific Computing Division of the National Center for Atmospheric Research (NCAR) before the 11 March 2011 M9.0 Sendai earthquake, respectively. The analysis shows pronounced enhancements in the GPS TEC and SLHF a few days prior to the earthquake event. The maximum increase in the GPS TEC was about 30 TECu with an extended spatial distribution on a geomagnetically quiet day (Dst ? −20 nT, between two moderate geomagnetic storms), 8 March, 3 days prior to the earthquake. This giant positive disturbance was possibly associated with the impending disastrous earthquake and contributed from the enhanced solar radiation. Moreover, there were several anomalous regions of SLHF on the global map, but an area of enhanced SLHF very close to the epicenter. The purpose of this paper is to report the existence of the changes in surface and ionosphere, and show the potential application of multi-source data to identify seismic precursors.     

Plasmaspheric electron content derived from GPS TEC and FORMOSAT-3/COSMIC measurements: Solar minimum condition

The plasmaspheric electron content (PEC) was estimated by comparison of GPS TEC observations and FORMOSAT-3/COSMIC radio occultation measurements at the extended solar minimum of cycle 23/24. Results are retrieved for different seasons (equinoxes and solstices) of the year 2009. COSMIC-derived electron density profiles were integrated up to the height of 700 km in order to retrieve estimates of ionospheric electron content (IEC). Global maps of monthly median values of COSMIC IEC were constructed by use of spherical harmonics expansion. The comparison between two independent measurements was performed by analysis of the global distribution of electron content estimates, as well as by selection specific points corresponded to mid-latitudes of Northern America, Europe, Asia and the Southern Hemisphere. The analysis found that both kinds of observations show rather similar diurnal behavior during all seasons, certainly with GPS TEC estimates larger than corresponded COSMIC IEC values. It was shown that during daytime both GPS TEC and COSMIC IEC values were generally lower at winter than in summer solstice practically over all specific points. The estimates of PEC (h > 700 km) were obtained as a difference between GPS TEC and COSMIC IEC values. Results of comparative study revealed that for mid-latitudinal points PEC estimates varied weakly with the time of a day and reached the value of several TECU for the condition of solar minimum. Percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 50–60%) during night-time and lesser values (25–45%) during day-time.     

Comparison of model and experimental ionospheric parameters at high latitudes

Modern use and study of the auroral region needs to attract a wider class of models for describing conditions of radio wave propagation in the ionosphere. In this paper the possibilities of the International Reference Ionosphere model, well-proven and widespread in the mid-latitudes, are investigated in the high latitude zone. Model and measured values of the critical frequency foF2 for two mid-latitude stations (Juliusruh and Goosebay) and four high-latitude ones (Loparskaya, Sodankyla, Sondrestrom, Thule) are compared. Deviations of medians, variations from day to day and solar activity trends seemed to be similar for both areas. This similarity is irrespective of the RZ12 index. Special attention is paid to the TEC parameter and its determination using 6 versions of models, a new version of the model IRI2010 (IRI-Plas) among them. It is shown that the IRI-Plas model significantly improves the definition of TEC in contrast to the versions of IRI2007 and the new model NeQuick. The use of the median of the experimental equivalent slab thickness, together with the current values of the TEC, increases by a factor of two the agreement between calculated and measured foF2 values as compared with the variations from day to day. This allows foF2 to be defined in near-real time.     

航空发动机总温热电偶校检问题

由于航空总温热偶气动构件的复杂性，校验问题一直悬而未决。制成后的电偶热电特性迁移，及配套特性变化强调了配套校验是必要的。本文在着重分析了以上问题后，介绍了自行研制的已获国家专利的ＳＴＴ－１Ａ系列总温热电偶校验器。     

Differential code bias estimation based on uncombined PPP with LEO onboard GPS observations

Differential Code Bias (DCB) is an essential correction that must be provided to the Global Navigation Satellite System (GNSS) users for precise position determination. With the continuous deployment of Low Earth Orbit (LEO) satellites, DCB estimation using observations from GNSS receivers onboard the LEO satellites is drawing increasing interests in order to meet the growing demands on high-quality DCB products from LEO-based applications, such as LEO-based GNSS signal augmentation and space weather research. Previous studies on LEO-based DCB estimation are usually using the geometry-free combination of GNSS observations, and it may suffer from significant leveling errors due to non-zero mean of multipath errors and short-term variations of receiver code and phase biases. In this study, we utilize the uncombined Precise Point Positioning (PPP) model for LEO DCB estimation. The models for uncombined PPP-based LEO DCB estimation are presented and GPS observations acquired from receivers onboard three identical Swarm satellites from February 1 to 28, 2019 are used for the validation. The results show that the average Root Mean Square errors (RMS) of the GPS satellite DCBs estimated with onboard data from each of the three Swarm satellites using the uncombined PPP model are less than 0.18 ns when compared to the GPS satellite DCBs obtained from IGS final daily Global Ionospheric Map (GIM) products. Meanwhile, the corresponding average RMS of GPS satellite DCBs estimated with the conventional geometry-free model are 0.290, 0.210, 0.281 ns, respectively, which are significantly larger than those obtained with the uncombined PPP model. It is also noted that the estimated GPS satellite DCBs by Swarm A and C satellites are highly correlated, likely attributed to their similar orbit type and space environment. On the other hand, the Swarm receiver DCBs estimated with uncombined PPP model, with Standard Deviation (STD) of 0.065, 0.037 and 0.071 ns, are more stable than those obtained from the official Swarm Level 2 products with corresponding STD values of 0.115, 0.101, and 0.109 ns, respectively. The above indicates that high-quality DCB products can be estimated based on uncombined PPP with LEO onboard observations.