数字式活塞压力计的研制

介绍了一种集活塞压力计和数字压力计优点于一身的数字式活塞压力计,其改变了传统活塞压力计的设计方案,并在传动密封和系统校准技术方面有了很大的创新,对于现场校准和提高压力计量校准的自动化程度有深远意义。     

New Insights on Geomagnetic Storms from Model Simulations Using Multi-Spacecraft Data

The forecast of the terrestrial ring current as a major contributor to the stormtime Dst index and a predictor of geomagnetic storms is of central interest to ‘space weather’ programs. We thus discuss the dynamical coupling of the solar wind to the Earth's magnetosphere during several geomagnetic storms using our ring current-atmosphere interactions model and coordinated space-borne data sets. Our model calculates the temporal and spatial evolution of H⁺, O⁺, and He⁺ ion distribution functions considering time-dependent inflow from the magnetotail, adiabatic drifts, and outflow from the dayside magnetopause. Losses due to charge exchange, Coulomb collisions, and scattering by EMIC waves are included as well. As initial and boundary conditions we use complementary data sets from spacecraft located at key regions in the inner magnetosphere, Polar and the geosynchronous LANL satellites. We present recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric ring current. Near minimum Dst there is a factor of ∼ 10 variation in the intensity of the dominant ring current ion specie with magnetic local time, its energy density reaching maximum in the premidnight to postmidnight region. We find that the O⁺ content of the ring current increases after interplanetary shocks and reaches largest values near Dst minimum; ∼ 60% of the total ring current energy was carried by O⁺ during the main phase of the 15 July 2000 storm. The effects of magnetospheric convection and losses due to collisions and wave-particle interactions on the global ring current energy balance are calculated during different storm phases and intercompared. This revised version was published online in August 2006 with corrections to the Cover Date.     

直升机低速飞行特性与意外右偏航

根据国外有关参考资料，对直升机丧尾桨推力导致意想不右偏航进行了讨论分析，简单介绍了直升机飞行时的四种飞行特性，（风标稳定性、尾桨涡环状态、主旋翼桨盘旋涡影响，丧失前飞升力）在意外右偏航中的作用和特点，以及改出方法和实施改出的应急措施，为飞行人员保证飞行安全提供了参考依据。     

用数字电压表检定标准电池的测量不确定度评定

介绍了用数字电压表检定高等级标准电池的操作方法，并对其测量不确定度进行了分析与评定。     

由稳态飞行确定纵向气动导数

研究了从稳态对称飞行数据估计气动导数的一种方法，要估计的导数是纵向静稳定性和操纵性导数，尾翼产生的阻尼导数、速度对升力和俯仰力矩系数影响的导数，其方法是基于扩展的纵向静稳定性和操纵性理论以及相应的飞行试验数据表示方法，对于大多数气导数，假设飞行测量数据是以平衡曲线和ＣＬ（α）曲线形式给出的，导数估计表达式是由已知常数，直接或非直接测量量的代数关系式构成，估计精度用结果标准误差或系统误差带表示。所研     

基于整体叶盘环形摩擦阻尼器减振分析及设计

为抑制叶片-盘耦合振动,设计了一种适应整体叶盘结构的环形摩擦阻尼器。拓展了1阶谐波平衡法和整体-局部统一滑动模型在带环形摩擦阻尼器的循环对称结构叶盘减振分析中的应用。使用该方法对实际发动机叶盘在简谐激励下的振动响应进行了仿真计算,结果表明:环形摩擦阻尼器对于某发动机叶盘的0节径4阶危险模态振动有明显抑制作用,且减振效果与阻尼器的质量、安装位置有关,在选定的安装位置最高可使振幅降低75%。在阻尼器结构确定的情况下,利用仿真结果给出了最优的设计方案,包括阻尼器的质量和安装设计。     

用于压电料位计的微弱信号检测电路设计

设计了一种用于压电料位计的微弱信号检测电路,从防积分饱和电荷放大、带通滤波、精密检波、两级比较和逻辑控制五个方面介绍了其工程实现。能够实现单极性电源供电处理交流信号,实时监测料位计输出电荷大小,并转换为开关信号输出;具备灵敏度调节功能,可以根据不同物料的阻尼特性,有针对性地设置动作阈值;能够根据用户需要设置输出电平极性,提高了料位计的灵活性和适应性。结合理论计算、仿真分析和试验测试,验证了设计的合理性和正确性。     

基于北斗/GNSS精密时频量值传递综述

介绍了北斗/GNSS精密时间频率量值传递技术及其应用研究进展,通过对北斗共视比对技术的研究,设计出利用北斗共视与国家授时中心GNSS CV精密时间服务系统进行比对,从而实现用户与标准时间UTC的溯源完成基于GNSS CV技术的时间频率计量服务系统设计,创新性地提出提高北斗共视比对技术以及研制多模多频GNSS CV量值传递设备的研究方向。     

The influence of the spatial and temporal collocation windows on the comparisons of the ionospheric characteristic parameters derived from COSMIC radio occultation and digisondes

GPS radio occultation (RO) ionospheric products obtained by Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) mission during the year of 2014 and the observations from 3 digisonde stations which are located at different latitudes are used to study the influence of different time and space collocation windows on the comparisons of the ionospheric characteristic parameters (ICPs), including the peak density and peak height, derived from the two techniques. The results show that the correlation coefficients (CC) and the standard deviation of the absolute biases (SDAB) between the ICPs derived from the two techniques vary distinctly under different spatial and time collocation windows. Generally, the CC (SDAB) of the ICPs decrease (increase) as the size of the collocation window increases in time dimension or in space dimension. The rate of change of the statistic parameters with the increase in the size of the collocation window in time dimension and space dimension is analyzed for each digisonde station. It is found that within the collocation window of $\left(60\mathrm{m}\mathrm{i}\mathrm{n},{20}^{°},{20}^{°}\right)$, the influence of the increase of $1^{°}$ in the space window on the statistical comparison is much more significant than that of the increase of 1?min in the time window, and it is suggested that there can be appropriate relaxation on the time window within the threshold of 60?min to get a balance between the quality of the comparison results and the number of the matched pairs. In addition, it is found that the same variations in the longitude window and in the latitude window may have different influences on the comparison results when the horizontal gradients in electron density are distinctly different along different directions at the digisonde station, and strict space collocation window is preferred when comparing the observations from COSMIC RO with those from the digisonde station in such cases.     

一种激光陀螺闭锁阈值的测试方法研究

闭锁效应是二频机抖激光陀螺的最重要误差,其主要来源于光路中的背向散射。通过对自洽场方程组的分析,给出了光强与频差的表达式,继而得到一种新的闭锁阈值测试方法。通过搭建相关测试系统,并对比传统的转台渐进降速测试的闭锁阈值,结果表明新方法得到的测试值与陀螺实测精度具有更好的吻合性,这对预估和分析激光陀螺性能具有较好的指导意义。