插装式液控能源选择阀的设计与分析

针对液压系统油源的安全性及可靠性问题，提出油源冗余设计方法，即多油源供给多负载，当某一油源发生故障时能源选择阀切断故障油源，由其他油源给负载提供基本液压能源，系统能完成必须的服役性能。针对液压系统能源选择阀存在的频繁换向与振动问题，提出一种插装式液控能源选择阀，其先导阀采用锥阀和可变阻尼形式，主阀采用三台肩且终端有缓冲功能的滑阀。建立了插装式液控能源选择阀的数学模型，分析了能源选择阀在两种模拟故障下的切换压力及切换时间、油源压力脉动等特性。理论分析结果表明，油源压力阶跃和线性变化时，某能源选择阀切换时间分别为5 ms和7 ms。当压力发生波动时，主阀不会发生振动，还可通过液控先导阀结构设计来控制切换压力和回复压力大小。     

Deorbiter CubeSat mission design

This paper presents the mission design for a CubeSat-based active debris removal approach intended for transferring sizable debris objects from low-Earth orbit to a deorbit altitude of 100 km. The mission consists of a mothership spacecraft that carries and deploys several debris-removing nanosatellites, called Deorbiter CubeSats. Each Deorbiter is designed based on the utilization of an eight-unit CubeSat form factor and commercially-available components with significant flight heritage. The mothership spacecraft delivers Deorbiter CubeSats to the vicinity of a predetermined target debris, through performing a long-range rendezvous maneuver. Through a formation flying maneuver, the mothership then performs in-situ measurements of debris shape and orbital state. Upon release from the mothership, each Deorbiter CubeSat proceeds to performing a rendezvous and attachment maneuver with a debris object. Once attached to the debris, the CubeSat performs a detumbling maneuver, by which the residual angular momentum of the CubeSat-debris system is dumped using Deorbiter’s onboard reaction wheels. After stabilizing the attitude motion of the combined Deorbiter-debris system, the CubeSat proceeds to performing a deorbiting maneuver, i.e., reducing system’s altitude so much so that the bodies disintegrate and burn up due to atmospheric drag, typically at around 100 km above the Earth surface. The attitude and orbital maneuvers that are planned for the mission are described, both for the mothership and Deorbiter CubeSat. The performance of each spacecraft during their operations is investigated, using the actual performance specifications of the onboard components. The viability of the proposed debris removal approach is discussed in light of the results.     

一种基于VPL 的元器件快速建模方法

为了更好地落实航空电子模块的可制造性设计审查工作,结合航空电子模块产品特点和技术要求,建设了基于Valor软件的PCB/PCBA设计与检测自动化分析系统.元器件模型库作为该系统的必要组成部分,其覆盖范围和数据精度对审查结果至关重要.本文将从元器件模型库建设必要性、建设过程和建模工艺要求三个方面进行阐述,并提出一种基于Valor VPL的元器件快速建模方法,应用结果表明,该方法能够高效构建满足系统审查精度的元器件模型,使大规模元器件模型库的建设成为可能.     

Development and performance evaluation of tropospheric scintillation model on Ku-band satellite link over Akure,Nigeria

Existing amplitude scintillation prediction models often perform less satisfactorily when deployed outside the regions where they were formulated. This necessitates the need to evaluate the performance of scintillation models developed in one region using data data from other regions while documenting their relative errors. Due to its variation with elevation angle, frequency, other link parameters and meteorological factors, we employed three years (January 2016 to December 2018) of concurrently measured satellite radio beacons and tropospheric weather parameters to develop a location-based amplitude scintillation prediction model over the Earth-space path of Akure (7.17^oN, 5.18^oE), South-western Nigeria. The satellite beacon measurement used Tektronix Y400 NetTek Analyzer at 1 s integration time while meteorological parameters, namely; temperature, pressure and relative humidity were measured using Davis Vantage Vue weather station at 1 min integration time. Comparative study of the model’s performance with nine (9) existing scintillation prediction models indicates that the best and worst performing models, in terms of root mean square error (RMSE), are the Statistical Temperature and Refractivity (STN) and direct physical and statistical prediction (DPSP) models with values 11.48 and 51.03 respectively. Also, worst month analysis indicates that April, with respective enhancement and fade values of 0.88 and 0.90 dB for 0.01% exceedance, is the overall worst calendar month for amplitude scintillation.     

弹载变转速定量泵高动态压力控制特性分析

传统弹载电液伺服系统的液压能源采用有刷直流电机驱动恒压变量泵的方式，泵源压力在导弹飞行过程中设定值恒定，但在平飞段过程长、负载小，对能源压力需求低，造成弹上能源总利用率不高的问题，提出无刷直流电机驱动小排量液压泵的压力控制泵源的设计，在低气动负载阶段适当降低系统压力，进而降低节流损失与泄漏量，提高能量利用率。分析了变转速定量泵的流量压力特性曲线，通过建立基于变转速压力控制泵源的位置电液伺服系统数学模型与仿真模型，分析了变转速定量泵压力控制系统在典型工况下的位置跟踪、系统压力变化与能量利用效率，验证了压力控制系统能够在导弹平飞段保证位置伺服系统跟踪正常的前提下，能有效提高系统效率，证明了变转速定量泵压力控制系统的有效性与可行性。     

先进战斗机过失速机动大气数据融合估计方法

可控的过失速机动是先进战斗机超机动性能的重要标志，飞机飞行包线的扩大已超出传统的大气数据系统测量范围，可靠的迎角、侧滑角、总压、静压等飞行大气数据是制约先进战斗机过失速机动中飞行控制的关键因素。以中国推力矢量验证机为对象，基于过失速机动飞行试验的数据，开展大气参数估计与验证研究。结合过失速机动的时间与空间特性，研究了基于风速、地速、空速矢量和惯性姿态、导航参数的大气参数融合计算方法；针对过失速大迎角状态下飞机周围气流非定常、模型非线性导致的融合大气参数误差的复杂特性，进一步构建深度神经网络，对机动状态融合迎角、侧滑角的强非线性误差进行拟合。仿真和飞行试验表明：该方法可在大迎角飞行状态下实现主要大气参数的融合估计，过失速机动过程中融合迎角误差优于2.3°，融合得到的大气参数可为过失速大迎角机动飞行控制提供可靠的大气参数状态反馈。     

部署retro-GEO巡视器的月球借力飞行轨道分析

retro-GEO是指逆行（retrograde）地球静止轨道（geostationary Earth orbit, GEO），该轨道与GEO轨道高度相同或相近，但倾角为180°，安装在retro-GEO卫星上的巡视器可每12h对GEO带空间资产附近碎片环境安全预警。直接西向发射retro-GEO卫星存在地面测控和发射能耗较大的困难。基于平面四体模型，为降低设计变量敏感性，以近月点参数为设计变量，建立了部署retro-GEO巡视器的月球借力飞行轨道设计模型，利用轨道动力学模型延拓策略，得到该类轨道绕月后返回地球飞行时长只能约为114.79h，该结论可用于求解该类轨道高精度轨道动力学模型解。     

Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

双模块下颌式内转进气道/圆锥前体一体化布局研究

为实现三维内转进气道的内收缩流场与圆锥前体的外压缩流场的良好匹配，提出了一种双模块下颌式内转进气道/圆锥前体(Double-modules Chin Inward-turning Inlet and Conical Forebody，DCII/CF)一体化设计方法，获得一种新颖的双发并置、侧向安装的DCII/CF一体化布局。针对该布局形式，开展了DCII/CF一体化构型与传统的单模块内转进气道/圆锥前体(Single-module Inward-turning Inlet and Conical Forebody，SII/CF)一体化构型的数值对比研究。结果表明：DCII/CF一体化布局不仅为内转进气道提供了优秀的前体附面层排移效果，还有效避免了传统SII/CF布局中前体附面层与进气道内部流场之间的相互干扰。在Ma∞=6.0设计状态，DCII/CF一体化布局的进气道总压恢复系数相较传统的SII/CF布局有了显著提高，从0.403提高至0.482；但由于前体附面层的排移，该布局的捕获流量略有降低， SII/CF的流量系数为0.956，该布局则为0.917。而在非设计状态，该布局形式同样具备较好的总压恢复性能，在Ma∞=5.0与Ma∞=4.0的总压恢复系数分别达到了0.586和0.682，明显高于SII/CF的总压恢复系数0.507和0.619。     

27-day variation in solar-terrestrial parameters: Global characteristics and an origin based approach of the signals

The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ～27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ～27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation.