基于遗传算法的涡扇发动机多变量加速寻优控制

研究了变几何涡扇发动机不等式约束下的遗传算法最优加速控制规律，在全飞行包线内进行了仿真计算。通过分析多变量变几何涡扇发动机加速过程的特点和性能要求，用离散化加速模型结合遗传算法，使得加速过程最优。仿真计算表明该控制律可以保证变几何涡扇发动机在全飞行包线内稳定工作，且加速时间最短。     

惯导平台式重力测量技术实现及应用

详细阐述了解析方位双轴惯导平台式重力测量的工作原理,并通过基于方位余弦积的惯导力学编排解决了极区工作问题。在常规平台式重力测量数据处理方法的基础上,针对高动态环境提出了基于Kalman滤波的运动扰动修正方法。在此基础上研制了ZL11-1A型国产惯导平台式海洋重力仪。通过与国外主流重力仪产品海上同船作业比对,结果表明,该型重力仪在高海况下测量精度依然优于1mGal,满足重力测量作业要求。     

新型磁悬浮振动陀螺的设计与分析研究

振动陀螺是一种利用哥氏效应检测角速度的传感器,其谐振子的结构精度和阻尼均匀性限制了陀螺性能的提升。为减小谐振子结构与支撑锚点的影响,提出了一种全新概念的磁悬浮振动陀螺。该陀螺利用电磁悬浮的方法将谐振子悬空,从而简化了谐振子为无支撑锚点的集中质量块,降低了其结构精度要求,消除了机械结构阻尼,最终达到提升陀螺性能的目的。基于经典振动陀螺模型,理论分析了磁悬浮振动陀螺的基本工作原理,并说明了谐振子误差对陀螺性能的影响规律,设计了新型磁悬浮振动陀螺的结构,并对该结构的磁感应强度进行了仿真分析。仿真结果证明,悬浮质量块振动稳定,具有较好的磁场均匀性。最后对陀螺样机进行了测试,其固有频率为20Hz,标度因子约为1.6mV/[(°)/s],测试结果验证了所提磁悬浮振动结构的陀螺效应。     

Acceleration of interplanetary pick-up ions and anomalous cosmic rays

It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath.     

电磁测力系统研究

介绍了电磁测力系统中静磁场分析与优化、通电线圈位置控制方法及提高线性度的自校准方法。运用Maxwell 3D进行仿真计算，得到了相对优化的磁密及磁均匀性，通过控制通电线圈在磁场中位置及分段线性微分技术，提高了电磁测力准确度。构建了试验装置，对比试验数据表明，该研究措施对于提高电磁测力准确度取得了较好效果。     

螺旋相位板生成涡旋电磁波仿真研究

涡旋电磁波的产生方式有多种,使用涡旋相位板即为其中重要的一种方式。该文对螺旋相位板产生涡旋电磁波的情况进行了仿真.通过仿真。给出了在喇叭天线口面上覆盖螺旋相位板时生成的涡旋电磁波的幅度相位分布。     

小型电磁辐射敏感度自动测试系统的设计

介绍电磁辐射敏感度自动测试系统组成、工作原理和设计方法，叙述了硬件配置、系统控制、数据采集处理等软件设计。其中较详细地介绍了光纤式场强数据采集部分的设计。     

振动传感器的微加速度动态校准

阐述了高灵敏度振动传感器在超低频微小加速度下进行动态校准的校准装置工作原理、校准方法 ,分析了其校准不确定度。该装置采用曲率半径为 10m的虚拟摆结构 ,从较强的环境干扰噪声中利用数字滤波技术成功地拾检微弱振动信号 ,使微小标准加速度获得复现。该装置可在 (0 .0 0 1～ 0 .1)Hz超低频率范围内和 (1× 10 -6～ 1× 10 -2 )m s2 微小加速度范围内实现高准确度激光绝对校准和比较法校准 ,其校准不确定度达 0 .5%。     

Electromagnetic waves observed by Venus Express at periapsis: Detection and analysis techniques

The magnetometer on Venus Express was designed to be able to obtain 128 Hz samples of the magnetic field from two sensors in a gradiometer configuration. This mode is used around periapsis to determine whether the signals reported at low altitudes near 100 Hz, had the properties of electromagnetic waves generated by electric discharges in the Venus atmosphere. The lack of a magnetic cleanliness program and the shortness of the magnetometer boom make this a challenging measurement. Fortunately the signals are sufficiently strong that they can be easily resolved with rather straightforward analysis techniques.     

Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.