Energetic Particles Investigation (EPI)

The Energetic Particles Investigation (EPI) instrument operates during the pre-entry phase of the Galileo Probe. The major science objective is to study the energetic particle population in the innermost regions of the Jovian magnetosphere — within 4 radii of the cloud tops — and into the upper atmosphere. To achieve these objectives the EPI instrument will make omnidirectional measurements of four different particle species — electrons, protons, alpha-particles, and heavy ions (Z > 2). Intensity profiles with a spatial resolution of about 0.02 Jupiter radii will be recorded. Three different energy range channels are allocated to both electrons and protons to provide a rough estimate of the spectral index of the energy spectra. In addition to the omnidirectional measurements, sectored data will be obtained for certain energy range electrons, protons, and alpha-particles to determine directional anisotropies and particle pitch angle distributions. The detector assembly is a two-element telescope using totally depleted, circular silicon surfacebarrier detectors surrounded by a cylindrical tungsten shielding with a wall thickness of 4.86 g cm^-2. The telescope axis is oriented normal to the spherical surface of the Probe's rear heat shield which is needed for heat protection of the scientific payload during the Probe's entry into the Jovian atmosphere. The material thickness of the heat shield determines the lower energy threshold of the particle species investigated during the Probe's pre-entry phase. The EPI instrument is combined with the Lightning and Radio Emission Detector (LRD) such that the EPI sensor is connected to the LRD/EPI electronic box. In this way, both instruments together only have one interface of the Probe's power, command, and data unit.     

Broadening of Fe X (6374 Å) profiles above the limb in a coronal hole

Profiles of the visible Fe X (6374 Å) coronal emission line as a function of height above the limb were obtained out to 1.16 solar radii in a coronal hole using the NSO/Sacramento Peak Observatory Coronagraph, Universal Spectrograph and a CCD camera. These are the first coronal line profiles obtained as a function of height in a coronal hole from the ground. Analysis of the line widths suggests a large component of nonthermal broadening which increases with height ranging from 40 to 60 km/s, depending upon the assumed temperature or thermal component of the profile.     

高精度光纤陀螺高带宽信号检测方案

研究兼顾静态性能和力学环境适应性的信号检测方案是高精度光纤陀螺实用化的迫切要求.分析了高精度光纤陀螺全数字闭环信号检测过程,推导了系统的闭环传递函数.一般的基频调制使检测系统的采样周期长、带宽低,反馈不能很好地补偿因力学环境产生的高频噪声信号,会破坏系统闭环,产生较大的动态误差.设计了三倍频调制/解调数字闭环信号检测方案,使采样周期是基频调制方案的1/3,有效提高了系统带宽.两种方案的力学环境实验和静态实验结果对比说明,三倍频方案明显提高了高精度光纤陀螺的力学环境适应性,同时静态性能不受影响,能够满足实际应用的要求.      

Daytime VHF amplitude scintillations recorded at an Indian low-latitude station,Waltair (17.7°N, 83.3°E) during 1997–2003

In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased.     

基于DDPG算法的变体飞行器自主变形决策

针对变体飞行器的自主变形决策问题,提出了一种基于深度确定性策略梯度(DDPG)算法的智能二维变形决策方法。以可同时变展长及后掠角的飞行器为研究对象,利用DATCOM计算气动数据,并通过分析获得变形量与气动特性之间关系;基于给定的展长和后掠角变形动力学方程,设计DDPG算法学习步骤;针对对称和不对称变形条件下的变形策略进行学习训练。仿真结果表明:所提算法可以快速收敛,变形误差保持在3%以内,训练好的神经网络提高了变体飞行器对不同飞行任务的适应性,可以在不同的飞行环境中获得最佳的飞行性能。      

Cf/Al复合材料管件的真空液相成型工艺研究

以高模高强碳纤维M40J(6K)增强铝基复合管为研究对象，研究了真空反压液相浸渗工艺中，纤维束丝分散技术、预制件压缩强度提高技术及碳纤维涂层对管件成型及性能的影响。结果表明：SiCp可以起分散作用，有利于浸渍；加入10％的偏磷酸盐的预制件经680℃真空去胶后的压缩性能满足浸渗要求，纤维保持了较好的平直度且分布均匀。C-Al2O3涂层对复合材料的性能有较大影响，经涂层处理后的预制件所制备出的复合材料的强度比未经涂层处理的提高了13％左右。所制备的复合材料的比强度、比模量较高，密度小于2．5g／cm^3。     

基于协调权的案例学习群决策分类方法

基于案例学习的决策方法具有易于理解、贴近 实际决策过程的优点,成为当前决策领域的一个研究热点。文中针对如何有效地集成不同决 策专家提供的案例信息,提出了一种基于协调权的案例学习群决策模型用以解决多属性分类 决策问题。该方法首先针对各决策者给出不同案例数据,通过构建混合整数规划模型,识别 出具有一致案例信息重要度最大化的典型案例集。然后设计了分类阈值远离程度最大化模型 ,以此确定兼容各个决策者案例信息的指标权重（协调权）和最优分类阈值,由此构建一致 性的效用函数并应用获得的阈值进行分类决策。最后通过案例研究以及与其他模型的比较分 析,验证了方法的可行性。     

单片机控制无刷直流电动机速度伺服系统

介绍了一种稀土永磁无刷直流方波电动机速度伺服系统，该系统以８０９８单片机为核心，外加ＧＡＬ芯片构成控制器，主回路开关器件采用ＩＧＢＴ，用ＥＸＢ８４０驱动，组成功率变换电路，实现了ＰＷＭ波单极半调制方式的电机伺服控制。     

基于故障行为的惯导产品贮存寿命试验设计

以典型惯导产品加速度计贮存寿命评估为例,提出了一种基于故障行为模型的加速退化试验设计方法,解决了缺乏预试验数据情况下试验应力水平设计的问题。在通过对产品特性和主机理分析基础上,确定表征产品贮存寿命特征参数及试验应力,构建了考虑材料等分散性的加速度计故障行为模型,用以描述参数加速时变规律的特性。在试验应力最高水平确定的情况下,基于给定置信度和故障行为模型,以高应力水平下退化量的置信下限与低应力水平下退化量的置信上限不交叉为原则,采用基于仿真的加速退化试验设计方法,优化确定低应力和中间应力水平,从而设计给出试验剖面,并给出了加速退化试验方案优选流程,最终从备选方案集中确定加速度计试验最优方案。通过实际案例分析,验证了该方法的有效性。      

微型飞行器低雷诺数流场显示试验研究

在南航非定常风洞内,对一盘状微型飞行器的气动特性进行了测力和流场显示实验,给出了不同迎角下微型飞行器的空间流场显示结果.研究表明:随着迎角的增加,在机翼上表面开始形成前缘分离涡,并且前缘涡的尺度和强度不断增加.迎角继续增大,前缘涡首先在后缘开始破裂,并不断前移,最终导致微型飞行器的失速.模型上前缘分离涡的形成、发展和破裂是导致盘状微型飞行器气动力特性产生变化的根本原因.