弹射救生系统大迎角大侧滑角气动特性工程计算方法研究

对弹射救生系统的气动特性进行了分析,发展了一套快速获取其气动特性的工程计算方法,并对某战斗机弹射救生系统的大迎角大侧滑角气动力特性进行了计算.结果表明,工程计算结果与风洞试验数据一致性良好.     

Electrostatic accelerometer with bias rejection for gravitation and Solar System physics

Radio tracking of interplanetary probes is an important tool for navigation purposes as well as for testing the laws of physics or exploring planetary environments. The addition of an accelerometer on board a spacecraft provides orbit determination specialists and physicists with an additional observable of great interest: it measures the value of the non-gravitational acceleration acting on the spacecraft, i.e. the departure of the probe from geodesic motion.     

The effect of the longitudinal propagating waves on the electron acceleration in the reconnecting current sheet

Based upon the most efficient electron acceleration near the midplane of 3D non-neutral driven reconnecting current sheet (RCS) and the electrostatic wave excitation by the drift Maxwellian distribution of electrons in Vlasov simulation, we assume that the electrostatic waves mainly propagate opposite to the reconnecting electric field and investigated how these waves affect the electron acceleration. The main results are: (1) when the electron’s velocity equals to the phase speed of the waves, they will be trapped and have the different accelerating characteristics from the untrapped electrons through solving the momentum equations of electrons analytically; (2) the test particle simulations further prove that the number of the energetic electrons decreases with the increasing intensity of unstable waves, and the distribution of the energetic electrons takes on the double power-law.     

基于光敏树脂分析的3D打印加速度传感器设计

MEMS加速度传感器所采用的硅微机械加工技术存在个性化定制、小批量生产成本方面的不足，而3D打印技术的优势就在于无需模具的自由化定制、一机多用实现低成本产品生产，3D打印的发展趋势就是实现微纳尺度结构的制造。在此背景下，采用光固化立体成型技术设计了一种3D打印压阻式加速度传感器结构。传感器基底使用耐高温光敏树脂制作，并采用丝网印刷工艺在基底表面印制导电碳浆形成应变计结构。为此，首先对耐高温光敏树脂的相关热学与机械性能进行分析。通过测试，得到该光敏树脂固化后的起始分解温度等热力学参数。其次，通过控制光敏树脂紫外光固化时间，取得了较好杨氏模量和弯曲强度的树脂，且为该加速度传感器的结构仿真优化与制作工艺提供了必需数据与重要依据。除此之外，还对所设计的碳浆应变计结构进行了测试，得到了有效灵敏系数。通过以上工作，为最终实现3D打印加速度传感器的制作做好铺垫，助力3D打印技术与MEMS传感器技术相融合。     

某型飞机后减速板抗振动损伤设计分析

某型飞机后减速板在部队使用中 ,由于振动损伤原因 ,多次出现减速板梁断裂、蒙皮裂纹等故障 ,经分析 ,确定了能抗振动疲劳的打孔加型材结构改进方案 ,并经实际飞行测试取得了满意效果。本文是对后减速板的抗振动损伤设计思想和方法进行简要介绍 ,为类似问题的处理提供借鉴。     

用影响因子评估弹射座椅多模态控制输入参数

为提供弹射座椅多模态控制输入参数选择的理论依据,通过计算机仿真,比较分析了俯仰角、滚转角、滚转角速度、下沉率、迎角、侧滑角等弹射启动时飞机状态参数对弹射轨迹(垂直方向)和安全救生高度的影响。参考评估期刊的影响因子,提出了安全高度影响因子法,并计算出在同等弹射条件下(速度和高度)各参数的平均影响因子,得出各参数对救生高度的影响程度及变化规律,确定了俯仰角、滚转角和下沉率是影响救生高度的三个主要参数。     

弹射救生用人体数学模型

 利用人体弹射试验数据建立起人体动力学特性的数学模型(简称人体数学模型)。模型的动态响应特性分析可以解决一些与弹射有关的人体工程学问题。根据人体的最大动态超调,结合椎骨强度可确定人体耐受弹射加速度的限度。从防护角度出发,分析座垫对人体受力的影响和人体响应的时相特点而要求座垫厚度必需很薄。还提出改善弹射动力和确定测试系统性能指标的依据。将模型用于弹射实践可以减少人体试验,对人体安全和研制生产都极其有利。     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.     

CME-geometry and cosmic-ray anisotropy observed by a prototype muon detector network

We analyze the cosmic-ray anisotropy observed by a prototype network of muon detectors during geomagnetic storms associated with coronal mass ejections (CMEs). The network currently consists of multidirectional surface muon detectors at Nagoya (Japan) and Hobart (Australia), together with a prototype detector at São Martinho (Brazil) which has been in operation since March, 2001. In this report, we analyze the anisotropy recorded in both the muon detector and neutron monitor (the Spaceship Earth) networks and find significant enhancements of cosmic-ray anisotropy during geomagnetic storms. Following the analysis by Bieber and Evenson [Bieber, J.W., Evenson, P. CME geometry in relation to cosmic ray anisotropy. Geophys. Res. Lett. 25 (1998) 2955–2958] for the neutron monitor data at 10 GeV, we also derive cosmic-ray density gradients from muon data at higher-energy (50 GeV), possibly reflecting the larger-scale geometry of CMEs causing geomagnetic storms. We particularly find in some events the anisotropy enhancement clearly starting prior to the storm onset in both the muon and neutron data. This is the first result of the CME-geometry derived from simultaneous observations of the anisotropy with networks of multidirectional muon detectors and neutron monitors.     

磁重联区Alfven波及新生离子的加速

利用二维混合数值模拟研究了有速度驱动、低等离子体β值情况下的磁场重联过程，结果表明磁重联过程可以产生Alfven波，该Alfven波动对重新区中的新生离子作用，使得新生离子经历投掷角散射方程，具有球壳分布特征，部分新生离子得到加速，其获得的最大能量约为4（miVA0^2/2)，此加速过程所需的加速时间在100／Ωi量级，是一个极快的加速机制，加速粒子能谱为双幂律谱。