降落伞初始充气阶段数值模拟

首先建立了初始充气模型 ;将前体、伞绳及伞衣离散为一系列弹性连接的质量节点 ,伞衣内部流场为一维不可压流 ;最后利用模型计算了初始充气阶段伞衣形状变化、伞衣投影面积变化及伞绳张力     

Substorms in the inner plasma sheet

Thin Current Sheets (TCS) are regularly formed prior to substorm breakup, even in the near-Earth plasma sheet, as close as the geostationary orbit. A self-consistent kinetic theory describing the response of the plasma sheet to an electromagnetic perturbation is given. This perturbation corresponds to an external forcing, for instance caused by the solar wind (not an internal instability). The equilibrium of the configuration of this TCS in the presence of a time varying perturbation is shown to produce a strong parallel thermal anisotropy (T T) of energetic electrons and ions (E>50keV) as well as an enhanced diamagnetic current carried by low energy ions (E<50keV). Both currents tend to enhance the confinement of this current sheet near the magnetic equator. These results are compared with data gathered by GEOS-2 at the geostationary orbit, where the magnetic signatures of TCS, and parallel anisotropics are regularly observed prior to breakup. By ensuring quasi-neutrality everywhere we find, when low frequency electromagnetic perturbations are applied, that although the magnetic field line remains an equipotential to the lowest order in T_e/T_i, a field-aligned potential drop exists to the next order in (T_e/T_i). Thus the development of a TCS implies the formation of a field-aligned potential drop ( few hundred volts) to ensure the quasi-neutrality everywhere. For an earthward directed pressure gradient, a field-aligned electric field, directed towards the ionosphere, is obtained, on the western edge of the perturbation (i.e. western edge of the current sheet). Thus field aligned beams of electrons are expected to flow towards the equatorial region on the western edge of the current sheet. We study the stability of these electron beams and show that they are unstable to “High Frequency” (HF) waves. These “HF” waves are regularly observed at frequencies of the order of the proton gyrofrequency (f_H+) just before, or at breakup. The amplitude of these HF waves is so large that they can produce a strong pitch-angle diffusion of energetic ions and a spatial diffusion that leads to a reduction of the diamagnetic current. The signature of a fast ion diffusion is indeed regularly observed during the early breakup; it coincides with the sudden development of large amplitude transient fluctuations, ballooning modes, observed at much lower frequencies (fH+). These results suggest that the HF waves, generated by field-aligned electron beams, provide the dissipation which is necessary to destabilize low frequency (ballooning) modes.     

近地球赤道面轨道上磁性刚体卫星的混沌运动

讨论地球磁场中非自旋磁性刚体卫星在近赤道平面圆轨道上平面天平动的混沌问题.利用Melnikov方法预测出现混沌的可能性并数值验证混沌的存在性.研究表明地球磁场的周期扰动能引起卫星的混沌运动,扰动增大则混沌加强.      

三维LDV光学系统技术方案的研究

通过自行设计制造色分离器、一维发射系统、提升反射镜组针丹麦ＤＡＮＴＥＣ的二维ＬＤＶ改造为三维ＬＤＶ。提出了镀膜分光和紫光滤光片提纯相结合的最佳分色方案并研制了镀膜分色片、紫光波光片这两种关键部件。通过联调作校准试验,证明本三维ＬＤＶ系统完全达到了设计技术指标。     

基于PDCA的EWIS设计质量提升研究与应用

为了全面提升军用飞机线束及线束敷设设计质量,从设计源头根本性改善外场线路问题,从系统设计的角度出发,开展了EWIS (电气线路互联系统)设计质量控制的新流程、新方法和新技术的研究和应用。根据设计质量问题和改进需求分析结果,提出了基于PDCA (质量环)的质量控制方法,并将其应用到实践中,完善了EWIS技术文件体系,形成了EWIS精细化设计及检查验证流程,提高了设计要求的提出、实现、验证和持续完善能力,在此基础上优化了对重量特性的控制过程,极大提高了设计质量和效率,对提升飞机EWIS设计质量具有参考意义。     

液氧煤油火箭海上发射基本方案及关键技术分析

海上发射火箭在提升火箭运载能力、降低残骸坠落风险等方面具有极大优势。我国已成功实施多型固体火箭海上发射任务,相比固体火箭,液氧煤油火箭具有更高的比冲和环保性。根据液氧煤油火箭陆基发射的特点规律和固体火箭海上发射任务流程及实施方案,研究了海射系统港口基地、海上发射船、运载火箭、保障船等运行的基本方案,提出海上发射任务实施流程,分析了牵制释放、连接器零秒脱落和自动对接、无人值守推进剂加注技术在海上发射火箭中的重要意义,以及需要解决的关键技术难题。     

精密热控技术在太极一号卫星上的应用

为探测空间引力波,中国科学院提出了太极计划,其第一步是通过近地轨道卫星太极一号对核心载荷的关键技术进行验证.由于温度稳定性直接影响干涉仪测距和加速度的测量精度,太极一号卫星提出了(T±0.1)K的高精度、高稳定度温控指标.针对该指标要求设计热控方案,从热组件的选取到单机设备的应用均依照高指标进行控制.为了保证方案实施的...     

Cd1-xZnxS体系红外光谱及发射率特性

制备了Cd1-xZnxS三元系半导体材料。利用X射线衍射(XRD)对其结构进行了表征,结果表明实验所得样品均为纤锌矿结构。建立了Cd1-xZnxS混晶替位模型,根据所建模型和晶格振动理论,对Cd1-xZnxS红外光谱特性进行探讨。研究了Cd1-xZnxS三元系半导体材料红外发射率特性,Cd1-xZnxS在3~5μm波段的发射率远远低于8~14μm波段的发射率,这与材料的红外吸收机制和光谱特性有关;Cd1-xZnxS半导体材料的红外发射率随着烧结温度的提高而降低,这是由于温度升高,晶格畸变减小并逐渐趋近于完整晶格。     

金属热防护系统多层隔热材料的传热分析及参数优化

采用能量平衡方程和离散坐标法近似地建立了金属热防护系统多层隔热材料的一维稳态传热的数学模型,并利用遗传算法和纤维隔热材料的有效导热系数试验数据求解传热反问题,从而得到了模型中的纤维隔热材料的辐射衰减系数、反照率和隔热屏表面辐射发射系数。最后,由实验测得了多层隔热材料的有效导热系数,验证了采用优化参数后,多层隔热材料的传热模型的正确性。