帧转移面阵CCD电子像移补偿设计

文章通过分析像移对面阵CCD成像的影响,针对面阵CCD运动成像中影响图像MTF的速度误差和积分级数来设计具有电子像移补偿功能的面阵CCD积分时序,并完成了软件仿真和硬件电路测试,在实际CCD成像电路中验证了像移补偿时序。     

降落伞特性对伞舱系统运动稳定性的影响

建立了伞舱系统刚性连接和弹性连接时的数学模型,针对联盟号飞船回收系统进行了动力学仿真。分析了降落伞侧向力系数、吊带长度、降落伞和载荷质量比以及吊带性质对伞舱系统运动稳定性的影响,其结论可为伞舱回收系统的设计提供参考。     

周边桁架可展天线展开过程动力学分析及控制

 基于多刚体系统动力学的Lagrange方法,采用独立的Lagrange广义坐标,考虑耗散力、铰链处扭簧的驱动力及索网预张力对展开过程的影响,建立了周边桁架可展天线展开过程的动力学模型,给出了基于力控制的展开过程控制策略,得出了展开过程驱动力的变化与天线位形变化之间的关系,根据所规划好的天线展开运动得出相应的驱动力。编制了仿真程序进行算例分析,研究了初速度、阻尼及重力对天线展开过程的影响,实现了考虑驱动扭簧的刚度、关节中的阻尼、重力及索网预张力影响的周边桁架可展天线展开过程的动力学分析与控制。实验仿真结果验证了该方法的有效性。     

自旋弹头的自适应变结构控制研究

对自旋弹头实现末端机动的变质心控制系统进行了研究。采用牛顿力学方法重新建立了自旋弹头的姿态运动模型。在此基础上,采用自适应变结构控制方法设计了变质心控制系统,对弹头内部质量块的偏移运动进行控制,进而准确地控制自旋弹头的姿态运动。仿真结果表明：所设计的变质心控制系统具有快速性和较高的控制精度,实现了对自旋弹头姿态角的准确控制。     

不同初始温度下等离子体对H2/Air混合物燃烧影响

等离子体助燃过程是一个非平衡的,瞬时的,极不均匀的物理化学过程,活性粒子在等离子体助燃计算中是一个关键难题。文章建立H2/Air燃烧的化学动力学模型,计算与分析了在非平衡等离子体条件下,气体放电产生的活性粒子(O,H)和活性基(OH)在不同初始温度下对燃烧过程中参与燃烧的组分以及温度和压力的影响,为航空发动机燃烧室等离子体助燃实验研究和实际应用提供理论依据。数学模型的计算结果表明等离子体助燃可以提高反应效率,缩短延迟时间,增加燃烧温度,火焰传播速率,强烈影响H2/Air混合物燃烧效果。     

轨道运动对高轨卫星成像的影响及补偿

针对三轴稳定静止轨道气象卫星图像运动补偿技术,分析了轨道运动误差源对有效载荷成像仪成像光轴的影响.基于轨道确定数据,采用空间成像矢量修正方法,对轨道运动引起的光轴偏离进行补偿.根据高分辨率成像对光轴高指向精度的指标要求,研究了轨道确定误差和有效载荷伺服控制系统误差对图像配准精度的影响关系,并指出了进一步提高图像配准精度的措施.仿真结果表明了补偿方法的可行性.     

舰船运动对某无人机发射安全的影响研究

探讨了舰面运动(舰面纵摇、横摇和垂荡运动)对舰载无人机火箭助推发射安全的影响。数值分析表明,舰面纵摇可能导致飞机起飞后撞上甲板,是舰面运动中最危险的因素。舰面横摇对飞机离舰后最大下沉量的影响相比纵摇为小,若无人机在甲板上布置的位置适当,则可以实现安全发射。     

球形重力场下的视线动力学方程

以交会对接问题为背景,建立了球形重力场下的视线动力学方程,其简化形式可以描述平面重力场下的相对运动。该方程直接描述了视线参数和机动策略之间的关系,可广泛应用于相对运动问题的机动策略研究。     

Charged particle dynamics in the combined field of two rotating magnetic dipoles: A numerical investigation of the parametric effect on the equatorial motions

In this contribution we study some aspects of the dynamics of a charged particle in the field produced by two magnetic dipoles that rotate in circular orbits around their common center of mass under their mutual Newtonian attraction. More precisely, we numerically investigate the evolution of the regions of the particle motion on the equatorial plane of each dipole and we explore their parametric variation. We focus our investigation on those problem parameters that are related with the magnetic fields and the masses of the primaries. The obtained preliminary results show that for each particular set of the above parameters and for certain values of energy these regions are bounded, and therefore the motion of the particle is confined inside them.     

December 2006 solar extreme events and their influence on the near-Earth space environment: “Universitetskiy-Tatiana” satellite observations

The Russian microsatellite “Universitetskiy-Tatiana” was launched on Jan. 20, 2005 and was both a scientific and educational mission. Its two main aims were declared as: (1) monitoring of the energetic particles dynamics in the near-Earth space environment after solar events and during quiet times, (2) educational activities based on experimental data obtained from the spacecraft. In this paper observations acquired during Dec. 5–16, 2006, known as “Solar Extreme Events 2006”, were analyzed. The “Universitetskiy-Tatiana” microsatellite orbit permits one to measure both solar energetic particle dynamics, variations of the boundary of solar particle penetration, as well as relativistic and sub-relativistic electrons of the Earth’s outer radiation belt during and after magnetic storms. Both relativistic electrons of the Earth’s outer radiation and solar energetic particles are an important source of radiation damage in near-Earth space. Therefore, the presented experimental results demonstrate the successful application of a small educational spacecraft both for scientific and educational programs.