Solar Gamma-Ray Spectroscopy

Interactions of ions accelerated in solar flares produce gamma-ray lines and continuum and neutrons. These emissions contain a rich set of observables that provides information about both the accelerated ions and the environment where the ions are transported and interact. Ion interactions with the various nuclei present in the ambient medium produce gamma-ray lines at unique energies. How abundance information is extracted from the measurements is discussed and results from analyses of a number of solar flares are presented. The analyses indicate that the composition of the ambient gas where the ions interact (typically at chromospheric densities) is different from that of the photosphere and more like the composition of the corona, exhibiting low-FIP elemental enhancements that may vary from flare to flare. Evidence for increased Ne/O and the photospheric ³He abundance is also discussed.     

The Local Bubble and Interstellar Material Near the Sun

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff, has a bulk velocity of ∼19 km s⁻¹ in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet flow direction is included.     

Stellar flares

Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed.     

基于改进A^*算法的无人机快速轨迹规划方法

针对旋翼无人机在三维障碍物环境中自主飞行时路径搜索速度慢、轨迹生成通常忽略无人机动力学特性的问题,发展一种基于改进A^*算法并同时考虑无人机动力学特性和运动学性能的快速轨迹规划方法。首先,在三维障碍物环境中运用改进A^*算法通过剔除部分网格节点降低A^*算法的节点计算量,提升算法的路径搜索速度;其次,以最小化飞行轨迹的四阶导数作为目标函数,以路径点处的位置、速度、加速度等各阶导数作为约束条件优化飞行轨迹;最后,在三维障碍物环境中对比A^*算法改进前后的路径搜索结果,并对优化的飞行轨迹进行仿真飞行测试。结果表明:改进A^*算法大幅降低了A^*算法的节点计算量,显著提升了路径搜索速度;且无人机能够始终以较小位置误差沿优化轨迹光滑连续飞行。     

10 Gbit/s伪随机序列光纤通信系统PMD补偿

光纤通信线路检测到的电功率随差分群延迟变化,可作为PMD补偿的反馈控制信号。给出了这一变化关系的理论计算和曲线并通过实验验证这一关系,确定电压信号与DGD的变化关系。建立了一套完整的实验系统,并考虑了影响反馈电压信号的多种因素以及减小这些影响的措施。通过眼图给出的实验结果说明了补偿的效果,还通过误码测试仪测量了补偿前后的接收灵敏度的改变以定量说明补偿的效果,最后比较了不同情况下的补偿结果。     

共轴式直升机旋翼气动干扰对航向操纵的影响

利用共轴式旋翼风洞实验结果，结合轻型共轴式直升机M16飞行中的现象，分析了上下旋翼气动干扰对共轴式直升机过渡飞行中航向操纵的影响。介绍了直升机由悬停转入垂直上升、平飞中加减速和转入爬升与下滑等过程中，由于上下旋翼干扰发生了变化，使直升机航向发生偏转后飞机的反应情况，以及在这种情况下应进行的相应操纵。所得结果对研究共轴式直升机的操稳特性有重要意义。     

翼型动失速和非定常载荷的综合翼型数据方法

本文给出受迫谐振翼型的动失速工程估算方法。本方法基于凤洞试验，综合分析翼型动、稳态特性之间的差别与动、稳态条件之间的关系，建立一套估算动、稳态特性之间差别的经验公式，修正稳态特性，得到相应的动态特性。用本方法计算了三种翼型不同动态条件（包括深失速和后掠）的动失速特性，并与测量和文献结果进行了比较，结果符合得相当好。     

有效载荷／运载火箭耦合分析的频域方法

盘算尖响函数综合技术导出了用耦合频响函数和无有效载荷的运载火箭界面加速度响应表示的有效载荷／运载火箭耦合动力分析的频域方法，给出了以自由界面的运载火箭模态分数放自由界面或固定界面有效载荷模态参数构成的耦合频响函数表达式。     

直升机涡环状态试验数据处理研究

采用神经网络误差反向传播算法,以旋翼涡环状态试验数据为基础,研究了桨叶负扭度对直升机涡环状态特性的影响,分析了负扭度变化对旋翼扭矩、拉力平均值及脉动幅度的影响。计算结果表明,神经网络模型能够准确预测桨叶负扭度对直升机涡环状态的影响。