少烟高固体含量丁羟推进剂配方研究

通过理论计算和初步实验，证实少烟高固体含量丁羟推进剂是实用的。研究表明，铝粉含量对Ｉ＾０ｓｐ、燃气中Ａｌ２Ｏ３含量、ρ有显著影响，降低铝粉含量，比冲大幅度下降；ＲＤＸ代替部分ＡＰ，烯气中ＨＣ１、Ｈ２Ｏ含量降低，但（ＣＯ＋Ｈ２）含量增加，增加了燃气的二次火焰，低铝粉配方中，ＲＤＸ不能提高比冲；增加固体含量，能明显提高比冲和密度，是提高能量特性的有效途径；提高压强，比冲增加，燃气中Ｈ２Ｏ％和ＣＯ＋Ｈ２     

硼粉在推进剂中应用研究

对硼粉与粘合剂要容性，硼粉表面处理及其在固体推进剂配方中的应用进行了研究。表明硼粉中杂质含量是影响其与粘合剂相容性的重要因素。     

空间可展结构卷尺铰链的设计与分析

卷尺弹簧是形状类似钢卷尺的一种构件,是一种单层开口柱面壳。可以利用其壳体屈曲性能,设计和研制出一种铰链结构。这种铰链结构具有独特的力学性能,它可以利用折叠时积聚的弹性应变能实现结构的自动展开而不需要其它的动力装置;在展开之后,又能够靠自身的刚度提供大型可展结构所需的锁定力,而不需要另外加设锁定装置。这种铰链可用于大型航天可展结构中,如可展的太阳翼等。     

复合固体推进剂脱模型的研究

研究了复合固体推进剂颗粒界面的脱湿机理。运用弹笥－粘弹性对应笥原理建立了复合固体推进剂粘弹性脱湿两相球颗粒分析模型，利用能量守恒得到了脱湿时间的控制方程，并导出了以界面粘结能表示的临界脱湿应力的简洁表达式。计算结果表明，颗粒的体积分数、粒径和加载速率对脱湿时间有显著的影响。     

空间太阳能发电和微波与电离层相互作用

本文第一部分研究了空间太阳能热发电，基于所提的评价动力系统的准则，比较了三种热力学系统，并给出了一些参数变化对闭式回热Ｂｒａｙｔｏｎ循环系统的影响，本文第二部分对微波速对电离层中电子的加速和受热进行了数值研究，得出了一些结果。     

Present status of very high energy gamma ray observations

Recent results from observations of the southern sky objects are summarized. The unpulsed, persistent very high energy (VHE) emission from the gamma ray pulsars, the Crab and PSR1706-44, is discussed. A process of energetic electrons ejection may take place from a variety of other objects such as from X-ray binaries, similarly to the pulsars. Such an effect may be seen also in pair halos around extragalactic VHE gamma ray emitters, the observational study of which is still in a preliminary stage in the southern hemisphere.     

飞机座舱盖热疲劳试验系统的热经济分析

 依据热经济分析理论 ,并结合对飞机座舱盖热疲劳试验系统的运行模拟 ,找出了系统的关键能耗元件 ,针对它的热惯性是造成系统潜在高耗能的主要原因 ,提出了在关键能耗元件加隔热层的改进方案。对某型号座舱盖 100飞行小时试验 ,模拟计算结果的比较表明 ,改进方案能使试验能耗下降 37%。     

复合材料切削表面粗糙度测试方法的研究

利用先进的TalyScan150型表面粗糙度测试仪，采用不同测试手段和不同测试参数对复合材料切削试样表面进行测量、计算，得出复合材料切削表面粗糙度；通过比较分析，得到了适用于复合材料切削表面粗糙度测试的手段及参数，建立了复合材料切削表面粗糙度的测试方法，该方法为全面评价复合材料表面质量提供了测试基础。     

新型热流计测量技术的探索研究

目前的热流计在测量热量时需要测量供热管道的流量以及进出口温度,然后再对其进行积分计算.其技术非常复杂,而且精度低,仪器成本高,难以普及.为了解决这一系列问题,本文主要依据能量守恒定律提出了一种新型的能量测量装置,并对该装置的测量原理进行了理论分析.通过数值模拟,在理论上对其进行了验证.数值模拟的结果证实该型热流计测量结果与系统流体的流量无关,这也是本测量方法不同于其它常规热流计的优点之一,摆脱了流量对能量测量的影响,同时也简化了计算过程,大大降低了成本.     

Energy flux in the Earth's magnetosphere: Storm – substorm relationship

Three ways of the energy transfer in the Earth's magnetosphere are studied. The solar wind MHD generator is an unique energy source for all magnetospheric processes. Field-aligned currents directly transport the energy and momentum of the solar wind plasma to the Earth's ionosphere. The magnetospheric lobe and plasma sheet convection generated by the solar wind is another magnetospheric energy source. Plasma sheet particles and cold ionospheric polar wind ions are accelerated by convection electric field. After energetic particle precipitation into the upper atmosphere the solar wind energy is transferred into the ionosphere and atmosphere. This way of the energy transfer can include the tail lobe magnetic field energy storage connected with the increase of the tail current during the southward IMF. After that the magnetospheric substorm occurs. The model calculations of the magnetospheric energy give possibility to determine the ground state of the magnetosphere, and to calculate relative contributions of the tail current, ring current and field-aligned currents to the magnetospheric energy. The magnetospheric substorms and storms manifest that the permanent solar wind energy transfer ways are not enough for the covering of the solar wind energy input into the magnetosphere. Nonlinear explosive processes are necessary for the energy transmission into the ionosphere and atmosphere. For understanding a relation between substorm and storm it is necessary to take into account that they are the concurrent energy transferring ways. This revised version was published online in August 2006 with corrections to the Cover Date.