固体火箭发动机性能蜕变的压强补偿

介绍了采用缩小喷管喉径的方法，对固体火箭发动机燃烧室压强和推力进行补偿，以达到延长发动机使用寿命的目的。     

亚,超声速旋涡流动特征的定性分析研究

本文研究了沿其轴向运动的亚声速和超声速旋涡的性状，指出两者完全不同。在加速区，于涡轴附近，亚声速旋涡的横截面流线即横截面上的速度场的向量线为由外向内转的稳定螺旋点形态，空间流线沿其轴向是收缩的，而超声速旋涡的横截面流线为由内向外转的不稳定螺旋点形态，空间流线沿其轴向是散开的。在减速区，两者的情况也恰好相反，此外，当旋涡由加速区过渡到减速区时，两者横截面流线方程在涡轴附近的Ｈｏｐｆ分叉情况也不同，亚     

热防护系统高温纤维隔热毡传热及有效热导率分析

针对重复使用运载器热防护系统纤维隔热毡内部导热和辐射的耦合换热问题进行了分析,应用有限差分法建立了纤维隔热毡的数值分析模型.通过数值求解传热方程,计算了稳态的有效热导率.计算结果表明辐射和气体传导是纤维隔热毡内的主要传热方式,辐射作用随压力和试样密度的增加而降低,在试样温度高的一侧辐射是主要的传热方式,而在温度低的一侧气体传导为主要的传热方式;试样的有效热导率随纤维的平均直径、压力和温差的增加而增加,随试样密度的增加而降低.本文的计算结果与文献中的实验结果吻合较好,可以为纤维隔热毡及热防护系统的优化设计提供理论参考.     

The magnetotail and substorms

The tail plays a very active and important role in substorms. Magnetic flux eroded from the dayside magnetosphere is stored here. As more and more flux is transported to the magnetotail and stored, the boundary of the tail flares more, the field strength in the tail increases, and the currents strengthen and move closer to the Earth. Further, the plasma sheet thins and the magnetic flux crossing the neutral sheet lessens. At the onset of the expansion phase, the stored magnetic flux is returned from the tail and energy is deposited in the magnetosphere and ionosphere. During the expansion phase of isolated substorms, the flaring angle and the lobe field strength decrease, the plasma sheet thickens and more magnetic flux crosses the neutral sheet.In this review, we discuss the experimental evidence for these processes and present a phenomenological or qualitative model of the substorm sequence. In this model, the flux transport is driven by the merging of the magnetospheric and interplanetary magnetic fields. During the growth phase of substorms the merging rate on the dayside magnetosphere exceeds the reconnection rate in the neutral sheet. In order to remove the oversupply of magnetic flux in the tail, a neutral point forms in the near earth portion of the tail. If the new reconnection rate exceeds the dayside merging rate, then an isolated substorm results. However, a situation can occur in which dayside merging and tail reconnection are in equilibrium. The observed polar cap electric field and its correlation with the interplanetary magnetic field is found to be in accord with open magnetospheric models.     

航空发动机燃油与控制系统的研究与展望

归纳和分析了国内外军用航空发动机燃油与控制系统的研制现状和今后的发展方向 ,简要介绍和评述了主燃油控制、加力燃油控制、尾喷口控制、防喘控制、发动机状态监视 ,特别是FADEC系统的技术特点、方案选择和研究动向。从中可以看出 ,这些方面的技术进步推动了航空发动机的发展     

The Genesis Solar-Wind Collector Materials

Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high purity materials will be exposed to the solar wind and then returned to Earth for laboratory analysis. There is a suite of fifteen types of ultra-pure materials distributed among several locations. Most of the materials are mounted on deployable panels (‘collector arrays’), with some as targets in the focal spot of an electrostatic mirror (the ‘concentrator’). Other materials are strategically placed on the spacecraft as additional targets of opportunity to maximize the area for solar-wind collection. Most of the collection area consists of hexagonal collectors in the arrays; approximately half are silicon, the rest are for solar-wind components not retained and/or not easily measured in silicon. There are a variety of materials both in collector arrays and elsewhere targeted for the analyses of specific solar-wind components. Engineering and science factors drove the selection process. Engineering required testing of physical properties such as the ability to withstand shaking on launch and thermal cycling during deployment. Science constraints included bulk purity, surface and interface cleanliness, retentiveness with respect to individual solar-wind components, and availability. A detailed report of material parameters planned as a resource for choosing materials for study will be published on a Genesis website, and will be updated as additional information is obtained. Some material is already linked to the Genesis plasma data website (genesis.lanl.gov). Genesis should provide a reservoir of materials for allocation to the scientific community throughout the 21st Century. This revised version was published online in August 2006 with corrections to the Cover Date.     

复合材料锥壳0°铺层的自动铺放成型方法研究

研究了一种基于自动铺带技术的复合材料锥壳0°铺层成型方法：根据锥壳构件尺寸将等宽预浸带数控分切成预定尺寸的直角梯形预浸带片，按特定方式铺放到锥壳表面并使每两片拼成一个等腰梯形单元，多个等腰梯单元形构成锥壳的0°铺层；并针对这种成型方法设计了一种实现锥壳0°铺层自动成型的装置。采用该方法及其设备可以实现锥壳0°铺层的自动化制造，提高成型效率、降低废料率、稳定工艺质量，降低装备制造成本。     

欧拉方程多重网格方法及三维跨声速大迎角流动数值计算

本文给出一种粗、细网格时间步长可调整匹配至最优组合的多重网格方法以获得在最细网格上最大的加速收敛效益，二重网格中节省机时可达３５％。文中的数值方法可用于飞行器跨声速大迎角无粘有旋的涡干扰流场的模拟研究。     

气膜冷却流场的实验研究和数值模拟的分析

用Ｘ型双丝热线探头对扇形气膜孔射流下游流场的测量结果表明，湍流因射流的注入而显著增强，并存在十分明显的各向非同性。传统的应力和速度梯度的涡粘关系仍然适用于气膜冷却流场，但应该在不同的方向上分别对湍流粘性系数进行修正。标准ｋ－ε湍流模型可成功地模拟孔内流动和流向倾角α较小时的掺混气膜冷却流场，但在α较大时的孔中线附近区域内的流场模拟是不成功的，并导致冷却效率的模拟失败。     

稳态周向混合畸变对压气机特性和流场的影响

用完全径向平衡方程加多扇平行压气机模型处理复杂畸变流场的方法，计算出进口流场组合参数畸变对压气机特性和性能的影响，并得出了压气机在进口畸变条件下流场的详细情况。