真空羽流场的 N-S 和 DSMC 耦合数值模拟

根据调姿发动机真空羽流场的特点,采用差分求解Ｎ－Ｓ方程数值模拟喷管内流场,用ＤＳＭＣ方法数值模拟喷管外羽流场,得到了符合流动规律的数值模拟结果。为姿控发动机喷管设计提供了参考,并为真空羽流污染研究打下了良好的基础。     

非自模化区域内动叶叶尖间隙对气动-声学性能的影响

本文对非自模化区域内小型风机的气动－声学性能进行了实验研究,详细了在非自模化区域内动叶叶尖间隙对气动－声学性能的影响,并与自模化区域内的影响作了对比分析,得到了在非自模化区域内动叶径向间隙对气动－声学性能的修正,计算结果与实测值吻合良好。初步提示了非自模化区域内动叶叶尖间隙对气动－声学性能影响的机理。     

喷管潜入段二维两相冷流实验

建立了喷管潜入段二维两相冷流实验设备,进行了相应的实验。实验清晰地显示了在潜入喷管进口背壁凹区旋涡的产生、稳定、消失,以及粒子的冲刷、粘贴、脱落、沉积等反复作用的复杂现象,它们与流动的雷诺数、粒子的含量和尺寸、潜入喷管进口处的形状和潜入深度、背壁型面等因素有关。     

A Functionally Redundant Altimeter

A scheme to provide redundant sensor data in an automatic control system using the principle of functional redundancy is described. Normally there are three redundant radar altimeters used in the terminal phase of automatic landing of jet transport airplanes. This scheme replaces one of these altimeters with a data processing scheme based on a Kalman filter. The filter is driven by altitude rate and acceleration signals from the air data computer and vertical accelerometer. A special initialization technique employs the two altimeter signals. The feasibility of this scheme is indicated by tests in which data obtained from these several sensors during flight tests are used to drive the functionally redundant altimeter.     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Coronal Observations of CMEs

CMEs have been observed for over 30 years with a wide variety of instruments. It is now possible to derive detailed and quantitative information on CME morphology, velocity, acceleration and mass. Flares associated with CMEs are observed in X-rays, and several different radio signatures are also seen. Optical and UV spectra of CMEs both on the disk and at the limb provide velocities along the line of sight and diagnostics for temperature, density and composition. From the vast quantity of data we attempt to synthesize the current state of knowledge of the properties of CMEs, along with some specific observed characteristics that illuminate the physical processes occurring during CME eruption. These include the common three-part structures of CMEs, which is generally attributed to compressed material at the leading edge, a low-density magnetic bubble and dense prominence gas. Signatures of shock waves are seen, but the location of these shocks relative to the other structures and the occurrence rate at the heights where Solar Energetic Particles are produced remains controversial. The relationships among CMEs, Moreton waves, EIT waves, and EUV dimming are also cloudy. The close connection between CMEs and flares suggests that magnetic reconnection plays an important role in CME eruption and evolution. We discuss the evidence for reconnection in current sheets from white-light, X-ray, radio and UV observations. Finally, we summarize the requirements for future instrumentation that might answer the outstanding questions and the opportunities that new space-based and ground-based observatories will provide in the future.     

雷达罩应用5258树脂基复合材料的试验研究

通过试验研究了雷达罩所用主要材料5258环氧树脂、预浸料和复合材料制备方法，进行了这些材料及结构的拉伸、弯曲、剪切和介电常数等性能的测试，结果表明5258树脂基体制备的复合材料均具有良好的力学和电学性能，能够满足雷达罩的设计要求。     

影响某型燃机转子轴向力关键因素分析

燃气轮机转子的轴向力是燃机总体设计的重要指标之一。为了研究影响轴向力的因素,针对某型燃机,通过建立轴向力仿真平台,计算不同装机状态燃机的轴向力载荷,并结合大量整机试车与轴向力实测数据,分析影响该载荷的关键因素。研究与实测表明：运行工况、涡轮导向器喉道面积、封严结构等均构成影响轴向力的关键因素;调整封严直径、喉道面积可以大范围地调整转子轴向力,调整封严间隙值能对轴向力进行微小的调整。