模型旋翼风洞试验中变距拉杆载荷的测量

桨叶变距拉杆操纵载荷是旋翼设计的重要参数之一。在参考了常规飞机模型风洞试验测力元件及国外测量方法的基础上,研制了具有足够刚度和强度,且有较高载荷灵敏度的新式变距拉杆测力元件,解决了高刚度与高的载荷灵敏度要求这一矛盾。同时采用了信号放大技术,将其成功地应用于旋翼模型试验,并获得了操纵载荷这一重要参数     

低速闭口风洞模型张线支撑及内天平测量系统的研制

“张线支撑及内天平测量系统”已在ＦＬ－８ 闭口风洞中调试、使用。该系统使用了套管天平,套管内杆是天平与模型相连,与天平相连的套管是支撑体,张线的一端与套管的前后吊点相连,张线的另一端与风洞上转盘齿圈上的张紧机构和风洞下转盘下的配重相连。该系统的角度变化范围,模型侧吊时, α＝ ±３６０°,β＝ ±６５°,模型正吊时,α＝ ±６５°,β＝ ±３６０°实验表明：张线支撑与尾撑和腹撑相比,消除了由于支杆引起的模型振动,其支架干扰变小,试验数据质量有了进一步的提高     

弹性模型实验技术

介绍了火箭弹性模型实验技术,包括模型对火箭的质量分布、刚度分布的模拟,模型的加工制做,激振机构的研制,支撑元件的研制以及几期实验的结果综合。     

TUNNEL INTERFERENCE IN UNSTEADY POST-STALL EXPERIMENTS

ＴＵＮＮＥＬＩＮＴＥＲＦＥＲＥＮＣＥＩＮＵＮＳＴＥＡＤＹＰＯＳＴ┐ＳＴＡＬＬＥＸＰＥＲＩＭＥＮＴＳＺｈａｎｇＷｅｎｈｕａ，ＤｉｎｇＫｅｗｅｎ，ＨｕａｎｇＤａ，ＬｉＺｈｉｑｉａｎｇ，ＺｈａｎｇＱｉｎｇｌｉ（６ｔｈＤｅｐｔ．ＮａｎｊｉｎｇＵｎｉｖｅｒｓｉ...     

钝体涡激力参数的识别

涡激振是柔性结构易发生的气动弹性现象。本文通过风洞试验，研究了均匀流场中弹性支承的二维刚性模型的强激力，提出了一种识别涡激力模型中未知参数的方法。用本文的方法，进行了三种钝体模型的风洞试验。     

FL-1风洞绘图软件

本文介绍了用于 FL-1风洞实验的绘图软件结构、功能和操作。     

The nature of the luminous blue variable AG carinae

After many years of permanence at minimum, the luminous blue variable AG Car started in mid 1990 a new brightening phase. We review the spectroscopic variations of the star since 1949, and discuss the nature of the circumstellar nebula. We give evidence that, like in Car, also in AG Car dust is continuously condensing from the stellar wind. We suggest that the star could be partially reddened by the circumstellar dust, which could affect the estimates of the stellar distance. An extended HII halo is present outside the ring nebula, which should be associated with the wind of a previous cooler evolutionary stage of AG Car.     

Composition of anomalous cosmic rays and implications for the heliosphere

We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the Voyager 1 and 2 spacecraft during the period 1994/157-313 to determine several parameters of interest to heliospheric studies. We estimate that the strength of the solar wind termination shock is 2.42 (–0.08, +0.04). We determine the composition of ACRs by estimating their differential energy spectra at the shock and find the following abundance ratios: H/He = 5.6 (–0.5, ⁺0.6), C/He = 0.00048 ± 0.00011, N/He = 0.011 ± 0.001, O/He = 0.075 ± 0.006, and Ne/He = 0.0050 ± 0.0004. We correlate our observations with those of pickup ions to deduce that the long-term ionization rate of neutral nitrogen at 1 AU is 8.3 × 10^–7 s^–1 and that the charge-exchange cross section for neutral N and solar wind protons is 1.0 × 10^–15 cm² at 1.1 keV. We estimate that the neutral C/He ratio in the outer heliosphere is 1.8(–0.7, +0.9) × 10^–5. We also find that heavy ions are preferentially injected into the acceleration process at the termination shock.     

地球同步轨道高能电子增强事件预报方法

分析了地球同步轨道高能电子通量增强事件的发生规律及其与太阳风和行星际磁场参数的关系，并在此基础上建立了基于人工神经网络的高能电子增强事件模式，经实测数据检验，预报模式可以对未来1天的高能电子通量进行预报，误差为8．2％，达到了较高水平．     

汽车空调风道设计对车内噪声的影响

空调风道的设计与布置合理与否直接影响车内环境的舒适性.风道设计中要求风道的气流噪声必须控制在允许的范围内.风道中压力损失是使得车厢内产生气流噪声的原因之一,在此通过分析风道中产生压力损失的原因和对某汽车整车送风系统的计算流体力学（CFD, Computational Fluid Dynamics）分析和实际测试,说明减小风道压力损失可使车内噪声得到降低.