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.     

跨声速风洞试验段低噪声壁板模型的声学试验

介绍了跨声速风洞试验段低噪声壁板模型的声学试验。实验结果表明：（1）斜孔所产生的边缘音是最主要的声源；（2）用加网和加隔片都是抑制边缘音的有效方法；（3）文献[1]介绍的低噪声壁板的方法具有实用性。     

复杂大跨屋面脉动风压风洞试验研究

介绍了复杂大跨屋面的脉动风压风洞试验研究方法和广州国际会议展览中心屋面脉动风压风洞试验的结果，并对结果进行了分析。分析表明：风压系数平均值分布规律性明显，能体现屋面流场分布情况；均方根值则在一定程度上反映出气流分离和旋涡脱落情况。复杂大跨屋面上表面主要分布为负压，迎风边缘及突出部位较大，低凹处及尾流区域较小；下表面风压分布具有钝体外形的特点，内压的大小与开门状态有关。     

旋转导弹风洞六自由度自由飞动导数实验研究

风洞六自由度自由飞实验,是国内首次开展的一项新的风洞实验研究。实验设备为0.2米×0.2米的超声速风洞,求流马赫数为2和2.5。当超声速流场建立后,将以每分钟一万多转的高速旋转导弹模型,向实验段上游发射。模型在风洞观察窗区飞行时,用高速立体摄影拍摄模型飞行姿态随时间的变化。然后根据飞行姿态记录,通过数据辨识,求得俯仰力矩系数斜率,俯仰阻尼力矩系数和马格努斯力矩系数。实验精度优于国外弹道靶自由飞实验结果,尤其是动导数数据取得了满意的结果。     

复杂地形低空三维风场数值仿真方法

设计了飞机超低空飞行的复杂山地地形,基于球绕流理论,建立了低空复杂地形及其上空三维过山气流的工程化模拟方法,并进行了算例仿真和分析.该方法可以提供低空三维风场模型,并能满足分析飞机低空飞行动力学特性的需要.     

Heliospheric Physics: Linking the Sun to the Magnetosphere

Research into the heliospheric structure and its relation to the solar boundary is at an impasse. After successful predictions by Parker about the zeroth-order behavior of the heliospheric magnetic field and the solar wind, the heliospheric community struggles to make substantive progress toward a predictive model describing the connections between the Sun and its space environment, between the closed corona and the open corona extending to the planets. This is caused by our lack of understanding of the basic processes heating the corona and transporting open magnetic field. We detail the models used to describe this connectivity, from potential field source surface models to full MHD techniques. We discuss the current limitations of both approaches. Finally, we address a recent attempt to advance our understanding beyond these limitations. At this point in time the proposed theory remains controversial in the community, but it addresses important shortcomings of current approaches outlined above.