飞行器级间段跨声速脉动压力特性试验

通过脉动压力风洞试验测量，对比分析了跨声速（马赫数介于0.75~1.2）不同锥角和锥长大小的级间段对锥柱外形飞行器局部脉动压力的影响规律。结果表明，肩部脉动压力主要由以低频为主导的激波振荡所致，能量集中在100 Hz左右的窄带区间，且表现为随着马赫数增加，脉动压力系数峰值先增大后减小，并随着肩部激波的后移而不断向后推移。此外，通过对比分析5种不同锥角模型（10°、12.7°、15.3°、20°、25°）的脉动压力系数最大值发现，随着锥角的增加，脉动压力表现出当锥角小于15°时先平缓增加，随着锥角增大脉动压力系数增加幅度进一步加大的趋势。对比分析不同锥长模型的结果发现，锥长对局部脉动压力的最大峰值几乎没有影响，影响的只是脉动压力在肩部作用区域的大小以及峰值出现的马赫数范围，且表现为锥柱级间段越长其作用范围越大，对应于峰值的马赫数区间越宽。     

内埋武器机弹分离相容性研究进展综述

为满足新型有人或无人作战飞机高隐身、高速和高机动性等要求，作战飞机普遍采用武器内埋挂载方式。当高速气流流过内埋武器舱的空腔时，将引发边界层分离、舱口附近会存在复杂的剪切流动、舱内会产生极为恶劣的噪声环境等非定常流动现象，这些复杂的非定常流动现象严重影响内埋武器机弹分离相容性（ASSC）。首先，给出内埋武器机弹分离相容性的重要研究意义；接着，重点介绍内埋武器机弹分离相容性的研究进展；最后，论述和总结了国内外采用4种方法（理论分析与建模、风洞试验、数值模拟和飞行试验）研究内埋武器机弹分离相容性及其流动控制方法的进展，指出内埋武器机弹分离相容研究存在的主要问题，并给出几点建议。     

Classification of solar wind structures and intense geomagnetic storm alarms with self-organizing maps

Intense geomagnetic storms (D_st < −100 nT) usually occur when a large interplanetary duskward-electric field (with Ey > 5 mV m⁻¹) lasts for more than 3 h. In this article, a self-organizing map (SOM) neural network is used to recognize different patterns in the temporal variation of hourly averaged Ey data and to predict intense storms. The input parameters of SOM are the hourly averaged Ey data over 3 h. The output layer of the SOM has a total of 400 neurons. The hourly Ey data are calculated from solar wind data, which are provided by NSSDC OMNIWeb and ACE spacecraft and contain information on 143 intense storms and a fair number of moderate storms, weak storms and quiet periods between September 3, 1966 and June 30, 2002. Our results show that SOM is able to classify solar wind structures and therefore to give timely intense storm alarms. In our SOM, 21 neurons out of 400 are identified to be closely associated with the intense storms and they successfully predict 134 intense storms out of the 143 ones selected. In particular, there are 14 neurons for which, if one or more of them are present, the occurrence probability of intense storms is about 90%. In addition, several of these 14 neurons can predict big magnetic storm (D_st  −180 nT). In summary, our method achieves high accuracy in predicting intense geomagnetic storms and could be applied in space environment prediction.     

CONTOUR DESIGN AND PRACTICE FOR A LOW RADAR CROSS SECTION VEHICLE

ＣＯＮＴＯＵＲＤＥＳＩＧＮＡＮＤＰＲＡＣＴＩＣＥＦＯＲＡＬＯＷＲＡＤＡＲＣＲＯＳＳＳＥＣＴＩＯＮＶＥＨＩＣＬＥＺｈａｎｇＺｈｏｎｇａｎ；ＷａｎｇＬｕｅ（ＲｅｓｅａｒｃｈＩｎｓｔｉｔｕｔｅｏｆＰｉｌｏｔｌｅｓｓＡｉｒｃｒａｆｔ，ＮａｎｊｉｎｇＵｎｉｖｅ...     

彩色氦气泡在风洞试验中的应用

彩色氦气泡流动显示是一极好的新技术。在风洞中应用彩色氦气泡进行流动显示已于1984年3月在哈尔滨空气动力研究所实现了,获得了丰富多采的彩色迹线,摄制了清晰的彩色录象和彩色照片。不久之后,进行了轿车、面包车、高楼、船舵、鱼鳞波表面、细长体、圆柱体、降落伞和各种飞机模型的试验。 本文描述了彩色氦气泡流动显示技术,介绍了在风洞中进行流动显示的一般装置、基本原理和应用。     

EXPERIMENTAL STUDY OF TURBULENT WINGBODY JUNCTION AND WAKE FLOW

ＥＸＰＥＲＩＭＥＮＴＡＬ　ＳＴＵＤＹ　ＯＦ　ＴＵＲＢＵＬＥＮＴ　ＷＩＮＧＢＯＤＹ　ＪＵＮＣＴＩＯＮ　ＡＮＤ　ＷＡＫＥＦＬＯＷＫａｎｇＨｏｎｇｗｅｎ；ＦａｎＭｅｎｇ；ＷｅｉＺｈｏｎｇｌｅｉ（ＤｅｐａｒｔｍｅｎｔｏｆＭｅｃｈａｎｉｃｓ，ＰｅｋｉｎｇＵｎｉ...     

PROBLEMS OF WINDBLAST

ＰＲＯＢＬＥＭＳＯＦＷＩＮＤＢＬＡＳＴＺｈａｎｇＹｕｎｒａｎ；ＷｕＧｕｉｒｏｎｇ（ＩｎｓｔｉｔｕｔｅｏｆＳｐａｃｅＭｅｄｉｃｏ－Ｅｎｇｉｎｅｅｒｉｎｇ，Ｂｅｉｊｉｎｇ，Ｃｈｉｎａ，１０００９４）ＰＲＯＢＬＥＭＳＯＦＷＩＮＤＢＬＡＳＴ￥ＺｈａｎｇＹｕｎ...     

SEPARATION CONTROL FOR THE OUTWING OF A STRAKE－WING BY ROTATING CONE PLACED NEAR THE LEADING EDGE

ＳＥＰＡＲＡＴＩＯＮＣＯＮＴＲＯＬＦＯＲＴＨＥＯＵＴＷＩＮＧＯＦＡＳＴＲＡＫＥ－ＷＩＮＧＢＹＲＯＴＡＴＩＮＧＣＯＮＥＰＬＡＣＥＤＮＥＡＲＴＨＥＬＥＡＤＩＮＧＥＤＧＥ￥ＬｕＺｈｉｙｏｎｇ（ＢｅｉｊｉｎｇＵｎｉｖｅｒｓｉｔｙｏｆＡｅｒｏｎａｕｔｉｃｓａｎ...     

Working group 3: Coronal streamers

The working group on coronal streamers convened on the first day of the 2nd SOHO Workshop, which took place in Marciana Marina, Isola d'Elba, 27 September –1 October 1993. Recent progress in streamer observational techniques and theoretical modeling was reported. The contribution of streamers to the mass and energy supply for the solar wind was discussed. Moreover, the importance of thin electric current sheets for determining both the gross dynamical properties of streamers and the fine-scale filamentary structure within streamers, was strongly emphasized. Potential advances to our understanding of these areas of coronal physics that could be made by the contingent of instruments aboard SOHO were pointed out.