克服旋转导弹螺旋运动的方法研究

本文结合旋转导弹自身的特点，提出了一种通过主动控制弹体内部活动质量块的运动来克服旋转弹螺旋运动的方法，这将有助于提高旋转导弹的合中精度。文中针对大气层外飞行的旋转导弹进行仿真研究，计算结果证实了该方法的有效性和可行性。     

多分支管道若干流动现象和特性的探讨

在稳定的多分支管道流动中，对于相同的主管道流量，各分支管道中可以有不同的稳定流动状况与之对应．分支管道中的稳定流动状态，不仅取决于主管道中的流量，而且取决于主管道和分支管道中的流量调整变化过程．实验表明：对于具有相同尺寸，相同几何形状的多个分支管道而言，分支管道距主管道入口端的位置顺序越靠前，则通过该分支管道的流量越小．虽然实验中的多分支管道流动是属于非常复杂的湍流，但实验表明主管道的流量与各分支管道的流量之间存在一简单的线性关系．实验还表明，主管道入口的壁面静压与备分支管道出口的壁面静压之间存在抛物线关系．     

尾迹对涡轮动叶全表面气膜冷却效率的影响

采用压敏漆（PSP）测量技术研究了尾迹对涡轮动叶气膜冷却效率的影响，测试叶片带有11排圆柱形气膜孔。获得了不同质量流量比和尾迹斯特劳哈尔数（Sr=0，0.12，0.36）条件下全表面气膜冷却效率分布的试验数据，结果表明：随着尾迹Sr数的增加，叶片前缘区域径向平均气膜冷却效率最大降低幅度达36.5%，吸力面径向平均气膜冷却效率最大降低幅度达53.5%，压力面径向平均气膜冷却效率最大降低幅度达24.2%；尾迹对前缘和吸力面气膜冷却效率的影响大于压力面；随着质量流量比增加，尾迹的影响减小；在进行涡轮动叶表面气膜冷却结构设计时，不考虑尾迹效应会增加设计风险。     

Coronal mass ejections acceleration problem

A statistical study of acceleration and its error of coronal mass ejections (CMEs) observed by the Large Angle Spectrometric Coronagraph (LASCO) is performed. A total of 5594 CMEs events have been analyzed by using a least-square method and using the error in the height measures. We verify that slower CMEs (velocities in the interval from 200 to 500 km s⁻¹) tend to have a positive acceleration (about 1 m s⁻²) at heights above 5 solar radii, while less than 10% CMEs show an average negative acceleration (about −2.2 m s⁻²) as they propagate from 5 to 30 solar radii. For most individual CMEs one can not say if they are accelerated or decelerated, only for 8% of all observed CMEs events one can extract the sign of the acceleration in the 5–30 solar radii.     

一次火箭流量对RBCC性能影响的数值和实验研究

利用三维两相数值计算方法和地面直联试验系统,开展了不同来流速度下一次火箭流量变化对发动机性能的影响。数值研究结果表明,在不同来流条件下,一次流流量的增加对发动机推力和比冲的贡献不同,在低速条件时,一次火箭流量的增加对来流空气的加热以及缩短二次燃料的雾化蒸发时间和距离起着积极的作用,对性能的提高有一定作用;当来流速度较高时,过大一次流流量对流动通道产生了阻塞效应,造成对推力和比冲贡献作用的减小。试验结果验证了数值研究得到的规律,特别在高马赫数条件下,一次火箭流量的增加对推力和比冲的贡献是减小的,且飞行速度越高,这种贡献越小。无论低速还是高速来流条件,存在着一个优化的一次流流量,这对提高发动机性能有很大好处。     

气膜冷却传热传质类比研究

应用SSTκ-ω湍流模型,对三维粘性掺混流场进行了数值模拟,得到了切向入射的超声速氢气膜在不同吹风比和被冷却面上的绝热温比分布,并通过冷却剂分布情况详细研究了其形成原因。计算结果表明：吹风比是决定超声速气膜冷却效果的重要因素,吹风比增大,冷却效果随之提高;不同曲率的曲面上,冷却效率的分布规律不同,凹面上冷却效果最好,这与低速气膜冷却不同;离散孔在被冷却面中心和两侧的冷却效果存在明显差异,引入一定的侧向倾角使这种差异趋向消失。     

卫星质心三轴快速测量配重新工艺

文章介绍在某型号的结构星质心测试中,克服了传统工艺的局限性,采用了新的测试工艺,利用倾斜法对卫星三个坐标轴上的质心位置进行快速测量并配重,节省了时间,在实践中取得了很好的效果。     

原子氧环境下磁力矩器用聚合物材料的质损和红外光谱分析

文章利用新型的原子氧环境模拟设备进行真空和原子氧试验,通过质量损失测量和FT-IR分析,对试样的质量损失率(SAML)和表面成分的变化进行了研究。试验结果表明:真空环境会导致材料产生质量损失,4种材料中真空质损最大相差24倍;原子氧作用导致聚合物材料产生质量损失,4种材料中质量损失率最大相差25倍;原子氧与有机硅物质反应能够形成保护层,可以抑制原子氧对材料内部的进一步侵蚀。FT-IR分析结果表明,原子氧作用导致环氧材料的-N消失,O元素百分比含量升高,硅橡胶的化学键被破坏,并导致新的O-H和C-H的生成。     

A study on radio-loud interacting/non-interacting CMEs-associated SEPs and solar flares

We have established a data set of 58 major hybrid SEP events associated with meter-to-decahectometer wavelength (m-to-DH) type II bursts, solar flares, and radio-load CMEs during the period of 1997–2014. The main focus of our study is to address the following two questions: Does the interaction of CMEs play a role in the enhancement of SEP intensity? Is there any difference in the seed population, and parent eruptions in the SEP events with and without CME interactions? Hence, the sample of 58 events is classified into two sets: (i) 35 non-interacting-CME-associated SEP events; (ii) 23 interacting-CME-associated SEP events. All the characteristics of SEPs, their associated CMEs/flares and the relationships between them are statistically analyzed and compared. Some of the basic attributes and relative elemental abundances (Fe/O ratios) of the both the sets are also compared. The results indicate that the seed particles in non-interacting-CME-associated SEP events are mostly from solar wind/coronal materials. But in the case of interacting-CME-associated SEP events, it may be associated with both flare material from preceding flares and coronal materials from solar wind/preceding CMEs. The correlation studies reveal that there are clear correlations between logarithmic peak intensity of SEP events and properties of CMEs (space speed: cc?=?0.56) and solar flares (peak intensity: cc?=?0.40; integrated flux: cc?=?0.52) for non-interacting-CME-associated SEP events. But these correlations are absent for the interacting-CME-associated events. In addition, the results suggest that interaction of primary CMEs with their preceding CMEs plays an important role in the enhancement of peak intensity of SEPs at least for a set of m-to-DH type II bursts associated SEP events.     

Interpretation of the SOHO/UVCS observations of two CME-driven shocks

We report on the analysis of two fast CME-driven shocks observed with the UltraViolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO). The first event, detected on 2002 March 22 at 4.1 R_⊙ with the UVCS slit placed in correspondence with the flank of the expanding CME surface, represents the highest UV detection of a shock obtained so far with the UVCS instrument in the corona. The second one, detected on 2002 July 23 at 1.6 R_⊙ with the UVCS slit placed in correspondence with the front of the expanding CME surface, shows an anomalous deficiency of ion heating with respect to what observed in previous CME/shocks observed by UVCS, possibly reflecting the effect of different coronal plasma conditions over the solar cycle. From the two different sets of observations we derived an estimate for the shock compression ratio X, which turns out to be X = 2.4 ± 0.2 and X = 2.2 ± 0.1, respectively, for the first and second event. Comparison between the two events provides complementary perspectives on the dynamical evolution of CME-driven shocks.