三角翼低速动态大攻角气动特性试验研究

对后掠角分别为X=60°、70°和80°尖前缘平板三角翼模型和一个前缘后掠角为（76° 40°）的双三角翼模型在低速风洞中作大攻角俯仰摩波运动，振幅am=30°、60°和90°，缩减频率K=0.01～0.12，基于根弦长雷诺数Re=2.76×10^5～8.23×10^5。进行了六分量动态气动载荷测量，动态流动显示和70°三角翼上翼面非定常压力测量，并分别与对应的静态试验结果比较。分析了运动参数包括缩减频率、振幅和Re数、后掠角对气流动态迟滞特性的影响。     

风洞试验中风剖面的模拟及近流场特性分析

首先简单介绍了日本东京工艺大学风工程研究中心新建的开环流低速边界层风洞中风剖面模拟的试验情况.基于试验结果,采用被广泛应用的三角尖劈加上布置粗糙元的方法,成功地模拟出日本建筑学会定义的四类不同场地对应的风剖面.通过对试验数据的比较分析,就所采用的立方体粗糙元及三角尖劈对最终模拟得到的风剖面特性的影响进行了比较分析.其次,对风剖面模拟及特性判定中的几个重要问题,如三角尖劈的形状优化、风速功率谱的一致性、积分尺度的分析方法等进行了分析.最后,基于以上分析,对在边界层风洞中模拟预定的风剖面提出几点参考意见.     

角速度波动率测量的数据处理和不确定度分析

本文在对角速度波动率测量技术研究的基础上，提出了一些自己的看法，并对一些相关术语进行了定义，同时，对角速度波动率测量方法的不确定度评定进行了分析。最后，通过数据处理软件对实验数据进行了分析和验证。     

单向玻璃纤维增强环氧树脂低温冲击拉伸性能的试验研究

 在经改进后配有低温装置的杆-杆型冲击拉伸装置上,对单向玻璃纤维增强环氧树脂在室温、-50℃、-100℃和-150℃的冲击性能进行了研究。结果表明该材料有温度相关性,所研制的装置性能良好,便于应用。     

WALL INTERFERENCE CORRECTIONS FORHIGH-LIFT EXPERIMENT

ＷＡＬＬＩＮＴＥＲＦＥＲＥＮＣＥＣＯＲＲＥＣＴＩＯＮＳＦＯＲＨＩＧＨ－ＬＩＦＴＥＸＰＥＲＩＭＥＮＴＺｈａｎｇＷｅｎｈｕａ（Ｆａｃｕｌｔｙ６０３ｏｆＮａｎｊｉｎｇＵｎｉｖｅｒｓｉｔｙｏｆＡｅｒｏｎａｕｔｉｃｓａｎｄＡｓｔｒｏｎａｕｔｉｃｓ，Ｎａｎｊｉｎ...     

A320系列机型绿点速度特性分析

绿点速度是空客系列机型特有的光洁构型、一发失效条件下的最佳操纵速度。为了研究绿点速度的设计依据,利用空客PEP性能软件计算A320系列机型光洁构型、一发失效条件下、不同校正表速所对应的爬升角、等待燃油流量和飘降下滑角,分析了绿点速度状态、最大升阻比状态下的爬升、等待、飘降性能与最佳爬升/等待/飘降性能相互之间的关系。结果表明:绿点速度小于最大升阻比速度,随着飞行高度增加逐渐逼近最大升阻比速度;绿点速度下的爬升/等待/飘降性能对应于最大升阻比性能、最佳爬升/等待/飘降性能的均值。     

侧向喷流的一种直接实验模拟

研究了侧向喷流的一种直接实验模拟技术,旨在探讨喷流力直接作用在天平上时,侧向喷流对气动载荷的影响及其增益情况。本文的直接模拟是通过一种通气式应变天平实现的。研究中分析了有关模拟原则,妥善处理了诸如高压气体密封、天平变形引发的漂移、干扰等相关技术问题,并在一尖拱柱构型上实现了多种条件下的直接模拟,给出了来流条件和喷口参数条件对法向力、俯仰力矩增益因子的影响。最后,就实验结果进行了适当讨论和评述。     

高速风洞引射式进排气动力模拟试验研究

为了测定具有埋入式进气道的某航弹发动机进排气对航弹的气动影响量 ,采用引射式动力模拟器在FL 7高速风洞 ,首次在国内成功地进行了高速风洞进排气动力模拟试验。试验模型缩比为 1∶1 0 ,M =0 .7,P0j/P∞ =2 .62 ,Cφ=0 .79。试验结果表明 ,有动力后XD,CL,CD增加 ,Cma减少。试验表明在高速风洞中对于小尺寸的试验模型 ,采用引射式动力模拟器开展进排气动力模拟试验是一种简便适用的好方法     

Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs

Coronal mass ejections (CMEs) observed near the Sun via LASCO coronographic imaging are the most important solar drivers of geomagnetic storms. ICMEs, their interplanetary, near-Earth counterparts, can be detected in situ, for example, by the Wind and ACE spacecraft. An ICME usually exhibits a complex structure that very often includes a magnetic cloud (MC). They can be commonly modelled as magnetic flux ropes and there is observational evidence to expect that the orientation of a halo CME elongation corresponds to the orientation of the flux rope. In this study, we compare orientations of elongated CME halos and the corresponding MCs, measured by Wind and ACE spacecraft. We characterize the MC structures by using the Grad–Shafranov reconstruction technique and three MC fitting methods to obtain their axis directions. The CME tilt angles and MC fitted axis angles were compared without taking into account handedness of the underlying flux rope field and the polarity of its axial field. We report that for about 64% of CME–MC events, we found a good correspondence between the orientation angles implying that for the majority of interplanetary ejecta their orientations do not change significantly (less than 45 deg rotation) while travelling from the Sun to the near-Earth environment.     

Coronal mass ejection detection using wavelets,curvelets and ridgelets: Applications for space weather monitoring

Coronal mass ejections (CMEs) are large-scale eruptions of plasma and magnetic field that can produce adverse space weather at Earth and other locations in the Heliosphere. Due to the intrinsic multiscale nature of features in coronagraph images, wavelet and multiscale image processing techniques are well suited to enhancing the visibility of CMEs and suppressing noise. However, wavelets are better suited to identifying point-like features, such as noise or background stars, than to enhancing the visibility of the curved form of a typical CME front. Higher order multiscale techniques, such as ridgelets and curvelets, were therefore explored to characterise the morphology (width, curvature) and kinematics (position, velocity, acceleration) of CMEs. Curvelets in particular were found to be well suited to characterising CME properties in a self-consistent manner. Curvelets are thus likely to be of benefit to autonomous monitoring of CME properties for space weather applications.