串列多支柱主起落架布局飞机的起飞载荷研究

大型军用运输机、民航客机广泛采用可视为前三点式(前起落架组、左主起落架组、右主起落架组)的多支柱起落架布局方案.通常,此类飞机的最大起飞质量高达数百吨,起飞滑跑速度也较大,因此,起飞情况是起落架强度设计的重点.本文基于前三点式起落架计算理论,以及对An-124、An-225飞机起落架设计方案的研究,提出一类串列多支柱多轮主起落架的起飞情况地面载荷算法.     

不对称静子尾迹流场激振力分析及计算方法

为降低转子叶片在前排静子尾迹流场激振情况下的动应力,提高转子叶片疲劳寿命,对不对称静子叶片分布进行流场分析,研究在不对称静子分布非谐情况下,转子所受到的尾迹流场的激振力频谱及幅值.研究表明不对称静子分布非谐设计下,转子所受到的激振力由静子均布情况下的单频率高幅值激振转变为多频率成分低幅值激振力,通过对各个频率成分幅值的计算分析,得到了不对称静子分布非谐设计可有效降低转子叶片受到的尾流激振力,提高疲劳寿命的结论.同时,对不对称静子分布的三维流场计算,提出了简化计算方法,可大大降低计算时间和对计算机硬件要求.      

高性能玻璃纤维增强树脂基复合材料拉-压疲劳行为

对LTX1240玻璃纤维/环氧复合材料开展拉-压疲劳试验,绘制S-N曲线进行疲劳寿命预测,利用扫描电镜观察疲劳试样断口形貌,分析其在拉-压循环载荷作用下的失效模式。结果表明:LTX1240玻璃纤维增强环氧树脂基复合材料的条件疲劳极限为278 MPa;失效过程为树脂基体最先破坏,接着界面分层乃至纤维拉伸、剪切破坏,它们相互作用形成了弥散损伤区并据此扩展发生材料断裂。     

Modeling and observations of the north–south ionospheric asymmetry at low latitudes at long deep solar minimum

Using the physics based model SUPIM and FORMOSAT-3/COSMIC electron density data measured at the long deep solar minimum (2008–2010) we investigate the longitude variations of the north–south asymmetry of the ionosphere at low latitudes (±30° magnetic). The data at around diurnal maximum (12:30–13:30 LT) for magnetically quiet (Ap ? 15) equinoctial conditions (March–April and September–October) are presented for three longitude sectors (a) 60°E–120°E, (b) 60°W–120°W and (c) 15°W–75°W. The sectors (a) and (b) have large displacements of the geomagnetic equator from geographic equator but in opposite hemispheres with small magnetic declination angles; and sector (c) has large declination angle with small displacement of the equators; vertical E × B drift velocities also have differences in the three longitude sectors. SUPIM investigates the importance of the displacement of the equators, magnetic declination angle, and E × B drift on the north–south asymmetry. The data and model qualitatively agree; and indicate that depending on longitudes both the displacement of the equators and declination angle are important in producing the north–south asymmetry though the displacement of the equators seems most effective. This seems to be because it is the displacement of the equators more than the declination angle that produces large north–south difference in the effective magnetic meridional neutral wind velocity, which is the main cause of the ionospheric asymmetry. For the strong control of the neutral wind, east–west electric field has only a small effect on the longitude variation of the ionospheric asymmetry. Though the study is for the long deep solar minimum the conclusions seem valid for all levels of solar activity since the displacement of the equators and declination angle are independent of solar activity.     

粗糙带对细长体大迎角流动非对称性的影响

通过模型表面压力分布测量和表面油流图谱显示等试验手段,在低湍流度风洞中探讨了模型头部不同形式的粗糙带对细长体大迎角条件下流动非对称性的影响.结果表明:"条型"粗糙带可以有效改善流动非对称性、降低当地侧向力;"环型"粗糙带可以改善模型表面的分离状态,但是却增强了流动非对称性;"条型 环型"粗糙带对于表面流谱的影响较为复杂.但是这些形式的粗糙带都不能完全消除流动非对称性所产生的侧向力.试验结果还展示出了大迎角状态下,流动非对称性的存在形式与表现特征.     

On the performance of IRI-2016 to predict the North-South asymmetry of the equatorial ionization anomaly around 73°E longitude

The ionospheric total electron content (TEC) in both northern and southern Equatorial anomaly regions are examined by using the Global Positioning System (GPS) based TEC measurements around 73°E Longitude in the Asian sector. The TEC contour charts obtained at SURAT (21.16°N; 72.78°E; 12.9°N Geomagnetic Lat.) and DGAR (7.27°S; 72.37°E; 15.3°S Geomagnetic Lat.) over 73°E longitude during a very low solar activity phase (2009) and a moderate solar activity (2012) phase are used in this study. The results show the existence of hemispheric asymmetry and the effects of solar activity on the EIA crest in occurrence time, location and strength. The results are also compared with the TEC derived by IRI-2016 Model and it is found that the North-South asymmetry at the EIA region is clearly depicted by IRI-2016 with some discrepancies (up to 20% in the northern hemisphere at SURAT and up to 40% in the southern hemisphere at DGAR station for June Solstice and up to 10% both for SURAT and DGAR for December Solstice). This discrepancy in the IRI-2016 model is found larger during the year 2012 than that during the solar minimum year 2009 at both the hemispheres. Further, an asymmetry index, (A_i) is determined to illustrate the North-South asymmetry observed in TEC at EIA crest. The seasonal, annual and solar flux dependence of this index are investigated during both solstices and compared with the TEC derived by IRI.     

Second order experimental statistics of rain attenuation at Ka band in a tropical location

Some second order rain attenuation statistics such as fade duration and fade slope are investigated on the basis of experimental measurements of received signals using the GSAT-14 satellite beacon signal at 20.2 GHz for three years (2014–2016) over the tropical location Ahmedabad (23.02 ⁰E, 72.51⁰N), India with an Elevation angle of 63⁰. Existing models of fade duration are compared with experimental data in this study and exponent of power law model of fade duration at Ka band is further explored. A new model for fade duration for Ka band for tropical locations is proposed where the constant of exponent of attenuation in the power law is found to be 0.143 instead of 0.055 used in ITU-R. Other relevant parameters for implementation of fade mitigation technique to prevent the link outage like cumulative distribution of signal fade rate, maximum and minimum fade rise and fade fall are also studied. Fade slope asymmetry over tropical region is also investigated. Keeping in view of exploiting the commercial launch of Ka band in Indian region there is an urgent need for validation of the existing models of fade slope (specially looking into fade symmetry) and fade duration. It will help the SATCOM (Satellite Communication) link designer to improve closed loop fade mitigation technique to minimize the possible link failure/link outage over the tropical region.     

Dy和Yd类变压器联结组的微机判别

三相变压器的联结组标号必须判别确定。选较复杂的 Dy和 Yd类联结组为例 ,对其进行理论分析 ,获得作筛选法判别基准的理想计算值的规律性。在实测时考虑三相电源电压不对称的影响 ,用实测计算值代替理想计算值作判别基准。经微机的硬件与软件系统联试 ,能对全部联结组标号快捷地判别 ,不仅能判定对与错 ,还能指出错误联成何种标号     

细长旋成体大迎角非定常运动数值研究

利用DES方法对处于非对称流态下的细长旋成体进行了俯仰和偏航振荡的数值模拟,观察细长体气动特性尤其是背风面非对称分离涡的变化。计算结果表明在大迎角非对称多涡系情况下,固定频率和振幅的非定常运动可以改变流场结构和气动力,对细长体背风面流态有巨大的影响。俯仰振荡对非对称分离涡有明显的控制作用,抑制流场的非对称性,使分离涡趋于对称;而固定频率的偏航振荡则破坏背风面分离涡的稳定性,激励非对称背涡产生随时间变化的周期性脱落。所进行的非定常运动与细长体流场耦合作用研究在国内外研究尚少。     

喉部不对称对微喷管性能影响

以FLUENT 6.1软件为工具,利用数值计算求解二维稳态可压缩Navier-Stokes(N-S)方程,模拟了微喷管内超声速流体流动,分析了喷管喉部结构不对称对喷管内部的流场和喷管性能的影响.这种喉部结构不对称是由于喉部上下顶点在x方向偏离一定距离所造成的.数值计算结果表明,喷管喉部在流体流动方向的不对称,将导致喷管内部流体流场不平衡性,使得流量增大,喷管出口的x方向推力增加,y方向产生了多余的推力.