CZ2F火箭POGO振动信号特征频率提取

CZ2F运载火箭在第5次飞行过程中意外出现了"8Hz"POGO振动现象,该振动频率对箭体的稳定性和航天员安全产生了严重的影响。为解决这一振动问题,必须精确分析该频率的持续时间和振动量级。通过研究HHT(Hilbert-Huang Transform,希尔伯特-黄变换)方法,结合火箭振动信号特点设计了特征频率提取算法,成功地提取了CZ2F火箭飞行中的"8Hz"POGO振动频率,为有效解决"8 Hz"POGO振动问题提供了技术支撑。     

原位自生TiB2/Al复合材料车削参数多目标优化方法

原位自生TiB2/Al复合材料具有密度小、比强度高、高耐磨等特点,在航空航天领域具有广泛的应用前景.主要针对TiB2/Al复合材料车削参数对表面粗糙度的影响进行探索性研究.首先,以车削速度、进给速度、车削深度为对象,基于单因素试验研究了车削参数控制域.进一步在控制域内设计正交试验,并基于试验结果研究了表面粗糙度与车削参数的映射关系,推导了材料去除率模型.最后,以表面粗糙度和材料去除率为优化目标,提出并研究了基于GA-Pareto的车削参数多目标优化方法,并通过试验验证了该方法的可行性和有效性.     

热处理对激光增材制造Ti2AlNb基合金组织及性能的影响

利用激光增材制造技术制备出Ti-22Al-25Nb合金薄壁试样,分析了沉积态和热处理态试样的宏观形貌、相组成和显微组织,以及不同制度热处理态试样的组织和室温拉伸性能.结果表明,沉积态试样相组成沿沉积高度方向呈现由B2+O+α2→B2+O→B2的变化趋势;热处理态试样的微观组织和相组成均匀,由B2、O、α23相组成;经930℃保温2h空冷的固溶处理和800℃保温24h空冷的时效处理后,合金室温拉伸性能好,抗拉强度为1017MPa,断后伸长率为6.0％.     

TA12钛合金电子束焊接的显微组织和力学性能

采用电子束焊接对10mm TA12钛合金进行了焊接,焊缝表面形成良好.对TA12钛合金电子束焊接试样进行了金相分析和静力试验、冲击试验和扫描电镜(SEM)分析.结果表明,焊接接头熔合区、热影响区和母材区的微观组织差别明显;随着等轴α相体积分数的减少,接头塑性和冲击韧性值降低,但是拉伸强度变化不大.     

“嫦娥二号”卫星L2点角动量管理

对“嫦娥二号”(CE-2)卫星进入环绕日地拉格朗日L2点的李萨如轨道后卫星喷气卸载所产生的影响进行了研究.提出了一种利用光压力矩辅助卫星太阳电池翼角度调整进行角动量管理的方法.在轨试验表明,太阳光压强度足够对飞行在L2点环绕轨道上的CE-2卫星进行角动量管理,可以大幅度减少动量轮在轨喷气卸载的次数,有利于CE-2卫星的轨道维持.     

Comparison of ionosphere characteristic parameters obtained by ionosonde with IRI-2007 model over Southeast Asia

In this work, the foF2 and hmF2 parameters at the conjugate points near the magnetic equator of Southeast Asia are studied and compared with the International Reference Ionosphere (IRI) model. Three ionosondes are installed nearly along the magnetic meridian of 100°E; one at the magnetic equator, namely Chumphon (10.72°N, 99.37°E, dip angle 3.0°N), and the other two at the magnetic conjugate points, namely Chiang Mai (18.76°N, 98.93°E, dip angle 12.7°N) and Kototabang (0.2°S, 100.30°E, dip angle 10.1°S). The monthly hourly medians of the foF2 and hmF2 parameters are calculated and compared with the predictions obtained from the IRI-2007 model from January 2004 to February 2007. Our results show that: the variations of foF2 and hmF2 predicted by the IRI-2007 model generally show the similar feature to the observed data. Both parameters generally show better agreement with the IRI predictions during daytime than during nighttime. For foF2, most of the results show that the IRI model overestimates the observed foF2 at the magnetic equator (Chumphon), underestimates at the northern crest (Chiang Mai) and is close to the measured ones at the southern crest of the EIA (Kototabang). For hmF2, the predicted hmF2 values are close to the hmF2(M3000F2_OBS) during daytime. During nighttime, the IRI model gives the underestimation at the magnetic equator and the overestimation at both EIA crests. The results are important for the future improvements of the IRI model for foF2 and hmF2 over Southeast Asia region.     

骨特异性转录因子Runx2对抗空间骨丢失效应的初步研究

为了构建稳定过表达Runx2 (骨特异性转录因子)的C2C12 (小鼠成肌细胞)和MG63 (前成骨细胞)细胞株, 并用于研究Runx2在对抗空间骨丢失效应中的作用. 利用实时定量聚合酶链式反应鉴定Runx2下游基因I型胶原、碱性磷酸酶表达情况, 在二维回转器中培养稳定细胞株, 通过定量聚合酶链式反应,观察在模拟失重效应下Runx2基因对其下游基因表达的影响. 结果表明, 通过筛选获得稳定转染的C2C12-Runx2和MG63-Runx2细胞株, 经鉴定都能过表达Runx2. 转染后的细胞 I 型胶原和碱性磷酸酶mRNA表达增高. 回转组与对照组相比, MG63, C2C12-Runx2, MG63-Runx2细胞的I型胶原和碱性磷酸酶mRNA表达降低, 但在模拟失重效应下, 转染细胞中I型胶原和碱性磷酸酶的mRNA表达下降程度明显低于未转染细胞株. 所构建的C2C12-Runx2和MG63-Runx2细胞株比较稳定, 并证实Runx2能部分对抗失重引起的成骨特异性分子的降低.      

星载单频GPS数据的电离层延迟改正方法分析

利用C/A码单点定位对LEO(Low Earth Orbit)卫星上的电离层延迟改正方法——"电离层比例因子法"进行了分析研究.计算的CHAMP卫星的轨道结果表明:采用电子密度峰值高度(hmF2,F2 region maximum electron density height)平均值和瞬时值计算的电离层比例因子α变化范围分别为0.3~0.4和0.2~0.65之间,两者最大差异可达0.3,相比较而言,hmF2瞬时值的结果更加合理,并且相应的大地高H方向的系统偏差要降低0.05~0.3m左右;与双频无电离层组合的普通单点定位结果相比表明该方法能较好地消除电离层一阶项所引入的H方向上的系统偏差;该方法适用的LEO卫星轨道高度范围大致在200~ 600km之间,当轨道高度超过700km时,该方法并不适用.     

星载全球大气波动成像仪研究

在卫星上对中间层顶区域的气辉辐射成像观测, 对于全球大气波动的监测和研究具有重要的意义. 利用TDICCD对O₂A (0-0)气辉进行成像观测, 计算了曝光积分时间、信噪比和能达到的最高空间分辨率, 分析了地球自转对空间分辨率的影响, 在此基础上提出一种星载全球大气波动成像仪方案, 该方案可以观测垂直波长大于10km的大气波动, 最高水平分辨率可以达到0.33km.      

A new global version of M(3000)F2 prediction model based on artificial neural networks

A new version of global empirical model for the ionospheric propagation factor, M(3000)F2 prediction is presented. Artificial neural network (ANN) technique was employed by considering the relevant geophysical input parameters which are known to influence the M(3000)F2 parameter. This new version is an update to the previous neural network based M(3000)F2 global model developed by Oyeyemi et al. (2007), and aims to address the inadequacy of the International Reference Ionosphere (IRI) M(3000)F2 model (the International Radio Consultative Committee (CCIR) M(3000)F2 model). The M(3000)F2 has been found to be relatively inaccurate in representing the diurnal structure of the low latitude region and the equatorial ionosphere. In particular, the existing hmF2 IRI model is unable to reproduce the sharp post-sunset drop in M(3000)F2 values, which correspond to a sharp post-sunset peak in the peak height of the F2 layer, hmF2. Data from 80 ionospheric stations globally, including a good number of stations in the low latitude region were considered for this work. M(3000)F2 hourly values from 1987 to 2008, spanning all periods of low and high solar activity were used for model development and verification process. The ability of the new model to predict the M(3000)F2 parameter especially in the low latitude and equatorial regions, which is known to be problematic for the existing IRI model is demonstrated.