熵产控制体方法对压气机近零间隙流动损失的演变规律

以澄清近零间隙流动结构及流动损失随间隙的变化规律为目标,提出熵产控制体分析方法,可精确量化流场任意位置的局部不可逆损失.数值模拟发现,间隙在0.4%叶高范围内(称近零间隙)效率水平最高且出现一对应峰值效率最高的最佳非零间隙.熵产控制体分析表明:通道内总熵产随间隙变化规律与效率一致;间隙变化对动叶端区20%~80%弦长范围内的熵产改变最为明显,主导了总熵产的变化;间隙变化时熵产改变的流动区域不同,这是由于动叶端区主导损失的流动结构发生改变造成的.进一步结合流场结构,探讨近零间隙流动损失演变的可能原因:间隙为零时壁面剪切力是造成损失的主导因素;最佳间隙时流动均匀,损失最小.      

基于变导叶调节的涡扇发动机加速过程优化控制

提出了一种利用变导叶调节,基于可行序列二次规划算法的涡扇发动机加速过程优化控制方法,研究发现,通过在发动机加速过程中对压缩部件导叶角度的适应性调节,可以优化压气机和风扇在过渡态的空气流量,使得燃油在满足各方面约束条件下以最大可能的速度增加,从而提升了发动机加速性能.最后,与常规两变量加速过程优化方法进行了对比研究:在相同目标函数和约束条件下,分别进行了两控制量(主燃油和尾喷管喉道面积)、增加风扇导叶调节或压气机变导叶的三控制量的加速优化控制仿真,结果表明,所提出的方法在优化过程中可以使得燃油最大可能速率高于常规方法,且发现压气机导叶角在优化过程的作用优于风扇导叶角,优化后的工作点加速路径紧贴喘振裕度限制边界,且各个约束严格在可行域范围内,3种方案的加速时间分别为5.5,4.9s和4.5s.     

具有吸附性的平板型轨道分子屏离轴区域真空特性的研究

轨道分子屏真空系统,是利用分子屏轨道飞行速度远大于轨道环境大气的平均热运动速度,使空间环境对分子屏产生理想的抽速,在尾部形成气体分子的稀化区,达到极高真空.对平板型轨道分子屏,现有的文献中,仅仅计算了沿对称轴线的压力分布,然而,由于实际的分子屏试验,试件是具有一定尺寸的三维物体。仅仅获得对称轴线上的真空信息是不够的,需要对偏离对称轴线的空间点,进行分析计算.文章针对具有吸附性的平板型轨道分子屏,对偏离对称轴线的压力分布计算,提出了一套计算方法,对500km 的轨道高度,计算结果表明:当考察点与分子屏表面的距离(=|Z0|)小于1.0m,偏离对称轴线的距离小于1.6m 时,真空度维持在优于10~(-10)Pa 的数量级。建议在这一尺度范围进行材料试验。     

Nighttime ionosphere–thermosphere coupling observed during an intense geomagnetic storm

The electrodynamics of the ionosphere in the tropical region presents various scientific aspects, which remain subject of intensive investigations and debates by the scientific community. During the year 2002, in a joint project between the Universidade do Vale do Paraíba (UNIVAP) and Universidade Luterana do Brasil (ULBRA), a chain of three Canadian Advanced Digital Ionosondes (CADIs) was established nearly along the geomagnetic meridian direction, for tropical ionospheric studies, such as, changes and response due to geomagnetic disturbances and thermosphere–ionosphere coupling and the generation and dynamics of ionospheric irregularities, in the Brazilian sector. The locations of the three ionosondes stations are São José dos Campos (23.2°S, 45.9°W, dip latitude 17.6°S – under the southern crest of equatorial ionospheric anomaly), Palmas (10.2°S, 48.2°W, dip latitude 5.5°S – near the magnetic equator) and Manaus (2.9°S, 60.0°W, dip latitude 6.4°N – between the geographic and geomagnetic dip equators). It should be pointed out that Palmas and Manaus are located on the opposite sides of the magnetic equator but both are south of the geographic equator. The three CADIs work in time-synchronized mode and obtain ionograms every 5 min. This configuration of the ionospheric sounding stations allowed us to study the F-region dynamics during geomagnetically disturbed period in the meridional direction. Just after the installation and testing of the three CADIs, on September 05, 2002 a coronal mass ejection (CME) left the Sun and about 2 days after the CME left the Sun, it reached the Earth’s magnetosphere and complex and multi step events took place during the period September 07–09. In the study we note that the equatorial stations located north (Manaus, dip latitude 6.4°N) and south (Palmas, dip latitude 5.5°S) of the dip equator presented significant F-layer height asymmetries during the storm main phase. In addition, the low-latitude station SJC (dip latitude 17.6°S) presented decrease in the F-layer densities (negative phase), whereas Palmas presented increase in the F-layer densities (positive phase) during the main phase. This was followed by positive phase at both the stations. During the first night of the recovery phase a strong formation and evolution of large-scale ionospheric irregularities (equatorial spread-F (ESF)) was observed, but on the second night of the recovery phase, there was strong and almost simultaneous sporadic E (Es) formation at all three stations. During the presence of Es, spread-F formation is not observed, indicating the suppression of spread-F, possibly by sporadic E.     

提高河南经济外向度的对策建议

河南省的对外开放取得了很大发展,进出口总额不断提高,引进外资数量逐年增长。然而,河南省对外开放力度与全国平均水平及沿海发达地区相比,一直处于较弱势地位,外贸的控制力和竞争力较弱,这在一定程度制约了河南经济的进一步发展。提高河南经济的对外开放度,主要应从以下几个方面入手：（1）走出利用外资的认识误区,努力提高利用外资的质量和水平。（2）营造良好的投资环境,改善对外开放的发展条件。（3）探索引进外资的动力机制,搞好引资工作。（4）建立健全对外贸易服务体系,进一步扩大外贸出口规模。（5）鼓励“走出去”,加强对外经济技术合作。（6）在加快对外开放的同时,加快对内开放。     

Effects of solar activity variations on the low latitude topside nighttime ionosphere

We have studied the topside nighttime ionosphere of the low latitude region using data obtained from DMSP F15, ROCSAT-1, KOMPSAT-1, and GUVI on the TIMED satellite for the period of 2000–2004, during which solar activity decreased from its maximum. As these satellites operated at different altitudes, we were able to discriminate altitude dependence of several key ionospheric parameters on the level of solar activity. For example, with intensifying solar activity, electron density was seen to increase more rapidly at higher altitudes than at lower altitudes, implying that the corresponding scale height also increased. The density increased without saturation at all observed altitudes when plotted against solar EUV flux instead of F10.7. The results of the present study, as compared with those of previous studies for lower altitudes, indicate that topside vertical scale height increases with altitude and that, when solar activity increases, topside vertical scale height increases more rapidly at higher altitudes than at lower altitudes. Temperature also increased more rapidly at higher altitudes than at lower altitudes as solar activity increased. In addition, the height of the F2 peak was seen to increase with increasing solar activity, along with the oxygen ion fraction measured above the F2 peak. These results confirm that the topside ionosphere rises and expands with increasing solar activity.     

Model of a fluxtube with a twisted magnetic field in the stratified solar atmosphere

We build a single vertical straight magnetic fluxtube spanning the solar photosphere and the transition region which does not expand with height. We assume that the fluxtube containing twisted magnetic fields is in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity. Incorporating specific forms of current density and gas pressure in the Grad–Shafranov equation, we solve the magnetic flux function, and find it to be separable with a Coulomb wave function in radial direction while the vertical part of the solution decreases exponentially. We employ improved fluxtube boundary conditions and take a realistic ambient external pressure for the photosphere to transition region, to derive a family of solutions for reasonable values of the fluxtube radius and magnetic field strength at the base of the axis that are the free parameters in our model. We find that our model estimates are consistent with the magnetic field strength and the radii of Magnetic bright points (MBPs) as estimated from observations. We also derive thermodynamic quantities inside the fluxtube.     

Connection between winter mesopause region temperatures and diurnal LF reflection height variations measured at Collm

Scale height, H, estimates are calculated from the decrease/increase of ionospheric virtual reflection heights of low-frequency (LF) radio waves at oblique incidence in suitably defined morning intervals around sunrise during winter months. The day-to-day variations of H qualitatively agree with daily mean temperature variations around 90 km from meteor radar measurements. Since mesospheric long-period temperature variations are generally accepted to be the signature of atmospheric planetary waves, this shows that LF reflection height measurements can be used for monitoring the dynamics of the upper middle atmosphere. The long-term variations of monthly mean H estimates have also been analysed. There is no significant trend, which is in agreement with other measurements of mesopause region temperature trends.     

后掠平板横流不稳定性

本文研究了无限后掠平板三维边界层的横流不稳定性，证明行进波和定常波几平同时失稳，且行进波比定常波更不稳定；     

航空工业人才培养的探讨与研究

本文运用人力资本的概念分析了航空工业人才培养的重要性，同时根据人才成长的规律，结合航空工业的特点，得出了相应的人才培养的途径和方法。