民航飞行员飞行错觉的应对

飞行员的飞行错觉一直是威胁飞行安全的一大隐患,历来是航空医学、航空心理学等领域的研究热点,但其在民航飞行中没有受到足够重视。本文通过查阅近40年来发生的由飞行错觉引起的严重民航飞行事故,结合其他学者的研究结果,提出飞行错觉应在民航飞行中受到更大程度的重视;基于近20年来国内外有关飞行错觉产生机制和训练方法与效果的研究成果,给出了以下应对飞行错觉的建议:从多层面检查前庭;筛选飞行员时增加场独立和视觉空间认知能力的测量;改变飞行仪表显示方式;飞行错觉恢复训练的模拟机程序(针对视性错觉的除外)应使用动态的背景。     

Influence of lunar topography on simulated surface temperature

The surface temperature of the Moon is one of the essential parameters for the lunar exploration, especially to evaluate the Moon thermophysical features. The distribution of the temperature is heavily influenced by the Moon topography, which, however, is rarely studied in the state-of-art surface temperature models. Therefore, this paper takes the Moon topography into account to improve the surface temperature model, Racca model. The main parameters, such as slopes along the longitude and latitude directions, are estimated with the topography data from Chang’E-1 satellite and the Horn algorithm. Then the effective solar illumination model is then constructed with the slopes and the relative position to the subsolar point. Finally, the temperature distribution over the Moon surface is obtained with the effective illumination model and the improved Racca model. The results indicate that the distribution of the temperature is very sensitive to the fluctuation of the Moon surface. The change of the surface temperature is up to 150 K in some places compared to the result without considering the topography. In addition, the variation of the surface temperature increases with the distance from the subsolar point and the elevation, along both latitude and longitude directions. Furthermore, the simulated surface temperature coincides well with the brightness temperature in 37 GHz observed by the microwave sounder onboard Chang’E-2 satellite. The corresponded emissivity map not only eliminates the influence of the topography, but also hints the inherent properties of the lunar regolith just below the surface. Last but not the least, the distribution of the permanently shadowed regions (PSRs) in the lunar pole area is also evaluated with the simulated surface temperature result.     

空乘大学生心理健康现状调查与对策分析

心理健康对于学生的成长成才具有至关重要的作用。文章针对飞行学院2009级和2010级空乘专业学生进行了心理健康现状调查,分析了目前学院学生的心理健康整体水平和成长需求,为学院在制订学生心理健康培养对策时提供理论参考。     

利用并联氙气瓶温差补偿航天器质心偏移的可行性研究

在以往航天器研制中,一般通过增加配重的方式对航天器质心偏移进行补偿.这种质心补偿方式占用了运载火箭承载能力资源,降低了航天器的有效承载能力.针对常规质心补偿方式的弱点,利用电推进航天器上氙气高密度填充的特点,提出了一种通过氙气瓶温度控制对航天器质心偏移进行补偿的方法,减少了航天器配重的使用需求.氙气瓶温差对航天器质心偏...     

飞行员培养中思想政治理论课教育教学改革探索

飞行专业培养的是从事特殊职业的飞行员,飞行专业思想政治教育有其不同于一般大学生的地方。本文总结了飞行员培养对象的特点,调查了用人单位订单式培养飞行员的特殊要求,研究了飞行员培养中思想政治理论课教育教学的特殊规律,探索了飞行员培养中思想政治理论课教育教学改革的方向。     

西南地区飞行计划统一管理模式探讨

本文主要对西南地区飞行计划管理制作方式和发展趋势进行了讨论,结合国内外飞行计划管理运行模式和西南地区的运行特点,分析了西南地区现行飞行计划管理模式存在的问题,对统一制作管理飞行计划的必然性、优势及可行性进行了探讨,以建立更加完善、科学的飞行计划管理运行模式。     

飞机着陆进近穿越风切变的轨迹响应

大气紊流和风切变对飞行活动影响较大,尤以低空风切变危害最大,严重威胁着民航飞行的安全。鉴于飞行器对抗大气扰动的实际能力有限,正确的飞行对策是回避或改出危险的大气扰动区。本文对某训练飞机着陆进近遭遇风切变时飞机轨迹的变化进行了模拟仿真计算。结果表明,采用恒定迎角策略,即采用最大允许迎角（抖动迎角）和最大油门时,改出效果最佳。同时计算出了某训练飞机在水平风为0时,所能抵抗的最大垂直阵风强度;以及在垂直阵风为0时,所能抵抗的最大水平风强度。     

高温磁悬浮轴承励磁绕组制造技术

针对国内外高温励磁绕组存在的缺陷与不足,提出了一种新型的迷宫形励磁绕组结构,首先通过电火花线切割制造出单层迷宫形线圈,并在线圈匝间和层间充分均匀地填充耐高温绝缘材料;然后通过真空钎焊工艺实现多层迷宫形线圈的牢固焊接,最后将焊接成型的多层线圈封装成迷宫形绕组,并应用于单自由度高温磁悬浮轴承试验台中,实现了550℃被悬浮物体近20h的稳定悬浮.研究结果表明:线圈焊缝的高温电阻值小,抗剪切强度满足要求,焊缝的金相组织致密均匀;绕组匝间和层间绝缘性能良好;迷宫形励磁绕组在原理和工艺上是可行的.对高温悬浮试验后的迷宫形绕组内部形貌进行观察后发现封装线圈的高温绝缘材料存在一定的缺陷,有待进一步研究.      

Gyrosynchrotron Radiation of Interplanetary CMEs

CMEs (Coronal Mass Ejections) are an important means of energy release in the solar corona. Solar Polar Orbit Radio Telescope (SPORT) is a mission being proposed for observing the propagation of interplanetary CMEs from solar polar orbit. The main payload onboard SPORT is a synthetic aperture interferometric radiometer, which receives radio emission of interplanetary CMEs. It is identified that there are mainly three radio emission mechanisms of CMEs, i.e., bremsstrahlung, gyrosynchrotron emission and plasma emission. Among these emission types, bremsstrahlung emission is the main emission mechanism of the high-density plasma clouds of interplanetary CMEs. Gyrosynchrotron emission is the continuous emission generated by high-energy electrons from CMEs, while plasma emission is the main mechanism of transient radio bursts from CMEs. In this paper, the gyrosynchrotron emission of interplanetary CMEs is focused on. Firstly, the mechanism of gyrosynchrotron emission is reviewed. Secondly, a review of the physical parameter models of background solar wind and interplanetary CMEs is presented. After these, the brightness temperature and polarization of gyrosynchrotron emission of interplanetary CMEs are calculated and analyzed. Finally, the detectability of gyrosynchrotron emission of interplanetary CMEs by radio meters is discussed briefly.