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401.
袁鑫磊 《中国民航飞行学院学报》2013,24(4):38-40
A320系列飞机在运行中有时会出现低速滑行时滑偏的现象,给航班的安全、正点运行带来了很大的压力.本文分析了引起滑偏的原因,给出针对此类故障的快速处理建议及排故方法,以期节省排除此类故障的时间,对缓解航班运行压力提供帮助. 相似文献
402.
Rodrigo A. Miranda Abraham C.-L. Chian Erico L. Rempel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
We analyze the multifractal scaling of the modulus of the interplanetary magnetic field near and far upstream of the Earth’s bow shock, measured by Cluster and ACE, respectively, from 1 to 3 February 2002. The maximum order of the structure function is carefully estimated for each time series using two different techniques, to ensure the validity of our high-order statistics. The first technique consists of plotting the integrand of the pth order structure function, and the second technique is a quantitative method which relies on the power-law scaling of the extreme events. We compare the scaling exponents computed from the structure functions of magnetic field differences with the predictions obtained by the She–Lévêque model of intermittency in anisotropic magnetohydrodynamic turbulence. Our results show a good agreement between the model and the observations near and far upstream of the Earth’s bow shock, rendering support for the modelling of universal scaling laws based on the Kolmogorov phenomenology in the presence of sheet-like dissipative structures. 相似文献
403.
Periodic Variations of Drag Coefficient for the ANDE Spherical Satellites During its Lifetime 下载免费PDF全文
A drag coefficient (CD) inversion method is introduced to study the variations of the drag coefficient for orbital satellites with spherical geometry. Drag coefficients of the four micro satellites in the Atmospheric Neutral Density Experiment (ANDE) are compiled out with this new method. The Lomb-Scargle Periodgram (LSP) analysis of the four ANDE satellites' CD series has shown that there are obvious 5, 7, 9, and 27 days' period in those data. Interesting results are found through comparing the LSP analysis with series of the daily solar radio flux at 10.7 cm (F10.7 index), the Ap index, and the daily averaged solar wind speed at 1AU. All series in the same time interval have an obvious period of about 27 days, which has already been explained as the association with the 27 days' solar rotation. The oscillating periods less than 27 days are found in series of CD, Ap and solar wind speed at 1AU, e.g., the 5, 7, 9 days period. However, these short periods disappeared in the time series of F10.7 index. The same periodicities of 5, 7, 9 days in Ap and solar wind are presented at the same time interval during the declining phase of solar cycle 23. While in the ascending phase of solar cycle 24, these short oscillations are not so obvious as that in the declining phase of solar cycle 23. These results provide definite evidence that the CD variations with period of 5, 7 and 9 days are produced by a combination of space weather effects caused by the solar wind and geomagnetic activity. 相似文献
404.
针对飞航导弹单独使用时SINS存在姿态估计精度随时间降低的问题,提出了基于未知地标被动观测的SINS俯仰姿态误差估计方法。首先,根据飞航导弹中制导段飞行的特点,把SINS俯仰姿态误差估计问题转化为攻角估计问题。然后,在不改变导弹巡航路径的前提下,利用弹上成像导引头对视场内任意未知地标连续被动观测,分别提出了弹体坐标系和速度坐标系下的攻角估计方法,并分析了观测噪声对量测方程系数的影响。最后,利用平均去噪的思想对估计结果进行处理,提高了SINS俯仰姿态误差的估计精度。仿真结果表明:两种方法都能有效估计出飞航导弹SINS俯仰姿态量测误差。 相似文献
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设计一种双级径向旋流器,采用数值模拟的方法研究了旋流器的燃烧性能。计算结果表明:旋流器第Ⅱ级叶片安装角在40°~60°范围内,燃烧室内速度分布相差较小;燃烧室内温度分布与旋流器叶片安装角没有呈现规律性的变化关系;所研究的燃烧室结构,旋流器第Ⅱ级叶片安装角为60°的燃烧室燃烧性能更好。 相似文献
409.
在第23至第24太阳活动周的峰年之间,太阳活动谷年具有持续时间长,极低F10.7太阳辐射通量(低至65)和超长期的零太阳黑子数记录等特点,因此是观测和研究在这种特殊背景下热层大气变化的极好机会.尤其是能充分理解和掌握在宁静环境下热层大气密度对弱太阳活动和小地磁扰动的响应特性.本文利用高度650 km以上星载大气密度探测器2007—2009年的连续探测数据进行分析,结果表明,在太阳辐射通量F10.7极低值期间,较高热层大气密度对F10.7的起伏具有更显著的响应变化.当F10.7由70降至65时,日均大气密度会有4~5倍的显著降变,远大于通常大气模式中的降变值.同样在F10.7极低值期间,较高热层大气密度对小地磁扰动也具有显著的响应增变,当日Kp指数之和由23增至30时,较高热层大气密度则会有80%~160%的强增变. 相似文献
410.
Stefano Della Torre Pavol Bobik Matteo J. Boschini Cristina Consolandi Massimo Gervasi Davide Grandi Karel Kudela Simonetta Pensotti Pier Giorgio Rancoita Davide Rozza Mauro Tacconi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We implemented a 2D Monte Carlo model to simulate the solar modulation of galactic cosmic rays. The model is based on the Parker’s transport equation which contains diffusion, convection, particle drift and energy loss. Following the evolution in time of the solar activity, we are able to modulate a local interstellar spectrum (LIS), that we assumed isotropic beyond the termination shock, down to the Earth position inside the heliosphere. In this work we focused our attention to the cosmic ray positron fraction at energy below ∼10 GeV, showing how the particle drift processes could explain different results for AMS-01 and PAMELA. We compare our modulated spectra with observations at Earth, and then make a prediction of the cosmic ray positron fraction for the AMS-02 experiment. 相似文献