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1.
航空发动机熄火预测是重要关键问题之一,湍流和化学反应的非线性相互作用使预测非常困难。本文采用大涡模拟(LES)对湍流进行高精度模拟,采用概率密度函数输运方程湍流燃烧模型(TPDF)耦合JL4、Z66和H73三种化学反应机理,对预混丙烷钝体熄火现象和规律进行研究。JL4的反应机理最简单,反应释热快,局部放热高,火焰宽度大,火焰两侧温度梯度大,燃烧更加趋于稳定,无法模拟出熄火状态。H73机理绝热火焰温度低,火焰温度低,回流区中部OH含量高;在近熄火状态,大量CO被氧化,释放热量过高导致无法模拟出熄火现象。Z66机理可以模拟出火焰正常状态,在低当量比下也可以模拟出熄火状态。本文算例中,局部Da数大于1的区域超过35%则会发生熄火。 相似文献
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雷电空间电磁场一直是电磁领域研究的热门,成熟的算法例如有限时域差分法(FDTD),传输线矩阵法(TLM)以及频域的矩量法(MoM)在计算雷电问题方面都有广泛的应用。由于计算流体力学(CFD)中的Euler方程与电磁学中的Maxwell方程有着相同的守恒形式,而且采用间断伽辽金方法(DG)已经在流场问题上得到广泛的尝试,因此引入了基于计算流体力学的DG方法来离散时域Maxwell方程,并采用网格分区并行技术加速计算,使用基于DG的圆球雷达散射截面积(RCS)算例进行测试,数值结果一致表明DG算法在求解电磁场问题上的可行性,之后通过计算一段近场雷电通道的电场分布并与解析解、某算法仿真解对比,数据基本吻合,说明该方法适合于雷电电磁场的计算。 相似文献
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可控的过失速机动是先进战斗机超机动性能的重要标志,飞机飞行包线的扩大已超出传统的大气数据系统测量范围,可靠的迎角、侧滑角、总压、静压等飞行大气数据是制约先进战斗机过失速机动中飞行控制的关键因素。以中国推力矢量验证机为对象,基于过失速机动飞行试验的数据,开展大气参数估计与验证研究。结合过失速机动的时间与空间特性,研究了基于风速、地速、空速矢量和惯性姿态、导航参数的大气参数融合计算方法;针对过失速大迎角状态下飞机周围气流非定常、模型非线性导致的融合大气参数误差的复杂特性,进一步构建深度神经网络,对机动状态融合迎角、侧滑角的强非线性误差进行拟合。仿真和飞行试验表明:该方法可在大迎角飞行状态下实现主要大气参数的融合估计,过失速机动过程中融合迎角误差优于2.3°,融合得到的大气参数可为过失速大迎角机动飞行控制提供可靠的大气参数状态反馈。 相似文献
4.
Fault mode probability factor based fault-tolerant control for dissimilar redundant actuation system
This paper presents a Fault Mode Probability Factor (FMPF) based Fault-Tolerant Control (FTC) strategy for multiple faults of Dissimilar Redundant Actuation System (DRAS) composed of Hydraulic Actuator (HA) and Electro-Hydrostatic Actuator (EHA). The long-term service and severe working conditions can result in multiple gradual faults which can ultimately degrade the system performance, resulting in the system model drift into the fault state characterized with parameter uncertainty. The paper proposes to address this problem by using the historical statistics of the multiple gradual faults and the proposed FMPF to amend the system model with parameter uncertainty. To balance the system model precision and computation time, a Moving Window (MW) method is used to determine the applied historical statistics. The FMPF based FTC strategy is developed for the amended system model where the system estimation and Linear Quadratic Regulator (LQR) are updated at the end of system sampling period. The simulations of DRAS system subjected to multiple faults have been performed and the results indicate the effectiveness of the proposed approach. 相似文献
5.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(11):2551-2558
The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (Psw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some Psw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in Psw. It proved that the enhancement of Psw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the Psw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the Psw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. 相似文献
6.
Facundo L. Poblet Francisco Azpilicueta 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2275-2289
The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ~27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ~27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation. 相似文献
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介绍某些战术导弹折叠翼快速展开特性测试技术。详细地介绍了测量方法、项目、数据处理和主要结果。试验是在北京空气动力研究所一座低速风洞中进行的。试验结果表明,获得的数据具有很高精度和可靠性,重复性也是令人满意的。 相似文献