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21.
《中国航空学报》2023,36(3):220-240
Blade-health monitoring is intensely required for turbomachinery because of the high failure risk of rotating blades. Blade-Tip Timing (BTT) is considered as the most promising technique for operational blade-vibration monitoring, which obtains the parameters that characterize the blade condition from recorded signals. However, its application is hindered by severe undersampling and stringent probe layouts. An inappropriate probe layout can make most of the existing methods invalid or inaccurate. Additionally, a general conflict arises between the allowed and required layouts because of arrangement restrictions. For the sake of economy and safety, parameter identification based on fewer probes has been preferred by users. In this work, a spatial-transformation-based method for parameter identification is proposed based on a single-probe BTT measurement. To present the general Sampling-Aliasing Frequency (SAFE) map definition, the traditional time–frequency analysis methods are extended to a time-sampling frequency. Then, a SAFE map is projected onto a parameter space using spatial transformation to extract the slope and intercept parameters, which can be physically interpreted as an engine order and a natural frequency using coordinate transformation. Finally, the effectiveness and robustness of the proposed method are verified by simulations and experiments under uniformly and nonuniformly variable speed conditions. 相似文献
22.
为了对G-16EP型电瓶进行维护和保养,根据电瓶厂家规定和适航规范,总结了该型电瓶的充电和容量测试(放电)方法,指出了影响电瓶寿命的主要因素,为该型号电瓶的维护提供了参考。 相似文献
23.
24.
临近空间飞行器近年来得到了广泛的关注和研究。为克服传统飞艇和太阳能飞机尺寸大、抗风能力差的缺点,本文提出了一种升浮一体飞行器概念方案,并对其总体参数设计方法进行研究。以能量平衡分析为核心,建立了太阳能电池系统、燃料电池系统、推进系统等子系统的数学模型,给出了适合于该飞行器的总体参数设计方法,并对总体设计参数进行了研究。结果表明,升浮一体飞行器相对于传统飞艇,体积下降了53%,长度下降了22%,起飞重量下降了4%。相对于固定翼太阳能飞机,翼展下降了52%,机翼面积减小了56%,起飞重量下降了3.5%。该类飞行器总体参数对飞行速度非常敏感,飞行速度从30 m/s提高至40 m/s时,起飞重量增加约1倍,艇体体积增大77%。提高太阳能电池、燃料电池和螺旋桨效率可有效降低起飞重量,且升浮一体飞行器比传统飞艇对上述参数更敏感。 相似文献
25.
操纵负荷系统是人在回路仿真系统中的负载模拟装置,它要完成对飞行员十分敏感的驾驶杆力和脚蹬力的仿真,其部件模型的设计满足了操纵负荷系统的通用性。此操纵负荷系统在某型机工程模拟器上的应用测试结果表明,该设计符合直升机飞行模拟器鉴定标准的C级要求。 相似文献
26.
In this paper we review the possible mechanisms for production of non-thermal electrons which are responsible for the observed
non-thermal radiation in clusters of galaxies. Our primary focus is on non-thermal Bremsstrahlung and inverse Compton scattering,
that produce hard X-ray emission. We first give a brief review of acceleration mechanisms and point out that in most astrophysical
situations, and in particular for the intracluster medium, shocks, turbulence and plasma waves play a crucial role. We also
outline how the effects of the turbulence can be accounted for. Using a generic model for turbulence and acceleration, we
then consider two scenarios for production of non-thermal radiation. The first is motivated by the possibility that hard X-ray
emission is due to non-thermal Bremsstrahlung by nonrelativistic particles and attempts to produce non-thermal tails by accelerating
the electrons from the background plasma with an initial Maxwellian distribution. For acceleration rates smaller than the
Coulomb energy loss rate, the effect of energising the plasma is to primarily heat the plasma with little sign of a distinct
non-thermal tail. Such tails are discernible only for acceleration rates comparable or larger than the Coulomb loss rate.
However, these tails are accompanied by significant heating and they are present for a short time of <106 years, which is also the time that the tail will be thermalised. A longer period of acceleration at such rates will result
in a runaway situation with most particles being accelerated to very high energies. These more exact treatments confirm the
difficulty with this model, first pointed out by Petrosian (Astrophys. J. 557:560, 2001). Such non-thermal tails, even if possible, can only explain the hard X-ray but not the radio emission which needs GeV or
higher energy electrons. For these and for production of hard X-rays by the inverse Compton model, we need the second scenario
where there is injection and subsequent acceleration of relativistic electrons. It is shown that a steady state situation,
for example arising from secondary electrons produced from cosmic ray proton scattering by background protons, will most likely
lead to flatter than required electron spectra or it requires a short escape time of the electrons from the cluster. An episodic
injection of relativistic electrons, presumably from galaxies or AGN, and/or episodic generation of turbulence and shocks
by mergers can result in an electron spectrum consistent with observations but for only a short period of less than one billion
years. 相似文献
27.
大规模场景的沉浸式投影系统大都以环幕作为显示设备,而由环幕造成的几何失真使系统真实感大大降低。从环幕产生失真的几何原理出发,通过建立投影平面和成像面之间的坐标映射关系,生成了一种几何失真校正的理论模型。同时,研究了一种适于通用加速计算的图形硬件架构CUDA,基于其多线程的硬件执行机制,通过将几何失真的校正矩阵组织成纹理进行多重纹理贴图映射,设计了预失真校正的硬件加速算法,该算法还利用基于权值的超采样技术对加速中的走样进行了设计。最后,对该方法的校正效率和效果进行了实验验证,证明该方法具有更高的场景交互速度和很好的校正效果。 相似文献
28.
This paper presents an application of the recent relativistic HLLC approximate Riemann solver by Mignone & Bodo to magnetized
flows with vanishing normal component of the magnetic field. The numerical scheme is validated in two dimensions by investigating
the propagation of axisymmetric jets with toroidal magnetic fields. The selected jet models show that the HLLC solver yields
sharper resolution of contact and shear waves and better convergence properties over the traditional HLL approach. 相似文献
29.
为降低航空发动机涡轮盘失效风险并提高使用寿命,将主动热载荷管理技术应用于预置裂纹的涡轮盘模型,采用通用权函数法计算裂纹应力强度因子进而分析轮盘寿命,研究经主动热载荷管理的轮盘上能量分布对轮盘寿命的影响,探索轮盘上热边界载荷与寿命的关联性和变化规律,并通过有限元仿真模拟初步分析其作用机理。结果表明:主动热载荷管理技术通过优化轮盘的温度分布,可以有效地降低裂纹附近的应力,延缓裂纹的扩展,显著的提高寿命和安全性,当热边界载荷系数分别取0.05和0.10时,轮盘相应的寿命分别增加12.2%和26.1%。 相似文献
30.