高精度稠粘流体压力传感器

一种高精度流体压力传感器,这种传感器除适用于测量普通气体、液体的压力外,特别适用于稠粘流体的压力测量。文中着重阐述了这种传感器的工作原理、结构特点及性能指标,并简要介绍了设计中的一些考虑,指出了这种传感器的发展潜力和应用前景。     

分开排气式喷管喷流噪声预测及试验研究

为揭示涡扇发动机分开排气式喷管喷流噪声的频谱分布和指向特性,对喷管缩比模型远声场喷流噪声进行了预测及试验研究,并开展了全尺寸喷管基准型及锯齿型喷流噪声的预测工作。结果表明:采用Tam & Auriault方法可以预测出喷流噪声的声压级值和空间指向分布,喷流噪声具有明显的指向性。与基准型喷管相比,锯齿型喷管具有良好的降噪效果;内外涵锯齿型喷管在中低频段的降噪效果优于内涵锯齿型喷管,在高频段的降噪效果差于内涵锯齿型喷管;在本文研究参数范围内,指向角小于88°时内外涵锯齿型喷管总声压级(OASPL)值高于内涵锯齿型喷管。     

环型超声速空气引射器零二次流流场数值研究

采用二维轴对称雷诺平均方程和标准κ-ε双方程湍流模型，数值研究了环型超声速引散器零二次流的流场结构及盲腔压强的变化，空间上采用二阶迎风格式进行耦合求解，时间上采用显示的Runge-Kutta方法进行迭代推进。结果表明，引射器几何参数不变的情况下，启动后的盲腔压强与引射气流总压之比为一常数；喷管马赫数不变情况下，喷管出口面积与混合室入口面积比越小，盲腔压强越低，扩压器性能越好，启动要求的总压越低，对超声速空气引射器的设计具有指导意义。     

Optimal nodal flyby with near-Earth asteroids using electric sail

The aim of this paper is to quantify the performance of an Electric Solar Wind Sail for accomplishing flyby missions toward one of the two orbital nodes of a near-Earth asteroid. Assuming a simplified, two-dimensional mission scenario, a preliminary mission analysis has been conducted involving the whole known population of those asteroids at the beginning of the 2013 year. The analysis of each mission scenario has been performed within an optimal framework, by calculating the minimum-time trajectory required to reach each orbital node of the target asteroid. A considerable amount of simulation data have been collected, using the spacecraft characteristic acceleration as a parameter to quantify the Electric Solar Wind Sail propulsive performance. The minimum time trajectory exhibits a different structure, which may or may not include a solar wind assist maneuver, depending both on the Sun-node distance and the value of the spacecraft characteristic acceleration. Simulations show that over 60% of near-Earth asteroids can be reached with a total mission time less than 100 days, whereas the entire population can be reached in less than 10 months with a spacecraft characteristic acceleration of 1 mm/s².     

利用常规风洞进行二元翼型试验的竖置全跨方法

采用竖置全跨试验方案,在CARDC(中国空气动力研究与发展中心)4米×3米风洞进行了几个二元翼型模型风洞试验。最初选用的模型是NASA GA(W)-1翼型,并作为校验模型。试验雷诺数高达4.69×100~6,攻角范围为-10～24°,试验结果相当满意。     

非定常风洞壁压特性研究

在低速风洞中用2组后掠角分别为70°和65°的三角翼模型进行过失速非定常运动,测量风洞洞壁上非定常壁压。研究风洞非定常壁压的延迟与频率特性。讨论了模型尺寸、缩减频率、前缘后掠角等对风洞非定常壁压的影响。     

空间站大面积太阳翼热分析

本文在一定的假设条件下，对空间站大面积太阳翼进行了系统的热流和温度场计算。在计算中利用矢量分析和坐标变换的方法求解出了太阳直接辐射1地球红外辐射和地球反照的辐射角系数，再根据传热学理论建立了瞬态热平衡方程，应用有限单元法对热平衡方程进行了求解。本文通过计算给出了各项热流的大小及在总热流中所占的比例和太阳民办的瞬态温度场分布，对空间站大面积太阳翼设计及热控制具有一定的参考价值。     

Coronal radio-sounding detection of a CME during the 1997 Galileo solar conjunction

Frequency fluctuations of the Galileo S-band radio signal were recorded nearly continuously during the spacecraft’s solar conjunction from December 1996 to February 1997. A strong propagating disturbance, most probably associated with a coronal mass ejection (CME), was detected on 7 February when the radio ray path proximate point was on the west solar limb at about 54 solar radii from the Sun. The CME passage through the line of sight is characterized by a significant increase in the fluctuation intensity of the recorded frequency and by an increase in the plasma speed from about 234 km s⁻¹ up to about 755 km s⁻¹. These velocity estimates are obtained from a correlation analysis of frequency fluctuations recorded simultaneously at two widely-separated ground stations. The density turbulence power spectrum is found to steepen behind the CME front. The Galileo radio-sounding data are compared with SOHO/LASCO observations of the CME in the corona and with WIND spacecraft data near the Earth’s orbit.     

Solar wind turbulence during the solar cycle deduced from Galileo coronal radio-sounding experiments

Seven coronal radio-sounding campaigns were carried out during the active lifetime of the Galileo spacecraft in the years 1994–2002. The observational data analyzed in the present work are S-band frequency fluctuation measurements recorded during the solar conjunctions at different phases of solar activity cycle #23, specifically: periods near solar maximum (three conjunctions), near solar minimum (three conjunctions) and during the ascending phase (one conjunction). These data are all applicable to low heliographic latitudes, i.e. to the slow solar wind. The rms frequency fluctuation and power-law index of the frequency fluctuation temporal spectra are determined as a function of heliocentric distance. The turbulence power spectrum tends to be flatter inside ca. 20 solar radii during all phases of the solar cycle. This coincides with a transition in the flow from the inner acceleration region to the outer region of constant velocity. The radial falloff rate and absolute level of the rms frequency fluctuation are essentially invariant over the solar cycle.     

径向磁气组合轴承系统的动态性能

为探究磁轴承失效时能否减轻转子跌落带来的损害,将人字槽径向动压气体轴承引入磁轴承转子系统,研究磁气组合轴承对系统动态性能的影响和动压气体轴承的支承特性。采用有限差分法和小扰动法求解气膜厚度方程和雷诺方程,研究动压气体轴承的静动态特性。对磁轴承电磁力进行了分析,采用磁轴承不完全微分PID（比例-积分-微分）控制策略,对系统进行了理论模态分析和试验模态分析,完成了系统高速旋转试验,测试了动压气体轴承在不同偏心率和转速下的承载力。结果表明,引入动压气体轴承可提高系统的动态性能,在磁轴承失效造成高速转子跌落瞬间,偏心率趋近于1,两个径向动压气体轴承能够产生较大承载力,减轻转子跌落造成的损害。