谐振式加速度计自激振荡电路性能评价方法的研究

针对谐振式加速度计成品率不高、精度低等问题,以石英振梁加速度计为例,采用引进标准信号,将谐振电路作为"黑盒子",对其开展独立的评价.通过评价电路的驱动电压幅值稳定性、移相稳定性、全温幅值/相位对称性等指标,与加速度计实际指标建立了一一对应的关系,为加速度计研制与性能提升提供了有效依据.实际运用表明,电路噪声性能、温度性...     

翅片位置对复合式减涡器减阻性能影响数值模拟

为了探索翅片-管复合式减涡器的翅片安装位置对共转盘腔径向内流压力损失的影响规律,对不同转速、翅片周向位置及安装角度下的去旋系统开展了数值研究,得到了不同工况下共转盘腔径向内流的流场结构及压力损失分布曲线。研究结果表明:减涡管能引导流体径向流入,并降低流体的旋流比;相比于管式减涡器,翅片-管复合式减涡器能明显降低盘腔内的总压损失;在不同旋转雷诺数下,翅片的周向安装位置α及安装角β均存在最佳值;在中、高旋转雷诺数下,最佳值分别为α=9°,β=30°,最佳结构下总压损失较基础模型低40%左右;改变翅片周向位置及安装角度可以明显改变气流进入减涡管的角度,在较优情况下,可以减小流体流入减涡管的阻力及在减涡管内的流动阻力,整体上减小了盘腔内总压损失。     

GNSS single frequency ionospheric range delay corrections: NeQuick data ingestion technique

A study of the performance of the NeQuick model and the Klobuchar model for GNSS single frequency range delay correction on a global scale was done using data for moderate solar activity. In this study NeQuick was used in the way intended for Galileo. This study is to assess the performance of the two models at each ionospheric geographic region during moderate solar activity as previously published studies were concentrated only on high solar activity. The results obtained showed that NeQuick outperformed Klobuchar for the whole year at the three geographical regions of the ionosphere. In terms of monthly root mean square of mismodeling, NeQuick outperformed Klobuchar by 15 TECU or more at low-latitudes, 5 TEC or more at mid-latitudes, and 1 TECU or more at high-latitudes.     

Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm

The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30–45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere.     

浅凹槽底壁横向燃料喷射对流动和燃烧特性的影响

模拟了高度30km,飞行马赫数6的超声速燃烧室流场和燃烧特性.通过对固定长度、不同深度的一组浅凹槽底壁燃料横向喷射的燃烧室的冷态与燃烧工况进行数值计算,并将其和传统壁面横向喷射方式进行比较,发现引入浅凹槽底壁喷射结构能有效减弱流场的激波系强度,明显降低燃烧流场的总压损失;凹槽前壁面和喷流柱之间形成稳定的亚声速回流区,能够稳定火焰,这在较大深度凹槽会更明显.引入浅凹槽一定程度降低了横向射流穿透深度,这也导致燃烧效率相比传统壁面横向喷射结构有一定下降.     

槽道射流及端壁抽吸对角区分离的组合控制研究

为优化叶片吸力面流动分离结构,探究对于角区分离更好的流动控制方法,以一大弯角扩压静子叶栅为研究对象,对叶片进行全叶高槽道结构处理,并在其基础上于槽道出口前进行端壁抽吸槽结构处理.在来流马赫数为0.7,来流攻角为-8°～6°工况下,对原型叶栅、全叶高开槽叶栅及组合流动控制叶栅进行性能计算及对比.结果表明:全叶高开槽方案能...     

接受孔形状对预旋供气系统内气流流动影响研究

为对比不同形状接受孔的预旋系统内气流流动特性,通过数值模拟方法,对带有不同形状接受孔的预旋系统进行了研究。研究发现:收缩型接受孔入口截面气流流通面积较大,相对速度较小,在预旋系统中的性能最优,其次是类梯型,最后是直孔型。同一旋转雷诺数下,带收缩型接受孔的预旋系统无量纲温降较直孔型提高5.8%,总压损失系数降低3.0%。三种类型接受孔的预旋系统无量纲温降和总压损失系数均随进出口压比的增加而增大,在相同压比下,收缩型接受孔预旋系统无量纲温降最大,总压损失系数最小。     

Relative amplitude of the total electron content variations depending on geomagnetic activity

We developed a method of estimation of a relative amplitude dI/I of the total electron content (TEC) variations in the ionosphere as deduced from the data of the global GPS receivers network. To obtain statistically significant results we picked out three latitudinal belts provided in the Internet by the maximum number of GPS sites. They are high-latitudinal belt (50–80°N, 200–300°E; 59 sites), mid latitude belt (20–50°N, 200–300°E; 817 sites), and equatorial belt (±20°N, 0–360°E; 76 sites). The results of the analysis of the diurnal and latitudinal dependencies of dI/I and dI/I distribution probability for 52 days with different levels of geomagnetic activity are presented. It was found that on average the relative amplitude of the TEC variations varies within the range 0–10% proportionally to the value of the K_p geomagnetic index. In quiet conditions the relative amplitude dI/I of the TEC variations at night significantly exceeds the daytime relative amplitude. At high levels of magnetic field disturbances, the geomagnetic control of the amplitude of TEC variations at high and middle latitudes is much more significant than the regular diurnal variations. At the equatorial belt, on average, the amplitude of TEC variations in quiet and disturbed periods almost does not differ. The obtained results may be useful for development of the theory of ionospheric irregularities.