Comparison of electron density measurements from CSES and Swarm satellites with GNSS ionospheric tomography data

Electron density measurements obtained from China Seismo‐Electromagnetic Satellite (CSES) and Swarm-B can play an increasingly important role in the study of ionosphere above F2 peak height. This study presented a comprehensive comparison of electron density products obtained from Langmuir probe mounted on CSES and Swarm-B with ionospheric tomography for a whole year period of 2019. CSES was fully compared with Swarm-B on a global scale, including both absolute and relative differences, and a new index called NFI was developed to better quantify the similarity between two latitudinal profiles of electron density. CSES and Swarm-B were then compared with tomography respectively in four regions, roughly located in America, Europe, Australia and China. Results indicated that CSES data are consistent with Swarm-B, as NFI values exceed 0.6 for most of the analyses. Tomography and Swarm-B were found to have a good agreement as their biases are less than 0.2 × 10⁵ el/cm³ in general. For the comparison between CSES and tomography, the bias increased to around 0.6 × 10⁵ el/cm³ but the standard deviation changed slightly, validating the underestimation of electron density by CSES. The spatiotemporal comparisons of CSES and Swarm-B with tomography showed that: 1) the differences in electron density were relatively low in middle latitudes and increased rapidly in the regions of equatorial ionization anomaly; 2) Swarm-B has a better consistent with tomography than CSES, but both are capable of detecting ionosphere anomalies such as midlatitude arcs; and 3) CSES and Swarm-B both can capture the seasonal changes of electron density, while their values are basically smaller than those from tomography in Spring and Summer months.     

肋参数对液氧甲烷发动机推力室强化换热的影响

为深入研究带肋推力室强化传热的机理，对带肋液氧/甲烷推力室的燃烧与再生冷却进行了流动与传热耦合分析，并针对不同肋高和肋数目进行了参数化分析。结果表明:引入等效平均热流密度的概念可以准确描述带肋推力室中的实际传热过程;平均热流密度总是随着肋数目的增加而减小，当肋高恒定时，由于总换热面积增大，等效平均热流密度会随着肋数目的增加而增大;而当总表面积恒定时，等效平均热流密度会随肋数目的增加而减小。此外，盲目地增大总换热面积并不一定能改善传热强化，甚至会在某些情况下恶化传热，因此在设计过程中也应该结合其他肋参数进行综合考虑。     

遥感卫星多路数据传输系统同频共用方法

为节省频率资源，遥感卫星通常采用扩频体制实现多路数据的同频共用传输，针对通道间容易引起相互干扰的问题进行了研究，通过改进码分多址干扰估算模型，对采用平衡Gold码序列扩频系统抗干扰容限上界进行预测。在满足国际电信联盟（ITU）对卫星辐射功率通量密度约束条件下，提出了一种基于直接序列扩频体制的两路业务数据同频共用传输方法。仿真结果表明：当载波频率2GHz左右，两路辐射源的EIRP之差不大于8～15dBw时可以实现同频共用传输；如对信号扩频带宽进行差异化处理，则其相互兼容性还可进一步提高。     

齿轮故障识别的密度峰值聚类欠定盲源分离算法

为提高盲源分离算法在振动源数目估计问题中的噪声鲁棒性，提出了一种基于密度峰值聚类的欠定盲源分离算法。对预处理后的信号提取单源点，通过密度峰值聚类对单源点进行聚类得到混合矩阵的估计值。通过基于压缩感知模型对源信号进行重构，得到分离信号。为验证所提算法分离准确性和噪声鲁棒性，用所提算法对不同信噪比下的仿真信号进行分离，结果显示：在信噪比不低于4 dB时，所提算法均可以准确分离出源信号，算法的准确性和鲁棒性得到验证。设计旋转部件故障诊断试验台对所提算法在实际应用中的有效性进行验证，对实测复合故障振动信号进行分离，试验结果表明该算法成功分离出观测信号中的锥齿轮和行星齿轮单一故障特征，有助于工程中旋转部件故障诊断。     

Lift enhancement based on virtual aerodynamic shape using a dual synthetic jet actuator

The Dual Synthetic Jet Actuator (DSJA) is used to develop a new type of lift enhancement device based on circulation control, and to control the flow over the two-dimensional (2D) NACA0015 airfoil. The lift enhancement device is composed of a DSJA and a rounded trailing edge (Coanda surface). The two outlets of the DSJA eject two jets (Jet 1 and Jet 2). Jet 1 ejects from the upper trailing edge, which increases the circulation of airfoil with the help of the Coanda surface. Jet 2 ejects from the lower trailing edge, which acts as a virtual flap. The Reynolds number based on the airfoil chord length and free flow velocity is 250000. The results indicate that the circulation control method based on Dual Synthetic Jet (DSJ) has good performance in lift enhancement, whose control effect is closely related to momentum coefficient and reduced frequency. With the increase of the reduced frequency, the control effect of the lift enhancement is slightly reduced. As the momentum coefficient increases, the control effect becomes better. When the angle of attack is greater than 4°, the increments of lift coefficients under the control of DSJ are larger than those under the control of the steady blowing at a same momentum coefficient. The maximum lift augmentation efficiency can reach 47 when the momentum coefficient is 0.02, which is higher than the value in the case with steady blowing jet circulation control.     

不同机织结构碳布针刺后拉伸性能

针刺后碳布拉伸强力的大小决定了针刺预制体的性能,研究针刺后碳布拉伸强力可以为针刺工艺

参数优化、提高预制体性能提供重要参考。本文研究了不同机织结构碳布针刺前、后的拉伸性能及影响拉伸强力

的主要因素。在3K 平纹碳布、3K 斜纹碳布及3K 缎纹碳布中,3K 斜纹碳布具有较高的拉伸强力、较大的拉伸强

力保留率,针刺工艺性最好。在一定的针刺工艺下,碳布各层拉伸强力可以用函数y = A1 伊e-x / t1 + y0 来模拟,其中

A1、t1、y0为常数。针刺密度是影响针刺后碳布拉伸强力及强力保留率的主要因素,最终针刺密度决定了针刺后碳

布拉伸强力的大小。3K 斜纹碳布在针刺密度为26 针/ cm2 时,经、纬向的拉伸强力与未针刺时相比分别下降了

42.0%和49.1%;当针刺密度为32 针/ cm2时,其经、纬向拉伸强力则分别下降了71.4%和78郾8%。

     

TA15粉末冶金产品热等静压成形工艺过程的数值模拟

针对高品质粉末冶金新产品的研发,为了减少其研发周期、降低试验成本,采用Marc模拟软件,对轴承座产品的热等静压近净成形过程进行了有限元数值模拟。结果表明:经工艺成形后,产品几何外形尺寸变化较大,相对密度整体达到0.98,局部尖端位置相对密度仅为0.85,对此提出了改进包套结构和芯模结构形式、局部增加装粉量等方案,提高局部位置致密度,保证产品整体质量,为产品的实际生产提供了理论指导作用。     

The global response of terrestrial ionosphere to the December 2015 space weather event

This paper investigates the ionospheric storm of December 19–21, 2015, which was initiated by two successive CME eruptions that caused a G3 space weather event. We used the in situ electron density (N_e) and electron temperature (T_e) and the Total Electron Content (TEC) measurements from SWARM-A satellite, as well as the O/N₂ observations from TIMED/GUVI to study the ionospheric impact. The observations reveal the longitudinal and hemispherical differences in the ionospheric response to the storm event. A positive ionospheric storm was observed over the American, African and Asian regions on 20 December, and the next day showed a negative storm. Both these exhibited hemispheric differences. A positive storm was observed over the East Pacific region on 21 December. It is seen that the net effect of both the disturbance dynamo electric field and composition differences become important in explaining the observed variability in topside ionospheric densities. In addition, we also discuss the T_e variations that occurred as a consequence of the space weather event.     

Orbital error propagation considering atmospheric density uncertainty

Due to the influence of various errors, the orbital uncertainty propagation of artificial celestial objects while orbit prediction is required, especially in some applications such as conjunction analysis. In the orbital error propagation of artificial celestial objects in low Earth orbits (LEOs), atmospheric density uncertainty is one of the important factors that require special attention. In this paper, on the basis of considering the uncertainties of position and velocity, the atmospheric density uncertainty is also taken into account to further investigate the orbital error propagation of artificial celestial objects in LEOs. Artificial intelligence algorithms are introduced, the MC Dropout neural network and the heteroscedastic loss function are used to realize the correction of the empirical atmospheric density model, as well as to provide the quantification of model uncertainty and input uncertainty for the corrected atmospheric densities. It is shown that the neural network we built achieves good results in atmospheric density correction, and the uncertainty quantization obtained from the neural network is also reasonable. Moreover, using the Gaussian mixture model - unscented transform (GMM-UT) method, the atmospheric density uncertainty is taken into account in the orbital uncertainty propagation, by adding a sampled random term to the corrected atmospheric density when calculating atmospheric density. The feasibility of the GMM-UT method considering atmospheric density uncertainty is proved by the further comparison of abundant sampling points and GMM-UT results (with and without considering atmospheric density uncertainty).     

空中交通复杂性研究进展

空中交通复杂性是空中交通态势的本质属性，是空中交通管制工作负荷的主要驱动因素。空中交通复杂性的科学评价是实现空中交通精细化管理的关键，也是当前空管领域研究热点。本文介绍了国内外空中交通复杂性的研究团队，梳理了空中交通复杂性与工作负荷、安全水平等相互之间的区别和联系，并详细分析了现有研究的具体研究路线。在分析新一代空中交通管理系统特征的基础上，对空中交通复杂性的未来研究趋势和方向进行了展望。