A coordinated study of field-aligned currents and Pc5 ULF waves during ejecta 1997

We show examples of long period Pc5 magnetic field pulsations near field-aligned current (FAC) regions in the high-latitude magnetosphere, observed by INTERBALL-Au, and coordinated with POLAR, GOES-9 and ground-based observations during 11 January and 11 April 1997. Identification of corresponding magnetosphere regions and subregions is provided by electrons and protons in the energy-range of 0.01–100 keV measured onboard the spacecraft. The ULF Pc5 wave occurrence is observed in both upward and downward FACs. A fairly good correlation is demonstrated between these ULF Pc5 waves and the consecutive injection of magnetosheath low energy protons. The constancy of the observed frequency peak at 1.8 mHz during quite unsteady solar wind pressure conditions could be reconciled with the surface wave mode model. The 3.1 mHz peak location area probably resembles field-line fluctuations with an interesting appearance of poloidal mode oscillation. It is suggested that the 1.3 mHz wave and its harmonic 2.6 mHz represent global compressional oscillations.     

月球图像传输与处理的分析和仿真

需要一个平台对探月卫星,探月图像传输和处理进行研究. 嫦娥一号月球图像的传输与处理的仿真,结合了链路分析,采用MATLAB GUI 和虚拟现实设计工具。由于图像在深空传输中,距离较远,信号会受到很大的衰减,传输质量会受到噪声干扰的严重影响。因此要对系统链路进行严格的预算分析,包括考虑地球大气产生的影响,以确保信号传输质量满足要求,另外还要通过适当算法提高图像的清晰度。这种仿真方法对探月图像传输的研究奠定了基础,并且对降低探月成本有一定的帮助。     

近地空间磁场梯度分布特性及磁力效应研究

以国际地磁参考场模型IGRF11为基础,推导出地球磁场梯度分布公式,并对近地空间磁场分布特点进行了分析。由基本磁力学可知,带强磁体的航天器在地磁环境中不仅受到磁力矩作用,还将受到与地磁梯度相关的磁力的影响。根据地磁环境下的磁体受力机理,文章讨论了以弱磁力改变轨道倾角的方法,并通过数值仿真验证了其有效性。     

Inner core wobble and free core nutation of pulsar PSR B1828-11

PSR B1828-11 has long-term, highly periodic and correlated variations in pulse shape and a slow-down rate with period variations of approximately 1000, 500 and 250 days [Stairs, I.H., Lyne, A.G., Shemar, S.L. Evidence for free precession in a pulsar. Nature 406, 484–486, 2000]. There are three potential explanations of pulses time-of-arrival from a pulsar. These are related to the interior of the neutron star, planetary bodies, free precession and nutation. We use the Hamiltonian canonical method of Getino (1995) for analyzing the dynamically symmetric pulsar PSR B1828-11, consisting of a rigid crust, elliptical liquid outer core and solid inner core. Using the theory of differential rotation of a pulsar, we investigate the dependence on Chandler wobble period, inner core wobble, retrograde free core nutation and prograde free inner core nutation from ellipticity of the inner crystal core, outer liquid core and total pulsar.     

TC11钛合金片层组织热变形球化动力学过程

通过热压缩试验研究了TC11钛合金退火态片层组织在两相区980℃,950℃,850℃,应变速率0.001s-1,0.01s-1条件下,变形程度30%～70%范围内的热变形过程.分析了热变形参数对变形行为和片层组织球化过程的影响,并根据片层组织球化分数演变特征,建立了修正的Avrami 片层组织球化动力学方程,与试验数据吻合较好.     

10mm厚TC11钛合金电子束焊接熔池传热与流动行为研究

采用ANSYS软件中的Flotran模块,建立了基于高斯面热源与峰值热流递增的旋转体热源相结合的新型复合热源模型,合理地模拟了10mm厚TC11钛合金平板的电子束焊接熔池传热与流动行为。结果表明:计算熔池边界与真实焊缝的熔合线轮廓吻合较好,均呈现电子束焊接典型的"钉子形"焊缝。     

TC11材料高低周疲劳裂纹萌生与扩展特性研究

通过对航空发动机叶片用TC11材料在高低周复合载荷下进行裂纹扩展试验,研究了TC11材料高低周复合疲劳裂纹扩展规律,得到了高低周载荷条件下的裂纹稳态扩展曲线及断口特征。其结果可对风扇/压气机叶片抗高低周复合载荷下的裂纹扩展能力进行分析和评估,为下一代先进航空发动机设计提供技术支撑。     

数据链测试仿真评估中的信道与链路干扰仿真技术

信道和链路干扰仿真是数据链测试仿真评估系统的关键技术之一。在局域网下模拟数据链系统真实运行的无线环境的非理想特性,需要对典型应用环境的信道条件、干扰特征进行分析和建模,仿真验证数据链系统在不同环境条件下的性能。本文首先分析了几类常见的信道和链路干扰仿真工具相关模块的原理和机制,研究并提出了传输时延、信道与链路干扰、链路级仿真方法及方案,并对几个关键问题进行了分析并提出解决方案。该研究在数据链测试仿真评估系统中的验证效果良好,能够为数据链系统可靠性、稳定性提供无线信道和链路干扰模拟工具,从而为数据链系统的设计提供参考和依据。     

Analysis of ionospheric TEC response to solar and geomagnetic activities at different solar activity stages

Studying the relationship of total electron content (TEC) to solar or geomagnetic activities at different solar activity stages can provide a reference for ionospheric modeling and prediction. On the basis of solar activity indices, geomagnetic activity parameters, and ionospheric TEC data at different solar activity stages, this study analyzes the overall variation relationships of solar and geomagnetic activities with ionospheric TEC, the characteristics of the quasi-27-day periodic oscillations of the three variables at different stages, and the delayed TEC response of solar activity by conducting correlation analysis, Butterworth band-pass filtering, Fourier transform, and time lag analysis. The following results are obtained. (1) TEC exhibits a significant linear relationship with solar activity at different solar activity stages. The correlation coefficients |R| are arranged as follows: |R|_EUV > |R|_F10.7 > |R|sunspot number. No significant linear relationship exists between TEC and geomagnetic activity parameters (|R| < 0.35). (2) TEC, solar activity indices, and geomagnetic activity parameters have a period of 10.5 years. The maximum amplitudes of the Fourier spectrum for TEC and solar activity indices are nearly 27 days and those of geomagnetic activity parameters are nearly 27 and 13.5 days. (3) The deviations of the quasi-27-day significant periodic oscillation of TEC and solar activity indices are consistent. (4) No evident relationship exists between the quasi-27-day periodic oscillation of TEC and geomagnetic activity parameters. (5) The delay time of TEC for the 10.7 cm solar radio flux and extreme ultraviolet is always consistent, whereas that for sunspot number varies at each stage.