Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

Collision Risk Mitigation in Geostationary Orbit

The short- and long-term effects of spacecraft explosions, as a function of the end-of-life re-orbit altitude above the geostationary orbit (GEO), were analyzed in terms of their additional contribution to the debris flux in the GEO ring. The simulated debris clouds were propagated for 72yrs, taking into account all the relevant orbital perturbations.The results obtained show that 6–7 additional explosions in GEO would be sufficient, in the long term, to double the current collision risk with sizable objects in GEO. Unfortunately, even if spacecraft were to re-orbit between 300 and 500km above GEO, this would not significantly improve the situation. In fact, an altitude increase of at least 2000km would have to be adopted to reduce by one order of magnitude the long-term risk of collision among geostationary satellites and explosion fragments. The optimal debris mitigation strategy should be a compromise between the reliability and effectiveness of spacecraft end-of-life passivation, the re-orbit altitude and the acceptable debris background in the GEO ring. However, for as long as the re-orbit altitudes currently used are less than 500km above GEO, new spacecraft explosions must be avoided in order to preserve the geostationary environment over the long term.     

航天器的防污染技术

简单介绍了航天器污染的概念,污染对航天器的损害,航天器污染研究的重要性,以及国内外航天器防污染研究概况。着重介绍真空热试验中的污染控制方法。引入航天器自污染的概念,介绍消除航天器自污染的有效办法是真空烘烤。     

网络最大流与最小割集的矩阵算法

本文给出了解决运输问题为中心的一类特殊的线性规划问题的新的、简便的算法。网络最大流与最小割集的矩阵算法,不仅能解决许多这类问题,而且能使最小费用流、分配问题和运输问题容易通过计算机来实现。     

A first step towards proton flux forecasting

We present a preliminary version of a potential tool for real time proton flux prediction which provides proton flux profiles and cumulative fluence profiles at 0.5 and 2 MeV of solar energetic particle events, from their onset up to the arrival of the interplanetary shock at the spacecraft position (located at 1 or 0.4 AU). Based on the proton transportation model by Lario et al. [Lario, D., Sanahuja, B., Heras, A.M. Energetic particle events: efficiency of interplanetary shocks as 50 keV E < 100 MeV proton accelerators. Astrophys. J. 509, 415–434, 1998] and the magnetohydrodynamic shock propagation model of Wu et al. [Wu, S.T., Dryer, M., Han, S.M. Non-planar MHD model for solar flare-generated disturbances in the Heliospheric equatorial plane. Sol. Phys. 84, 395–418, 1983], we have generated a database containing “synthetic” profiles of the proton fluxes and cumulative fluences of 384 solar energetic particle events. We are currently validating the applicability of this code for space weather forecasting by comparing the resulting “synthetic” flux profiles with those of several real events.     

微束等离子焊接钛合金薄板保护规律的研究

 通过试验认为微束等离子焊接钛合金薄板的保护问题,关键在于控制施焊时焊缝处于700℃以上的加热范围,和700℃到400℃的冷却时间。并论证了以氧的污染层厚度作为钛合金焊接污染程度判据的合理性。本文采用电子探针法对氧污染层厚度进行了测定,求出污染方程。从而。使微束等离子焊接钛合金薄板的污染问题,可通过调整焊接规范进行控制。     

顺序函数法求解二维非稳态热传导逆问题

基于有限控制体积法对二维非稳态热传导问题的数值模拟，导出了处理二维非稳态热传导逆问题的顺序函数法，并用该方法来对一典型的圆环域边界条件反演问题进行了反演计算，结果表明，顺序函数法是求解二维非稳态热传导逆问题的有效方法，当测量噪声比较小时，顺序函数法能得出较高精度的反演结果；当测量噪声增大时，反演结果仍能较好地再现出精确解在空间和时间方向上的变化趋势，具有一定精度。     

新型阻燃Ti40合金TIG焊焊接性能研究

研究新型阻燃钛合金Ti40合金的TIG(tungest inert gas)焊焊接性能,采用金相、SEM等方法分析Ti40合金焊缝及热影响区的组织变化.结果表明,Ti40合金钨极氩弧焊焊缝室温、高温拉伸性能良好,冲击性能较低.焊接之后的热处理制度对组织有一定的改善.经500℃×100h热暴露后,晶界粗化,为连续α相.     

时效处理对T-250钢电子束焊接接头组织及性能的影响

采用金相显微镜、透射电镜观察了焊后不同时效状态下T— 2 5 0马氏体时效钢电子束焊缝的微观组织 ,测试了不同时效状态下焊接接头的室温强度、夏比缺口冲击韧性、显微硬度 ,并用扫描电镜分析了拉伸断口形貌。结果表明 :随时效温度的升高 ,焊缝区枝晶间逆转奥氏体析出量增加 ,焊缝缺口冲击韧性增大 ,断口韧窝增大 ;但由于 5 0 0℃× 4h时效处理后焊缝马氏体孪晶较多而使其拉伸强度和缺口冲击韧性降低。经 4 80℃× 4h时效处理后 ,焊接接头强度具有最佳强韧性配合     

大厚度铝合金飞行器结构的焊接

介绍了采用熔化极脉冲氦弧焊工艺焊接大厚度铝合金燃料箱的优越性。