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1.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(11):2551-2558
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 (Psw) 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 Psw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in Psw. It proved that the enhancement of Psw 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 Psw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the Psw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. 相似文献
2.
偏心撞击对撞击式喷嘴雾化特性的影响 总被引:2,自引:0,他引:2
为研究偏心撞击对撞击式喷嘴雾化特性的影响,建立了求解自燃推进剂冷态射流撞击雾化过程的数值模拟方案,计算了不同偏心度条件下的射流撞击雾化过程。采用树形自适应加密算法直接求解不可压Navier-Stokes方程组,由分段线性的流体体积(VOF)方法对流体界面进行捕捉。结果表明偏心撞击会导致雾场发生偏转,当无量纲偏心度E为1/8时,雾场偏转角度约为9.2°,应控制加工偏差小于该值。随着偏心度的增大,液膜的偏转角度增大,理论推导得到的液膜偏转角度要小于数值计算得到的液膜偏转角度。正心撞击时燃料与氧化剂流强峰值接近,雾场的流强分布呈单峰分布。当发生偏心撞击时,由于燃料与氧化剂部分射流未参与撞击导致流强峰值出现交错,雾场的流强分布呈双峰分布,混合比的空间分布发生较大改变。正心撞击时撞击点下游液滴的速度分布近似呈轴对称分布,而偏心撞击之后的速度分布则呈中心对称分布。偏心撞击导致的射流动量损失使得雾化性能变差,当无量纲偏心度E为1/8时,一甲基肼(MMH)的Sauter平均直径增大约4.8%,四氧化二氮(NTO)的Sauter平均直径增大约5.8%。 相似文献
3.
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. 相似文献
4.
5.
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。 相似文献
6.
A. Aran B. Sanahuja D. Lario 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2333-2338
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. 相似文献
7.
转动坐标系中三维跨声速欧拉流的有限体积 TVD格式 总被引:4,自引:2,他引:4
在非惯性转动坐标系中,本文采用贴体网格、有限体积法离散和修正数值通量技术,将Harten的一维TVD格式推广到三维。由于转动使方程出现源项,文中通过对源项的巧妙处理,使修改后的格式能用于非齐次双曲守恒律方程组高分辨率的数值计算。为了加速解的收敛,提高显式时间推进的CFL数,本文采用隐式残值光顺技术。三维跨声速带非齐次源项欧拉方程的典型算例表明:捕捉的激波分辨率较高;激波前后没有发现大的数值波动和伪振荡现象;所得的跨声速流场解与实验较接近。 相似文献
8.
考虑可压缩与热传导的壁面函数边界条件及其应用 总被引:4,自引:0,他引:4
考虑到可压缩和热传导效应的壁面函数边界条件,被耦合到了采用k-ω两方程湍流模型、用有限体积法求解N-S方程的程序中。壁面函数基于耦合的速度和温度型,并且在边界层内的粘性子区和对数区内一致有效。引入壁面函数边界条件后,通过算例验证在y <100的范围内,得到的物面压力、摩阻、热流与实验结果比较,结果可靠。而无壁面函数边界条件时,要得到相同精度的结果,要求y ≈1。壁面函数的引入,为工程上准确预测飞行器在湍流流动中表面受力与气动热提供了保障。 相似文献
9.
顺序函数法求解二维非稳态热传导逆问题 总被引:2,自引:0,他引:2
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。 相似文献
10.
活性化焊剂对堆焊焊缝熔深的影响 总被引:1,自引:0,他引:1
在采用TIG焊接方法时,在奥氏体不锈钢的表面涂敷一层活性化焊剂进行焊接,会影响焊缝熔深的变化。研究结果表明:在相同焊接工艺参数下,与普通TIG焊相比,涂敷活性化焊剂对焊缝熔深有一定的影响,A—TIG焊的焊缝熔深要明显大于普通TIG焊的焊缝熔深,并且不同的活性化焊剂成分对焊缝熔深有不同的影响,活性化焊剂F5可使堆焊焊缝熔深达到6.39mm。 相似文献