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21.
高速铁路隧道初始压缩波一维流动模型的数值分析方法 总被引:2,自引:0,他引:2
基于隧道内空气流通截面是时间和距离的二元函数条件与一维流动理论,提出了高速列车驶入设有缓冲结构隧道端口时产生初始压缩波的数值分析方法。一维流动理论采用考虑摩擦、传热以及空气质交换等因素的一维可压缩非定常不等熵流动模型。数值分析方法采用广义黎曼变量特征线法。与国外有关未设缓冲结构、开孔型与未开孔型缓冲结构的隧道端口三种情况的现车试验结果进行了比较,表明本文所建方法正确、合理,能够模拟计算多种类型缓冲结构条件下的压缩波波动规律。 相似文献
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以汽油/空气两相混气为可爆混合物,采用汽油机点火和半导体高能点火系统,实验研究了不同点火频率对脉冲爆震室中不同位置脉冲爆震波压力的影响,结果发现,充满度大,产生的紊流强度大,有利于爆震波的形成;在大多数情况下,用低能量(50mJ)的点火系统点火时,点火频率大于实际产生的爆震频率;用高能(IJ)点火系统时,可缩短烯向爆震转变(DDT)的距离,易产生爆震,所得爆震波的峰值压力明显增大,所得结果可为脉冲爆震发动机的设计、爆震点火系统选型提供重要参考。 相似文献
24.
Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for
interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of
electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions
as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory
is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are
bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
25.
平板叶片斜撞击瞬态响应的计算分析 总被引:1,自引:0,他引:1
采用有限元法,对平板叶片在不同鸟撞击角度下的非线性瞬态响应进行了数值分析研究.结果表明,平板叶片在不同撞击角度下的弯曲变形、到达最大变形的时间及残余变形随着撞击角度的增加而增大;平板叶片的扭转变形随着撞击角度的增加先增大后减少,撞击角度在小于30°及90°附近对平板叶片的扭转变形影响很小. 相似文献
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基于响应面法进行了二维混合压缩超燃冲压发动机进气道的多目标优化研究.采用均匀试验设计确定试验方案,运用计算流体动力学求解进气道的性能.根据分析结果构造了响应面近似模型,该模型采用了完全二阶多项式模型.通过响应面近似模型的优化,实现了超燃冲压发动机进气道优化,得到了Pareto最优集.结果表明,采用均匀试验设计和响应面法可以大大减小数值模拟的计算量,提高优化效率. 相似文献
28.
本文采用SOUSYVHF雷达1987年6月22日至6月29日在挪威Andφya(69°N,10°E)的观测数据,研究中层惯性重力波传播的统计特征.21个周期为数小时的准单色波例子,在垂直方向上有确定的相位移动,表明它们是惯性内重力波.通过分析波相关水平扰动速度的矢端曲线,获得了水平传播矢量的大小和方向的分布,大多数(76%)波具有西向传播的波矢分量,似乎与中层顶具有强的西向背景风有关;水平传播速度的大小与中层高度上典型的观测值一致.本文分析结果还表明在极区中不仅存在向上的能量传输,也存在强烈的向下的能量传输. 相似文献
29.
Mukul Kumar Wang Chi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):640-652
We study the Propagation and damping properties of Alfvén gravity waves in the presence of the vertical magnetic field in the viscous solar plasma under influence of the background flow by deriving a fourth order dispersion relation in terms of the Doppler shifted frequency. We derive the dispersion relation under WKB and Boussinesq approximation. We study the damping of Alfvén gravity waves for the wave frequencies less than and greater than the Brunt-Väisälä frequency. We find that the Brunt-Väisälä frequency divides the frequency ranges where the weakly or strongly damped oscillations occur. The background flow exhibits a strong effect on weakly damped oscillations and a weak effect on the strongly damped oscillations. We also notice that the damping of both the strong and weakly damped oscillations depend on the Brunt-Väisälä frequency and wave number. The effect of the background flow is also being governed by the Brunt-Väisälä frequency and wave number. We also study the properties of gravity wave mode after filtering the Alfvén wave mode by minimizing the magnetic field and noticed that the background flow shows a very strong effect on the gravity wave mode. 相似文献
30.
P. Alexander R. Ruscica A.A. Sörensson C.G. Menéndez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Adequate representations of diverse dynamical processes in general circulation models (GCM) are necessary to obtain reliable simulations of the present and the future. The parameterization of orographic gravity wave drag (GWD) is one of the critical components of GCM. It is therefore convenient to evaluate whether standard orographic GWD parameterizations are appropriate. One alternative is to study the generation of gravity waves (GW) with horizontal resolutions that are higher than those used in current GCM simulations. Here we assess the seasonal pattern of topographic GW momentum flux (GWMF) generation for the late 20th and 21st centuries in a downscaling using the Rossby Centre regional atmospheric model under the Intergovernmental Panel on Climate Change A1B emission conditions. We focus on one of the world’s strongest extra-tropical GW zones, the Andes Mountains at mid-latitudes in the Southern Hemisphere. The presence of two GCM sub-grid scale structures locally contributing to GWMF (one positive and one negative) is found to the East of the mountains. For the late 21st century the strength of these structures during the GW high season increases around 23% with respect to the late 20th century, but the GWMF average over GCM grid cell scales remains negative and nearly constant around −0.015 Pa. This constitutes a steady significant contribution during GW high season, which is not related to the GWMF released by individual sporadic strong GW events. This characteristic agrees with the fact that no statistically significant variation in GWMF at source level has been observed in recent GCM simulations of atmospheric change induced by increases in greenhouse gases. 相似文献