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151.
The magnetopause is in continuous motion and shock waves and impulsive acceleration events can occur. As an example, we show
that the interaction of an interplanetary shock with the bow shock can generate a shock wave that after passing through the
magnetosheath can interact with the magnetopause. In fluid dynamics, when a shock wave encounters a fluid discontinuity, the
interface may become unstable and form bubbles and spikes. We consider this Richtmyer-Meshkov instability in magnetohydrodynamics.
At the dayside magnetopause, the instability tends to be stabilized by the magnetic field. However, the shock wave interaction
can initiate magnetic field reconnection for the southward IMF, which may be important in strong interplanetary shock events.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
152.
G. Uma P.S. Brahmanandam V.K.D. Srinivasu D.S.V.V.D. Prasad P.V.S. Rama Rao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1736-1743
In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased. 相似文献
153.
《中国航空学报》2020,33(10):2527-2534
Studies on the high-lift mechanisms of butterfly gliding flights shed light on the design of the micro air vehicles. The flow field around a simplified Danaus plexippus model is investigated using the hydrogen bubble visualization and the Particle Image Velocimetry (PIV) techniques. There are three near-wall topological patterns with different Angles of Attack (AoAs): the separation bubble, the Leading-Edge Vortex (LEV) and the high AoAs flow. For the separation bubble pattern, two saddles and two foci form in the middle of the model. The features of the LEV pattern are the leading-edge separation lines. The topological characteristics of the separation lines are changed by the interaction between the LEV and the Wing-Tip Vortex (WTV). For the high AoAs flow pattern, four unstable foci are found at the forewing and the hindwing respectively. The angle between the trajectory of the WTV and the model increases with increasing AoA even though the slope of the WTV angle versus AoA curve declines at the moderate AoAs. 相似文献
154.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(6):2954-2966
The Two-stream Instability (TSI) generation is studied analytically in the lunar ionosphere. The TSI is a tiny perturbation in the electron plasma density, due to which an electric field grows with time and this growth is facilitated by the electron plasma in the background. In lunar ionosphere, the TSI comes into existence when the solar wind interacts unhindered with the tenuous lunar electron plasma in the surface bound exosphere. In this study, the conditions which allow the TSI to form and the subsequent instability growth with time i.e. the growth factor, is estimated. Initially, the threshold condition for the TSI to take place is determined. Thereafter, the solar wind and lunar plasma parameter contribution to trigger TSI is investigated along with the effect of these parameters in the evolution of TSI. The plasma TSI evolution with the passage of time is also depicted in phase space diagram with Particle-In-Cell simulations. 相似文献
155.
This study numerically investigated a single stage centrifugal compressor ‘‘Radiver’’ with a wedge diffuser and several tandem-designed impellers to explore the flow phenomena within the tandem impeller and the potential to enhance compressor performance. The results demonstrate that tandem design and clocking fraction (λs) significantly affects the compressor performance. The compressor stage with tandem impellers of Series A of boundary layer growth interruption alone are observed to have a widely operating range but efficiency and total pressure ratio penalty compared with that of conventional impeller. The tandem impeller with at least the same impeller efficiency as the conventional design is considered as a critical design criteria so that further modification process based on the flow characteristic of tandem impeller is necessary. In order to restrain the inducer wake and exducer shock losses, parameters modification of blade angle and thickness distributions are necessary and the modified tandem impeller of Series B is obtained. The modified tandem impeller with 25% clocking arrangement shows an 8.45% stall margin increase and maintains the total pressure ratio and efficiency as the conventional design, which proves the potential of tandem impeller to improve compressor stage performance. It is noteworthy that the tandem impellers of Radiver have not shown obviously balanced exit flow field and the fundamental mechanism of stall margin extending of tandem impeller lies on the improved impeller/diffuser matching performance resulting from the incidence angle variation at diffuser inlet. 相似文献
156.
The technology development related to aerodynamics is leading to ever increasing loads of wings, airfoils and turbine and compressor blades. The increase in aerodynamic forces is often leading to flow separation and depreciation of the aerodynamic performance of flying objects or propulsion systems. Flow control methods are required to avoid these negative effects. In the recent two decades the flow control by means of air-jet vortex generators has been also intensively investigated. In this method a streamwise vortex is introduced by an oblique jet. The necessity to supply air by a pipe system may be considered a disadvantage. In order to eliminate this feature, it has been proposed to put out a rod instead of a jet. It has been shown that the application of a rod can introduce the same effect as a jet, as long as the streamwise vortex generation is concerned and appropriate dimensions are used. The present paper focuses on the influence of rod vortex generators on a flow pattern downstream. The results presented here concern experimental and numerical investigations and provide guidelines for the design of a new flow control method dedicated mainly to external flows. 相似文献
157.
采用数值模拟方法研究了延伸冲击孔冲击冷却系统的冷却特性,分析了3个冲击雷诺数和5个冲击孔延伸长度对冲击腔内流动与换热特性的影响,给出了靶面努塞尔数分布、靶面压力分布、中心截面流速与综合换热性能的变化。结果表明:延伸冲击孔可以有效地防止横流对冲击射流的偏转作用,同时使射流出口更加贴近冲击靶面壁面,冲击速度更高,可以明显提高靶面的换热系数,并使整个靶面上的换热系数分布也更加均匀。冲击冷却的冷却性能随着冲击孔延伸长度的增加而增加,相较于传统冲击冷却(baseline),在L/d=2.5时靶面平均努塞尔数提升达15%以上,但压力损失也相对较高;对比不同延伸长度冲击孔的综合换热性能,发现存在最佳的L/d取值范围使冲击冷却系统获得最佳的综合冷却性能。在本研究范围内,最佳的L/d= 2.5。 相似文献
158.
应用N- S方程压力修正算法和k- ε两方程湍流模型,对端弯叶片和基准(无端弯)叶片的平面叶栅进行了三维粘性数值模拟。在采用简单交错网格的情况下,通过对计算控制体通量的速度进行修正的方法解决了N- S方程压力修法算中遇到的压力场和速度场呈锯齿状分布的问题。用实验测量值对本数值模拟方法的精度和可靠性进行了检验 相似文献
159.
160.
部分球壳分布离子流激发的电磁不稳定性 总被引:1,自引:1,他引:0
在离子环束流和低频电磁波相互作用的过程中廓了环束流将演化成具有投掷角展宽的部分球壳速度分布离子流,其投掷角展宽随时间增大,低频右旋电磁不稳定性增长率峰值,总的说来也逐渐增大,并向高频短波方向移动,与此相反,低频左旋电磁不稳定性增长率峰值,当投掷 角展宽等于0时,大于右旋不稳定性峰值,但随着投掷角展宽增加而迅速低于右 性增长率峰值,并向工波方向移动。 相似文献