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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Impact of the rippling of a perpendicular shock front on ion dynamics
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Impact of the rippling of a perpendicular shock front on ion dynamics

机译:垂直冲击波前的波纹对离子动力学的影响

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Both hybrid/full particle simulations and recent experimental results have clearly evidenced that the front of a supercritical quasi-perpendicular shock can be rippled. Recent two-dimensional simulations have focused on two different types of shock front rippling: (1) one characterized by a small spatial scale along the front is supported by lower hybrid wave activity, (2)the other characterized by a large spatial scale along the front is supported by the emission of large amplitude nonlinear whistler waves. These two rippled shock fronts are self-consistently observed when the static magnetic field is perpendicular to(so called B0-OUT case)or within(so called B0-IN case)the simulation plane, respectively. On the other hand, several studies have been made on the reflection and energization of incoming ions with a shock but most have been restricted to a one dimensional shock profile only(no rippling effects). Herein, two-dimensional test particle simulations based on strictly perpendicular shock profiles chosen at a fixed time in twodimensional Particle-in-cell(PIC)simulations, are performed in order to investigate the impact of the shock front ripples on incident ion(H+)dynamics. The acceleration mechanisms and energy spectra of the test-ions(described by shell distributions with different initial kinetic energy)interacting with a rippled shock front are analyzed in detail. Both B0-OUT and B0-IN cases are considered separately; in each case, y-averaged(front rippling excluded)and non-averaged(front rippling included)profiles will be analyzed. Present results show that: (1)the incident ions suffer both shock drift acceleration(SDA)and shock surfing acceleration(SSA)mechanisms. Moreover, a striking feature is that SSA ions not only are identified at the ramp but also within the foot which confirms previous 1-D simulation results; (2)the percentage of SSA ions increases with initial kinetic energy, a feature which persists well with a rippled shock front; (3)furthermore, the ripples increase the porosity of the shock front, and more directly transmitted(DT)ions are produced; these strongly affect the relative percentage of the different identified classes of ions(SSA, SDA and DT ions), their average kinetic energy and their relative contribution to the resulting downstream energy spectra; (4)one key impact of the ripples is a strong diffusion of ions(in particular through the frontiers of their injection angle domains and in phase space which are blurred out)which leads to a mixing of the different ion classes. This diffusion increases with the size of the spatial scale of the front ripples; (5)through this diffusion, an ion belonging to a given category(SSA, SDA, or DT)in y-averaged case changes class in non-averaged case without one-to-one correspondence.
机译:混合/全粒子模拟和最近的实验结果都清楚地证明了超临界准垂直冲击的前部会产生波纹。最近的二维模拟关注于两种不同类型的激波前波荡:(1)一种特征是沿着前波的小空间尺度受到较低混合波活动的支持;(2)另一种特征是沿着波前的大空间尺度。大振幅的非线性惠斯勒波的发射支持了前端。当静磁场分别垂直于(称为B0-OUT情况)或位于模拟平面内(称为B0-IN情况)时,这两个波纹激波锋面是自洽的。另一方面,已经对冲击引起的入射离子的反射和通电进行了几项研究,但大多数研究仅限于一维冲击分布(无波纹效应)。在本文中,基于二维固定粒子中的固定时间选择的严格垂直冲击轮廓进行了二维测试粒子模拟,以研究冲击前波动对入射离子(H +)的影响动力学。详细分析了与波纹激波前部相互作用的测试离子(由具有不同初始动能的壳分布描述)的加速机理和能谱。 B0-OUT和B0-IN情况是分开考虑的;在每种情况下,将分析y平均(排除前波纹)和非平均(包括前波纹)轮廓。目前的结果表明:(1)入射离子同时具有激波漂移加速度(SDA)和激波冲浪加速度(SSA)机制。此外,一个显着的特征是,SSA离子不仅在坡道处被识别,而且在脚部也被识别,这证实了先前的一维模拟结果。 (2)SSA离子的百分比随着初始动能的增加而增加,这种特征在波纹激波前部持续存在; (3)此外,波纹会增加激波前沿的孔隙率,并产生更直接传输的(DT)离子;这些因素会严重影响不同类别的离子(SSA,SDA和DT离子)的相对百分比,其平均动能及其对产生的下游能谱的相对贡献; (4)波纹的一个关键影响是离子的强烈扩散(尤其是通过其注入角域的边界以及在模糊的相空间中),这导致了不同离子类别的混合。这种扩散随着前波纹的空间尺度的大小而增加; (5)通过这种扩散,在y平均情况下属于给定类别(SSA,SDA或DT)的离子在非平均情况下改变类别而没有一一对应关系。

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