首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Van Allen Probe Observations of Disappearance,Recovery and Patchiness of Plasmaspheric Hiss Following Two Consecutive Interplanetary Shocks: First Results
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Van Allen Probe Observations of Disappearance,Recovery and Patchiness of Plasmaspheric Hiss Following Two Consecutive Interplanetary Shocks: First Results

机译:范艾伦辐射探测器的观察消失,恢复和破碎的连续两个后Plasmaspheric嘶嘶声星际冲击:第一的结果

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We present, for the first time, a plasmaspheric hiss event observed by the Van Allen probes in response to two successive interplanetary (IP) shocks occurring within an interval of ~2 h on December 19, 2015. The first shock arrived at 16:16 UT and caused disappearance of hiss for ~30 min. Combined effect of plasmapause crossing, significant Landau damping by suprathermal electrons and their gradual removal by magnetospheric compression led to the disappearance of hiss. Calculation of electron phase space density and linear wave growth rates showed that the shock did not change the growth rate of whistler waves within the core frequency range of plasmaspheric hiss (0.1-0.5 kHz) during this interval making conditions unfavorable for the generation of hiss. The recovery began at ~16:45 UT which is attributed to an enhancement in local plasma instability initiated by the first shock-induced substorm and additional possible contribution from chorus waves. This time, the wave growth rate peaked within the core frequency range (~350 Hz). The second shock arrived at 18:02 UT and generated patchy hiss persisting up to ~19:00 UT. It is shown that an enhanced growth rate and additional contribution from shock-induced poloidal Pc5 mode (periodicity ~240 s) ultralow frequency (ULF) waves resulted in the excitation of hiss waves during this period. The hiss wave amplitudes were found to be additionally modulated by background plasma density and fluctuating plasmapause location. The investigation highlights the important roles of IP shocks, substorms, ULF waves, and background plasma density in the variability of plasmaspheric hiss.
机译:我们现在,第一次,plasmaspheric嘶嘶声范艾伦辐射探测器观察到的事件应对连续两个星际(IP)冲击发生在一个时间间隔中~ 2 h2015年12月19日。16:16 UT,嘘~ 30的消失分钟。等离子体层顶的共同影响下,重大suprathermal朗道阻尼电子和他们逐步撤消磁性层的压缩了消失的嘶嘶声。相空间密度和线性波的增长率表明,冲击改变不了增长惠斯勒波速度在核心频率plasmaspheric嘘范围(0.1 - -0.5 kHz)期间这个区间使条件不利嘘的一代。16 ~但这是归因于一个改进在当地发起的等离子体不稳定性第一个触觉亚暴和额外的可能的贡献从合唱。时间,在核心波增长率达到顶峰频率范围(~ 350赫兹)。抵达18:02 UT嘶嘶声和生成的不完整的坚持~晚7:00 UT。提高增长率和额外的贡献从触觉极向Pc5模式(周期性~ 240年代)超低频(ULF)波了嘶嘶声激发的波在这时期。另外调制的背景等离子体密度和波动的等离子体层顶位置。调查强调了重要的角色IP的冲击,为亚暴,ULF波,和背景等离子体密度的变化plasmaspheric嘶嘶声。

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