地球等离子体层嘶声的内部源区  

Internal source of plasmaspheric hiss on Earth

作　　者：苏振鹏 刘倪纲[3] 何兆国 吴志勇 Su Zhenpeng;Liu Nigang;He Zhaoguo;Wu Zhiyong(CAS Key Laboratory of Geospace Environment,Department of Geophysics and Planetary Sciences,University of Science and Technology of China,Hefei 230026,China;CAS Center for Excellence in Comparative Planetology,Hefei 230026,China;Planetary Environmental and Astrobiological Research Laboratory(PEARL),School of Atmospheric Sciences,Sun Yat-sen University,Zhuhai 519082,China)

机构地区：[1]中国科学技术大学地球和空间科学学院,合肥230026 [2]中国科学院比较行星学卓越创新中心,合肥230026 [3]中山大学大气科学学院行星环境与宜居性研究实验室,珠海519082

出　　处：《地球与行星物理论评》2022年第4期454-465,共12页Reviews of Geophysics and Planetary Physics

基　　金：国家自然科学基金面上资助项目(41774170,42174185);国家自然科学基金青年科学基金资助项目(42004140)。

摘　　要：地球等离子体层是向阳侧中低纬度电离层沿着闭合磁力线向上的自然延伸,其中所出现的一类频率覆盖数十赫兹至数千赫兹的哨声模波动称为等离子体层嘶声.自发现以来,等离子体层嘶声就被广泛认为是沉降损失辐射带高能电子的主要等离子体波动之一.但是,等离子体层嘶声的起源一直没有定论.潜在的来源分成两类:一类为等离子体层内部背景等离子体噪声,另一类为等离子体层外部波动.2012年发射升空的Van Allen Probes搭载了完备的磁层粒子、场和波动探测仪器,为这一问题的解决带来了新的机遇.本文综述了近5年来利用Van Allen Probes探索等离子体层嘶声内部源区的研究工作,强调背景等离子体噪声可以通过高能电子线性和非线性不稳定性叠加放大成可观测的嘶声,突出内源的广泛分布特性,即在结构上涵盖等离子体层核心和羽流,在地方时上涵盖向阳和背阳侧等离子体层,在径向距离上涵盖外层和内层等离子体层.Plasmasphere is an upward extension of the ionosphere at low and middle latitudes along the closed magnetic field lines rooted in the Earth,where the trapped whistler-mode waves in the frequency range from tens to thousands of Hertz are named as plasmaspheric hiss.Since its discovery,plasmaspheric hiss has been considered an important plasma wave to drive the precipitation loss of the Van Allen radiation belt electrons.However,the origin of plasmaspheric hiss has long been under debate.There have been two classes of sources proposed for the plasmaspheric hiss:(1)background plasma noises inside the plasmasphere and(2)other plasma waves outside the plasmasphere.In 2012,the Van Allen Probes mission capable of measuring an enormous range of particles,fields and waves was launched,providing an unprecedented opportunity to investigate the origin of plasmaspheric hiss.Here we briefly review the progress on the internal sources of plasmaspheric hiss during the recent five years.It has been suggested the background plasma noises can be amplified to the plasmaspheric hiss by a combination of linear and nonlinear instabilities of energetic electrons.During geomagnetically active times,energetic electrons are transported from the magnetotail into the plasmaspheric body and plume.The linear growth rate of whistler-mode waves destabilized by these energetic electrons exhibits an analogous frequency-dependence to the observed hiss power spectral density.When the seed wave amplitude exceeds a threshold,the nonlinear instability can act and then amplify the seed wave to the observable level.Such internal sources could exist over a broad range of magnetic local times,radial distances,and other structures of the plasmasphere.

关 键 词：等离子体层 等离子体层嘶声 内部源区 

分 类 号：P354[天文地球—空间物理学]