{"title":"地磁风暴恢复阶段背景水平密度不规则对两个哨声模式波的调制","authors":"Xu Liu, W. Gu, Z. Xia, Lunjin Chen, R. Horne","doi":"10.23919/USNC-URSIRSM52661.2021.9552349","DOIUrl":null,"url":null,"abstract":"The plasmasphere is a vast torus shape region of the inner magnetosphere, filled with dense $\\left(\\sim 1-10^{6} \\# / \\text{cm}^{-3}\\right)$ and cold (less than $10 \\text{eV})$ ions and electrons. The outer boundary of the plasmasphere, called plasmapause, is a sharp plasma density boundary that separates closed and open drift paths for cold plasmas. Distinct plasmapause with sharp density variations are only 16% of the observed plasmapause and are preferred to occur at the post-midnight and dawnside than the duskside. Most of the plasmapause, however, is accompanied by significant density irregularities. These density irregularities are thought to play an important role in wave excitation and propagation, such as the excitation of the electromagnetic ion cyclotron (EMIC) waves and magnetosonic (MS) waves, and the propagation of EMIC wave and MS waves.","PeriodicalId":365284,"journal":{"name":"2021 USNC-URSI Radio Science Meeting (USCN-URSI RSM)","volume":"4 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-08-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Two Whistler-Mode Waves Modulation By Background-Level Density Irregularity During The Recovery Phase of A Geomagnetic Storm\",\"authors\":\"Xu Liu, W. Gu, Z. Xia, Lunjin Chen, R. Horne\",\"doi\":\"10.23919/USNC-URSIRSM52661.2021.9552349\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The plasmasphere is a vast torus shape region of the inner magnetosphere, filled with dense $\\\\left(\\\\sim 1-10^{6} \\\\# / \\\\text{cm}^{-3}\\\\right)$ and cold (less than $10 \\\\text{eV})$ ions and electrons. The outer boundary of the plasmasphere, called plasmapause, is a sharp plasma density boundary that separates closed and open drift paths for cold plasmas. Distinct plasmapause with sharp density variations are only 16% of the observed plasmapause and are preferred to occur at the post-midnight and dawnside than the duskside. Most of the plasmapause, however, is accompanied by significant density irregularities. These density irregularities are thought to play an important role in wave excitation and propagation, such as the excitation of the electromagnetic ion cyclotron (EMIC) waves and magnetosonic (MS) waves, and the propagation of EMIC wave and MS waves.\",\"PeriodicalId\":365284,\"journal\":{\"name\":\"2021 USNC-URSI Radio Science Meeting (USCN-URSI RSM)\",\"volume\":\"4 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-08-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2021 USNC-URSI Radio Science Meeting (USCN-URSI RSM)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.23919/USNC-URSIRSM52661.2021.9552349\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2021 USNC-URSI Radio Science Meeting (USCN-URSI RSM)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.23919/USNC-URSIRSM52661.2021.9552349","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
等离子层是内磁层的一个巨大的环状区域,充满了密集的$\left(\sim 1-10^{6} \# / \text{cm}^{-3}\right)$和冷的(小于$10 \text{eV})$)离子和电子。等离子体层的外边界,称为等离子体顶,是一个尖锐的等离子体密度边界,它将冷等离子体的封闭和开放漂移路径分开。具有明显密度变化的等离子体ause只有16个% of the observed plasmapause and are preferred to occur at the post-midnight and dawnside than the duskside. Most of the plasmapause, however, is accompanied by significant density irregularities. These density irregularities are thought to play an important role in wave excitation and propagation, such as the excitation of the electromagnetic ion cyclotron (EMIC) waves and magnetosonic (MS) waves, and the propagation of EMIC wave and MS waves.
Two Whistler-Mode Waves Modulation By Background-Level Density Irregularity During The Recovery Phase of A Geomagnetic Storm
The plasmasphere is a vast torus shape region of the inner magnetosphere, filled with dense $\left(\sim 1-10^{6} \# / \text{cm}^{-3}\right)$ and cold (less than $10 \text{eV})$ ions and electrons. The outer boundary of the plasmasphere, called plasmapause, is a sharp plasma density boundary that separates closed and open drift paths for cold plasmas. Distinct plasmapause with sharp density variations are only 16% of the observed plasmapause and are preferred to occur at the post-midnight and dawnside than the duskside. Most of the plasmapause, however, is accompanied by significant density irregularities. These density irregularities are thought to play an important role in wave excitation and propagation, such as the excitation of the electromagnetic ion cyclotron (EMIC) waves and magnetosonic (MS) waves, and the propagation of EMIC wave and MS waves.