Radio sounding from IMAGE: New perspectives on field aligned density irregularities, Z and whistler mode diagnostics, and proton cyclotron harmonic echoes

D. L. Carpenter, T. Bell, V. Sonwalkar
{"title":"Radio sounding from IMAGE: New perspectives on field aligned density irregularities, Z and whistler mode diagnostics, and proton cyclotron harmonic echoes","authors":"D. L. Carpenter, T. Bell, V. Sonwalkar","doi":"10.1109/URSIGASS.2011.6051105","DOIUrl":null,"url":null,"abstract":"The operating frequency of the Radio Plasma Imager (RPI) instrument on the IMAGE satellite extended from 3 kHz to 3 MHz. This wide range made possible free-space O and X mode sounding from altitudes on both sides of the plasmasphere boundary layer (PBL) while also making possible wave injection in the whistler-mode and Z-mode domains at altitudes less than ≈ 10,000 km. We briefly review new findings in four areas: (i) density irregularities in the PBL and within the plasmasphere; (ii) upward Z-mode probing along geomagnetic field lines from within a Z-mode propagation ‘cavity’ (iii) downward probing from 4500–7000 km altitude using whistler-mode waves that undergo two fundamentally different types of reflection; (iv) strong coupling of RPI pulses to the local proton plasma","PeriodicalId":325870,"journal":{"name":"2011 XXXth URSI General Assembly and Scientific Symposium","volume":"79 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2011-10-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"2011 XXXth URSI General Assembly and Scientific Symposium","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/URSIGASS.2011.6051105","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

The operating frequency of the Radio Plasma Imager (RPI) instrument on the IMAGE satellite extended from 3 kHz to 3 MHz. This wide range made possible free-space O and X mode sounding from altitudes on both sides of the plasmasphere boundary layer (PBL) while also making possible wave injection in the whistler-mode and Z-mode domains at altitudes less than ≈ 10,000 km. We briefly review new findings in four areas: (i) density irregularities in the PBL and within the plasmasphere; (ii) upward Z-mode probing along geomagnetic field lines from within a Z-mode propagation ‘cavity’ (iii) downward probing from 4500–7000 km altitude using whistler-mode waves that undergo two fundamentally different types of reflection; (iv) strong coupling of RPI pulses to the local proton plasma
无线电探测图像:场对准密度不规则,Z和惠斯勒模式诊断和质子回旋加速器谐波回波的新视角
IMAGE卫星上无线电等离子体成像仪(RPI)的工作频率从3khz扩展到3mhz。这种宽范围使得从等离子层边界层(PBL)两侧的高度进行自由空间O和X模式探测成为可能,同时也使得在小于≈10,000 km的高度在哨子模式和z模式域中注入波成为可能。我们简要回顾了四个方面的新发现:(1)PBL和等离子体层内的密度不规则性;(ii)从z模式传播“腔”内沿地磁场线向上探测z模式;(iii)从4500-7000公里高度向下探测,使用经过两种根本不同反射类型的哨子模式波;(iv) RPI脉冲与局部质子等离子体的强耦合
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信