题名 | Excitation of extraordinary modes inside the source of Saturn's kilometric radiation |
作者 | |
通讯作者 | Chen, Yao |
发表日期 | 2023-10-11
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DOI | |
发表期刊 | |
ISSN | 0004-6361
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EISSN | 1432-0746
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卷号 | 678 |
摘要 | The electron cyclotron maser instability (ECMI) of extraordinary mode waves was investigated with the parameters observed in Saturn's kilometric radiation (SKR) sources. Previous studies employed simplified dispersion relations, and did not consider the excitation of the relativistic (R) mode. This mode is introduced by considering the relativistic effect in plasmas consisting of both cold and hot electrons. Using particle-in-cell simulations, we investigated the excitation of R and X modes based on the measured data. Using the reported value of the density ratio of energetic to total electrons n(e)/n(0) = 24%, the most unstable mode is the R mode. The escaping X-mode emissions are amplified only if the energetic electrons are dominant with n(e)/n(0) >= 90%. For these cases, only the X mode is excited and the R mode disappears due to its strong coupling. The results are well in line with the linear kinetic theory of ECMI. The properties of both the R and X modes are consistent with the observed SKR emissions. This raises questions about the nature of the measured electric field fluctuations within "presumed" SKR sources. The study provides new insights into the ECMI process relevant to SKR emission mechanisms. |
关键词 | |
相关链接 | [来源记录] |
收录类别 | |
语种 | 英语
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学校署名 | 其他
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资助项目 | NSFC["11973031","12203031","12103029"]
; China Postdoctoral Science Foundation[2022TQ0189]
; Natural Science Foundation of Shandong Province[ZR2021QA033]
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WOS研究方向 | Astronomy & Astrophysics
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WOS类目 | Astronomy & Astrophysics
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WOS记录号 | WOS:001084576600001
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出版者 | |
EI入藏号 | 20234414989321
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EI主题词 | Cyclotrons
; Electric fields
; Electrons
; Hot electrons
; Masers
; Numerical methods
; Satellites
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EI分类号 | Satellites:655.2
; Extraterrestrial Physics and Stellar Phenomena:657.2
; Electricity: Basic Concepts and Phenomena:701.1
; Electronic Components and Tubes:714
; Numerical Methods:921.6
; Particle Accelerators:932.1.1
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ESI学科分类 | SPACE SCIENCE
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来源库 | Web of Science
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引用统计 |
被引频次[WOS]:2
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成果类型 | 期刊论文 |
条目标识符 | http://sustech.caswiz.com/handle/2SGJ60CL/582834 |
专题 | 理学院_地球与空间科学系 |
作者单位 | 1.Shandong Univ, Inst Frontier & Interdisciplinary Sci, Qingdao 266237, Shandong, Peoples R China 2.Shandong Univ, Inst Space Sci, Jinan 264209, Shandong, Peoples R China 3.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen, Guangdong, Peoples R China 4.Inst Solar Terr Phys, Irkutsk 664033, Russia |
推荐引用方式 GB/T 7714 |
Ning, Hao,Chen, Yao,Li, Chuanyang,et al. Excitation of extraordinary modes inside the source of Saturn's kilometric radiation[J]. ASTRONOMY & ASTROPHYSICS,2023,678.
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APA |
Ning, Hao,Chen, Yao,Li, Chuanyang,Ye, Shengyi,Kuznetsov, Alexey,&Wu, Siyuan.(2023).Excitation of extraordinary modes inside the source of Saturn's kilometric radiation.ASTRONOMY & ASTROPHYSICS,678.
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MLA |
Ning, Hao,et al."Excitation of extraordinary modes inside the source of Saturn's kilometric radiation".ASTRONOMY & ASTROPHYSICS 678(2023).
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条目包含的文件 | 条目无相关文件。 |
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