DOI: | 10.1002/2013GL057967
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论文题名: | Saturn's magnetospheric dynamics |
作者: | Thomsen M.F.
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刊名: | Geophysical Research Letters
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ISSN: | 0094-8462
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EISSN: | 1944-8193
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出版年: | 2013
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卷: | 40, 期:20 | 起始页码: | 5337
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结束页码: | 5344
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语种: | 英语
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英文关键词: | magnetosphere
; Saturn
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Scopus关键词: | Fast rotation
; Magnetic reconnections
; Magnetospheric dynamics
; Magnetospheric plasmas
; Mass-transport process
; Radial diffusion
; Recent progress
; Saturn
; Dynamics
; Interplanetary flight
; Magnetoplasma
; Magnetosphere
; Jupiter
; magnetosphere
; mass transport
; Moon
; plasma
; radial diffusion
; Saturn
; solar wind
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英文摘要: | The dynamics of Saturn's magnetosphere are driven by two major features of the system: First, the dominant source of magnetospheric plasma is the icy moon Enceladus, located deep within the magnetosphere; and second, like Jupiter, Saturn is a very fast rotator, with a rotational period of only 10.7 h. The dynamical imperative is to rid the magnetosphere of the continuously supplied plasma, and the fast rotation provides the mechanisms to do so. Thus, magnetospheric dynamics are intimately related to mass transport processes, including radial diffusion, flux tube interchange, magnetic reconnection, and plasmoid formation. We review recent progress and new questions relating to these processes at Saturn. Key Points Centrifugal interchange and tail reconnection move plasma toward the solar wind Cassini observations and numerical simulations illuminate these processes Ultimate loss processes for Saturnian plasma are not yet quantitatively known ©2013. American Geophysical Union. All Rights Reserved. |
URL: | https://www.scopus.com/inward/record.uri?eid=2-s2.0-84886712175&doi=10.1002%2f2013GL057967&partnerID=40&md5=4f4de6b51d289790bc73037c669951b9
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Citation statistics: |
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资源类型: | 期刊论文
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标识符: | http://119.78.100.158/handle/2HF3EXSE/5726
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Appears in Collections: | 气候减缓与适应
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作者单位: | Planetary Science Institute, 1700 East Fort Lowell, Tucson, AZ 85719-2395, United States
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Recommended Citation: |
Thomsen M.F.. Saturn's magnetospheric dynamics[J]. Geophysical Research Letters,2013-01-01,40(20).
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