GSTDTAP  > 气候变化
DOI10.1029/2018GL078891
Standing Alfven Waves in Jupiter's Magnetosphere as a Source of similar to 10-to 60-Min Quasiperiodic Pulsations
Manners, H.1; Masters, A.1; Yates, J. N.1,2
2018-09-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:17页码:8746-8754
文章类型Article
语种英语
国家England; Spain
英文摘要

Energy transport inside the giant magnetosphere at Jupiter is poorly understood. Since the Pioneer era, mysterious quasiperiodic (QP) pulsations have been reported. Early publications successfully modeled case studies of similar to 60-min (rest-frame) pulsations as standing Alfven waves. Since then, the range of periods has increased to similar to 10-60 min, spanning multiple data sets. More work is required to assess whether a common QP modulation mechanism is capable of explaining the full range of wave periods. Here we have modeled standing Alfven waves to compute the natural periods of the Jovian magnetosphere, for varying plasma sheet thicknesses, field line lengths, and Alfven speeds. We show that variability in the plasma sheet produces eigenperiods that are consistent with all the reported observations. At least the first half-dozen harmonics (excluding the fundamental) may contribute but are indistinguishable in our analysis. We suggest that all QP pulsations reported at Jupiter may be explained by standing Alfven waves.


Plain Language Summary A magnetized planet produces a global magnetic field that deflects the solar wind, surrounding the planet in a magnetic cavity called a magnetosphere. Jupiter is surrounded by the largest magnetosphere in the solar system. Many aspects of how energy is transported and deposited around Jupiter's magnetosphere remain mysterious. One such mystery is semiperiodic pulsations that have been observed by spacecraft orbiting Jupiter. These pulsations have been observed in measurements of the magnetic field, the density of the magnetospheric plasma, and emissions from the auroral regions at the planet's poles. In this study we investigate whether at least some of these pulsations could be the result of the magnetosphere resonating, similar to a ringing bell. The magnetic field can be treated as being composed of lines of magnetic force, and, when perturbed, these lines of force behave like vibrating strings. Using a simple model, we have calculated the frequencies at which these magnetic strings resonate. We found that the resonant frequencies are consistent with all the reported pulsations. This shows that a large body of pulsations can be explained by a single phenomenon, one that constitutes a mechanism for storing, transporting, and dissipating energy around the entire magnetospheric environment.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000445727500006
WOS关键词FIELD LINE RESONANCES ; LOW-FREQUENCY WAVES ; HYDROMAGNETIC-WAVES ; ULF WAVES ; MAGNETIC PULSATIONS ; CURRENT SHEET ; RADIO-BURSTS ; EARTH ; ULYSSES ; EMISSIONS
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/25563
专题气候变化
作者单位1.Imperial Coll London, Blackett Lab, Space & Atmospher Phys Grp, London, England;
2.European Space Agcy, European Space Astron Ctr, Madrid, Spain
推荐引用方式
GB/T 7714
Manners, H.,Masters, A.,Yates, J. N.. Standing Alfven Waves in Jupiter's Magnetosphere as a Source of similar to 10-to 60-Min Quasiperiodic Pulsations[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(17):8746-8754.
APA Manners, H.,Masters, A.,&Yates, J. N..(2018).Standing Alfven Waves in Jupiter's Magnetosphere as a Source of similar to 10-to 60-Min Quasiperiodic Pulsations.GEOPHYSICAL RESEARCH LETTERS,45(17),8746-8754.
MLA Manners, H.,et al."Standing Alfven Waves in Jupiter's Magnetosphere as a Source of similar to 10-to 60-Min Quasiperiodic Pulsations".GEOPHYSICAL RESEARCH LETTERS 45.17(2018):8746-8754.
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Manners, H.]的文章
[Masters, A.]的文章
[Yates, J. N.]的文章
百度学术
百度学术中相似的文章
[Manners, H.]的文章
[Masters, A.]的文章
[Yates, J. N.]的文章
必应学术
必应学术中相似的文章
[Manners, H.]的文章
[Masters, A.]的文章
[Yates, J. N.]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。