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Using Jupiter's gravitational field to probe the Jovian convective dynamo
Kong, Dali1,4; Zhang, Keke1,2; Schubert, Gerald3
刊名SCIENTIFIC REPORTS
2016-03-23
卷号6
ISSN号2045-2322
DOI10.1038/srep23497
英文摘要Convective motion in the deep metallic hydrogen region of Jupiter is believed to generate its magnetic field, the strongest in the solar system. The amplitude, structure and depth of the convective motion are unknown. A promising way of probing the Jovian convective dynamo is to measure its effect on the external gravitational field, a task to be soon undertaken by the Juno spacecraft. We calculate the gravitational signature of non-axisymmetric convective motion in the Jovian metallic hydrogen region and show that with sufficiently accurate measurements it can reveal the nature of the deep convection.
WOS研究方向Science & Technology - Other Topics
语种英语
出版者NATURE PUBLISHING GROUP
WOS记录号WOS:000372607300002
内容类型期刊论文
源URL[http://119.78.226.72/handle/331011/32839]  
专题中国科学院上海天文台
通讯作者Zhang, Keke
作者单位1.Univ Exeter, Ctr Geophys & Astrophys Fluid Dynam, Exeter EX4 4QE, Devon, England
2.Macau Univ Sci & Technol, Lunar & Planetary Sci Lab, Macau, Peoples R China
3.Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA
4.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Planetary Sci, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Kong, Dali,Zhang, Keke,Schubert, Gerald. Using Jupiter's gravitational field to probe the Jovian convective dynamo[J]. SCIENTIFIC REPORTS,2016,6.
APA Kong, Dali,Zhang, Keke,&Schubert, Gerald.(2016).Using Jupiter's gravitational field to probe the Jovian convective dynamo.SCIENTIFIC REPORTS,6.
MLA Kong, Dali,et al."Using Jupiter's gravitational field to probe the Jovian convective dynamo".SCIENTIFIC REPORTS 6(2016).
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