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 |
DOI | 10.1038/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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