Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1002/2018GL077312 |
A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits | |
Connerney, J. E. P.1,2; Kotsiaros, S.1,3; Oliversen, R. J.1; Espley, J. R.1; Joergensen, J. L.4; Joergensen, P. S.4; Merayo, J. M. G.4; Herceg, M.4; Bloxham, J.5; Moore, K. M.5; Bolton, S. J.6; Levin, S. M.7 | |
2018-03-28 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS |
ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2018 |
卷号 | 45期号:6页码:2590-2596 |
文章类型 | Article |
语种 | 英语 |
国家 | USA; Denmark |
英文摘要 | A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic field observations acquired by the Juno spacecraft during its first nine polar orbits about the planet. Observations acquired during eight of these orbits provide the first truly global coverage of Jupiter's magnetic field with a coarse longitudinal separation of similar to 45 degrees between perijoves. The magnetic field is represented with a degree 20 spherical harmonic model for the planetary ("internal") field, combined with a simple model of the magnetodisc for the field ("external") due to distributed magnetospheric currents. Partial solution of the underdetermined inverse problem using generalized inverse techniques yields a model ('Juno Reference Model through Perijove 9") of the planetary magnetic field with spherical harmonic coefficients well determined through degree and order 10, providing the first detailed view of a planetary dynamo beyond Earth. |
英文关键词 | Jupiter magnetosphere Juno mission magnetic field dynamo generation planetary magnetic field |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000430106000004 |
WOS关键词 | GEOMAGNETIC-FIELD ; SECULAR VARIATION ; MAGNETOSPHERE ; SPACECRAFT ; SPECTRUM |
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/28047 |
专题 | 气候变化 |
作者单位 | 1.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA; 2.Space Res Corp, Annapolis, MD 21403 USA; 3.Univ Maryland, College Pk, MD 20742 USA; 4.Tech Univ Denmark, Lyngby, Denmark; 5.Harvard Univ, Cambridge, MA 02138 USA; 6.Southwest Res Inst, San Antonio, TX USA; 7.Jet Prop Lab, Pasadena, CA USA |
推荐引用方式 GB/T 7714 | Connerney, J. E. P.,Kotsiaros, S.,Oliversen, R. J.,et al. A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(6):2590-2596. |
APA | Connerney, J. E. P..,Kotsiaros, S..,Oliversen, R. J..,Espley, J. R..,Joergensen, J. L..,...&Levin, S. M..(2018).A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits.GEOPHYSICAL RESEARCH LETTERS,45(6),2590-2596. |
MLA | Connerney, J. E. P.,et al."A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits".GEOPHYSICAL RESEARCH LETTERS 45.6(2018):2590-2596. |
条目包含的文件 | 条目无相关文件。 |
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。
修改评论