A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits

التفاصيل البيبلوغرافية
العنوان: A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits
المؤلفون: Connerney, J. E. P, Kotsiaros, S, Oliversen, R. J, Espley, J. R, Joergensen, J. L, Joergensen, P. S, Merayo, J. M. G, Herceg, M, Bloxham, J, Moore, K. M, Bolton, S. J, Levin, S. M
المصدر: Geophysical Research Letters. 45(6)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2018.
سنة النشر: 2018
مصطلحات موضوعية: Lunar And Planetary Science And Exploration
الوصف: 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 ~45 deg 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.
نوع الوثيقة: Report
اللغة: English
تدمد: 1944-8007
0094-8276
DOI: 10.1002/2018GL077312
URL الوصول: https://ntrs.nasa.gov/citations/20180004823
ملاحظات: NNN12AA01C

80GSFC17M0002

NNM06AA75C

80GSFC17C0003
رقم الأكسشن: edsnas.20180004823
قاعدة البيانات: NASA Technical Reports
الوصف
تدمد:19448007
00948276
DOI:10.1002/2018GL077312