Measurement of Jupiter’s asymmetric gravity field

被引：0
|
作者：
L. Iess
W. M. Folkner
D. Durante
M. Parisi
Y. Kaspi
E. Galanti
T. Guillot
W. B. Hubbard
D. J. Stevenson
J. D. Anderson
D. R. Buccino
L. Gomez Casajus
A. Milani
R. Park
P. Racioppa
D. Serra
P. Tortora
M. Zannoni
H. Cao
R. Helled
J. I. Lunine
Y. Miguel
B. Militzer
S. Wahl
J. E. P. Connerney
S. M. Levin
S. J. Bolton
机构：
[1] Sapienza Università di Roma,
[2] Jet Propulsion Laboratory,undefined
[3] California Institute of Technology,undefined
[4] Weizmann Institute of Science,undefined
[5] Observatoire de la Côte d’Azur,undefined
[6] Lunar and Planetary Laboratory,undefined
[7] University of Arizona,undefined
[8] California Institute of Technology,undefined
[9] Southwest Research Institute,undefined
[10] Università di Bologna,undefined
[11] Università di Pisa,undefined
[12] University of Zurich,undefined
[13] Cornell University,undefined
[14] University of California,undefined
[15] NASA Goddard Space Flight Center,undefined
来源：
Nature | 2018年 / 555卷
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学科分类号：
摘要：
Precise Doppler tracking of the Juno spacecraft in its polar orbit around Jupiter is used to determine the planet’s gravity harmonics, showing north–south asymmetry caused by atmospheric and interior flows.
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页码：220 / 222
页数：2
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