Gravitational signature of Jupiter's deep zonal flows

Authors
Citation
Wb. Hubbard, Gravitational signature of Jupiter's deep zonal flows, ICARUS, 137(2), 1999, pp. 357-359
Citations number
15
Categorie Soggetti
Space Sciences
Journal title
ICARUS
ISSN journal
00191035 → ACNP
Volume
137
Issue
2
Year of publication
1999
Pages
357 - 359
Database
ISI
SICI code
0019-1035(199902)137:2<357:GSOJDZ>2.0.ZU;2-D
Abstract
Calculations predict that, if Jupiter's observed zonal flows persist to a d epth similar to 1000 km below the cloud layers (corresponding to a pressure similar to 10 kbar), they will produce gravity anomalies on the order of a few mgal in high-degree zonal components of the gravitational field, refer enced to the field expanded to tenth degree. This signature would be detect able by a low-periapse Jupiter orbiter with a sensitivity to accelerations at the same level as the Galileo orbiter. (C) 1999 Academic Press.