activity
20172022
most citedComparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core

396 citations · 765 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP20211 cited

Theory of Figures to the 7th order and the interiors of Jupiter and Saturn

N. Nettelmann, N. Movshovitz, D. Ni +6

Interior modeling of Jupiter and Saturn has advanced to a state where thousands of models are generated that cover the uncertainty space of many parameters. This approach demands a…

astro-ph.EP202137 cited

Jupiter's Temperate Belt/Zone Contrasts Revealed at Depth by Juno Microwave Observations

L. N. Fletcher, F. A. Oyafuso, M. Allison +12

Juno Microwave Radiometer (MWR) observations of Jupiter's mid-latitudes reveal a strong correlation between brightness temperature contrasts and zonal winds, confirming that the ba…

astro-ph.EP202121 cited

Constraints on the latitudinal profile of Jupiter's deep jets

E. Galanti, Y. Kaspi, K. Duer +7

The observed zonal winds at Jupiter's cloud tops have been shown to be closely linked to the asymmetric part of the planet's measured gravity field. However, other measurements sug…

astro-ph.EP202110 cited

Lightning generation in moist convective clouds and constraints on the water abundance in Jupiter

Yury S. Aglyamov, Jonathan Lunine, Heidi N. Becker +7

Recent Juno observations have greatly extended the temporal and spatial coverage of lightning detection on Jupiter. We use these data to constrain a model of moist convection and l…

astro-ph.EP202036 cited

Storms and the Depletion of Ammonia in Jupiter: II. Explaining the Juno Observations

Tristan Guillot, Cheng Li, Scott Bolton +8

Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars, a…

astro-ph.EP2020146 cited

The water abundance in Jupiter's equatorial zone

Cheng Li, Andrew Ingersoll, Scott Bolton +20

Oxygen is the most common element after hydrogen and helium in Jupiter's atmosphere, and may have been the primary condensable (as water ice) in the protoplanetary disk. Prior to t…