Authors: Thomas Ronnet, Olivier Mousis, and Pierre Vernazza
2017 The Astrophysical Journal84592.
Provider: AAS Journals
Caption: Figure 2.
Radial velocity profiles of the gas as a function of the height above the midplane at different distances from Jupiter. Solid and dashed lines correspond to profiles calculated with α = 1 × 10−4 and 5 × 10−4, respectively.