  The asymmetric gravity field measured by the Juno spacecraft allowed
estimation of the depth of Jupiter's zonal jets, showing that the winds extend
approximately $3000$ km beneath the cloud-level. This estimate was based on an
analysis using a combination of all measured odd gravity harmonics $J_{3}$,
$J_{5}$, $J_{7}$, and $J_{9}$, but the wind profile dependence on each of them
separately has not been investigated. Furthermore, these calculations assumed
the meridional profile of the cloud-level wind extends to depth. However, it is
possible that the interior jet profile varies from that of the cloud-level as
hinted by the Juno microwave measurement that find a smoother nadir brightness
temperature profile at depth compared to the cloud-level. Here we analyze in
detail the possible meridional and vertical structure of Jupiter's deep
jet-streams. We find that each odd gravity harmonic constrains the flow at a
different depth, with $J_{3}$ being the most dominant at depths below $3000$
km, $J_{5}$ being the most restrictive overall, and $J_{9}$ not constraining
the flow at all if the other odd harmonics are within the measurement range.
Interior flow profiles constructed from perturbations to the cloud-level winds
allow a more extensive range of vertical wind profiles, yet when the profiles
differ substantially from the cloud-level, the ability to match the gravity
data reduces significantly. Overall, we find that while interior wind profiles
that do not resemble the cloud-level are possible, they are statistically
unlikely. However, slightly smoother profiles, which resemble the Juno's
microwave radiometer temperature profile at depth, are still compatible with
the gravity measurements.
