Stable layers in Jupiter's interior modify the background density, creating a degeneracy with the vertical wind profile that prevents unique determination of jet depth from gravity data alone.
Monthly Notices of the Royal Astronomical Society , volume=
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.EP 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Implications of a Stable Layer on the Vertical Structure of Jet Streams on Jupiter
Stable layers in Jupiter's interior modify the background density, creating a degeneracy with the vertical wind profile that prevents unique determination of jet depth from gravity data alone.