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The actual correspondence still depends on cloud and haze distributions and varies across different regions of Jupiter (Sromovsky & Fry, 2010, 2018)

The model assumes the absence of aerosols in Jupiter's atmosphere, that incoming solar radiation is dissipated only through gas absorption or Rayleigh scattering · 2010

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Jovian Zonal Winds Revealed from Cassini/VIMS Observations

astro-ph.EP · 2026-05-07 · unverdicted · novelty 5.0

A new correlation method applied to Cassini/VIMS data measures Jupiter zonal winds at multiple altitudes, revealing weaker tropospheric vertical shear than previously reported.

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  • Jovian Zonal Winds Revealed from Cassini/VIMS Observations astro-ph.EP · 2026-05-07 · unverdicted · none · ref 12

    A new correlation method applied to Cassini/VIMS data measures Jupiter zonal winds at multiple altitudes, revealing weaker tropospheric vertical shear than previously reported.