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Influence of Penetration Depth on Jets on Giant Planets: Equatorial Jet Direction, Jet Numbers, and Jet Energy Fraction

  • Authors: Yaoxuan Zeng, Wanying Kang, Glenn R. Flierl, Geoffrey K. Vallis

Yaoxuan Zeng et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 8.

KE spectrum. Snapshots of the KE (u2/2 + v2/2) spectra from simulations with ε = 2.9 × 10−11 and μ = 10−7. The blue line shows the simulated KE spectrum. The green, red, and black dashed lines indicate the theoretical slopes of −3, −5/3, and −5, respectively. The transition wavenumbers ne, nβ, and nRh are also marked, where nβ and nRh are estimated using the averaged β across the domain.

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