Superrotation on Venus: Driven By Waves Generated By Dissipation of the Transterminator Flow
Hector Javier Durand-Manterola

TL;DR
This paper proposes a novel mechanism involving wave generation in Venus's cryosphere, driven by transterminator flow dissipation, which can transfer sufficient energy to sustain the planet's atmospheric superrotation.
Contribution
It introduces a new wave-driven mechanism for Venus's superrotation, supported by energy calculations and an experimental model, addressing previous explanatory gaps.
Findings
Transterminator flow provides enough energy to sustain superrotation.
Wave amplitudes of 10^-4 m at 1 Hz can transfer dissipated energy.
Superrotation could restart within 1.4 million years if stopped.
Abstract
Context: The superrotation phenomenon in the atmosphere on Venus has been known since the late 60's. But until now no mechanism proposed has satisfactorily explained this phenomenon. Objective: The aim of this research is to propose a mechanism, until now never considered, which could drive the atmosphere of Venus in its superrotation. This mechanism involves the transfer of the transterminator ionospheric flow momentum to the lower atmosphere via pressure waves generated in the cryosphere of Venus. The mechanism proposed presents a source of energy sufficiently strong to allow the transfer of energy despite dissipation. Method: The energy flow which transports the transterminator flow and the energy lost by the viscosity in the superrotating atmosphere were calculated. Both results were compared to establish if there is sufficient energy in the transterminator flow to drive the…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Fluid dynamics and aerodynamics studies
