The Potential Importance of Non-Local, Deep Transport on the Energetics, Momentum, Chemistry, and Aerosol Distributions in the Atmospheres of Earth, Mars and Titan
Scot Rafkin

TL;DR
This paper reviews non-local, deep transport mechanisms in Earth's atmosphere and explores their potential presence and significance in the atmospheres of Mars and Titan, highlighting their impact on atmospheric composition and dynamics.
Contribution
It extends the understanding of deep atmospheric transport processes from Earth to Mars and Titan, emphasizing their possible roles in planetary atmospheres.
Findings
Deep convective clouds drive vertical transport in Earth’s atmosphere.
Analogous deep transport mechanisms are suggested for Mars and Titan.
Evidence supports the significance of non-local deep transport in extraterrestrial atmospheres.
Abstract
A review of non-local, deep transport mechanisms in the atmosphere of Earth provides a good foundation for examining whether similar mechanisms are operating in the atmospheres of Mars and Titan. On Earth, deep convective clouds in the tropics constitute the upward branch of the Hadley Cell and provide a conduit through which energy, moisture, momentum, aerosols and chemical species are moved from the boundary layer to the upper troposphere and lower stratosphere. This transport produces mid-tropospheric minima in quantities such as water vapor and moist static energy and maxima where the clouds detrain. Analogs to this terrestrial transport are found in the strong and deep thermal circulations associated with topography on Mars and with Mars dust storms. Observations of elevated dust layers on Mars further support the notion that non-local deep transport is an important mechanism in…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Atmospheric Ozone and Climate
