Dynamics of atmospheres with a non-dilute condensible component

TL;DR

This paper explores the climate dynamics of atmospheres with a significant condensible component, revealing unique circulation patterns and implications for runaway greenhouse phenomena through analytical and simulation approaches.

Contribution

It provides the first comprehensive analysis of non-dilute atmospheres, combining analytical results with GCM simulations to reveal their distinctive features.

Findings

Weak horizontal temperature gradients in non-dilute atmospheres

Circulations are largely barotropic despite rapid rotation

Relative humidity approaches 100% as atmospheres become more non-dilute

Abstract

The diversity of characteristics for the host of recently discovered exoplanets opens up a great deal of fertile new territory for geophysical fluid dynamics, particularly when the fluid flow is coupled to novel thermodynamics, radiative transfer or chemistry. In this paper, we survey one of these new areas-the climate dynamics of atmospheres with a non-dilute condensible component, defined as the situation in which a condensible component of the atmosphere makes up a substantial fraction of the atmospheric mass within some layer. Non-dilute dynamics can occur for a wide range of condensibles, generically applying near both the inner and the outer edges of the conventional habitable zone and in connection with runaway greenhouse phenomena. It also applies in a wide variety of other planetary circumstances. We first present a number of analytical results developing some key features of non-dilute atmospheres, and then show how some of these features are manifest in simulations with a general circulation model adapted to handle non-dilute atmospheres. We find that non-dilute atmospheres have weak horizontal temperature gradients even for rapidly rotating planets, and that their circulations are largely barotropic. The relative humidity of the condensible component tends towards 100% as the atmosphere becomes more non-dilute, which has important implications for runaway greenhouse thresholds. Non-dilute atmospheres exhibit a number of interesting organized convection features, for which there is not yet any adequate theoretical understanding.