On the dual nature of atmospheric escape
Darius Modirrousta-Galian, Jun Korenaga

TL;DR
This paper reveals that atmospheric escape involves a smooth transition between collisional hydrodynamic flow and collisionless ballistic particles, challenging the traditional binary classification and offering a unified model.
Contribution
It introduces a two-channel framework that unifies hydrodynamic and kinetic descriptions of atmospheric escape, advancing beyond classical dichotomous models.
Findings
Collisionless particles influence the flow at all altitudes.
Flow profiles resemble Parker breeze solutions.
Escape involves a gradual shift from collisional to collisionless behavior.
Abstract
Planetary atmospheres cannot remain hydrostatic at all altitudes because they approach finite density at infinite radius, implying infinite mass. Classical treatments address this in two directions: either retain a hydrostatic structure while allowing particles in the high-velocity tail to decouple and escape in a Jeans-type manner, or promote the gas to a continuum outflow to obtain a transonic Parker-type solution. The usual criterion compares the local mean free path to the sonic point radius. If the mean free path is shorter, the atmosphere is hydrostatic with an imposed Jeans escape flux; if it is longer, the gas is hydrodynamic with Jeans escape neglected. Here, we show that hydrogen-rich atmospheres do not separate cleanly into hydrodynamic and Jeans-escape regimes. At any radius, some particles still collide and behave as a fluid, while others have already experienced their last…
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Taxonomy
TopicsFluid dynamics and aerodynamics studies · Solar and Space Plasma Dynamics · Spacecraft Dynamics and Control
