English

Buoyancy-Driven Entrainment in Dry Thermals

Fluid Dynamics 2020-03-18 v2 Earth and Planetary Astrophysics Atmospheric and Oceanic Physics

Abstract

\citet{turner1957} proposed that dry thermals entrain because of buoyancy (via a constraint which requires an increase in the radius aa). This however, runs counter to the scaling arguments commonly used to derive the entrainment rate, which rely on either the self-similarity of \citet{scorer1957} or the turbulent entrainment hypothesis of \citet{morton1956}. The assumption of turbulence-driven entrainment was investigated by \citet{lecoanet2018}, who found that the entrainment efficiency ee varies by less than 20%20\% between laminar (Re = 630) and turbulent (Re = 6300) thermals. This motivated us to utilize Turner's argument of buoyancy-controlled entrainment in addition to the thermal's vertical momentum equation to build a model for thermal dynamics which does not invoke turbulence or self-similarity. We derive simple expressions for the thermals' kinematic properties and their fractional entrainment rate ϵ\epsilon and find close quantitative agreement with the values in direct numerical simulations. In particular, our expression for entrainment rate is consistent with the parameterization ϵB/w2\epsilon \sim B/w^2, for Archimedean buoyancy BB and vertical velocity ww. We also directly validate the role of buoyancy-driven entrainment by running simulations where gravity is turned off midway through a thermal's rise. The entrainment efficiency ee is observed to drop to less than 1/3 of its original value in both the laminar and turbulent cases when g=0g=0, affirming the central role of buoyancy in entrainment in dry thermals.

Keywords

Cite

@article{arxiv.1906.07224,
  title  = {Buoyancy-Driven Entrainment in Dry Thermals},
  author = {Brett McKim and Nadir Jeevanjee and Daniel Lecoanet},
  journal= {arXiv preprint arXiv:1906.07224},
  year   = {2020}
}

Comments

12 pages, 8 figures

R2 v1 2026-06-23T09:56:07.041Z