Evolution of highly buoyant thermals in a stratified layer

Citation
A. Brandenburg et J. Hazlehurst, Evolution of highly buoyant thermals in a stratified layer, ASTRON ASTR, 370(3), 2001, pp. 1092-1102
Citations number
12
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS
ISSN journal
14320746 → ACNP
Volume
370
Issue
3
Year of publication
2001
Pages
1092 - 1102
Database
ISI
SICI code
1432-0746(200105)370:3<1092:EOHBTI>2.0.ZU;2-E
Abstract
The buoyant rise of thermals (i.e. bubbles of enhanced entropy, but initial ly in pressure equilibrium) is investigated numerically in three dimensions for the case of an adiabatically stratified layer covering 6-9 pressure sc ale heights. It is found that these bubbles can travel to large heights bef ore being braked by the excess pressure that builds up in order to drive th e gas sideways in the head of the bubble. Until this happens, the momentum of the bubble grows ass described by the time-integrated buoyancy force. Th is validates the simple theory of bubble dynamics whereby the mass entrainm ent of the bubble provides an effective braking force well before the bubbl e stops ascending. This is quantified by an entrainment parameter alpha whi ch is calculated from the simulations and is found to he in good agreement with the experimental measurements. This work is discussed in the context o f contact binaries whose secondaries could be subject to dissipative heatin g in the outermost layers.