Abstract
The evaporation of a droplet by non-uniform heating is numerically investigated in order to understand the
mechanism of the fuel-vapor jet eruption observed in the flame spread of a droplet array under microgravity
condition. The phenomenon was believed to be mainly responsible for the enhanced flame spread rate through
a droplet cloud at microgravity conditions. A modified Eulerian-Lagrangian method with a local phase change
model is utilized to describe the interfacial dynamics between liquid droplet and surrounding air. It is found
that the localized heating creates a temperature gradient along the droplet surface, induces the corresponding
surface tension gradient, and thus develops an inner flow circulation commonly referred to as the Marangoni
convection. Furthermore, the effect also produces a strong shear flow around the droplet surface, thereby
pushing the fuel vapor toward the wake region of the droplet to form a vapor jet eruption. A parametric study
clearly demonstrated that at realistic droplet combustion conditions the Marangoni effect is indeed responsible
for the observed phenomena, in contrast to the results based on constant surface tension approximation
Original language | English (US) |
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Title of host publication | 52nd Aerospace Sciences Meeting |
Publisher | American Institute of Aeronautics and Astronautics (AIAA) |
ISBN (Print) | 9781624102561 |
DOIs | |
State | Published - Jan 10 2014 |