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On the interface instability during rapid evaporation in microgravity

Technical Report ·
DOI:https://doi.org/10.2172/537364· OSTI ID:537364
 [1]
  1. Los Alamos National Lab., NM (United States). Theoretical Div.
The rapid evaporation of a superheated liquid (vapor explosion) under microgravity conditions is studied by direct numerical simulation. The time-dependent Navier-Stokes and energy equations coupled to the interface dynamics are solved using a two-dimensional finite-difference/front-tracking method. Large interface deformations, topology change, latent heat, surface tension and unequal material properties between the liquid and vapor phases are included in the simulations. A comparison of numerical results to the exact solution of a one-dimensional test problem shows excellent agreement. For the two-dimensional rapid evaporation problem, the vapor volume growth rate and unstable interface dynamics are studied for increasing levels of initial liquid superheat. As the superheat is increased the liquid-vapor interface experiences increasingly unstable energetic growth. These results indicate that heat transfer plays a very important role in the instability mechanism leading to vapor explosions. It is suggested that the Mullins-Sekerka instability could play a role in the instability initiation mechanism.
Research Organization:
Los Alamos National Lab., NM (United States)
Sponsoring Organization:
Department of Defense, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States); National Science Foundation, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
537364
Report Number(s):
LA-UR--97-918; CONF-971115--1; ON: DE97005030; CNN: Grant NGT-51070; Grant CTS-9503208
Country of Publication:
United States
Language:
English