This paper presents a numerical study of thermal convection in a gravitational field. It compares the sedimentation processes of solid spherical particles and water droplets in a hydrocarbon medium by employing different approaches to calculate sedimentation velocity: Stokes' law and the Hadamard-Rybczynski formula. Investigations are conducted on the gravitational sedimentation of the dispersed phase for varying initial concentrations and particle/droplet radii. The densities of the droplets and particles are assumed to be identical. The results demonstrate that the flow profiles and sedimentation dynamics differ significantly between droplets and particles. This disparity becomes more pronounced with increasing size of the dispersed phase. In the case of emulsion dynamics, the differences also depend on the viscosity ratio between the dispersed phase and the dispersion medium.
Author Biographies
Sakhibgareev Emil Elvirovich, Ufa University of Science & Technology
Ufa University of Science & Technology, applied physics department, st. Zaki Validi, 32, Ufa, Republic of Bashkortostan, Russia
Musin Airat Akhmatovich, Ufa University of Science & Technology
applied physics department, st. Zaki Validi, 32, Ufa, Republic of Bashkortostan, Russia
ResearcherID: R-9142-2016 Scopus AuthorID: 36778696600 SPIN-код: 6233-9516 РИНЦ AuthorID: 528818
Kovaleva Liana Aronovna, Ufa University of Science & Technology
applied physics department,, st. Zaki Validi, 32, Ufa, Republic of Bashkortostan, Russia