Particle stratification in spiral concentrators occurs
due to the
combined action of gravitational and centrifugal forces. Spiral flows
have a free surface, shallow depths, and a transition from laminar
to turbulent behavior. The current study investigates the comparisons
of the flow field and bicomponent particle separation in high-gravity
spirals with conventional coal spirals, often termed low-gravity spirals.
A sensitive digital flow depth gauge is utilized to measure the fluid
depth across the spiral trough. A high-speed motion camera is utilized
to measure the free surface velocity via a tracer tracking approach.
This flow visualization technique incorporates lycopodium powder as
tracer particles to capture the free surface flow field on a dark
background. Further, the two-phase flow is modeled for these designs
by utilizing the volume of fluid model (VOF), incorporating the Reynolds
stress model and RNG k–ε turbulence
models. Comparisons were made on the flow patterns between high-gravity
and low-gravity spirals, which differ in their trough profiles. High-gravity
spiral concentrators exhibit greater depths, free surface velocities,
secondary circulations, and turbulence intensities toward the outer
edges compared to low-gravity spirals. The discrete phase model (DPM)
is employed for particle tracking, thereby understanding particle
segregation radially along the spiral trough. Performance data on
bicomponent particle separation is presented to compare the separation
effectiveness of high- and low-gravity spirals. Heavy mineral ore,
such as chromite, is computationally tested with high- and low-gravity
spirals, and it was found that low-gravity spirals are ineffective
in achieving satisfactory particle separation. Also, the results demonstrate
that each spiral has its own distinct size range for effectively separating
particles. The DPM model predictions were validated against in-house
experiments conducted with monocomponent silica material, and a reasonable
match was found with the experimental data.