Computational fluid dynamics is used to investigate designs for rotating me
mbrane disk filters. Simulations have been run for the case of water permea
ting through a membrane disk rotating in a pressurized housing. The water w
as assumed to be Newtonian, incompressible, non-fouling and isothermal. A k
-epsilon model was used to describe turbulent how in the vessel surrounding
the rotating disk. Similar to a nonporous disk, the rotation of the membra
ne disk induces a recirculating flow pattern of the fluid within the vessel
. However, the centrifugal force acting on the permeate may locally increas
e the permeate side pressure above the feed side pressure resulting in a ne
gative local transmembrane pressure. Hence, a portion of the membrane is su
bject to a reversed flow of permeate which reduces effectiveness of membran
e area and may damage the membrane. This 'back pressure' phenomenon can be
avoided by a careful choice of the operating conditions and design paramete
rs. The propensity for 'back pressure' is higher when the membrane is more
permeable but can be reduced by increasing the feed flow rate or decreasing
the disk diameter (i.e. the membrane area). (C) 1999 Elsevier Science S.A.
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