Show simple item record

contributor authorPekmen Geridonmez, Bengisen
date accessioned2019-03-17T10:11:47Z
date available2019-03-17T10:11:47Z
date copyright2/25/2019 12:00:00 AM
date issued2019
identifier issn0022-1481
identifier otherht_141_04_042501.pdf
identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4255985
description abstractIn this study, free convection in a cavity with differentially heated wavy walls is numerically investigated in the presence of a magnetic source. Polyharmonic spline radial basis function (RBF) is utilized to discretize the governing dimensionless equations formulated by stream function-vorticity. The effects of dimensionless Hartmann number, Rayleigh number, the number of undulations, amplitude of wave, and the location of magnetic source are visualized in streamlines and isotherms as well as calculating average Nusselt number through the heated wall. Results show that primary vortex in streamlines is altered with the impact of magnetic source. The augmentation of undulations and amplitude causes convective heat transfer to decrease if Ra = 105. The impact of location of magnetic source is noted close to the top wall.
publisherThe American Society of Mechanical Engineers (ASME)
titleFree Convection in a Wavy Walled Cavity With a Magnetic Source Using Radial Basis Functions
typeJournal Paper
journal volume141
journal issue4
journal titleJournal of Heat Transfer
identifier doi10.1115/1.4042782
journal fristpage42501
journal lastpage042501-9
treeJournal of Heat Transfer:;2019:;volume( 141 ):;issue: 004
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record