Please use this identifier to cite or link to this item:
http://dspace.aiub.edu:8080/jspui/handle/123456789/604
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Maleque, Kh. Abdul | - |
dc.contributor.author | Sattar, Md. Abdus | - |
dc.date.accessioned | 2022-06-14T10:20:08Z | - |
dc.date.available | 2022-06-14T10:20:08Z | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | 8 | en_US |
dc.identifier.issn | 0970-9991 | - |
dc.identifier.uri | http://dspace.aiub.edu:8080/jspui/handle/123456789/604 | - |
dc.description | vol-27, pp-211-228 | en_US |
dc.description.abstract | A steady three-dimensional MHD convective laminar incompressible boundary layer flow due to an infinite rotating disk in an axial uniform magnetic field is studied taking the effect of Hall current. It is assumed that the flow is laminar and the boundary layer thickness depends on the radial distance. Then, by introducing suitable similarity variable η, which is a function of≅ and r, the governing partial differential equations are reduced to nonlinear ordinary differential equations. The similarity equations are then solved numerically by Nachtsheim-Swigert iteration technique. The results are then shown in the form of graphs and tablets. | en_US |
dc.publisher | Journal Journal of Energy, Heat and Mass Transfer, Madras, India. Volume 27 Pages pp. 211-228 | en_US |
dc.title | MHD convection flow due to a rotating disk with hall effect | en_US |
dc.type | Article | en_US |
Appears in Collections: | Publication: Journal |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
FORMAT 1.docx | 5 MB | Microsoft Word XML | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.