Exact solutions for the incompressible viscous magnetohydrodynamic fluid of a rotating disk flow (Retracted article. See vol. 50, pg. 3135, 2015)

Turkyilmazoglu M.

MECCANICA, cilt.46, sa.5, ss.1085-1092, 2011 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 46 Sayı: 5
  • Basım Tarihi: 2011
  • Doi Numarası: 10.1007/s11012-010-9362-4
  • Dergi Adı: MECCANICA
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.1085-1092
  • Hacettepe Üniversitesi Adresli: Hayır

Özet

The main interest of the present paper is to generate exact solutions to the steady Navier-Stokes equations for the incompressible Newtonian viscous electrically conducting fluid flow motion due to a disk rotating with a constant angular speed. In place of the traditional von Karman's axisymmetric evolution of the flow, the rotational non-axisymmetric stationary conducting flow is taken into consideration here. As a consequence, for an external uniform magnetic field applied perpendicular to the plane of the disk, the governing equations allow an exact solution to develop, which is influenced by a fixed point on the disk and also is bounded everywhere in the normal direction to the wall.