Results 161 to 170 of about 62,331 (246)

Novel analytical perspectives on nonlinear instabilities of viscoelastic Bingham fluids in MHD flow fields. [PDF]

Sci Rep
Moatimid GM, Mohamed YM.
europepmc   +1 more source

Unsteady MHD flow of tangent hyperbolic ternary hybrid nanofluid in a darcy-forchheimer porous medium over a permeable stretching sheet with variable thermal conductivity. [PDF]

F1000Res
Tsegaye Moltot A, Haile Gorfie E, Awgichew Zergaw G, Dessie H.   +3 more
europepmc   +1 more source

Modeling of entropy optimization for hybrid nanofluid MHD flow through a porous annulus involving variation of Bejan number. [PDF]

Sci Rep, 2020
Shah Z, Sheikholeslami M, Kumam P, Ikramullah, Shafee A.   +4 more
europepmc   +1 more source

Mass Transpiration in Nonlinear MHD Flow Due to Porous Stretching Sheet. [PDF]

Sci Rep, 2019
Singh J, Mahabaleshwar US, Bognár G.
europepmc   +1 more source

MHD flow of Maxwell fluid with nanomaterials due to an exponentially stretching surface. [PDF]

Sci Rep, 2019
Farooq U, Lu D, Munir S, Ramzan M, Suleman M, Hussain S.   +5 more
europepmc   +1 more source

Analysis of dual solution for MHD flow of Williamson fluid with slippage. [PDF]

Heliyon, 2019
Lund LA, Omar Z, Khan I.
europepmc   +1 more source

Mathematical analysis of magnetohydrodynamic (MHD) flow of micropolar nanofluid under buoyancy effects past a vertical shrinking surface: dual solutions. [PDF]

Heliyon, 2019
Lund LA, Omar Z, Khan I.
europepmc   +1 more source

MHD Flow of Sodium Alginate-Based Casson Type Nanofluid Passing Through A Porous Medium With Newtonian Heating. [PDF]

Sci Rep, 2018
Khan A, Khan D, Khan I, Ali F, Karim FU, Imran M.   +5 more
europepmc   +1 more source

Effects of cross diffusion and heat generation on mixed convective MHD flow of Casson fluid through porous medium with non-linear thermal radiation. [PDF]

Heliyon, 2019
Patel HR.
europepmc   +1 more source

MHD equilibria of astrospheric flows

, 2005
The hot gas cavities around stars which have a stellar wind are called astrospheres. Between the outer interstellar medium and the stellar wind there forms a contact surface or boundary surface which is called an astropause. In this thesis the geometrical shape of such an astrosphere/astropause region is calculated consistently together with the flow ...
openaire   +1 more source