In order to describe the magnetohydrodynamical (MHD) winds/jets from a geometrically thin accretion disk with rotation, MHD equations are written in orthogonal curvilinear coordinates with axes parallel and perpendicular to the streamlines, respectively.
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Nonlinear magneto-radiative bioconvection of Casson penta-hybrid nanofluid with microorganisms under inclined magnetic field and quadratic radiation for drug delivery. [PDF]
Chari FN, Mahboobtosi M, Ganji DD.
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Recent advances in high- β N experiments and magnetohydrodynamic instabilities with hybrid scenarios in the HL-2A Tokamak. [PDF]
Chen W +28 more
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A magnetohydrodynamic mechanism for the formation of solar polar vortices. [PDF]
Dikpati M +5 more
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CONfirm: A Spectacular Galactic Scale MHD Powered Wind in ESO~320-G030
Gorski M +25 more
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Electroosmotic flow of Jeffrey ternary hybrid nanofluids in converging-diverging ciliary microvessels. [PDF]
Obalalu AM +4 more
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Integrated Magnetohydrodynamic Pump with Magnetic Composite Substrate and Laser-Induced Graphene Electrodes. [PDF]
Khan MA, Kosel J.
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Analytical solution for MHD nanofluid flow over a porous wedge with melting heat transfer. [PDF]
Ahmadi Azar A +4 more
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Microenvironment regulation in nanomaterial synthesis. [PDF]
Pang S +7 more
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Accreting White Dwarfs: An Unreview. [PDF]
Scaringi S, Knigge C, de Martino D.
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