This study investigates the stability of parallel buoyant magneto-convection in a rotating vertical porous medium filled with a Casson fluid. The vertical boundaries are considered isothermal rigid and kept at different uniform temperatures. Based on Darcy's law, the Navier–Stokes equation is employed. In a linear stability theory, the stability of an eigenvalue problem is found using the normal mode approach. The original three-dimensional problem is cast in an equivalent two-dimensional form using Squire's transformations. Subsequently, the two-dimensional stability of the eigenvalue problem is solved numerically using the Chebyshev collocation method. To determine the stability of the basic flow, the problem was originally solved in Gill's classical proof of 1969 [A. E. Gill, “A proof that convection in a porous vertical slab is stable,” J. Fluid Mech. 35, 545–547 (1969)]. Various basic state flow and magnetic fields were considered by varying the magnetic Prandtl number, ranging from 1×10−5 to 5×10−5. The critical stability conditions are exhibited, and the critical Rayleigh number (Rc), critical wave number (ac), and critical wave speed (cc) for the onset of convective instability are computed for different governing parameters. For the unsteady flow model, stability occurs through the marginal state mode within a certain range of Chandrasekhar numbers; however, the base flow remains stable throughout. The Casson fluid parameter and Darcy number significantly affect the neutral stability curve of the flow. Their combined influence contributes to the onset of instability in the Brinkman region. This interaction highlights the critical role of these parameters determining flow behavior.
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