Answers are grounded in this paper and cite their sources.
We perform a bifurcation analysis of a two-dimensional magnetic Rayleigh–Bénard problem using a numerical technique called deflated continuation. Our aim is to study the influence of the magnetic field on the bifurcation diagram as the Chandrasekhar number Q increases and compare it to the standard (non-magnetic) Rayleigh–Bénard problem. We compute steady states at a high Chandrasekhar number of Q=103 over a range of the Rayleigh number 0≤Ra≤105. These solutions are obtained by combining deflation with a continuation of steady states at low Chandrasekhar number, which allows us to explore the influence of the strength of the magnetic field as Q increases from low coupling, where the magnetic effect is almost negligible, to strong coupling at Q=103. We discover a large profusion of states with rich dynamics and observe a complex bifurcation structure with several pitchfork, Hopf, and saddle–node bifurcations. Our numerical simulations show that the onset of bifurcations in the problem is delayed when Q increases, while solutions with fluid velocity patterns aligning with the background vertical magnetic field are privileged. Additionally, we report a branch of states that stabilizes at high magnetic coupling, suggesting that one may take advantage of the magnetic field to discriminate solutions.
No takes yet. Share an insight, caveat, or question.
Laakmann et al. (2024) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: