Axisymmetric self-similar solutions to the MHD equations without magnetic diffusion

Abstract

We study the axisymmetric self-similar solutions $(\mathbf{u},\mathbf{B})$ to the stationary MHD equations without magnetic diffusion, where $\mathbf{B}$ has only the swirl component. Our first result states that in ${\mathbb{R}}^3\setminus \{0\}$, $\mathbf{u}$ is a Landau solution and $\mathbf{B}=0$. Our second result proves the triviality of axisymmetric self-similar solutions in the half-space ${\mathbb{R}}_{+}^3$ with the no-slip boundary condition or the Navier slip boundary condition.