smod_equil_RTI_KHI Submodule

This submodule defines Rayleigh-Taylor and Kelvin-Helmholtz instabilities in Cartesian geometry. This equilibrium is a specific case of the flow driven instabilities.

This equilibrium is taken from section 13.2, p. 487 (case c) in Goedbloed, H., Keppens, R., & Poedts, S. (2019). Magnetohydrodynamics of Laboratory and Astrophysical Plasmas. Cambridge University Press. DOI.


Uses


Contents


Module Procedures

module procedure RTI_KHI_eq module module subroutine RTI_KHI_eq(settings, grid, background, physics)

Arguments

TypeIntentOptionalAttributesName
type(settings_t), intent(inout) :: settings
type(grid_t), intent(inout) :: grid
type(background_t), intent(inout) :: background
type(physics_t), intent(inout) :: physics