From 8624a241053557f173f7329f0d9dc957de48709d Mon Sep 17 00:00:00 2001 From: ArseniyKholod <119304909+ArseniyKholod@users.noreply.github.com> Date: Sun, 11 Feb 2024 18:08:19 +0200 Subject: [PATCH] Update docs/literate/src/files/behind_the_scenes_simulation_setup.jl Co-authored-by: Daniel Doehring --- docs/literate/src/files/behind_the_scenes_simulation_setup.jl | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/docs/literate/src/files/behind_the_scenes_simulation_setup.jl b/docs/literate/src/files/behind_the_scenes_simulation_setup.jl index e59e89319a0..d6ba59be0b5 100644 --- a/docs/literate/src/files/behind_the_scenes_simulation_setup.jl +++ b/docs/literate/src/files/behind_the_scenes_simulation_setup.jl @@ -218,7 +218,7 @@ sol = solve(ode, CarpenterKennedy2N54(williamson_condition = false), dt = 0.01, # "right-hand-side function", `rhs!`, within Trixi.jl. # Trixi.jl includes a set of `rhs!` functions designed to compute `du`, i.e., -# ``\partial u/\partial t`` according to the structure +# ``\frac{\partial u}{\partial t}`` according to the structure # of the setup. These `rhs!` functions calculate interface, mortars, and boundary fluxes, in # addition to surface and volume integrals, in order to construct the `du` vector. This `du` vector # is then used by the time integration method to obtain the solution at the subsequent time step.