Explain parameters of ParametersEulerGravity

src/Trixi.jl

@@ -262,7 +262,10 @@ export SemidiscretizationHyperbolicParabolic
 export SemidiscretizationEulerAcoustics
 
 export SemidiscretizationEulerGravity, ParametersEulerGravity,
-       timestep_gravity_erk52_3Sstar!, timestep_gravity_carpenter_kennedy_erk54_2N!
+       timestep_gravity_erk51_3Sstar!,
+       timestep_gravity_erk52_3Sstar!,
+       timestep_gravity_erk53_3Sstar!,
+       timestep_gravity_carpenter_kennedy_erk54_2N!
 
 export SemidiscretizationCoupled
 

src/semidiscretization/semidiscretization_euler_gravity.jl

@@ -14,11 +14,29 @@
                              timestep_gravity=timestep_gravity_erk52_3Sstar!)
 
 Set up parameters for the gravitational part of a [`SemidiscretizationEulerGravity`](@ref).
+
+# Arguments
+- `background_density<:Real`: Constant background/reference density ρ₀ which is subtracted from the (Euler) density
+                              in the RHS source term computation of the gravity solver.
+- `gravitational_constant<:Real`: Gravitational constant G which needs to be in consistent units with the
+                                  density and velocity fields. 
+- `cfl<:Real`: CFL number used for the pseudo-time stepping to advance the hyperbolic diffusion equations into steady state.
+- `resid_tol<:Real`: Absolute tolerance for the residual of the hyperbolic diffusion equations which are solved to 
+                     (approximately) steady state.
+- `n_iterations_max::Int`: Maximum number of iterations of the pseudo-time gravity solver. 
+                           If `n_iterations <= 0` the solver will iterate until the residual is less or equal `resid_tol`. 
+                           This can cause an infinite loop if the solver does not converge!
+- `timestep_gravity`: Function to advance the gravity solver by one pseudo-time step.
+                      There are three optimized methods available: 
+                      1) `timestep_gravity_erk51_3Sstar!` (first-order),
+                      2) `timestep_gravity_erk52_3Sstar!` (second-order),
+                      3) `timestep_gravity_erk53_3Sstar!` (third-order).
+                      Additionally, `timestep_gravity_carpenter_kennedy_erk54_2N!` (fourth-order) can be used.
 """
 struct ParametersEulerGravity{RealT <: Real, TimestepGravity}
     background_density     :: RealT # aka rho0
     gravitational_constant :: RealT # aka G
-    cfl                    :: RealT
+    cfl                    :: RealT # CFL number for the gravity solver
     resid_tol              :: RealT # Hyp.-Diff. Eq. steady state tolerance
     n_iterations_max       :: Int   # Max. number of iterations of the pseudo-time gravity solver
     timestep_gravity       :: TimestepGravity
@@ -71,7 +89,7 @@ end
 A struct containing everything needed to describe a spatial semidiscretization
 of a the compressible Euler equations with self-gravity, reformulating the
 Poisson equation for the gravitational potential as steady-state problem of
-the hyperblic diffusion equations.
+the hyperbolic diffusion equations.
 - Michael Schlottke-Lakemper, Andrew R. Winters, Hendrik Ranocha, Gregor J. Gassner (2020)
   "A purely hyperbolic discontinuous Galerkin approach for self-gravitating gas dynamics"
   [arXiv: 2008.10593](https://arXiv.org/abs/2008.10593)