The firstOrderMusclUpdater computes an first order upwind discretization of the spatial component of a non-linear hyperbolic system, possibly with source terms:
where \(\mathbf{q}\) is a vector of conserved variables (e.g. density, momentum, total energy), \(\mathcal{F}\left( \mathbf{w} \right)\) is a non-linear flux tensor computed from a vector of primitive variables, (e.g. density, velocity, pressure), \(\mathbf{w} = \mathbf{w}(\mathbf{q})\) and \(\mathcal{S} \left( \mathbf{w} \right)\) is some source term.
The firstOrderMuscl updater accepts the parameters below, in addition to those required by Updater.
in
(string vector, required)out
(string vector, required)waveSpeeds
(string vector, optional)equations
(string vector, required)numericalFlux
(string, required)cfl
(float, optional)checkCfl
(bool, optional)sources
(string vector, optional)Equation
(block, required)Source
(block)The following block demonstrates the firstOrderMuscl updater used in combination with the mhdDednerEqn to compute \(\nabla \cdot \mathcal{F}\left(\mathbf{w} \right)\) with an externally supplied magnetic field:
<Updater hyper>
kind=firstOrderMuscl1d
onGrid=domain
# input nodal component arrays
in=[q backgroundB]
# output nodal component array
out=[qnew]
# input dynVector containing fastest wave speed
waveSpeeds=[waveSpeed]
# the numerical flux to use
numericalFlux= hlldFlux
# CFL number to use
cfl=0.3
# list of equations to solve
equations=[mhd]
<Equation mhd>
kind=mhdDednerEqn
gasGamma=1.4
externalBfield="backgroundB"
</Equation>
</Updater>