mod_wb_atmosphere Module Reference

Well-balanced atmosphere module. More...

Functions/Subroutines
subroutine, public	wb_atmos_init (pa, ra, grav, jmax, ds, gzone, grav_dir, irho, ip)
	Build grid-aligned HSE tables from a fine 1D reference profile.
subroutine, public	wb_atmos_set_w (ixil, ixol, w, x)
	Set w to the equilibrium state (rho, v=0, p) at each cell position.
subroutine, public	wb_atmos_get_eq (x_grav, rho_eq, p_eq)
	Equilibrium (rho, p) of the grid-aligned table at a coordinate x_grav along the gravity direction: the node value at a node, else log-linear between the two nodes around it.

Variables
double precision, dimension(:), allocatable, public	wb_pa
	Grid-aligned discrete HSE (built at finest AMR resolution).
double precision, dimension(:), allocatable, public	wb_ra
	equilibrium density
integer, public	wb_n_grid = 0
	table size

Detailed Description

Well-balanced atmosphere module.

Builds grid-aligned hydrostatic equilibrium tables at the finest AMR resolution from a user-provided fine 1D reference profile. Provides routines for setting the initial condition and boundary conditions from these tables.

The module is EoS-independent: it receives p(s) and rho(s) and never calls EoS routines. The multiplicative HSE recurrence uses T = p/rho which is valid for any equation of state.

Usage:

1. User integrates HSE to produce fine pa(:), ra(:) arrays
2. call wb_atmos_init(pa, ra, grav, jmax, ds, gzone, grav_dir)
3. call wb_atmos_set_w(ixI^L, ixO^L, w, x) in IC and BC routines
4. call phys_to_conserved(...) after set_w (user's responsibility)

Function/Subroutine Documentation

wb_atmos_get_eq()

subroutine, public mod_wb_atmosphere::wb_atmos_get_eq	(	double precision, intent(in)	x_grav,
		double precision, intent(out)	rho_eq,
		double precision, intent(out)	p_eq )

Equilibrium (rho, p) of the grid-aligned table at a coordinate x_grav along the gravity direction: the node value at a node, else log-linear between the two nodes around it.

Definition at line 184 of file mod_wb_atmosphere.t.

wb_atmos_init()

subroutine, public mod_wb_atmosphere::wb_atmos_init	(	double precision, dimension(:), intent(in)	pa,
		double precision, dimension(:), intent(in)	ra,
		double precision, dimension(:), intent(in)	grav,
		integer, intent(in)	jmax,
		double precision, intent(in)	ds,
		double precision, intent(in)	gzone,
		integer, intent(in)	grav_dir,
		integer, intent(in)	irho,
		integer, intent(in)	ip )

Build grid-aligned HSE tables from a fine 1D reference profile.

The fine table (pa, ra) spans [xmin - gzone, xmax + gzone] along the gravity direction, evenly spaced at ds. The gravity array grav(jmax) gives the gravitational acceleration at each fine table point.

The grid-aligned table is built at the finest AMR resolution using the multiplicative trapezoidal recurrence, which matches the discrete HSE that the WB reconstruction preserves.

Parameters

[in]	pa	fine pressure table
[in]	ra	fine density table
[in]	grav	fine gravity table
[in]	jmax	fine table size
[in]	ds	fine table spacing
[in]	gzone	ghost zone width (code units)
[in]	grav_dir	gravity direction (1, 2, or 3)
[in]	irho	w-array index for density
[in]	ip	w-array index for pressure

Definition at line 56 of file mod_wb_atmosphere.t.

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wb_atmos_set_w()

subroutine, public mod_wb_atmosphere::wb_atmos_set_w	(	integer, intent(in)	ixi,
		integer, intent(in)	l,
		integer, intent(in)	ixo,
			l,
		double precision, dimension(ixi^s, 1:nw), intent(inout)	w,
		double precision, dimension(ixi^s, 1:ndim), intent(in)	x )

Set w to the equilibrium state (rho, v=0, p) at each cell position.

The grid-aligned table is sampled at the cell centres: the node value on the finest level, which matches the trap-rule recurrence of the legacy_trap WB transform, and log-linear between the two nodes around the centre of a coarse cell

On exit: w(rho_) = rho_eq, w(mom(:)) = 0, w(p_) = p_eq. The caller must call phys_to_conserved afterwards.

Definition at line 165 of file mod_wb_atmosphere.t.

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Variable Documentation

wb_n_grid

integer, public mod_wb_atmosphere::wb_n_grid = 0

table size

Definition at line 32 of file mod_wb_atmosphere.t.

wb_pa

double precision, dimension(:), allocatable, public mod_wb_atmosphere::wb_pa

Grid-aligned discrete HSE (built at finest AMR resolution).

equilibrium pressure

Definition at line 30 of file mod_wb_atmosphere.t.

wb_ra

double precision, dimension(:), allocatable, public mod_wb_atmosphere::wb_ra

equilibrium density

Definition at line 31 of file mod_wb_atmosphere.t.