gravity.c

Gravity wave
- Results
- See also

Gravity wave

A similar test to the capillary wave but for a pure gravity wave, using the reduced gravity approach.

We use a constant-resolution grid, the Navier–Stokes solver for two-phase flows and reduced gravity.

#include "grid/multigrid.h"
#include "navier-stokes/centered.h"
#include "two-phase.h"
#include "reduced.h"
#include "prosperetti-gravity.h"

We make sure that the boundary conditions for the face-centered velocity field are consistent with the centered velocity field (this affects the advection term).

uf.n[left]   = 0.;
uf.n[right]  = 0.;
uf.n[top]    = 0.;
uf.n[bottom] = 0.;

We will store the accumulated error in se and the number of samples in ne.

double se = 0; int ne = 0;

int main() {

The domain is 2x2 to minimise finite-size effects. The viscosity is constant. The acceleration of gravity is 50.

  L0 = 2.;
  Y0 = -L0/2.;
  G.y = 50.;
  rho1 = 1, rho2 = 0.1;
  mu1 = mu2 = 0.0182571749236;
  TOLERANCE = 1e-6[*];

We vary the resolution to check for convergence.

  for (N = 16; N <= 128; N *= 2) {
    se = ne = 0;
    run();
  }
}

The initial condition is a small amplitude plane wave of wavelength unity.

event init (t = 0) {
  fraction (f, y - 0.01*cos (2.*pi*x));
}

By default tracers are defined at t-\Delta t/2. We use the first keyword to move VOF advection before the amplitude output i.e. at t+\Delta/2. This improves the results.

event vof (i++, first);

We output the amplitude at times matching exactly those in the reference file.

event amplitude (t += 0.00225584983639310905; t <= 1.66481717925811447992) {

To get an accurate amplitude, we reconstruct interface position (using height functions) and take the corresponding maximum.

  scalar pos[];
  position (f, pos, {0,1});
  double max = statsf(pos).max;

We output the corresponding evolution in a file indexed with the number of grid points N.

  char name[80];
  sprintf (name, "wave-%d", N);
  static FILE * fp = fopen (name, "w");
  fprintf (fp, "%g %g\n", t*16.032448313657, max);
  fflush (fp);

To compute the RMS error, we get data from the reference file prosperetti-gravity.h and add the difference to the accumulated error.

  se += sq(max - prosperetti[ne][1]); ne++;

  if (N == 64)
    output_facets (f, stdout);
}

At the end of the simulation, we output on standard error the resolution (number of grid points per wavelength) and the relative RMS error.

event error (t = end)
  fprintf (stderr, "%g %g\n", N/L0, sqrt(se/ne)/0.01);

Results

set xlabel 'tau'
set ylabel 'Relative amplitude'
plot '../prosperetti-gravity.h' u 2:4 w l t "Prosperetti", \
     'wave-128' every 10 w p t "Basilisk"

$Evolution of the amplitude of the gravity wave as a function of non-dimensional time \tau=\omega_0 t (script)$

Evolution of the amplitude of the gravity wave as a function of non-dimensional time \tau=\omega_0 t (script)

set xlabel 'Number of grid points'
set ylabel 'Relative RMS error'
set logscale y
set logscale x 2
set grid
plot [5:200][1e-4:1]'log' u 1:2 t "Basilisk" w lp, 2./x**2 t "Second order"

Convergence of the RMS error as a function of resolution (number of grid points per wavelength) (script)

src/test/gravity.c

Gravity wave

Results

See also