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some updates to the massive star slice plots #2759

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Feb 23, 2024
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18 changes: 13 additions & 5 deletions Exec/science/massive_star/analysis/massive_star_multi.py
Original file line number Diff line number Diff line change
Expand Up @@ -22,6 +22,13 @@ def make_plot(plotfile, prefix="plot", width_frac=0.1,

ds = CastroDataset(plotfile)

t_drive = 0.0
if "[*] castro.drive_initial_convection_tmax" in ds.parameters:
t_drive = ds.parameters["[*] castro.drive_initial_convection_tmax"]
elif "[*] castro.drive_initial_convection_tmax" in ds.parameters:
t_drive = ds.parameters["[*] castro.drive_initial_convection_tmax"]
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print(t_drive)

xmin = ds.domain_left_edge[0]
xmax = ds.domain_right_edge[0]

Expand Down Expand Up @@ -70,32 +77,33 @@ def make_plot(plotfile, prefix="plot", width_frac=0.1,

if f == "enuc":
# now do a contour of NSE
sp.annotate_contour("in_nse", ncont=1, clim=(0.5, 0.5), take_log=False,
plot_args={"colors": "k", "linewidths": 2})
if ("boxlib", "in_nse") in ds.derived_field_list:
sp.annotate_contour("in_nse", ncont=1, clim=(0.5, 0.5), take_log=False,
plot_args={"colors": "k", "linewidths": 2})

sp.set_axes_unit("cm")

fig = sp.export_to_mpl_figure((layout[0], layout[1]), axes_pad=(1.0, 0.4),
cbar_location=cbar_location, cbar_pad="2%")

fig.subplots_adjust(left=0.05, right=0.95, bottom=0.025, top=0.975)
fig.text(0.02, 0.02, f"time = {float(ds.current_time):8.2f} s",
fig.text(0.02, 0.02, f"$t - \\tau_\\mathrm{{drive}}$ = {float(ds.current_time) - t_drive:6.1f} s",
transform=fig.transFigure)
fig.set_size_inches(size)
fig.tight_layout()
extra = ""
if layout[0] >= layout[1]:
extra = "_vertical"

fig.savefig(f"{prefix}_{os.path.basename(plotfile)}_w{width_frac:04.2f}{extra}.pdf", pad_inches=0)
fig.savefig(f"{prefix}_{os.path.basename(plotfile)}_w{width_frac:04.2f}{extra}.pdf", pad_inches=0.1, bbox_inches="tight")


if __name__ == "__main__":

p = argparse.ArgumentParser()
p.add_argument("--vertical", action="store_true",
help="plot 2x2 or 1x4")
p.add_argument("--width_fraction", type=float, default=0.1,
p.add_argument("--width-fraction", type=float, default=0.1,
help="fraction of domain to show")
p.add_argument("plotfile", type=str, nargs=1,
help="plotfile to plot")
Expand Down
178 changes: 178 additions & 0 deletions Exec/science/massive_star/analysis/massive_star_sequence.py
Original file line number Diff line number Diff line change
@@ -0,0 +1,178 @@
#!/usr/bin/env python3

import argparse
import os

import matplotlib
import matplotlib.pyplot as plt
import numpy as np
from mpl_toolkits.axes_grid1 import ImageGrid

import yt
from yt.frontends.boxlib.api import CastroDataset
# assume that our data is in CGS
from yt.units import cm

matplotlib.use('agg')

times = [50, 100, 150, 200, 250]

def find_files(plist):

mask = np.zeros(len(times))
files_to_plot = []
for pfile in plist:
for k, t in enumerate(times):
if mask[k]:
continue
print(pfile)
ds = CastroDataset(pfile)
if ds.current_time >= t:
files_to_plot.append(pfile)
mask[k] = 1.0

return files_to_plot


def make_plot(field, pfiles, *,
width_frac=0.1,
size=(19.2, 10.8)):

fig = plt.figure()

if len(pfiles) > 8:
nrows = 3
ncols = (len(pfiles) + 1)//3
elif len(pfiles) >= 4:
nrows = 2
ncols = (len(pfiles) + 1)//2
else:
nrows = 1
ncols = len(pfiles)

grid = ImageGrid(fig, 111, nrows_ncols=(nrows, ncols),
axes_pad=0.2, cbar_pad=0.05,
label_mode="L", cbar_mode="single")

# get some metadata
ds = CastroDataset(pfiles[0])

t_drive = 0.0
if "[*] castro.drive_initial_convection_tmax" in ds.parameters:
t_drive = ds.parameters["[*] castro.drive_initial_convection_tmax"]
elif "[*] castro.drive_initial_convection_tmax" in ds.parameters:
t_drive = ds.parameters["[*] castro.drive_initial_convection_tmax"]
print(t_drive)

xmin = ds.domain_left_edge[0]
xmax = ds.domain_right_edge[0]

ymin = ds.domain_left_edge[1]
ymax = ds.domain_right_edge[1]

xctr = 0.0 * xmin
L_x = xmax - xmin

yctr = 0.5 * (ymin + ymax)
L_y = ymax - ymin

f = field

if f == "Temp" or f == "abar":
text_color = "white"
else:
text_color = "black"

for i in range(nrows * ncols):

if i < len(pfiles):
pf = pfiles[i]
else:
grid[i].remove()
continue

ds = CastroDataset(pf)

sp = yt.SlicePlot(ds, "theta", f,
center=[xmin + 0.5*width_frac*L_x, yctr, 0.0*cm],
width=[width_frac*L_x, width_frac*L_y, 0.0*cm],
fontsize="12")

sp.set_buff_size((2400,2400))

sp.annotate_text((0.05, 0.05),
f"$t - \\tau_\\mathrm{{drive}}$ = {float(ds.current_time) - t_drive:8.2f} s",
coord_system="axis",
text_args={"color": text_color})


if f == "Ye":
sp.set_zlim(f, 0.46, 0.5)
sp.set_log(f, False)
sp.set_cmap(f, "magma_r")
elif f == "abar":
sp.set_log(f, False)
sp.set_cmap(f, "viridis")
elif f == "enuc":
sp.set_log(f, True, linthresh=1.e12)
sp.set_zlim(f, -1.e20, 1.e20)
sp.set_cmap(f, "bwr")
elif f == "MachNumber":
sp.set_zlim(f, 1.e-4, 0.3)
sp.set_cmap(f, "plasma")
elif f == "magvel":
sp.set_zlim(f, 100.0, 2.e7)
sp.set_cmap(f, "viridis")
elif f == "magvort":
sp.set_cmap(f, "magma")
sp.set_zlim(f, 1.e-2, 5)

if f == "enuc":
# now do a contour of NSE
if ("boxlib", "in_nse") in ds.derived_field_list:
sp.annotate_contour("in_nse", levels=1, clim=(0.5, 0.5), take_log=False,
plot_args={"colors": "k", "linewidths": 2})

sp.set_axes_unit("cm")

plot = sp.plots[field]
plot.figure = fig
plot.axes = grid[i].axes
plot.cax = grid.cbar_axes[i]
if i < len(pfiles)-1:
grid[i].axes.xaxis.offsetText.set_visible(False)
if i > 0:
grid[i].axes.yaxis.offsetText.set_visible(False)

sp._setup_plots()

fig.set_size_inches(size)
fig.tight_layout()
extra = ""

fig.savefig(f"massive_star_{f}_w{width_frac:04.2f}.pdf", pad_inches=0.1, bbox_inches="tight")


if __name__ == "__main__":

p = argparse.ArgumentParser()
p.add_argument("--var", type=str, default="Temp",
help="variable to plot")
p.add_argument("--vertical", action="store_true",
help="plot 2x2 or 1x4")
p.add_argument("--width-fraction", type=float, default=0.1,
help="fraction of domain to show")
p.add_argument("plotfiles", type=str, nargs="+",
help="list of plotfiles to plot")

args = p.parse_args()

if args.vertical:
size = (7.5, 8.5)
else:
size = (19.2, 8.5)

plist = find_files(args.plotfiles)

make_plot(args.var, plist,
width_frac=args.width_fraction, size=size)