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makeplot.py
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126 lines (103 loc) · 3.72 KB
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"""
This script produces a reproduction of Figures 2 and 3 from Rodriguez+2011, the
dynamics of CoRoT-7b and c, using VPLANET's STELLAR, EQTIDE, and DISTORB modules.
David P. Fleming, University of Washington, 2018
"""
from __future__ import division, print_function
import matplotlib.pyplot as plt
import matplotlib as mpl
import numpy as np
import vplot as vpl
import sys
# Check correct number of arguments
if (len(sys.argv) != 2):
print('ERROR: Incorrect number of arguments.')
print('Usage: '+sys.argv[0]+' <pdf | png>')
exit(1)
if (sys.argv[1] != 'pdf' and sys.argv[1] != 'png'):
print('ERROR: Unknown file format: '+sys.argv[1])
print('Options are: pdf, png')
exit(1)
#Typical plot parameters that make for pretty plot
mpl.rcParams['figure.figsize'] = (10,8)
mpl.rcParams['font.size'] = 16.0
# Load data
output = vpl.GetOutput()
# Extract data
time = output.b.Time/1.0e6 # Scale to Myr
ecc1 = output.b.Eccentricity
ecc2 = output.c.Eccentricity
varpi1 = output.b.LongP
varpi2 = output.c.LongP
a1 = output.b.SemiMajorAxis
a2 = output.c.SemiMajorAxis
# Plot
fig, axes = plt.subplots(nrows=2, ncols=2, sharex=True)
color = "k"
## Upper left: a1 ##
axes[0,0].plot(time, a1, color="C3", zorder=-1, label="CoRoT-7b")
# Format
axes[0,0].set_xlim(time.min(),time.max())
axes[0,0].legend(loc="best")
axes[0,0].set_ylim(0.0165,0.019)
axes[0,0].set_ylabel("Semi-major Axis [AU]")
## Upper right: eccentricities ##
axes[0,1].plot(time, ecc1, color="C3", zorder=-1)
axes[0,1].plot(time, ecc2, color="C0", zorder=-1)
# Format
axes[0,1].set_xlim(time.min(),time.max())
axes[0,1].set_ylim(0.0,0.2)
axes[0,1].set_ylabel("Eccentricity")
## Lower left: a2 ##
axes[1,0].plot(time, a2, color="C0", zorder=-1, label="CoRoT-7c")
# Format
axes[1,0].set_xlim(time.min(),time.max())
axes[1,0].legend(loc="best")
axes[1,0].set_ylim(0.0459,0.0462)
axes[1,0].set_xlabel("Time [Myr]")
axes[1,0].set_ylabel("Semi-major Axis [AU]")
## Lower right: diff between longitude of periapses ##
varpiDiff = np.fabs(np.fmod(varpi1-varpi2, 360.0))
axes[1,1].scatter(time, varpiDiff, color="C3", s=10, zorder=-1)
# Format
axes[1,1].set_xlim(time.min(),time.max())
axes[1,1].set_ylim(0, 360)
axes[1,1].set_xlabel("Time [Myr]")
axes[1,1].set_ylabel(r"$\Delta \varpi$ [$^{\circ}$]")
# Final formating
fig.tight_layout()
for ax in axes.flatten():
# Rasterize
ax.set_rasterization_zorder(0)
# Set tick locations
ax.set_xticklabels(["0", "2", "4", "6", "8", "10"])
ax.set_xticks([0, 2, 4, 6, 8, 10])
# Show late-term ecc damping
inset1 = fig.add_axes([0.74, 0.735, 0.2, 0.2])
inset1.plot(time, ecc1, color="C3", zorder=20)
inset1.plot(time, ecc2, color="C0", zorder=20)
inset1.set_xlabel("Time [Myr]", fontsize=12)
inset1.set_ylabel("Eccentricity", fontsize=12)
inset1.set_xlim(8,10)
inset1.set_xticks([8, 9, 10])
inset1.set_xticklabels(["8", "9", "10"], fontsize=12)
inset1.set_yticks([1.0e-4, 1.0e-3, 1.0e-2])
inset1.set_yticklabels(["$10^{-4}$", "$10^{-3}$", "$10^{-2}$"], fontsize=12)
inset1.set_yscale("log")
# Show early apsidal locking
inset2 = fig.add_axes([0.74, 0.235, 0.2, 0.2])
inset2.scatter(time, varpiDiff, color="C3", s=10, zorder=20)
inset2.set_xlim(0.1,3)
inset2.set_ylim(0,360)
inset2.set_xscale("log")
inset2.set_yticks([0, 180, 360])
inset2.set_yticklabels(["0", "180", "360"], fontsize=12)
inset2.set_ylabel(r"$\Delta \varpi$ [$^{\circ}$]", fontsize=12)
inset2.set_xticks([0.1, 0.25, 0.5, 1, 2, 3])
inset2.set_xticklabels(["0.1", "0.25", "0.5", "1", "2", "3"], fontsize=12)
inset2.set_xlabel("Time [Myr]", fontsize=12)
if (sys.argv[1] == 'pdf'):
fig.savefig('ApseLock.pdf', bbox_inches="tight", dpi=600)
if (sys.argv[1] == 'png'):
fig.savefig('ApseLock.png', bbox_inches="tight", dpi=600)
#fig.savefig("Rodriguez2011_Figs23.pdf", bbox_inches="tight", dpi=600)