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!Basic_Simulation | ||
!Fragmentation | ||
!helio_gr_test | ||
!whm_gr_test | ||
!whm_gr_test | ||
!Chambers2013 |
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* | ||
!.gitignore | ||
!init_cond.py | ||
!aescattermovie.py |
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#!/usr/bin/env python3 | ||
import swiftest | ||
import numpy as np | ||
import matplotlib.pyplot as plt | ||
from matplotlib import animation | ||
import matplotlib.colors as mcolors | ||
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titletext = "Chambers (2013)" | ||
radscale = 2000 | ||
xmin = 0.0 | ||
xmax = 2.20 | ||
ymin = 0.0 | ||
ymax = 1.0 | ||
framejump = 1 | ||
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class AnimatedScatter(): | ||
"""An animated scatter plot using matplotlib.animations.FuncAnimation.""" | ||
def __init__(self, ds, param): | ||
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frame = 0 | ||
nframes = int(ds['time'].size / framejump) | ||
self.ds = ds | ||
self.param = param | ||
self.Rcb = self.ds['radius'].sel(name="Sun").isel(time=0).values[()] | ||
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self.clist = {'Initial conditions' : 'xkcd:faded blue', | ||
'Disruption' : 'xkcd:marigold', | ||
'Supercatastrophic' : 'xkcd:shocking pink', | ||
'Hit and run fragmentation' : 'xkcd:baby poop green'} | ||
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# Setup the figure and axes... | ||
fig = plt.figure(figsize=(8,4.5), dpi=300) | ||
plt.tight_layout(pad=0) | ||
# set up the figure | ||
self.ax = plt.Axes(fig, [0.1, 0.15, 0.8, 0.75]) | ||
self.ax.set_xlim(xmin, xmax) | ||
self.ax.set_ylim(ymin, ymax) | ||
fig.add_axes(self.ax) | ||
self.ani = animation.FuncAnimation(fig, self.update, interval=1, frames=nframes, init_func=self.setup_plot, blit=True) | ||
self.ani.save('aescatter.mp4', fps=60, dpi=300, extra_args=['-vcodec', 'libx264']) | ||
print('Finished writing aescattter.mp4') | ||
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def scatters(self, pl, radmarker, origin): | ||
scat = [] | ||
for key, value in self.clist.items(): | ||
idx = origin == key | ||
s = self.ax.scatter(pl[idx, 0], pl[idx, 1], marker='o', s=radmarker[idx], c=value, alpha=0.75, label=key) | ||
scat.append(s) | ||
return scat | ||
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def setup_plot(self): | ||
# First frame | ||
"""Initial drawing of the scatter plot.""" | ||
t, name, Gmass, radius, npl, pl, radmarker, origin = next(self.data_stream(0)) | ||
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# set up the figure | ||
self.ax.margins(x=10, y=1) | ||
self.ax.set_xlabel("Semimajor Axis (AU)", fontsize='16', labelpad=1) | ||
self.ax.set_ylabel("Eccentricity", fontsize='16', labelpad=1) | ||
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self.title = self.ax.text(0.50, 1.05, "", bbox={'facecolor': 'w', 'alpha': 0.5, 'pad': 5}, transform=self.ax.transAxes, | ||
ha="center") | ||
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self.title.set_text(f"{titletext} - Time = ${t*1e-6:6.2f}$ My with ${npl:4.0f}$ particles") | ||
slist = self.scatters(pl, radmarker, origin) | ||
self.s0 = slist[0] | ||
self.s1 = slist[1] | ||
self.s2 = slist[2] | ||
self.s3 = slist[3] | ||
leg = plt.legend(loc="upper right", scatterpoints=1, fontsize=10) | ||
for i,l in enumerate(leg.legendHandles): | ||
leg.legendHandles[i]._sizes = [20] | ||
return self.s0, self.s1, self.s2, self.s3, self.title | ||
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def data_stream(self, frame=0): | ||
while True: | ||
d = self.ds.isel(time = frame) | ||
name_good = d.name.where(d['status'] != 1, drop=True) | ||
name_good = name_good.where(name_good != "Sun", drop=True) | ||
d = d.sel(name=name_good) | ||
d['radmarker'] = (d['radius'] / self.Rcb) * radscale | ||
radius = d['radmarker'].values | ||
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radius = d['radmarker'].values | ||
Gmass = d['Gmass'].values | ||
a = d['a'].values | ||
e = d['e'].values | ||
name = d['name'].values | ||
npl = d['npl'].values | ||
radmarker = d['radmarker'] | ||
origin = d['origin_type'] | ||
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t = self.ds.coords['time'].values[frame] | ||
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yield t, name, Gmass, radius, npl, np.c_[a, e], radmarker, origin | ||
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def update(self,frame): | ||
"""Update the scatter plot.""" | ||
t, name, Gmass, radius, npl, pl, radmarker, origin = next(self.data_stream(framejump * frame)) | ||
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self.title.set_text(f"{titletext} - Time = ${t*1e-6:6.3f}$ My with ${npl:4.0f}$ particles") | ||
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# We need to return the updated artist for FuncAnimation to draw.. | ||
# Note that it expects a sequence of artists, thus the trailing comma. | ||
s = [self.s0, self.s1, self.s2, self.s3] | ||
for i, (key, value) in enumerate(self.clist.items()): | ||
idx = origin == key | ||
s[i].set_sizes(radmarker[idx]) | ||
s[i].set_offsets(pl[idx,:]) | ||
s[i].set_facecolor(value) | ||
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self.s0 = s[0] | ||
self.s1 = s[1] | ||
self.s2 = s[2] | ||
self.s3 = s[3] | ||
return self.s0, self.s1, self.s2, self.s3, self.title, | ||
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sim = swiftest.Simulation(simdir="fragglesim",read_old_output=True) | ||
print('Making animation') | ||
anim = AnimatedScatter(sim.data,sim.param) | ||
print('Animation finished') |
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#!/usr/bin/env python3 | ||
import swiftest | ||
import numpy as np | ||
from numpy.random import default_rng | ||
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# Initialize simulation object | ||
sim = swiftest.Simulation(simdir="fragglesim") | ||
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sim.set_parameter(compute_conservation_values=True, rotation=True, init_cond_format="EL",collision_model="fraggle",encounter_save="none") | ||
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# Add bodies described in Chambers (2013) Sec. 2.1, with the uniform spatial distribution and two bodies sizes (big and small) | ||
Nb = 14 | ||
Ns = 140 | ||
Mb = 2.8e-7 * 14 / Nb | ||
Ms = 2.8e-8 * 140 / Ns | ||
dens = 3000.0 / (sim.param['MU2KG'] / sim.param['DU2M']**3) | ||
Rb = (3 * Mb / (4 * np.pi * dens) )**(1.0 / 3.0) | ||
Rs = (3 * Ms / (4 * np.pi * dens) )**(1.0 / 3.0) | ||
mtiny = 1e-2 * Ms | ||
mininum_fragment_mass = 1e-4 * Ms | ||
rng = default_rng(seed=880334) | ||
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# Define the initial orbital elements of the big and small bodies | ||
avalb = rng.uniform(0.3, 2.0, Nb) | ||
avals = rng.uniform(0.3, 2.0, Ns) | ||
evalb = rng.uniform(0.0, 0.01, Nb) | ||
evals = rng.uniform(0.0, 0.01, Ns) | ||
incvalb = rng.uniform(0.0, 0.005 * 180 / np.pi, Nb) | ||
incvals = rng.uniform(0.0, 0.005 * 180 / np.pi, Ns) | ||
capomvalb = rng.uniform(0.0, 360.0, Nb) | ||
capomvals = rng.uniform(0.0, 360.0, Ns) | ||
omegavalb = rng.uniform(0.0, 360.0, Nb) | ||
omegavals = rng.uniform(0.0, 360.0, Ns) | ||
capmvalb = rng.uniform(0.0, 360.0, Nb) | ||
capmvals = rng.uniform(0.0, 360.0, Ns) | ||
Ipvalb = np.full((Nb,3), 0.4) | ||
Ipvals = np.full((Ns,3), 0.4) | ||
rotvalb = np.zeros_like(Ipvalb) | ||
rotvals = np.zeros_like(Ipvals) | ||
GMvalb = np.full(Nb, Mb * sim.GU) | ||
GMvals = np.full(Ns, Ms * sim.GU) | ||
Rvalb = np.full(Nb, Rb) | ||
Rvals = np.full(Ns, Rs) | ||
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# Give the bodies unique names | ||
nameb = [f"Big{i:03}" for i in range(Nb)] | ||
names = [f"Small{i:03}" for i in range(Ns)] | ||
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# Add the modern planets and the Sun using the JPL Horizons Database. | ||
sim.add_solar_system_body(["Sun","Jupiter","Saturn","Uranus","Neptune"]) | ||
sim.add_body(name=nameb, a=avalb, e=evalb, inc=incvalb, capom=capomvalb, omega=omegavalb, capm=capmvalb, Gmass=GMvalb, radius=Rvalb, rot=rotvalb, Ip=Ipvalb) | ||
sim.add_body(name=names, a=avals, e=evals, inc=incvals, capom=capomvals, omega=omegavals, capm=capmvals, Gmass=GMvals, radius=Rvals, rot=rotvals, Ip=Ipvals) | ||
sim.set_parameter(mtiny=mtiny, minimum_fragment_mass=mininum_fragment_mass) | ||
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sim.run(tstop=3e8, dt=6.0875/365.25, istep_out=60000, dump_cadence=1) | ||
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