Created
July 11, 2016 13:27
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Astrochem issue #53
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[files] | |
source = source.mdl | |
chem = osu2009.chm | |
# Physical paramaters | |
[phys] | |
chi = 1.0 | |
cosmic = 1e-15 | |
# Solver parameters | |
[solver] | |
ti = 1e-6 | |
tf = 1e7 | |
# Initial abundances | |
[abundances] | |
H2 = 0.5 | |
He = 0.14 | |
N = 2.14e-5 | |
O = 1.76e-4 | |
C(+) = 7.30e-5 | |
S(+) = 8.00e-8 | |
Si(+) = 8.00e-9 | |
Fe(+) = 3.00e-9 | |
Na(+) = 2.00e-9 | |
Mg(+) = 7.00e-9 | |
P(+) = 2.00e-10 | |
Cl(+) = 1.00e-9 | |
F = 6.68e-9 | |
e(-) = 7.31012e-5 | |
# Output | |
[output] | |
abundances = CO,HCO(+) |
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from astrochem import tools | |
from astrochem.wrapper import * | |
import numpy as np | |
import matplotlib.pyplot as plt | |
# Read the abundances computed by the command line version | |
time_co, abun_co_cl = tools.readabun("astrochem_output.h5", 'CO') | |
time_hcop, abun_hcop_cl = tools.readabun("astrochem_output.h5", 'HCO(+)') | |
# Compute the abundances with the Python version | |
p = phys() | |
p.chi = 1.0 | |
p.cosmic = 1e-15 | |
initial_abundances = { | |
"H2": 0.5, | |
"He": 0.14, | |
"N": 2.14e-5, | |
"O": 1.76e-4, | |
"C(+)": 7.30e-5, | |
"S(+)": 8.00e-8, | |
"Si(+)": 8.00e-9, | |
"Fe(+)": 3.00e-9, | |
"Na(+)": 2.00e-9, | |
"Mg(+)": 7.00e-9, | |
"P(+)": 2.00e-10, | |
"Cl(+)": 1.00e-9, | |
"F": 6.68e-9, | |
"e(-)": 7.31012e-5 | |
} | |
c = cell(av=20, nh=1e4, tgas=10, tdust=10) | |
s = solver(c, "osu2009.chm", p, 1e-15, 1e-6, initial_abundances, 1e4, 0.) | |
abun_co = [] | |
abun_hcop = [] | |
for ti in time_co: # use the same time values than for the CL version | |
abundances = s.solve(ti*365*24*3600, c) # time should be given in years !!!! | |
abun_co.append(abundances['CO']*.9) | |
abun_hcop.append(abundances['HCO(+)']) | |
# Plot the results | |
plt.xlabel("Time (years)") | |
plt.ylabel("Abundances") | |
plt.title("CO abundance") | |
plt.yscale('log') | |
plt.xscale('log') | |
plt.xlim([1e-6, 1e7]) | |
plt.ylim([1e-15, 1e-4]) | |
plt.plot(time_co, abun_co_cl, label="Command line") | |
plt.plot(time_co, abun_co, label="Python interface") | |
plt.legend() | |
fig = plt.gcf() | |
plt.show() |
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# Source model file example | |
# shell number, Av [mag], nH [cm^-3], Tgas [K], Tdust [K] | |
# | |
0 20.0 1e+04 10.0 10.0 |
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