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make_snapshot.py
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make_snapshot.py
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# -*- coding: utf-8 -*-
"""
Created on Fri Mar 21 15:11:31 2014
@author: ibackus
"""
__version__ = "$Revision: 1 $"
# $Source$
import pynbody
SimArray = pynbody.array.SimArray
import numpy as np
import gc
import os
import isaac
import calc_velocity
import ICgen_utils
import ICglobal_settings
global_settings = ICglobal_settings.global_settings
def snapshot_gen(ICobj):
"""
Generates a tipsy snapshot from the initial conditions object ICobj.
Returns snapshot, param
snapshot: tipsy snapshot
param: dictionary containing info for a .param file
"""
print 'Generating snapshot...'
# Constants
G = SimArray(1.0,'G')
# ------------------------------------
# Load in things from ICobj
# ------------------------------------
print 'Accessing data from ICs'
settings = ICobj.settings
# filenames
snapshotName = settings.filenames.snapshotName
paramName = settings.filenames.paramName
# particle positions
r = ICobj.pos.r
xyz = ICobj.pos.xyz
# Number of particles
nParticles = ICobj.pos.nParticles
# molecular mass
m = settings.physical.m
# star mass
m_star = settings.physical.M.copy()
# disk mass
m_disk = ICobj.sigma.m_disk.copy()
m_disk = isaac.match_units(m_disk, m_star)[0]
# mass of the gas particles
m_particles = m_disk / float(nParticles)
# re-scale the particles (allows making of lo-mass disk)
m_particles *= settings.snapshot.mScale
# -------------------------------------------------
# Assign output
# -------------------------------------------------
print 'Assigning data to snapshot'
# Get units all set up
m_unit = m_star.units
pos_unit = r.units
if xyz.units != r.units:
xyz.convert_units(pos_unit)
# time units are sqrt(L^3/GM)
t_unit = np.sqrt((pos_unit**3)*np.power((G*m_unit), -1)).units
# velocity units are L/t
v_unit = (pos_unit/t_unit).ratio('km s**-1')
# Make it a unit
v_unit = pynbody.units.Unit('{0} km s**-1'.format(v_unit))
# Other settings
metals = settings.snapshot.metals
star_metals = metals
# -------------------------------------------------
# Initialize snapshot
# -------------------------------------------------
# Note that empty pos, vel, and mass arrays are created in the snapshot
snapshot = pynbody.new(star=1,gas=nParticles)
snapshot['vel'].units = v_unit
snapshot['eps'] = 0.01*SimArray(np.ones(nParticles+1, dtype=np.float32), pos_unit)
snapshot['metals'] = SimArray(np.zeros(nParticles+1, dtype=np.float32))
snapshot['rho'] = SimArray(np.zeros(nParticles+1, dtype=np.float32))
snapshot.gas['pos'] = xyz
snapshot.gas['temp'] = ICobj.T(r)
snapshot.gas['mass'] = m_particles
snapshot.gas['metals'] = metals
snapshot.star['pos'] = SimArray([[ 0., 0., 0.]],pos_unit)
snapshot.star['vel'] = SimArray([[ 0., 0., 0.]], v_unit)
snapshot.star['mass'] = m_star
snapshot.star['metals'] = SimArray(star_metals)
# Estimate the star's softening length as the closest particle distance
snapshot.star['eps'] = r.min()
# Make param file
param = isaac.make_param(snapshot, snapshotName)
param['dMeanMolWeight'] = m
eos = (settings.physical.eos).lower()
if eos == 'adiabatic':
param['bGasAdiabatic'] = 1
param['bGasIsothermal'] = 0
param['dConstGamma']
gc.collect()
# -------------------------------------------------
# CALCULATE VELOCITY USING calc_velocity.py. This also estimates the
# gravitational softening length eps
# -------------------------------------------------
print 'Calculating circular velocity'
preset = settings.changa_run.preset
max_particles = global_settings['misc']['max_particles']
calc_velocity.v_xy(snapshot, param, changa_preset=preset, max_particles=max_particles)
gc.collect()
# -------------------------------------------------
# Estimate time step for changa to use
# -------------------------------------------------
# Save param file
isaac.configsave(param, paramName, 'param')
# Save snapshot
snapshot.write(filename=snapshotName, fmt=pynbody.tipsy.TipsySnap)
# est dDelta
dDelta = ICgen_utils.est_time_step(paramName, preset)
param['dDelta'] = dDelta
# -------------------------------------------------
# Create director file
# -------------------------------------------------
# largest radius to plot
r_director = float(0.9 * r.max())
# Maximum surface density
sigma_min = float(ICobj.sigma(r_director))
# surface density at largest radius
sigma_max = float(ICobj.sigma.input_dict['sigma'].max())
# Create director dict
director = isaac.make_director(sigma_min, sigma_max, r_director, filename=param['achOutName'])
## Save .director file
#isaac.configsave(director, directorName, 'director')
# -------------------------------------------------
# Wrap up
# -------------------------------------------------
print 'Wrapping up'
# Now set the star particle's tform to a negative number. This allows
# UW ChaNGa treat it as a sink particle.
snapshot.star['tform'] = -1.0
# Update params
r_sink = isaac.strip_units(r.min())
param['dSinkBoundOrbitRadius'] = r_sink
param['dSinkRadius'] = r_sink
param['dSinkMassMin'] = 0.9 * isaac.strip_units(m_star)
param['bDoSinks'] = 1
return snapshot, param, director