コード例 #1
0
def project(snapshot, scale, view, **kwargs):
    pps = kwargs.pop('pps', 500)
    sm = kwargs.pop('sm', 1.7)
    shiftx = kwargs.pop('shiftx', None)
    shifty = kwargs.pop('shifty', None)
    shiftz = kwargs.pop('shiftz', None)
    dens_lim = kwargs.pop('dens_lim', None)
    boxsize = float("".join(ch if ch.isdigit() else "" for ch in scale))
    unit = "".join(ch if not ch.isdigit() else "" for ch in scale)
    dens = snapshot.gas.get_number_density()
    xyz = snapshot.gas.get_coords(unit)
    uvw = snapshot.gas.get_velocities()
    hsml = snapshot.gas.get_smoothing_length(unit)

    print 'Calculating...'
    xyz = analyze.center_box(xyz, velocity=uvw, density=dens, **kwargs)
    xyz = set_view(view, xyz)
    x = xyz.x
    y = xyz.y
    z = xyz.z
    if shiftx:
        x += shiftx
    if shifty:
        y += shifty
    if shiftz:
        z += shiftz
    snapshot.update_sink_coordinates(x, y, z)
    # Artificially shrink sink smoothing lengths.
    for s in snapshot.sinks:
        hsml[s.index] *= .5
    data = snap.gas['x', 'y', 'z', 'ndensity',
                    'smoothing_length'].copy(deep=True)
    data = trim_view(boxsize, data, **kwargs)
    if dens_lim:
        arrs = [scalar, x, y, z, hsml]
        scalar, x, y, z, hsml = analyze.data_slice(scalar > dens_lim, *arrs)
    hsml = numpy.fmax(sm * hsml, boxsize / pps / 2)
    xi, yi = build_grid(boxsize, pps)
    zi = scalar_map(x, y, scalar, hsml, boxsize, pps, xi.shape)
    print '%s:: min: %.3e max: %.3e' % (loadable, zi.min(), zi.max())
    imscale = kwargs.pop('imscale', 'log')
    if imscale == 'log':
        zi = numpy.log10(zi)
        print 'log(%s):: min: %.3e max: %.3e' % (loadable, zi.min(), zi.max())
    else:
        print 'Returning raw (non-log) values!'
    return xi, yi, zi
コード例 #2
0
ファイル: visualize.py プロジェクト: astrosmith/pyGadget
def project(snapshot, scale, view, **kwargs):
    pps = kwargs.pop('pps',500)
    sm = kwargs.pop('sm',1.7)
    shiftx = kwargs.pop('shiftx',None)
    shifty = kwargs.pop('shifty',None)
    shiftz = kwargs.pop('shiftz',None)
    dens_lim = kwargs.pop('dens_lim', None)
    boxsize = float("".join(ch if ch.isdigit() else "" for ch in scale))
    unit = "".join(ch if not ch.isdigit() else "" for ch in scale)
    dens = snapshot.gas.get_number_density()
    xyz = snapshot.gas.get_coords(unit)
    uvw = snapshot.gas.get_velocities()
    hsml = snapshot.gas.get_smoothing_length(unit)

    print 'Calculating...'
    xyz = analyze.center_box(xyz, velocity=uvw, density=dens, **kwargs)
    xyz = set_view(view, xyz)
    x = xyz.x
    y = xyz.y
    z = xyz.z
    if shiftx:
        x += shiftx
    if shifty:
        y += shifty
    if shiftz:
        z += shiftz
    snapshot.update_sink_coordinates(x,y,z)
    # Artificially shrink sink smoothing lengths.
    for s in snapshot.sinks:
        hsml[s.index] *= .5
    data = snap.gas['x', 'y', 'z', 'ndensity', 'smoothing_length'].copy(deep=True)
    data = trim_view(boxsize, data, **kwargs)
    if dens_lim:
        arrs = [scalar,x,y,z,hsml]
        scalar,x,y,z,hsml = analyze.data_slice(scalar > dens_lim, *arrs)
    hsml = numpy.fmax(sm * hsml, boxsize/pps/2)
    xi,yi = build_grid(boxsize,pps)
    zi = scalar_map(x,y,scalar,hsml,boxsize,pps,xi.shape)
    print '%s:: min: %.3e max: %.3e' %(loadable, zi.min(),zi.max())
    imscale = kwargs.pop('imscale','log')
    if imscale == 'log':
        zi = numpy.log10(zi)
        print 'log(%s):: min: %.3e max: %.3e' %(loadable, zi.min(),zi.max())
    else:
        print 'Returning raw (non-log) values!'
    return xi,yi,zi
コード例 #3
0
ファイル: sink.py プロジェクト: astrosmith/pyGadget
def disk_properties(snapshot, sink_id, **kwargs):
    r_start = kwargs.pop('r_start', 50*1.49597871e13)
    r_step = kwargs.pop('r_step', 1.49597871e14)
    r_multiplier = kwargs.pop('multiplier', 1.2)
    verbose = kwargs.pop('verbose', True)
    n_min = kwargs.pop('n_min', 32)
    dens_lim = kwargs.pop('dens_lim', 1e6)
    orb_crit = kwargs.pop('orb_crit', 1.)
    disky_crit = kwargs.pop('disky_crit', .9)
    kepler_crit = kwargs.pop('kepler_crit', .8)

    redshift = snapshot.header.Redshift
    length_unit = 'cm'
    mass_unit = 'g'
    velocity_unit = 'cgs'
    snapshot.gas.units.set_velocity(velocity_unit)
    xyz = snapshot.gas.get_coords(length_unit)
    uvw = snapshot.gas.get_velocities()
    snapshot.update_sink_frame_ofR(xyz, uvw)

    dens = snapshot.gas.get_number_density('cgs')
    mass = snapshot.gas.get_masses(mass_unit)
    temp = snapshot.gas.get_temperature()
    csound = snapshot.gas.get_sound_speed()

    i = 0
    try:
        while snapshot.sinks[i].pid != sink_id:
            i += 1
    except IndexError:
        raise IndexError("Sink {} has not yet formed!".format(sink_id))
    else:
        sink = snapshot.sinks[i]
        sinkpos = (sink.x, sink.y, sink.z)
        sinkvel = (sink.vx, sink.vy, sink.vz)
        pos = snapshot.gas.get_coords(system='spherical',view='face',
                                      center=sinkpos, vcenter=sinkvel)
    vel = snapshot.gas.get_velocities(system='spherical')
    xyz = snapshot.gas.get_coords()
    uvw = snapshot.gas.get_velocities()
    snapshot.update_sink_frame_ofR(xyz, uvw)
    pos = numpy.nan_to_num(pos)
    vel = numpy.nan_to_num(vel)

    L9 = analyze.total_angular_momentum(*analyze.data_slice(dens > 1e9,
                                                            xyz,uvw,mass))
    uL9 = L9 / numpy.linalg.norm(L9)

    if dens_lim:
        arrs = [dens,pos,vel,xyz,uvw,mass,temp,csound]
        dslice = dens > dens_lim
        dens,pos,vel,xyz,uvw,mass,temp,csound = analyze.data_slice(dslice,
                                                                    *arrs)
    L = analyze.angular_momentum(xyz,uvw,mass)
    uL = L / numpy.linalg.norm(L, axis=1)[:, numpy.newaxis]
    disky = numpy.where((numpy.abs(vel[:,2])/numpy.abs(vel[:,0]) > orb_crit)
                    & (uL.dot(uL9) > disky_crit))[0]
    print disky.size, '"disky" particles',
    print '({}) percent'.format(float(disky.size)/dens.size * 100)

    inf = numpy.where(numpy.abs(vel[:,0])
                      / numpy.linalg.norm(vel, axis=1) > .5)[0]
    print inf.size, 'infalling particles',
    print '({}) percent'.format(float(inf.size)/dens.size * 100)

    orb = numpy.where((numpy.abs(vel[:,2])/numpy.abs(vel[:,0]) > orb_crit)
                   & (uL.dot(uL9) < disky_crit))[0]
    print orb.size, '"orbiting" particles',
    print '({}) percent'.format(float(orb.size)/dens.size * 100)

    notorb = numpy.where(numpy.abs(vel[:,2]) < numpy.abs(vel[:,0]))[0]
    print notorb.size, '"not orbiting" particles',
    print '({}) percent'.format(float(notorb.size)/dens.size * 100)

    print 'Data loaded.  Analyzing...'
    disk_properties = []
    vrot = vk = 1.
    n = old_n = r0 = 0
    r1 = r_start
    print "Starting at {:.2e} AU".format(r1/1.49e13)
    r2d = numpy.sqrt(xyz[:,0]**2 + xyz[:,1]**2)
    data = []
    while vrot/vk > kepler_crit  and n < disky.size:
        inR = numpy.where(pos[disky,0] <= r1)[0]
        n = inR.size
        if n > old_n and n > n_min:
            annulus = numpy.where((r2d[disky] > r0) & (r2d[disky] <= r1))[0]
            annulus = disky[annulus]
            radii = r2d[annulus]
            radius = radii.mean()
            vrot = vel[annulus, 2].mean()
            T = analyze.reject_outliers(temp[annulus]).mean()
            cs = analyze.reject_outliers(csound[annulus]).mean()
            H = cs * radius / vrot
            Mcyl = mass[annulus].sum()
            if annulus.size > 0:
                zmax = numpy.abs(xyz[annulus,2]).max()
            else:
                zmax = 0.0
            density = dens[annulus].mean()
            if numpy.isnan(density):
                density = dens.max()
            mdensity = density * constants.m_H / constants.X_h
            tff = numpy.sqrt(3 * numpy.pi / 32 / constants.GRAVITY / mdensity)

            tavg = analyze.reject_outliers(temp[inR]).mean()
            Mtot = mass[numpy.where(pos[:,0] <= radius)[0]].sum()
            vk = numpy.sqrt(6.6726e-8 * Mtot / radius) / 1e5

            Lj = cs*tff #Jeans Length
            Mj = mdensity * (4*numpy.pi/3) * Lj**3 / 1.989e33 #Jeans Mass
            H = cs * radius / vrot #Disk Scale Height

            rau = radius/1.49597871e13
            Msun = Mtot/1.989e33
            vrot = vrot / 1e5
            disk_properties.append((redshift,rau,density,Msun,Mcyl,
                                    vrot,vk,tff,T,tavg,cs,H,Lj,Mj,n))
            if verbose:
                print 'R = %.2e AU' %rau,
                print 'Mass enclosed: %.2e' %Msun,
                print 'density: %.3e' %density,
                print 'vrot: %.3e' %vrot,
                print 'npart: {}'.format(n)
        old_n = n
        r0 = r1
        r1 *= r_multiplier
    print 'snapshot', snapshot.number, 'analyzed.'
    return disk_properties