def generate_windows(window="blackman"):
datapath_db = data_paths.DataPath()
# first generate a window for the full physical volume
filename = datapath_db.fetch('simideal_15hr_physical', intend_read=True,
pick='1')
print filename
pcube = algebra.make_vect(algebra.load(filename))
pwindow = algebra.make_vect(fftutil.window_nd(pcube.shape, name=window),
axis_names=('freq', 'ra', 'dec'))
pwindow.copy_axis_info(pcube)
print pwindow.shape
algebra.save("physical_window.npy", pwindow)
# now generate one for the observed region and project onto the physical
# volume.
filename = datapath_db.fetch('simideal_15hr_beam', intend_read=True,
pick='1')
print filename
ocube = algebra.make_vect(algebra.load(filename))
owindow = algebra.make_vect(fftutil.window_nd(ocube.shape, name=window),
axis_names=('freq', 'ra', 'dec'))
owindow.copy_axis_info(ocube)
print owindow.shape
print owindow.axes
algebra.save("observed_window.npy", owindow)
pwindow = physical_gridding.physical_grid(owindow, refinement=2)
print pwindow.shape
algebra.save("observed_window_physreg.npy", pwindow)
def cross_power_est_highmem(arr1, arr2, weight1, weight2,
window="blackman", nonorm=False):
"""Calculate the cross-power spectrum of a two nD fields.
The arrays must be identical and have the same length (physically
and in pixel number) along each axis.
Same goal as above without the emphasis on saving memory.
This is the "tried and true" legacy function.
"""
if window:
window_function = fftutil.window_nd(arr1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
warr1 = arr1 * weight1
warr2 = arr2 * weight2
ndim = arr1.ndim
fft_arr1 = np.fft.fftshift(np.fft.fftn(warr1))
fft_arr2 = np.fft.fftshift(np.fft.fftn(warr2))
xspec = fft_arr1 * fft_arr2.conj()
xspec = xspec.real
# correct for the weighting
product_weight = weight1 * weight2
xspec /= np.sum(product_weight)
# make the axes
k_axes = tuple(["k_" + axis_name for axis_name in arr1.axes])
xspec_arr = algebra.make_vect(xspec, axis_names=k_axes)
info = {'axes': k_axes, 'type': 'vect'}
width = np.zeros(ndim)
for axis_index in range(ndim):
n_axis = arr1.shape[axis_index]
axis_name = arr1.axes[axis_index]
axis_vector = arr1.get_axis(axis_name)
delta_axis = abs(axis_vector[1] - axis_vector[0])
width[axis_index] = delta_axis
k_axis = np.fft.fftshift(np.fft.fftfreq(n_axis, d=delta_axis))
k_axis *= 2. * math.pi
delta_k_axis = abs(k_axis[1] - k_axis[0])
k_name = k_axes[axis_index]
info[k_name + "_delta"] = delta_k_axis
info[k_name + "_centre"] = 0.
#print k_axis
#print k_name, n_axis, delta_axis
xspec_arr.info = info
#print xspec_arr.get_axis("k_dec")
if not nonorm:
xspec_arr *= width.prod()
return xspec_arr
def cross_power_est_highmem(arr1, arr2, weight1, weight2,
window="blackman", nonorm=False):
"""Calculate the cross-power spectrum of a two nD fields.
The arrays must be identical and have the same length (physically
and in pixel number) along each axis.
Same goal as above without the emphasis on saving memory.
This is the "tried and true" legacy function.
"""
if window:
window_function = fftutil.window_nd(arr1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
warr1 = arr1 * weight1
warr2 = arr2 * weight2
ndim = arr1.ndim
fft_arr1 = np.fft.fftshift(np.fft.fftn(warr1))
fft_arr2 = np.fft.fftshift(np.fft.fftn(warr2))
xspec = fft_arr1 * fft_arr2.conj()
xspec = xspec.real
# correct for the weighting
product_weight = weight1 * weight2
xspec /= np.sum(product_weight)
# make the axes
k_axes = tuple(["k_" + axis_name for axis_name in arr1.axes])
xspec_arr = algebra.make_vect(xspec, axis_names=k_axes)
info = {'axes': k_axes, 'type': 'vect'}
width = np.zeros(ndim)
for axis_index in range(ndim):
n_axis = arr1.shape[axis_index]
axis_name = arr1.axes[axis_index]
axis_vector = arr1.get_axis(axis_name)
delta_axis = abs(axis_vector[1] - axis_vector[0])
width[axis_index] = delta_axis
k_axis = np.fft.fftshift(np.fft.fftfreq(n_axis, d=delta_axis))
k_axis *= 2. * math.pi
delta_k_axis = abs(k_axis[1] - k_axis[0])
k_name = k_axes[axis_index]
info[k_name + "_delta"] = delta_k_axis
info[k_name + "_centre"] = 0.
#print k_axis
#print k_name, n_axis, delta_axis
xspec_arr.info = info
#print xspec_arr.get_axis("k_dec")
if not nonorm:
xspec_arr *= width.prod()
return xspec_arr
def estimate_ps_3d(self, window="blackman"):
window_function = fftutil.window_nd(self.nbox1.shape, name=window)
self.nbox1 *= window_function
self.nbox2 *= window_function
self.ibox1 *= self.nbox1
self.ibox2 *= self.nbox2
self.subtract_mean()
normal = (self.nbox1 * self.nbox2).flatten().sum()
delta_v = self.boxunit**3
iput_1 = np.zeros(self.boxshape, dtype=complex)
#oput_1 = np.zeros(self.boxshape, dtype=complex)
#plan_1 = FFTW.Plan(iput_1, oput_1, direction='forward', flags=['measure'])
iput_1.imag = 0.
iput_1.real = self.ibox1
#FFTW.execute(plan_1)
oput_1 = np.fft.fftn(iput_1)
iput_2 = np.zeros(self.boxshape, dtype=complex)
#oput_2 = np.zeros(self.boxshape, dtype=complex)
#plan_2 = FFTW.Plan(iput_2, oput_2, direction='forward', flags=['measure'])
iput_2.imag = 0.
iput_2.real = self.ibox2
#FFTW.execute(plan_2)
oput_2 = np.fft.fftn(iput_2)
oput_1 = np.fft.fftshift(oput_1)
oput_2 = np.fft.fftshift(oput_2)
self.ps_3d = (oput_1 * oput_2.conj()).real
self.ps_3d *= delta_v/normal
del iput_1
del iput_2
del oput_1
del oput_2
gc.collect()
def calculate_mixing(weight_file1, weight_file2, bins, xspec_fileout,
mixing_fileout,
unitless=False, refinement=2, pad=5, order=1,
window='blackman', zero_pad=False, identity_test=False):
print "loading the weights and converting to physical coordinates"
weight1_obs = algebra.make_vect(algebra.load(weight_file1))
weight1 = bh.repackage_kiyo(pg.physical_grid(
weight1_obs,
refinement=refinement,
pad=pad, order=order))
weight2_obs = algebra.make_vect(algebra.load(weight_file2))
weight2 = bh.repackage_kiyo(pg.physical_grid(
weight2_obs,
refinement=refinement,
pad=pad, order=order))
if window:
window_function = fftutil.window_nd(weight1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
print "calculating the cross-power of the spatial weighting functions"
arr1 = algebra.ones_like(weight1)
arr2 = algebra.ones_like(weight2)
# no window applied here (applied above)
xspec = pe.cross_power_est(weight1, weight2, arr1, arr2,
window=None, nonorm=True)
# for each point in the cube, find |k|, k_perp, k_parallel
# TODO: speed this up by using one direct numpy call (not limiting)
k_mag_arr = binning.radius_array(xspec)
k_perp_arr = binning.radius_array(xspec, zero_axes=[0])
k_parallel_arr = binning.radius_array(xspec, zero_axes=[1, 2])
if unitless:
xspec = pe.make_unitless(xspec, radius_arr=k_mag_arr)
# NOTE: assuming lowest k bin has only one point in 3D k-space
# could make this floor of dimensions divided by 2 also
center_3d = np.transpose(np.transpose(np.where(k_mag_arr == 0.))[0])
# In the estimator, we devide by 1/sum(w1 * w2) to get most of the effect
# of the weighing. The mixing matrix here can be thought of as a correction
# that that diagonal-only estimate.
leakage_ratio = xspec[center_3d[0], center_3d[1], center_3d[2]] / \
np.sum(weight1 * weight2)
print "power leakage ratio: %10.5g" % leakage_ratio
xspec /= np.sum(weight1 * weight2)
print "partitioning the 3D kspace up into the 2D k bins"
(kflat, ret_indices) = bin_indices_2d(k_perp_arr, k_parallel_arr,
bins, bins)
# perform a test where the window function is a delta function at the
# origin so that the mixing matrix is identity
if identity_test:
xspec = algebra.zeros_like(xspec)
xspec[center_3d[0], center_3d[1], center_3d[2]] = 1.
# now save the window cross-power for downstream pooled users
algebra.save(xspec_fileout, xspec)
runlist = []
for bin_index in range(kflat.shape[0]):
bin_3d = ret_indices[repr(bin_index)]
if bin_3d is not None:
runlist.append((xspec_fileout, bin_index, bins, bin_3d, center_3d))
pool = multiprocessing.Pool(processes=(multiprocessing.cpu_count() - 4))
# the longest runs get pushed to the end; randomize for better job packing
random.shuffle(runlist)
results = pool.map(sum_window, runlist)
#gnuplot_single_slice(runlist[0]) # for troubleshooting
# now save the results for post-processing
params = {"unitless": unitless, "refinement": refinement, "pad": pad,
"order": order, "window": window, "zero_pad": zero_pad,
"identity_test": identity_test, "weight_file1": weight_file1,
"weight_file2": weight_file2, "bins": bins}
outshelve = shelve.open(mixing_fileout, "n")
outshelve["params"] = params # parameters for this run
outshelve["weight1"] = weight1 # weight map 1
outshelve["weight2"] = weight2 # weight map 2
outshelve["xspec"] = xspec # copy of the weight spectra
outshelve["kflat"] = kflat # 2D k bin vector
outshelve["bins_3d"] = ret_indices # indices to k3d for a 2d k bin
outshelve["results"] = results # mixing matrix columns
outshelve.close()
def cross_power_est(arr1, arr2, weight1, weight2, window="blackman"):
"""Calculate the radially average cross-power spectrum of a two nD fields.
The arrays must be identical and have the same length (physically
and in pixel number) along each axis.
Parameters
----------
arr1, arr2: np.ndarray
The cubes to calculate the cross-power spectrum of. If arr2 is
None then return the standard (auto-)power spectrum.
window: boolean
Apply an additional named window
"""
if window:
window_function = fftutil.window_nd(arr1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
warr1 = arr1 * weight1
warr2 = arr2 * weight2
ndim = arr1.ndim
fft_arr1 = np.fft.fftshift(np.fft.fftn(warr1))
fft_arr2 = np.fft.fftshift(np.fft.fftn(warr2))
xspec = fft_arr1 * fft_arr2.conj()
xspec = xspec.real
# correct for the weighting
product_weight = weight1 * weight2
xspec /= np.sum(product_weight)
# make the axes
k_axes = tuple(["k_" + axis_name for axis_name in arr1.axes])
xspec_arr = algebra.make_vect(xspec, axis_names=k_axes)
info = {'axes': k_axes, 'type': 'vect'}
width = np.zeros(ndim)
for axis_index in range(ndim):
n_axis = arr1.shape[axis_index]
axis_name = arr1.axes[axis_index]
axis_vector = arr1.get_axis(axis_name)
delta_axis = abs(axis_vector[1] - axis_vector[0])
width[axis_index] = delta_axis
k_axis = np.fft.fftshift(np.fft.fftfreq(n_axis, d=delta_axis))
k_axis *= 2. * math.pi
delta_k_axis = abs(k_axis[1] - k_axis[0])
k_name = k_axes[axis_index]
info[k_name + "_delta"] = delta_k_axis
info[k_name + "_centre"] = 0.
#print k_axis
#print k_name, n_axis, delta_axis
xspec_arr.info = info
#print xspec_arr.get_axis("k_dec")
xspec_arr *= width.prod()
return xspec_arr
def calculate_mixing(weight_file1,
weight_file2,
bins,
xspec_fileout,
mixing_fileout,
unitless=False,
refinement=2,
pad=5,
order=1,
window='blackman',
zero_pad=False,
identity_test=False):
print "loading the weights and converting to physical coordinates"
weight1_obs = algebra.make_vect(algebra.load(weight_file1))
weight1 = bh.repackage_kiyo(
pg.physical_grid(weight1_obs,
refinement=refinement,
pad=pad,
order=order))
weight2_obs = algebra.make_vect(algebra.load(weight_file2))
weight2 = bh.repackage_kiyo(
pg.physical_grid(weight2_obs,
refinement=refinement,
pad=pad,
order=order))
if window:
window_function = fftutil.window_nd(weight1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
print "calculating the cross-power of the spatial weighting functions"
arr1 = algebra.ones_like(weight1)
arr2 = algebra.ones_like(weight2)
# no window applied here (applied above)
xspec = pe.cross_power_est(weight1,
weight2,
arr1,
arr2,
window=None,
nonorm=True)
# for each point in the cube, find |k|, k_perp, k_parallel
# TODO: speed this up by using one direct numpy call (not limiting)
k_mag_arr = binning.radius_array(xspec)
k_perp_arr = binning.radius_array(xspec, zero_axes=[0])
k_parallel_arr = binning.radius_array(xspec, zero_axes=[1, 2])
if unitless:
xspec = pe.make_unitless(xspec, radius_arr=k_mag_arr)
# NOTE: assuming lowest k bin has only one point in 3D k-space
# could make this floor of dimensions divided by 2 also
center_3d = np.transpose(np.transpose(np.where(k_mag_arr == 0.))[0])
# In the estimator, we devide by 1/sum(w1 * w2) to get most of the effect
# of the weighing. The mixing matrix here can be thought of as a correction
# that that diagonal-only estimate.
leakage_ratio = xspec[center_3d[0], center_3d[1], center_3d[2]] / \
np.sum(weight1 * weight2)
print "power leakage ratio: %10.5g" % leakage_ratio
xspec /= np.sum(weight1 * weight2)
print "partitioning the 3D kspace up into the 2D k bins"
(kflat, ret_indices) = bin_indices_2d(k_perp_arr, k_parallel_arr, bins,
bins)
# perform a test where the window function is a delta function at the
# origin so that the mixing matrix is identity
if identity_test:
xspec = algebra.zeros_like(xspec)
xspec[center_3d[0], center_3d[1], center_3d[2]] = 1.
# now save the window cross-power for downstream pooled users
algebra.save(xspec_fileout, xspec)
runlist = []
for bin_index in range(kflat.shape[0]):
bin_3d = ret_indices[repr(bin_index)]
if bin_3d is not None:
runlist.append((xspec_fileout, bin_index, bins, bin_3d, center_3d))
pool = multiprocessing.Pool(processes=(multiprocessing.cpu_count() - 4))
# the longest runs get pushed to the end; randomize for better job packing
random.shuffle(runlist)
results = pool.map(sum_window, runlist)
#gnuplot_single_slice(runlist[0]) # for troubleshooting
# now save the results for post-processing
params = {
"unitless": unitless,
"refinement": refinement,
"pad": pad,
"order": order,
"window": window,
"zero_pad": zero_pad,
"identity_test": identity_test,
"weight_file1": weight_file1,
"weight_file2": weight_file2,
"bins": bins
}
outshelve = shelve.open(mixing_fileout, "n")
outshelve["params"] = params # parameters for this run
outshelve["weight1"] = weight1 # weight map 1
outshelve["weight2"] = weight2 # weight map 2
outshelve["xspec"] = xspec # copy of the weight spectra
outshelve["kflat"] = kflat # 2D k bin vector
outshelve["bins_3d"] = ret_indices # indices to k3d for a 2d k bin
outshelve["results"] = results # mixing matrix columns
outshelve.close()
def cross_power_est(arr1, arr2, weight1, weight2, window="blackman"):
"""Calculate the radially average cross-power spectrum of a two nD fields.
The arrays must be identical and have the same length (physically
and in pixel number) along each axis.
Parameters
----------
arr1, arr2: np.ndarray
The cubes to calculate the cross-power spectrum of. If arr2 is
None then return the standard (auto-)power spectrum.
window: boolean
Apply an additional named window
"""
if window:
window_function = fftutil.window_nd(arr1.shape, name=window)
weight1 *= window_function
weight2 *= window_function
warr1 = arr1 * weight1
warr2 = arr2 * weight2
ndim = arr1.ndim
fft_arr1 = np.fft.fftshift(np.fft.fftn(warr1))
fft_arr2 = np.fft.fftshift(np.fft.fftn(warr2))
xspec = fft_arr1 * fft_arr2.conj()
xspec = xspec.real
# correct for the weighting
product_weight = weight1 * weight2
xspec /= np.sum(product_weight)
# make the axes
k_axes = tuple(["k_" + axis_name for axis_name in arr1.axes])
xspec_arr = algebra.make_vect(xspec, axis_names=k_axes)
info = {'axes': k_axes, 'type': 'vect'}
width = np.zeros(ndim)
for axis_index in range(ndim):
n_axis = arr1.shape[axis_index]
axis_name = arr1.axes[axis_index]
axis_vector = arr1.get_axis(axis_name)
delta_axis = abs(axis_vector[1] - axis_vector[0])
width[axis_index] = delta_axis
k_axis = np.fft.fftshift(np.fft.fftfreq(n_axis, d=delta_axis))
k_axis *= 2. * math.pi
delta_k_axis = abs(k_axis[1] - k_axis[0])
k_name = k_axes[axis_index]
info[k_name + "_delta"] = delta_k_axis
info[k_name + "_centre"] = 0.
#print k_axis
#print k_name, n_axis, delta_axis
xspec_arr.info = info
#print xspec_arr.get_axis("k_dec")
xspec_arr *= width.prod()
return xspec_arr
