def momenta(self,chanrange=None,p=1):
"""abs(intensity)-weighted moment
Does somewhat better than signed intensity-weighted moment.
Parameters
----------
chanrange: range of channels over which to compute moment
[startchan, endchan]
p: the moment to compute (the power of the frequency in the sum)
Returns:
The computed moment
"""
# get the masked array
s = self.spec()
chupper = len(s)-1
chanrange = self._sanitizechanrange(chanrange,chupper)
sum_s = ma.sum(ma.abs(s[chanrange[0]:chanrange[1]+1]))
sum_sf = 0
mean = 0
if p > 1:
mean = self.moment(chanrange,p-1)
for i in range(chanrange[0],chanrange[1]+1):
sum_sf += ma.abs(s[i])*math.pow((self._freq[i]-mean),p)
return sum_sf/sum_s
def combine_nights(combined_catalog, filterlist, refcat):
header = [
'BEGIN CATALOG HEADER', 'nfields 13', ' ra 1 0 d degrees %10.6f',
' dec 2 0 d degrees %10.6f', ' id 3 0 c INDEF %3d'
]
for filt in filterlist:
header.append(' {} {:2d} 0 r INDEF %6.3f'.format(
filt,
len(header) - 1))
header.append(' {}err {:2d} 0 r INDEF %6.3f'.format(
filt,
len(header) - 1))
header += ['END CATALOG HEADER', '']
catalog = Table([refcat['ra'], refcat['dec'], refcat['id']],
meta={'comments': header},
masked=True)
for filt in filterlist:
mags = combined_catalog['mag'][combined_catalog['filter'] == filt]
median = np.median(mags, axis=0)
absdev_mag = mags - median
mad = np.median(np.abs(absdev_mag), axis=0) * np.sqrt(pi / 2)
mags.mask |= np.abs(absdev_mag) > 5 * mad
catalog[filt] = np.median(mags, axis=0)
catalog[filt + 'err'] = np.median(np.abs(mags - catalog[filt]),
axis=0) * np.sqrt(pi / 2)
return catalog
def momenta(self,chanrange=None,p=1):
"""abs(intensity)-weighted moment
Does somewhat better than signed intensity-weighted moment.
Parameters
----------
chanrange: range of channels over which to compute moment
[startchan, endchan]
p: the moment to compute (the power of the frequency in the sum)
Returns:
The computed moment
"""
# get the masked array
s = self.spec()
chupper = len(s)-1
chanrange = self._sanitizechanrange(chanrange,chupper)
sum_s = ma.sum(ma.abs(s[chanrange[0]:chanrange[1]+1]))
sum_sf = 0
mean = 0
if p > 1:
mean = self.moment(chanrange,p-1)
for i in range(chanrange[0],chanrange[1]+1):
sum_sf += ma.abs(s[i])*math.pow((self._freq[i]-mean),p)
return sum_sf/sum_s
def find_lines(peaks, fwhm, y=None, verbose=False):
if y is None:
y = np.arange(len(peaks))
# Делаем все строки одинаковой длины (по наидленнейшей)
peaks = np.array(list(zip_longest(*peaks)), dtype='float')
# if verbose:
# plt.plot(peaks.T, y, 'o')
# plt.show()
msk = np.isnan(peaks)
peaks = ma.array(peaks, mask=msk)
col = ['C' + str(j) for j in range(9)]
# print(len(peaks))
# print()
for i in range(len(peaks)):
f**k = peaks[i:]
line = f**k[0]
# msk = np.logical_not(np.isnan(line))
# k = ma.polyfit(y, line, 2)
# print(k)
est = np.ones(len(y)) * ma.median(line)
# est = np.polyval(k, y)
err = est - line
move_right = ma.filled((err > 5 * ma.median(ma.abs(err))), False)
move_left = ma.filled((err < -5 * ma.median(ma.abs(err))), False)
not_move = np.logical_not(move_right + move_left)
# plt.plot(y[not_move], f**k[0][not_move], '.' + col[i % 9])
# plt.plot(y, est, col[i % 9], ls='--')
# plt.plot(y[move_right], f**k[0][move_right], 'x' + col[i % 9])
# plt.plot(y[move_left], f**k[0][move_left], '+' + col[i % 9])
# plt.show()
# print(i)
# print(ma.mean(ma.abs(err)))
# print(ma.median(line))
# print()
if np.sum(move_right) > 0: # Те, что меньше медианы (слева)
nonearray = ma.array([[None] * np.sum(move_right.astype('int'))], mask=[[True] * np.sum(move_right.astype('int'))])
f**k[:, move_right] = ma.append(f**k[:, move_right][1:, :], nonearray, axis=0)
if np.sum(move_left) > 0:
nonearray = ma.array([[None] * np.sum(move_left.astype('int'))], mask=[[True] * np.sum(move_left.astype('int'))])
f**k[:, move_left] = ma.append(nonearray, f**k[:, move_left][:-1, :], axis=0)
# plt.plot(f**k[0], col[i%9])
peaks[i:] = f**k
plt.show()
peaks = peaks.T
msk = np.isnan(peaks)
peaks = ma.array(peaks, mask=msk)
good_lines = (np.sum(np.logical_not(msk), axis=0) > len(y) / 4.)
peaks = peaks[:, good_lines]
return peaks
def fitBearingDrift(self, trajectory, windowSize=None, plotFit=False):
lags = np.linspace(0, np.round(50. * trajectory.frameRate), 200)
tau = lags / trajectory.frameRate
if windowSize is None:
psi = unwrapma(trajectory.getMaskedPosture(trajectory.psi))
D = drift(psi, lags, trajectory.excluded)
sel = ~ma.getmaskarray(psi)
#p = np.polyfit(tau, D, 1)
p = np.polyfit(trajectory.t[sel], psi[sel], 1)
self.k_psi = p[0]
else:
def result(traj):
psi = traj.getMaskedPosture(traj.psi)
if float(len(psi.compressed())) / float(len(psi)) > 0.2:
psi = unwrapma(psi)
D = drift(psi, lags, traj.excluded)
sel = ~ma.getmaskarray(psi)
p = np.polyfit(traj.t[sel], psi[sel], 1)
return D, p[0]
else:
return ma.zeros((len(lags), )) * ma.masked, ma.masked
results = [
result(traj) for traj in trajectory.asWindows(windowSize)
]
D = ma.array([resulti[0] for resulti in results])
k = ma.array([resulti[1] for resulti in results])
self.k_psi = ma.abs(k).mean()
D = ma.abs(D).T.mean(axis=1)
if plotFit:
plt.plot(tau, D, 'k.')
plt.plot(tau, self.k_psi * tau, 'r-')
plt.xlabel(r'$\tau$ (s)')
plt.ylabel(r'$\langle |\psi(\tau) - \psi(0)| \rangle$ (rad)')
textstr = r'$\langle|k_\psi|\rangle=%.2f$ rad/s' % (self.k_psi)
props = dict(boxstyle='round', facecolor='wheat', alpha=0.5)
# place a text box in lower left in axes coords
ax = plt.gca()
ax.text(0.95,
0.05,
textstr,
transform=ax.transAxes,
fontsize=14,
horizontalalignment='right',
verticalalignment='bottom',
bbox=props)
plt.show()
def openImage(nameFile, intersection):
# this allows GDAL to throw Python Exceptions
gdal.UseExceptions()
band_num = 1
#Tvis-animated.gif
try:
src_ds = gdal.Open(nameFile)
except (RuntimeError, e):
print('Unable to open INPUT.tif')
print(e)
sys.exit(1)
try:
srcband = src_ds.GetRasterBand(band_num)
except (RuntimeError, e):
# for example, try GetRasterBand(10)
print('Band ( %i ) not found' % band_num)
print(e)
sys.exit(1)
gt1 = src_ds.GetGeoTransform()
Project = src_ds.GetProjection()
print(nameFile)
print(gt1)
xOrigin = gt1[0]
yOrigin = gt1[3]
pixelWidth = float(gt1[1])
pixelHeight = float(gt1[5])
xmin = intersection[0]
ymax = intersection[1]
xoff = int((xmin - xOrigin) / pixelWidth)
yoff = int((yOrigin - ymax) / pixelWidth)
xcount = int(
(np.abs(intersection[0]) - np.abs(intersection[2])) / pixelWidth)
ycount = int(
(np.abs(intersection[1]) - np.abs(intersection[3])) / pixelHeight)
#print nameFile
if (xoff == 0 and yoff == 0):
lc = srcband.ReadAsArray()
else:
#print nameFile
#print xoff
#print yoff
#print xcount
#print ycount
#if "MODIS" in nameFile:
#lc = srcband.ReadAsArray(xoff, yoff, int(xcount), int(ycount))
#else:
lc = srcband.ReadAsArray(xoff, yoff, int(xcount), int(ycount))
return src_ds, lc, gt1, Project
def _calc_correlation(self, values_1, values_2, conf_level=0.95):
""" Calculates Pearson's correlation coeffcient.
Arguments:
values_1 -- first data
values_2 -- second data
conf_level -- confidence level
Returns:
(corr_coeff, significance) -- correlation coefficient and significance arrays
"""
n_samples = values_1.shape[0] # Sample length
# Calculate Pearson's correlatiob coefficient
values_cov = ma.sum((values_1 - ma.mean(values_1, axis=0)) *
(values_2 - ma.mean(values_2, axis=0)),
axis=0)
corr_coef = values_cov / (ma.std(values_1, axis=0) *
ma.std(values_2, axis=0)) / n_samples
# Calculate significance using t-distribution with n-2 degrees of freedom.
deg_fr = n_samples - 2 # Degrees of freedom.
t_distr = ma.abs(
corr_coef *
ma.sqrt(deg_fr / (1. - corr_coef**2))) # Student's t-distribution.
prob = 0.5 + conf_level / 2 # Probability for two tails.
cr_value = student_t.ppf(prob, deg_fr) # Student's Critical value.
significance = ma.greater(t_distr, cr_value)
return corr_coef, significance
def ma_mad(x, axis=None):
"""Median absolute deviation"""
median_x = ma.median(x, axis=axis)
if axis is not None:
median_x = ma.expand_dims(median_x, axis=axis)
return ma.median(ma.abs(x - median_x), axis=axis)
def ray_intersect(self, orig, direction) -> ma.array:
normal = np.cross(self.a, self.b)
ndotray = ma.array(v3_dots(normal, direction))
ndotray.mask = ma.abs(ndotray) < 1e-3
d = v3_dots(normal, orig)
t = (v3_dots(normal, self.corner) + d) / ndotray
t.mask |= t < 0
pt = orig + t.reshape(-1, 1) * direction
# TODO: try an alternative to find points in a parallelogram (or plane)
# if that's easier. Maybe project onto a plane then use a parallelogram
# as a basis in 2d?
# https://stackoverflow.com/questions/59128744/raytracing-ray-vs-parallelogram
# edge 0
t.mask |= v3_dots(normal, np.cross(self.a, pt - self.corner)) < 0
# edge 1
t.mask |= v3_dots(normal, np.cross(pt - self.corner, self.b)) < 0
# edge 2
t.mask |= v3_dots(normal, np.cross(pt - self.corner - self.b,
self.a)) < 0
# edge 3
t.mask |= v3_dots(normal, np.cross(self.b,
pt - self.corner - self.a)) < 0
return t
def psi_trend(traj, maxMissing):
D = ma.array([tsstats.drift(tsstats.unwrapma(trajw.getMaskedPosture(trajw.psi)), lags, exclude=trajw.excluded)
for trajw in traj.asWindows(100.)
if fractionMissing(trajw)>maxMissing])
D[np.isnan(D)] = ma.masked
D = ma.abs(D).mean(axis=0)
if len(D) == 0:
D = ma.zeros((len(lags),))
D[:] = ma.masked
return D
def tdpep(t,fm,PG0):
"""
Transit-duration - Period - Epoch
Parameters
----------
fm : Flux with bad data points masked out. It is assumed that
elements of f are evenly spaced in time.
PG0 : Initial period grid.
Returns
-------
epoch2d : Grid (twd,P) of best epoch
df2d : Grid (twd,P) of depth epoch
count2d : number of filled data for particular (twd,P)
noise : Grid (twd) typical scatter
PG : The Period grid
twd : Grid of trial transit widths.
"""
assert fm.fill_value ==0
# Determine the grid of periods that corresponds to integer
# multiples of cadence values
PcadG,PG = P2Pcad(PG0)
# Initialize tdur grid.
twdMi = a2tdur( P2a( PG[0 ] ) ) /keptoy.lc
twdMa = a2tdur( P2a( PG[-1] ) ) /keptoy.lc
twdG = np.round(np.linspace(twdMi,twdMa,4)).astype(int)
rec2d = []
noise = []
for twd in twdG:
dM = mtd(t,fm.filled(),twd)
dM.mask = fm.mask | ~isfilled(t,fm,twd)
rec2d.append( pep(t[0],dM,PcadG) )
# Noise per transit
mad = ma.abs(dM)
mad = ma.median(mad)
noise.append(mad)
rec2d = np.vstack(rec2d)
make2d = lambda x : np.tile( np.vstack(x), (1,rec2d.shape[1] ))
rec2d = mlab.rec_append_fields(rec2d,'noise',make2d(noise))
rec2d = mlab.rec_append_fields(rec2d,'twd', make2d(twdG))
PG = np.tile( PG, (rec2d.shape[0],1 ))
rec2d = mlab.rec_append_fields(rec2d,'PG',PG)
s2n = rec2d['fom']/rec2d['noise']*rec2d['count']
rec2d = mlab.rec_append_fields(rec2d,'s2n', s2n )
return rec2d
def combine_nights(combined_catalog, filterlist, refcat):
header = ['BEGIN CATALOG HEADER',
'nfields 13',
' ra 1 0 d degrees %10.6f',
' dec 2 0 d degrees %10.6f',
' id 3 0 c INDEF %3d']
for filt in filterlist:
header.append(' {} {:2d} 0 r INDEF %6.3f'.format(filt, len(header) - 1))
header.append(' {}err {:2d} 0 r INDEF %6.3f'.format(filt, len(header) - 1))
header += ['END CATALOG HEADER', '']
catalog = Table([refcat['ra'], refcat['dec'], refcat['id']], meta={'comments': header}, masked=True)
for filt in filterlist:
mags = combined_catalog['mag'][combined_catalog['filter'] == filt]
median = np.median(mags, axis=0)
absdev_mag = mags - median
mad = np.median(np.abs(absdev_mag), axis=0) * np.sqrt(pi / 2)
mags.mask |= np.abs(absdev_mag) > 5 * mad
catalog[filt] = np.median(mags, axis=0)
catalog[filt+'err'] = np.median(np.abs(mags - catalog[filt]), axis=0) * np.sqrt(pi / 2)
return catalog
def fitBearingDrift(self, trajectory, windowSize=None, plotFit=False):
lags = np.linspace(0, np.round(50.*trajectory.frameRate), 200)
tau = lags / trajectory.frameRate
if windowSize is None:
psi = unwrapma(trajectory.getMaskedPosture(trajectory.psi))
D = drift(psi, lags, trajectory.excluded)
sel = ~ma.getmaskarray(psi)
#p = np.polyfit(tau, D, 1)
p = np.polyfit(trajectory.t[sel], psi[sel], 1)
self.k_psi = p[0]
else:
def result(traj):
psi = traj.getMaskedPosture(traj.psi)
if float(len(psi.compressed()))/float(len(psi)) > 0.2:
psi = unwrapma(psi)
D = drift(psi, lags, traj.excluded)
sel = ~ma.getmaskarray(psi)
p = np.polyfit(traj.t[sel], psi[sel], 1)
return D, p[0]
else:
return ma.zeros((len(lags),))*ma.masked, ma.masked
results = [result(traj) for traj in trajectory.asWindows(windowSize)]
D = ma.array([resulti[0] for resulti in results])
k = ma.array([resulti[1] for resulti in results])
self.k_psi = ma.abs(k).mean()
D = ma.abs(D).T.mean(axis=1)
if plotFit:
plt.plot(tau, D, 'k.')
plt.plot(tau, self.k_psi*tau, 'r-')
plt.xlabel(r'$\tau$ (s)')
plt.ylabel(r'$\langle |\psi(\tau) - \psi(0)| \rangle$ (rad)')
textstr = r'$\langle|k_\psi|\rangle=%.2f$ rad/s'%(self.k_psi)
props = dict(boxstyle='round', facecolor='wheat', alpha=0.5)
# place a text box in lower left in axes coords
ax = plt.gca()
ax.text(0.95, 0.05, textstr, transform=ax.transAxes, fontsize=14,
horizontalalignment='right', verticalalignment='bottom', bbox=props)
plt.show()
def s2n_known(d, t, fm):
"""
Compute the FFA S/N assuming we knew where the signal was before hand
Parameters
----------
d : Simulation Parameters
t : time
fm : lightcurve (maksed)
"""
# Compute the twd from the twdG with the closest to the injected tdur
tdur = keptoy.tdurMA(d)
itwd_close = np.argmin(np.abs(np.array(config.twdG) - tdur / config.lc))
twd_close = config.twdG[itwd_close]
dM = tfind.mtd(t, fm, twd_close)
# Fold the LC on the closest period we're computing all the FFA
# periods around the P closest. This is a little complicated, but
# it allows us to use the same functions as we do in the complete
# period scan.
Pcad0 = int(np.floor(d['P'] / config.lc))
t0cad, Pcad, meanF, countF = tfind.fold(dM, Pcad0)
iPcad_close = np.argmin(np.abs(Pcad - d['P'] / config.lc))
Pcad_close = Pcad[iPcad_close]
P_close = Pcad_close * config.lc
# Find the epoch that is closest to the injected phase.
t0 = t[0] + t0cad * config.lc # Epochs in days.
phase = np.mod(t0, P_close) / P_close # Phases [0,1)
# The following 3 lines compute the difference between the FFA
# phases and the injected phase. Phases can be measured going
# clockwise or counter clockwise, so we must choose the minmum
# value. No phases are more distant than 0.5.
dP = np.abs(phase - d['phase'])
dP = np.vstack([dP, 1 - dP])
dP = dP.min(axis=0)
iphase_close = np.argmin(dP)
phase_close = phase[iphase_close]
# s2n for the closest twd,P,phas
noise = ma.median(ma.abs(dM))
s2nF = meanF / noise * np.sqrt(countF)
s2nP = s2nF[iPcad_close] # length Pcad0 array with s2n for all the
# P at P_closest
s2n_close = s2nP[iphase_close]
return phase, s2nP, twd_close, P_close, phase_close, s2n_close
def my_polyfit(x, y, deg, degatt=0):
k = ma.polyfit(x, y, degatt)
res = my_poly(k, x)
resid = ma.abs(res - y)
medresid = ma.median(resid, axis=0)
if y.ndim != 1:
mask = ma.logical_not(ma.sum((resid > 3 * medresid), axis=1).astype('bool'))
else:
mask = (resid < 3 * medresid)
y = y[mask]
x = x[mask]
k = ma.polyfit(x, y, deg)
return(k, mask)
def transform_non_affine(self, a):
# NOTE: Critical to truncate valid range inside transform *and*
# in limit_range_for_scale or get weird duplicate tick labels. This
# is not necessary for positive-only scales because it is harder to
# run up right against the scale boundaries.
with np.errstate(divide='ignore', invalid='ignore'):
m = ma.masked_where((a <= -90) | (a >= 90), a)
if m.mask.any():
m = np.deg2rad(m)
return ma.log(ma.abs(ma.tan(m) + 1 / ma.cos(m)))
else:
a = np.deg2rad(a)
return np.log(np.abs(np.tan(a) + 1 / np.cos(a)))
def psi_trend(traj, maxMissing):
D = ma.array([
tsstats.drift(tsstats.unwrapma(trajw.getMaskedPosture(trajw.psi)),
lags,
exclude=trajw.excluded) for trajw in traj.asWindows(100.)
if fractionMissing(trajw) > maxMissing
])
D[np.isnan(D)] = ma.masked
D = ma.abs(D).mean(axis=0)
if len(D) == 0:
D = ma.zeros((len(lags), ))
D[:] = ma.masked
return D
def tdpep(t, fm, par):
"""
Transit-duration - Period - Epoch
Parameters
----------
fm : Flux with bad data points masked out. It is assumed that
elements of f are evenly spaced in time.
P1 : First period (cadences)
P2 : Last period (cadences)
twdG : Grid of transit durations (cadences)
Returns
-------
rtd : 2-D record array with the following fields at every trial
(twd,Pcad):
- noise
- s2n
- twd
- fields in rep
"""
PcadG = np.arange(par['Pcad1'], par['Pcad2'])
twdG = par['twdG']
assert fm.fill_value == 0
# Determine the grid of periods that corresponds to integer
# multiples of cadence values
try:
ntwd = len(twdG)
except:
ntwd = 1
rtd = []
for i in range(ntwd): # Loop over twd
twd = np.int(twdG[i])
dM = mtd(fm, twd)
func = lambda Pcad: ep(dM, Pcad)
rep = list(map(func, PcadG))
rep = np.hstack(rep)
r = np.empty(rep.size, dtype=tddtype)
for k in epdtype.names:
r[k] = rep[k]
r['noise'] = ma.median(ma.abs(dM))
r['twd'] = twd
r['t0'] = r['t0cad'] * config.lc + t[0]
rtd.append(r)
rtd = np.vstack(rtd)
rtd['s2n'] = rtd['mean'] / rtd['noise'] * np.sqrt(rtd['count'])
return rtd
def calc_directionality(dat, dist_range):
nbin = len(dat)
min_d,max_d = dist_range
if min_d < 0 or max_d < min_d:
raise ValueError('calc_insulation() requires 0 <= min_d <= max_d')
directionality = ma.zeros(nbin)
for i in xrange(nbin):
if i < max_d or i >= nbin-max_d:
directionality[i] = 0.0
else:
up = dat[i,(i-max_d):(i-min_d)].sum()
down = dat[i,(i+min_d):(i+max_d)].sum()
avg = (up+down)/2.0
directionality[i] = (up-down)/ma.abs(up-down)*((up-avg)**2/avg + (down-avg)**2/avg)
return directionality
def _find_fog_profiles(
self,
n_gates_for_signal_sum: int = 20,
signal_sum_threshold: float = 1e-3,
variance_threshold: float = 1e-15,
) -> np.ndarray:
"""Finds saturated (usually fog) profiles from beta_raw."""
signal_sum = ma.sum(ma.abs(
self.data["beta_raw"][:, :n_gates_for_signal_sum]),
axis=1)
variance = _calc_var_from_top_gates(self.data["beta_raw"])
is_fog = (signal_sum > signal_sum_threshold) | (variance <
variance_threshold)
logging.info(f"Cleaned {sum(is_fog)} profiles with fog filter")
return is_fog
def iterative_correction(self, max_iter=100, tolerance=1e-5):
totalBias = ma.ones(self.nbin, float)
mat = self.dat.copy()
for r in xrange(max_iter):
print('.', end='', file=sys.stderr)
binSum = mat.sum(axis=1)
mask = binSum==0
bias = binSum/binSum[~mask].mean()
bias[mask] = 1
bias -= 1
bias *= 0.8
bias += 1
totalBias *= bias
biasMat = bias.reshape(1,len(bias)) * bias.reshape(len(bias),1)
mat = mat / biasMat
if ma.abs(bias-1).max() < tolerance:
break
self.dat = mat
corr = totalBias[~mask].mean()
self.bias = totalBias/corr
self.corrected |= 0x1
def identifyReversals(self, transitionWindow=2.):
dpsi = self.getMaskedPosture(self.dpsi)
rev = ma.abs(dpsi) > np.pi / 2.
inRev = False
state = np.zeros(self.t.shape, int)
state[~rev] = 1
state[rev] = 2
state[ma.getmaskarray(rev)] = 0
self.state = state
revBoundaries = []
currentRev = ma.zeros((2, ))
for j in xrange(1, self.t.shape[0] - 2):
if not inRev:
if ((state[j] == 2 & state[j + 1] == 2) |
(state[j] == 2 & state[j + 1] == 0 & state[j + 2] == 2)):
if state[j - 1] == 0:
currentRev[0] = ma.masked
else:
currentRev[0] = j
inRev = True
else:
if ((state[j] == 1 & state[j + 1] == 1) |
(state[j] == 1 & state[j + 1] == 0 & state[j + 2] == 1)):
currentRev[1] = j
inRev = False
revBoundaries.append(currentRev.copy())
elif (state[j] == 0 & state[j + 1] == 0):
currentRev[1] = ma.masked
inRev = False
revBoundaries.append(currentRev.copy())
self.revBoundaries = ma.array(revBoundaries, dtype='int')
revEdges = self.revBoundaries[:].compressed()
for boundary in revEdges:
self.nearRev[
(self.t > boundary / self.frameRate - transitionWindow / 2.)
& (self.t < boundary / self.frameRate +
transitionWindow / 2.)] = True
def plot_glider(cube, cmap=plt.cm.viridis, figsize=(9, 3.75), track_inset=False):
data = apply_range(cube)
x = apply_range(cube.coord(axis="X"))
y = apply_range(cube.coord(axis="Y"))
z = apply_range(cube.coord(axis="Z"))
t = cube.coord(axis="T")
t = t.units.num2date(t.points.squeeze())
fig, ax = plt.subplots(figsize=figsize)
dist = distance(x, y)
z = ma.abs(z)
dist, _ = np.broadcast_arrays(dist[..., np.newaxis], z.filled(fill_value=np.NaN))
dist, z = map(ma.masked_invalid, (dist, z))
cs = ax.pcolor(dist, z, data, cmap=cmap, snap=True)
kw = dict(orientation="horizontal", extend="both", shrink=0.65)
cbar = fig.colorbar(cs, **kw)
if track_inset:
axin = inset_axes(
ax,
width=2,
height=2,
loc=4,
bbox_to_anchor=(1.15, 0.35),
bbox_transform=ax.figure.transFigure,
)
axin.plot(x, y, "k.")
start, end = (x[0], y[0]), (x[-1], y[-1])
kw = dict(marker="o", linestyle="none")
axin.plot(*start, color="g", **kw)
axin.plot(*end, color="r", **kw)
axin.axis("off")
ax.invert_yaxis()
ax.invert_xaxis()
ax.set_xlabel("Distance (km)")
ax.set_ylabel("Depth (m)")
return fig, ax, cbar
def identifyReversals(self, transitionWindow=2.):
dpsi = self.getMaskedPosture(self.dpsi)
rev = ma.abs(dpsi)>np.pi/2.
inRev = False
state = np.zeros(self.t.shape, int)
state[~rev] = 1
state[rev] = 2
state[ma.getmaskarray(rev)] = 0
self.state = state
revBoundaries = []
currentRev = ma.zeros((2,))
for j in xrange(1,self.t.shape[0]-2):
if not inRev:
if ((state[j]==2 & state[j+1]==2) |
(state[j]==2 & state[j+1]==0 & state[j+2]==2)):
if state[j-1] == 0:
currentRev[0] = ma.masked
else:
currentRev[0] = j
inRev = True
else:
if ((state[j]==1 & state[j+1]==1) |
(state[j]==1 & state[j+1]==0 & state[j+2]==1)):
currentRev[1] = j
inRev = False
revBoundaries.append(currentRev.copy())
elif (state[j]==0 & state[j+1]==0):
currentRev[1] = ma.masked
inRev = False
revBoundaries.append(currentRev.copy())
self.revBoundaries = ma.array(revBoundaries, dtype='int')
revEdges = self.revBoundaries[:].compressed()
for boundary in revEdges:
self.nearRev[(self.t>boundary/self.frameRate-transitionWindow/2.) &
(self.t<boundary/self.frameRate+transitionWindow/2.)] = True
def noiseyReg(t, dM, thresh=2):
"""
Noisey Region
If certain regions are much noisier than others, we should remove
them. A typical value of the noise is computed using a median
absolute deviation (MAD) on individual regions. If certain regions are
noiser by thresh, we mask them out.
Parameters
----------
dM : Single event statistic (masked array)
thresh : If region has MAD > thresh * typical MAD throw it out.
"""
tm = ma.masked_array(t, mask=dM.mask)
label = detrend.sepseg(tm)
sL = ma.notmasked_contiguous(label)
madseg = np.array([ma.median(ma.abs(dM[s])) for s in sL])
madLC = np.median(madseg) # Typical MAD of the light curve.
isNoisey = np.zeros(tm.size).astype(bool)
sNL = [] # List to keep track of the noisey segments
for s, mads in zip(sL, madseg):
if mads > thresh * madLC:
isNoisey[s] = True
sNL.append(s)
if len(sNL) != 0:
print "Removed following time ranges because data is noisey"
print "----------------------------------------------------"
for s in sNL:
print "%.2f %.2f " % (t[s.start], t[s.stop - 1])
return isNoisey
def peak(self,chanrange=None):
"""Return the peak intensity in the given channel range
If a mask exists, this function operates on the masked spectrum.
Parameters
----------
chanrange: range of channels over which to compute dispersion
[startchan, endchan]
Returns
----------
Maximum of the absolute value of the spectrum in the channel range
max(abs(spectrum[startchan:endchan]))
"""
s = self.spec()
chupper = len(s)-1
chanrange = self._sanitizechanrange(chanrange,chupper)
# Handle one-channel ranges.
if (chanrange[0] == chanrange[1]):
return s[chanrange[0]]
return ma.max(ma.abs(s[chanrange[0]:chanrange[1]]))
def peak(self,chanrange=None):
"""Return the peak intensity in the given channel range
If a mask exists, this function operates on the masked spectrum.
Parameters
----------
chanrange: range of channels over which to compute dispersion
[startchan, endchan]
Returns
----------
Maximum of the absolute value of the spectrum in the channel range
max(abs(spectrum[startchan:endchan]))
"""
s = self.spec()
chupper = len(s)-1
chanrange = self._sanitizechanrange(chanrange,chupper)
# Handle one-channel ranges.
if (chanrange[0] == chanrange[1]):
return s[chanrange[0]]
return ma.max(ma.abs(s[chanrange[0]:chanrange[1]]))
if np.all(group['dc1'][f0]):
dc0 = np.sum(np.power(group['dc1'][f0], -2))**-0.5
c0 = np.sum(
group['c1'][f0] * np.power(group['dc1'][f0], -2)) * dc0**2
else:
dc0 = 0.
c0 = np.mean(group['c1'][f0])
if np.all(group['dc2'][f1]):
dc1 = np.sum(np.power(group['dc2'][f1], -2))**-0.5
c1 = np.sum(
group['c2'][f1] * np.power(group['dc2'][f1], -2)) * dc1**2
else:
dc1 = 0.
c1 = np.mean(group['c2'][f1])
color = np.divide(m0 - m1 + z0 - z1, 1 - c0 + c1)
dcolor = np.abs(color) * np.sqrt(
np.divide(dm0**2 + dm1**2 + dz0**2 + dz1**2,
(m0 - m1 + z0 - z1)**2) +
np.divide(dc0**2 + dc1**2, (1 - c0 + c1)**2))
for row in group:
colors.append(color)
dcolors.append(dcolor)
targets[filters] = np.array(colors)
targets['d' + filters] = np.array(dcolors)
# calibrate all the instrumental magnitudes
zcol = [
color_to_use[row['filter']][0]
if color_to_use[row['filter']] else row['filter'] * 2
for row in targets
]
def manhattan(a, b):
"""
Manhattan distance between a and b
"""
return ma.abs(a.real - b.real) + ma.abs(a.imag - b.imag)
def euclid(a,b):
"""
Euclidian distance between a and b
"""
return ma.abs(a - b)
def __call__(self, value, clip=None):
# read in parameters
method = self.stretch
exponent = self.exponent
midpoint = self.midpoint
# ORIGINAL MATPLOTLIB CODE
if clip is None:
clip = self.clip
if np.iterable(value):
vtype = 'array'
val = ma.asarray(value).astype(np.float)
else:
vtype = 'scalar'
val = ma.array([value]).astype(np.float)
self.autoscale_None(val)
vmin, vmax = self.vmin, self.vmax
if vmin > vmax:
raise ValueError("minvalue must be less than or equal to maxvalue")
elif vmin == vmax:
return 0.0 * val
else:
if clip:
mask = ma.getmask(val)
val = ma.array(np.clip(val.filled(vmax), vmin, vmax),
mask=mask)
result = (val - vmin) * (1.0 / (vmax - vmin))
# CUSTOM APLPY CODE
# Keep track of negative values
negative = result < 0.
if self.stretch == 'Linear':
pass
elif self.stretch == 'Log':
# result = np.log(result * (self.midpoint - 1.) + 1.) \
# / np.log(self.midpoint)
result = ma.log10(result * (self.midpoint - 1.) + 1.) \
/ ma.log10(self.midpoint)
elif self.stretch == 'Sqrt':
result = ma.sqrt(ma.abs(result))
elif self.stretch == 'Arcsinh':
result = ma.arcsinh(result / self.midpoint) \
/ ma.arcsinh(1. / self.midpoint)
elif self.stretch == 'Arccosh':
result = ma.arccosh(result / self.midpoint) \
/ ma.arccosh(1. / self.midpoint)
elif self.stretch == 'Power':
result = ma.power(result, exponent)
elif self.stretch == 'Exp':
result = np.exp(result)
else:
raise Exception("Unknown stretch in APLpyNormalize: %s" %
self.stretch)
# Now set previously negative values to 0, as these are
# different from true NaN values in the FITS image
result[negative] = -np.inf
if vtype == 'Scalar':
result = result[0]
return result
def measure(mode, x, y, x0, x1, thresh=0):
""" return the a measure of y in the window x0 to x1
"""
xm = ma.masked_outside(x, x0, x1) # .compressed()
ym = ma.array(y, mask=ma.getmask(xm)) # .compressed()
if mode == 'mean':
r1 = np.mean(ym)
r2 = np.std(ym)
if mode == 'max' or mode == 'maximum':
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
if mode == 'min' or mode == 'minimum':
r1 = ma.min(ym)
r2 = xm[ma.argmin(ym)]
if mode == 'minormax':
r1p = ma.max(ym)
r1n = ma.min(ym)
if ma.abs(r1p) > ma.abs(r1n):
r1 = r1p
r2 = xm[ma.argmax(ym)]
else:
r1 = r1n
r2 = xm[ma.argmin(ym)]
if mode == 'median':
r1 = ma.median(ym)
r2 = 0
if mode == 'p2p': # peak to peak
r1 = ma.ptp(ym)
r2 = 0
if mode == 'std': # standard deviation
r1 = ma.std(ym)
r2 = 0
if mode == 'var': # variance
r1 = ma.var(ym)
r2 = 0
if mode == 'cumsum': # cumulative sum
r1 = ma.cumsum(ym) # Note: returns an array
r2 = 0
if mode == 'anom': # anomalies = difference from averge
r1 = ma.anom(ym) # returns an array
r2 = 0
if mode == 'sum':
r1 = ma.sum(ym)
r2 = 0
if mode == 'area' or mode == 'charge':
r1 = ma.sum(ym) / (ma.max(xm) - ma.min(xm))
r2 = 0
if mode == 'latency': # return first point that is > threshold
sm = ma.nonzero(ym > thresh)
r1 = -1 # use this to indicate no event detected
r2 = 0
if ma.count(sm) > 0:
r1 = sm[0][0]
r2 = len(sm[0])
if mode == '1090': #measure 10-90% time, also returns max
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
y10 = 0.1 * r1
y90 = 0.9 * r1
sm1 = ma.nonzero(ym >= y10)
sm9 = ma.nonzero(ym >= y90)
r1 = xm[sm9] - xm[sm1]
if mode == 'count':
r1 = ma.count(ym)
r2 = 0
if mode == 'maxslope':
return (0, 0)
slope = np.array([])
win = ma.flatnotmasked_contiguous(ym)
st = int(len(win) / 20) # look over small ranges
for k in win: # move through the slope measurementwindow
tb = range(k - st, k + st) # get tb array
newa = np.array(self.dat[i][j, thisaxis, tb])
ppars = np.polyfit(
x[tb], ym[tb],
1) # do a linear fit - smooths the slope measures
slope = np.append(slope, ppars[0]) # keep track of max slope
r1 = np.amax(slope)
r2 = np.argmax(slope)
return (r1, r2)
z0, dz0 = average_in_flux(group['z1'][f0], group['dz1'][f0])
z1, dz1 = average_in_flux(group['z2'][f1], group['dz2'][f1])
if np.all(group['dc1'][f0]):
dc0 = np.sum(np.power(group['dc1'][f0], -2))**-0.5
c0 = np.sum(group['c1'][f0] * np.power(group['dc1'][f0], -2)) * dc0**2
else:
dc0 = 0.
c0 = np.mean(group['c1'][f0])
if np.all(group['dc2'][f1]):
dc1 = np.sum(np.power(group['dc2'][f1], -2))**-0.5
c1 = np.sum(group['c2'][f1] * np.power(group['dc2'][f1], -2)) * dc1**2
else:
dc1 = 0.
c1 = np.mean(group['c2'][f1])
color = np.divide(m0 - m1 + z0 - z1, 1 - c0 + c1)
dcolor = np.abs(color) * np.sqrt(
np.divide(dm0**2 + dm1**2 + dz0**2 + dz1**2, (m0 - m1 + z0 - z1)**2)
+ np.divide(dc0**2 + dc1**2, (1 - c0 + c1)**2)
)
for row in group:
colors.append(color)
dcolors.append(dcolor)
targets[filters] = np.array(colors)
targets['d'+filters] = np.array(dcolors)
# calibrate all the instrumental magnitudes
zcol = [color_to_use[row['filter']][0] if color_to_use[row['filter']] else row['filter']*2 for row in targets]
zeropoint = np.choose(zcol == targets['zcol1'], [targets['z2'], targets['z1']])
dzeropoint = np.choose(zcol == targets['zcol1'], [targets['dz2'], targets['dz1']])
colorterm = np.choose(zcol == targets['zcol1'], [targets['c2'], targets['c1']])
dcolorterm = np.choose(zcol == targets['zcol1'], [targets['dc2'], targets['dc1']])
def pgram_max(t,fm,par):
"""
Periodogram: Check max values
Computes s2n for range of P, t0, and twd. However, for every
putative transit, we evaluate the transit depth having cut the
deepest transit and the second deepest transit. We require that
the mean depth after having cut the test max two values not be too
much smaller. Good at removing locations with 2 outliers.
Parameters
----------
t : t[0] provides starting time
fm : masked array with fluxes
par : dict with following keys
- Pcad1 (lower period limit)
- Pcad2 (upper period limit)
- twdG (grid of trial durations to compute)
Returns
-------
pgram : Record array with following fields
"""
ncad = fm.size
PcadG = np.arange(par['Pcad1'],par['Pcad2'])
get_frac_Pcad = lambda P : np.arange(P,P+1,1.0*P / ncad)
PcadG = np.hstack(map(get_frac_Pcad,PcadG))
twdG = par['twdG']
icad = np.arange(ncad)
dtype_pgram = [
('Pcad',float),
('twd',float),
('s2n',float),
('c',float),
('mean',float),
('t0',float),
('noise',float),
]
pgram = np.zeros( (len(twdG),len(PcadG)),dtype=dtype_pgram)
# dtype of the record array returned from tdpep()
dtype_temp = [
('c',int),
('mean',float),
('s2n',float),
('col',int),
('t0',float)
]
# Loop over different transit durations
for itwd,twd in enumerate(twdG):
res = foreman_mackey_1d(fm,twd)
dM = ma.masked_array(
res['depth_1d'],
~res['good_trans'].astype(bool),
fill_value=0
)
# Compute noise (robust, based on MAD) on twd timescales
noise = ma.median( ma.abs(dM) ) * 1.5
pgram[itwd,:]['noise'] = noise
pgram[itwd,:]['twd'] = twd
for iPcad,Pcad in enumerate(PcadG):
# Compute row and columns for folded data
row,col = wrap_icad(icad,Pcad)
ncol = np.max(col) + 1
nrow = np.max(row) + 1
icol = np.arange(ncol)
# Shove data and mask into appropriate positions
data = np.zeros((nrow,ncol))
mask = np.ones((nrow,ncol)).astype(bool)
data[row,col] = dM.data
mask[row,col] = dM.mask
# Sum along columns (clipping top 0, 1, 2 values)
datasum,datacnt = cumsum_top(data,mask,2)
# datasum[-1] are the is the summed columns having not
# clipped any values. Update results array. For t0, add
# half the transit with because column index corresponds
# in ingress
s = datasum[-1,:]
c = datacnt[-1,:]
r = np.zeros(ncol,dtype=dtype_temp)
r['s2n'] = -1
r['mean'] = s/c
r['s2n'] = s / np.sqrt(c) / noise
r['c'][:] = c
r['col'] = icol
r['t0'] = ( r['col'] + twd / 2.0) * config.lc + t[0]
# Compute mean transit depth after removing the deepest
# transit, datacnt[-2], and the second deepest transit,
# datacnt[-3]. The mean transit depth must be > 0.5 it's
# former value. Also, require 3 transits.
mean_clip1 = datasum[-2] / datacnt[-2]
mean_clip2 = datasum[-3] / datacnt[-3]
b = (
(mean_clip1 > 0.5 * r['mean'] ) &
(mean_clip2 > 0.5 * r['mean']) &
(r['c'] >= 3)
)
if ~np.any(b):
continue
rcut = r[b]
rmax = rcut[np.argmax(rcut['s2n'])]
names = ['mean','s2n','c','t0']
for n in names:
pgram[itwd,iPcad][n] = rmax[n]
pgram[itwd,iPcad]['Pcad'] = Pcad
# Compute the maximum return twd with the maximum s2n
pgram = pgram[np.argmax(pgram['s2n'],axis=0),np.arange(pgram.shape[1])]
return pgram
def measure(mode, x, y, x0, x1, thresh=0):
""" return the a measure of y in the window x0 to x1
"""
xm = ma.masked_outside(x, x0, x1) # .compressed()
ym = ma.array(y, mask=ma.getmask(xm)) # .compressed()
if mode == "mean":
r1 = np.mean(ym)
r2 = np.std(ym)
if mode == "max" or mode == "maximum":
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
if mode == "min" or mode == "minimum":
r1 = ma.min(ym)
r2 = xm[ma.argmin(ym)]
if mode == "minormax":
r1p = ma.max(ym)
r1n = ma.min(ym)
if ma.abs(r1p) > ma.abs(r1n):
r1 = r1p
r2 = xm[ma.argmax(ym)]
else:
r1 = r1n
r2 = xm[ma.argmin(ym)]
if mode == "median":
r1 = ma.median(ym)
r2 = 0
if mode == "p2p": # peak to peak
r1 = ma.ptp(ym)
r2 = 0
if mode == "std": # standard deviation
r1 = ma.std(ym)
r2 = 0
if mode == "var": # variance
r1 = ma.var(ym)
r2 = 0
if mode == "cumsum": # cumulative sum
r1 = ma.cumsum(ym) # Note: returns an array
r2 = 0
if mode == "anom": # anomalies = difference from averge
r1 = ma.anom(ym) # returns an array
r2 = 0
if mode == "sum":
r1 = ma.sum(ym)
r2 = 0
if mode == "area" or mode == "charge":
r1 = ma.sum(ym) / (ma.max(xm) - ma.min(xm))
r2 = 0
if mode == "latency": # return first point that is > threshold
sm = ma.nonzero(ym > thresh)
r1 = -1 # use this to indicate no event detected
r2 = 0
if ma.count(sm) > 0:
r1 = sm[0][0]
r2 = len(sm[0])
if mode == "1090": # measure 10-90% time, also returns max
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
y10 = 0.1 * r1
y90 = 0.9 * r1
sm1 = ma.nonzero(ym >= y10)
sm9 = ma.nonzero(ym >= y90)
r1 = xm[sm9] - xm[sm1]
if mode == "count":
r1 = ma.count(ym)
r2 = 0
if mode == "maxslope":
return (0, 0)
slope = np.array([])
win = ma.flatnotmasked_contiguous(ym)
st = int(len(win) / 20) # look over small ranges
for k in win: # move through the slope measurementwindow
tb = range(k - st, k + st) # get tb array
newa = np.array(self.dat[i][j, thisaxis, tb])
ppars = np.polyfit(x[tb], ym[tb], 1) # do a linear fit - smooths the slope measures
slope = np.append(slope, ppars[0]) # keep track of max slope
r1 = np.amax(slope)
r2 = np.argmax(slope)
return (r1, r2)
def measure(mode, x, y, x0, x1, thresh=0, slopewin=1.0):
""" return the a measure of y in the window x0 to x1
"""
xm = ma.masked_outside(x, x0, x1)# .compressed()
ym = ma.array(y, mask = ma.getmask(xm))# .compressed()
if mode == 'mean':
r1 = np.mean(ym)
r2 = np.std(ym)
if mode == 'max' or mode == 'maximum':
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
if mode == 'min' or mode == 'minimum':
r1 = ma.min(ym)
r2 = xm[ma.argmin(ym)]
if mode == 'minormax':
r1p = ma.max(ym)
r1n = ma.min(ym)
if ma.abs(r1p) > ma.abs(r1n):
r1 = r1p
r2 = xm[ma.argmax(ym)]
else:
r1 = r1n
r2 = xm[ma.argmin(ym)]
if mode == 'median':
r1 = ma.median(ym)
r2 = 0
if mode == 'p2p': # peak to peak
r1 = ma.ptp(ym)
r2 = 0
if mode == 'std': # standard deviation
r1 = ma.std(ym)
r2 = 0
if mode == 'var': # variance
r1 = ma.var(ym)
r2 = 0
if mode == 'cumsum': # cumulative sum
r1 = ma.cumsum(ym) # Note: returns an array
r2 = 0
if mode == 'anom': # anomalies = difference from averge
r1 = ma.anom(ym) # returns an array
r2 = 0
if mode == 'sum':
r1 = ma.sum(ym)
r2 = 0
if mode == 'area' or mode == 'charge':
r1 = ma.sum(ym)/(ma.max(xm)-ma.min(xm))
r2 = 0
if mode == 'latency': # return first point that is > threshold
sm = ma.nonzero(ym > thresh)
r1 = -1 # use this to indicate no event detected
r2 = 0
if ma.count(sm) > 0:
r1 = sm[0][0]
r2 = len(sm[0])
if mode == '1090': #measure 10-90% time, also returns max
r1 = ma.max(ym)
r2 = xm[ma.argmax(ym)]
y10 = 0.1*r1
y90 = 0.9*r1
sm1 = ma.nonzero(ym >= y10)
sm9 = ma.nonzero(ym >= y90)
r1 = xm[sm9] - xm[sm1]
if mode == 'count':
r1 = ma.count(ym)
r2 = 0
if mode == 'maxslope':
slope = []
win = ma.flatnotmasked_contiguous(ym)
dt = x[1]-x[0]
st = int(slopewin/dt) # use slopewin duration window for fit.
print('st: ', st)
for k, w in enumerate(win): # move through the slope measurementwindow
tb = range(k-st, k+st) # get tb array
ppars = np.polyfit(x[tb], ym[tb], 1) # do a linear fit - smooths the slope measures
slope.append(ppars[0]) # keep track of max slope
r1 = np.max(slope)
r2 = np.argmax(slope)
return(r1, r2)
if v in var2:
arr1 = var1[v][:]
arr2 = var2[v][:]
mask1 = ma.getmask(arr1)
mask2 = ma.getmask(arr2)
diffm1 = ma.where((mask1 == True) & (mask2 == False))
diffm2 = ma.where((mask2 == 1) & (mask1 == 0))
if len(diffm1[0]) > 0:
print(
"WARNING: SOME " + v +
" PIXEL ARE MASKED FOR THE FIRST FILE AND NOT FOR THE SECOND ONE"
)
if len(diffm2[0]) > 0:
print(
"WARNING: SOME " + v +
" PIXEL ARE MASKED FOR THE SECOND FILE AND NOT FOR THE FIRST ONE"
)
arr1 = ma.array(arr1, mask=mask2)
print(arr1.shape)
arr2 = ma.array(arr2, mask=mask1)
diff = ma.abs((arr1[:, 2] - arr2[:, 2])) * 100 / ma.abs(arr2[:, 2])
diffm = ma.where(diff > .5)
if len(diffm[0]) > 0:
print(arr1[diffm])
print(arr2[diffm])
for t in time[diffm]:
print(t)
print("WARNING NOT ALL VALUES ARE EQUAL FOR " + v + " VARIABLES")
def manhattan(a,b):
"""
Manhattan distance between a and b
"""
return ma.abs(a.real - b.real) + ma.abs(a.imag - b.imag)
def __fit__(self, rating, row=True):
if isinstance(rating, ma.MaskedArray):
self._rating = rating
else:
self._rating = ma.masked_equal(rating, 0)
self._mean = ma.mean(self._rating, axis=1, keepdims=True)
self._mean_center_rating = self._rating - self._mean
self._rating_filled = self._rating.filled(0)
if row:
self._sim = person(mean_center_rating=self._mean_center_rating)
else:
self._rating = self._rating.T
self._mean_center_rating = self._mean_center_rating.T
self._sim = person(mean_center_rating=self._mean_center_rating)
self._sim[np.diag_indices(self._sim.shape[0])] = -999
self._skip_columns = np.where(self._rating.count(axis=0) == 0)[0]
# params
self._neighborhood = np.argsort(self._sim, axis=1)[:,
-self.config.topk:]
self._neighborhood_idx = ([
int(i / self._neighborhood.shape[1])
for i in range(self._neighborhood.size)
], self._neighborhood.flatten())
if row:
self._m, self._n = rating.shape
else:
self._n, self._m = rating.shape
if "_weight" not in self.__dict__:
self._weight = np.random.randn(self._m, self.config.topk)
if "_m_bias" not in self.__dict__:
self._m_bias = np.random.randn(self._m)
if "_n_bias" not in self.__dict__:
self._n_bias = np.random.randn(self._n)
assert self._weight.shape[1] == self.config.topk
assert self._m_bias.shape[0] == self._m
assert self._n_bias.shape[0] == self._n
start = time.perf_counter()
step = self._epoch * self._n
for epoch in range(self._epoch, self.config.epochs):
self._epoch = epoch
for j in range(self._n):
if j in self._skip_columns:
continue
# forward
step += 1
_hat_rating, mid_data = self.__forward__(j)
_loss = self.__loss__(self._rating[:, j], _hat_rating)
logger.debug(
"[{:4d} step in {:4d} epoch\ttime:{:.2f}s] {}'s loss:{:.2f}"
.format(step, self._epoch,
time.perf_counter() - start, j, _loss))
# backward
_g_m_bias, _g_ngb_m_bias, _g_ngb_n_bias, _g_weight = self.__backward__(
_hat_rating, self._rating[:, j], mid_data[0], mid_data[1])
if not ma.any(_g_m_bias):
continue
for i, g in zip(self._neighborhood.flat, _g_ngb_m_bias.flat):
if g is not ma.masked:
_g_m_bias[i] += g
# check gradient
if self.config.check_gradient:
logger.debug("check gradient")
self.__check_gradient__(j, _g_weight, _g_m_bias,
_g_ngb_n_bias)
logger.debug(
"[gradient] max(m_bias): {}\tmax(n_bias): {}\tmax(weight):{}"
.format(ma.max(ma.abs(_g_m_bias)), ma.abs(_g_ngb_n_bias),
ma.max(ma.abs(_g_weight))))
# update gradient
self._m_bias -= self.config.lr / self._m * _g_m_bias + self.config.wdecay * self._m_bias
self._n_bias[
j] -= self.config.lr / self._m * _g_ngb_n_bias + self.config.wdecay * self._n_bias[
j]
self._weight -= self.config.lr / self._m * _g_weight + self.config.wdecay * self._weight
logger.debug(
"[{:4d} epoch\ttime:{:.2f}s] epoch loss:{:.2f}".format(
epoch,
time.perf_counter() - start,
self.__loss__(self._rating, self.__predict__())))
if epoch % self.config.save_per_epochs == 0:
self.save()
if self._epoch % self.config.save_per_epochs != 0:
self.save()
#select variable Salt = RomsNC.variables['salt'][:] Prime2 = (Salt - ma.mean(Salt))**2 varname = Prime2 #horizontal gradients ds_dx = gr.x_grad_rho(RomsFile, RomsGrd, varname) ds_dy = gr.y_grad_rho(RomsFile, RomsGrd, varname) #grid corrections xCor = gr.x_grad_GridCor_Rho(RomsFile, RomsGrd, varname) yCor = gr.y_grad_GridCor_Rho(RomsFile, RomsGrd, varname) #ratio x_rat = ma.array(ma.abs(xCor)/ma.abs(ds_dx)) y_rat = ma.array(ma.abs(yCor)/ma.abs(ds_dy)) #depth median ratio DM_ratx = ma.median(x_rat[0,:,:,:], axis = 0) DM_raty = ma.median(y_rat[0,:,:,:], axis = 0) #mask land values Land = ma.getmask(varname) Landdt = rt.AddDepthTime(RomsFile, Land) Xratio = ma.array(x_rat, mask = Land).flatten() Yratio = ma.array(y_rat, mask = Land).flatten() #remove mask
def euclid(a, b):
"""
Euclidian distance between a and b
"""
return ma.abs(a - b)
def mean_sigma_predictor(mean, sigma, z, sim, **not_used_kwargs):
return mean + sigma * ma.sum(sim * z, axis=1) / ma.sum(ma.abs(sim), axis=1)
def correct_dualPRF_cmean(radar,
field='velocity',
Nprf=3,
corr_method='median',
Nmin=2):
v_ma = radar.fields[field]['data']
vcorr_ma = v_ma.copy()
out_mask = np.zeros(v_ma.shape)
# Dual-PRF parameters
Vny = radar.instrument_parameters['nyquist_velocity']['data'][0]
prf_flag = radar.instrument_parameters['prf_flag']['data']
# Array with the primary Nyquist velocity corresponding to each bin
Nprf_arr = primary_vel(v_ma.shape, Nprf, prf_flag=prf_flag)
Vny_arr = Vny / Nprf_arr
for nsweep, sweep_slice in enumerate(radar.iter_slice()):
v0 = v_ma[sweep_slice] # velocity field
vp = Vny_arr[sweep_slice] # primary velocities
nprfp = Nprf_arr[sweep_slice] # dual-PRF factors
ref, out_mask[sweep_slice] = outlier_detector_cmean(v0,
Vny,
nprfp,
Nmin=Nmin)
# Convert non-outliers to zero for correction procedure
v0_out = v0 * out_mask[sweep_slice]
vp_out = vp * out_mask[sweep_slice]
ref_out = ref * out_mask[sweep_slice]
vp_out_L = vp_out.copy() # Only low PRF outliers
vp_out_L[nprfp == Nprf] = 0
dev = ma.abs(v0_out - ref_out)
nuw = np.zeros(v0.shape) # Number of unwraps (initialisation)
for ni in range(-Nprf, (Nprf + 1)):
# New velocity values for identified outliers
if abs(ni) == Nprf:
vcorr_out = v0_out + 2 * ni * vp_out_L
else:
vcorr_out = v0_out + 2 * ni * vp_out
# New deviation for new velocity values
dev_tmp = ma.abs(vcorr_out - ref_out)
# Compare with previous
delta = dev - dev_tmp
# Update unwrap number
nuw[delta > 0] = ni
# Update corrected velocity and deviation
vcorr_out_tmp = v0_out + 2 * nuw * vp_out
dev = ma.abs(vcorr_out_tmp - ref_out)
# Corrected velocity field
vcorr_ma[sweep_slice] = v0 + 2 * nuw * vp
return vcorr_ma, out_mask
def run(self):
""" Main method of the class. Reads data arrays, process them and returns results. """
self.logger.info('Started!')
# Get inputs
input_uids = self._data_helper.input_uids()
assert input_uids, 'Error! No input arguments!'
# Get parameters
parameters = None
if len(input_uids
) == MAX_N_INPUT_ARGUMENTS: # If parameters are given.
parameters = self._data_helper.get(
input_uids[INPUT_PARAMETERS_INDEX])
feature = self._get_parameter('Feature', parameters, DEFAULT_VALUES)
exceedance = self._get_parameter('Exceedance', parameters,
DEFAULT_VALUES)
condition = self._get_parameter('Condition', parameters,
DEFAULT_VALUES)
calc_mode = self._get_parameter('Mode', parameters, DEFAULT_VALUES)
self.logger.info('Calculation feature: %s', feature)
self.logger.info('Exceedance: %s', exceedance)
if condition is not None:
self.logger.info('Condition: %s', condition)
self.logger.info('Calculation mode: %s', calc_mode)
# Get outputs
output_uids = self._data_helper.output_uids()
assert output_uids, '(CalcExceedance::run) No output arguments!'
# Get time segments and levels
study_time_segments = self._data_helper.get_segments(
input_uids[STUDY_UID])
study_vertical_levels = self._data_helper.get_levels(
input_uids[STUDY_UID])
# Normals time segments should be set for year 1 (as set in a pdftails file)
normals_time_segments = deepcopy(study_time_segments)
percentile = self._data_helper.get_levels(input_uids[NORMALS_UID])[
0] # There should be only one level - percentile.
for segment in normals_time_segments:
segment['@beginning'] = '0001' + segment['@beginning'][4:]
segment['@ending'] = '0001' + segment['@ending'][4:]
# Read normals data
normals_data = self._data_helper.get(input_uids[NORMALS_UID],
segments=normals_time_segments)
study_data = self._data_helper.get(input_uids[STUDY_UID],
segments=study_time_segments)
if exceedance == 'low':
comparison_func = operator.lt
elif exceedance == 'high':
comparison_func = operator.gt
else:
self.logger.error('Error! Unknown exceedance value: \'%s\'',
exceedance)
raise ValueError
data_func = ma.max # For calc_mode == 'data' we calculate max over all segments.
input_description = self._data_helper.get_data_info(
output_uids[0])['description']
output_description = {'@title': input_description['@title']}
if feature != 'total':
output_description['@title'] = feature.capitalize(
) + ' of ' + output_description['@title']
for level in study_vertical_levels:
all_segments_data = []
for segment in study_time_segments:
normals_values = normals_data['data'][percentile][
segment['@name']]['@values']
study_values = study_data['data'][level][
segment['@name']]['@values']
study_time_grid = study_data['data'][level][
segment['@name']]['@time_grid']
# Remove Feb 29 from the study array (we do not take this day into consideration).
study_values = self._remove_feb29(study_values,
study_time_grid)
# Apply conditions if there are any.
if condition is not None:
self._apply_condition(study_values, condition)
# Compare values according chosen exceedance.
comparison_mask = comparison_func(study_values, normals_values)
# Perform calculation for the current time segment.
if feature == 'frequency': # We can just average 'True's to get a fraction and multiply by 100%.
one_segment_data = ma.mean(comparison_mask, axis=0) * 100
output_description['@units'] = '%'
if feature == 'intensity':
diff = ma.abs(study_values -
normals_values) # Calculate difference
diff.mask = ma.mask_or(
diff.mask, ~comparison_mask,
shrink=False) # and mask out unnecessary values.
one_segment_data = ma.mean(diff, axis=0)
output_description['@units'] = 'days'
if feature == 'duration':
one_segment_data = self._calc_duration(comparison_mask)
output_description['@units'] = 'days'
if feature == 'total':
study_values.mask = ma.mask_or(study_values.mask,
~comparison_mask,
shrink=False)
one_segment_data = ma.sum(study_values, axis=0)
output_description['@units'] = 'days'
# For segment-wise averaging send to the output current time segment results
# or store them otherwise.
if calc_mode == 'segment':
self._data_helper.put(
output_uids[0],
values=one_segment_data,
level=level,
segment=segment,
longitudes=study_data['@longitude_grid'],
latitudes=study_data['@latitude_grid'],
fill_value=study_data['@fill_value'],
meta=study_data['meta'],
description=output_description)
elif calc_mode == 'data':
all_segments_data.append(one_segment_data)
else:
self.logger.error(
'Error! Unknown calculation mode: \'%s\'', calc_mode)
raise ValueError
# For data-wise analysis analyse segments analyses :)
if calc_mode == 'data':
data_out = data_func(ma.stack(all_segments_data), axis=0)
# Make a global segment covering all input time segments
full_range_segment = deepcopy(
study_time_segments[0]
) # Take the beginning of the first segment...
full_range_segment['@ending'] = study_time_segments[-1][
'@ending'] # and the end of the last one.
full_range_segment[
'@name'] = 'GlobalSeg' # Give it a new name.
output_description[
'@title'] = 'Maximum ' + output_description['@title']
self._data_helper.put(output_uids[0],
values=data_out,
level=level,
segment=full_range_segment,
longitudes=study_data['@longitude_grid'],
latitudes=study_data['@latitude_grid'],
fill_value=study_data['@fill_value'],
meta=study_data['meta'],
description=output_description)
self.logger.info('Finished!')
