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Python

from __future__ import absolute_import, division
import numpy as np
from numpy import (pi, linalg, concatenate, sqrt)
from scipy.sparse import spdiags
from scipy.sparse.linalg import spsolve
import scipy.optimize as optimize
from scipy.signal import _savitzky_golay
from scipy.ndimage import convolve1d
from scipy.ndimage.morphology import distance_transform_edt
import warnings
from wafo.dctpack import dctn, idctn
__all__ = ['SavitzkyGolay', 'Kalman', 'HodrickPrescott', 'smoothn',
'HampelFilter', 'SmoothNd']
8 years ago
# noise = np.random.randn(2**8)/10
8 years ago
noise = [-0.0490483773397234, 0.07101522794824691, 0.043129450693516064, 0.07858516767729644, -0.04489848540755172, -0.012710090966021995, 0.022967442347004003, -0.1593564930543959, 0.14752458454255937, -0.1220055819473534, -0.030151822649201642, 0.009880871420067841, 0.0401050562035102, -0.10931262882008379, -0.14550620919429919, -0.06632845063372966, 0.07773893951749064, -0.009527784302072342, 0.06002486046176557, 0.11972670522904964, -0.14436696992162384, 0.06009486605688445, -0.05802790838575894, 0.16964239368289297, 0.09088881573238144, -0.003398259264109856, 0.059830811447018004, -0.08189024981767952, -0.05455483548325317, 0.056651518536760745, -0.05211609539593189, -0.07848323826083178, -0.03921692262168154, -0.04755275276447492, -0.05855172473750038, 0.06480280696345982, -0.05237889271019207, -0.05891912551792037, -0.04045907452295067, -0.09058522124919187, 0.1406515441218336, 0.15557979603588584, -0.09096515320242772, 0.1724190189462715, -0.04978942687488187, -0.0855435866249914, 0.09439718859306868, -0.14758639479507882, -0.07225230856508442, 0.008364508824556314, 0.06704423745152435, -0.01718113731784587, 0.07473943576290255, 0.028133087670974395, 0.026270590730899095, 0.13175770484080895, -0.01821821552644416, 0.11325945472394446, 0.04694754851273185, -0.23899404962137366, -0.1528175431702195, 0.151870532421663, -0.07353204927616248, 0.11604199430172217, -0.09111623325687843, -0.11887366073405607, -0.029872397510562025, 0.047672685028458936, -0.18340065977268627, 0.06896217941210328, 0.042997912112300564, 0.15416998299846174, -0.0386283794526545, 0.14070600624229804, 0.020984623041646142, -0.1892741373898864, 0.03253519397457513, -0.06182705494266229, -0.1326495728975159, 0.026234150321195537, 0.0550541170409239, 0.029275813927566702, 0.042742104678489906, -0.2170004668366198, -0.00035991761313413197, -0.0638872684868346, -0.11769436550364845, -0.017792813824766808, -0.022786402363044914, -0.10668279890162544, 0.05979507681729831, -0.1008100479486818, 0.0703474638610785, 0.1630534776572414, 0.06682406484481357, -0.0527228810042394, -0.046515310355062636, 0.04609515154732255, 0.11503753838360875, 0.11517599661346192, -0.05596425736274815, -0.06149119758833357, 0.10599964719188917, -0.012076380140185552, 0.0436828262270732, -0.03910174791470852, -0.03263251315745414, -0.012513843545007558, 0.004590611827089213, 0.0762719171282112, 0.06497715695411535, -0.003280826953794463, 0.13524154885565484, -0.020441364843140027, -0.09488214173137496, 0.1385755359902911, -0.23883052310744746, -0.10110537386421652, -0.1588981058869149, 0.06645444828058467, -0.2103306051703948, 0.15215327561190056, -0.03582175680076989, 0.013593833383013293, -0.11542058494732854, -0.05613268116816099, 0.012711037661355899, 0.04242805633100794, -0.011799315325220794, 0.12141794601099387, 0.054285270560662645, 0.07549385527022169, -0.04549437694653443, 0.11009856942530691, 0.05233482224379645, -0.042246830306136955, -0.1737197924666796, -0.10589427330127077, 0.04895472597843757, 0.06756519832636187, 0.083376600742245, -0.07502859751328732, -0.09493802498812245, -0.01058967186080922, -0.23759763247649018, 0.08439637862616411, -0.2021754550870607, 0.07365816800912013, 0.07435401663661081, 0.047992791325423556, -0.005250092450514997, 0.1693610927865244, 0.030338113772413154, -0.18010537945928004, 0.01744129379023785, 0.1902505975745975, -0.004598733688659104, 0.13663542585715657, -0.04100719174496187, -0.15406303185009937, -0.05297118247908407, 0.04435144348234146, 0.022377061632995063, 0.05491057192661079, -0.08473062163887303, -0.03907641665824873, 0.008686833182075315, -0.06053451866471732, -0.051735892949367854, -0.1902071038920444, 0.11508817132666356, 0.08903045262390544, -0.028537865059606825, -0.07160660523436188, 0.05994760363400714, 0.03637820115278829, 0.027604828657436364, 0.04168122074675033, -0.021707671111253164, 0.06770739385070886, -0.04848505599153394, -0.14377853380839264, 0.17448368721141166, -0.05972663746675887, -0.1615729579782888, -0.09508063624538736, -0.05501964872264433, -0.14370852991216054, -0.1025241548369181, -0.147
8 years ago
def _assert(cond, msg):
if not cond:
raise ValueError(msg)
class SavitzkyGolay(object):
r"""Smooth and optionally differentiate data with a Savitzky-Golay filter.
The Savitzky-Golay filter removes high frequency noise from data.
It has the advantage of preserving the original shape and
features of the signal better than other types of filtering
approaches, such as moving averages techniques.
Parameters
----------
n : int
the size of the smoothing window is 2*n+1.
degree : int
the degree of the polynomial used in the filtering.
Must be less than `window_size` - 1, i.e, less than 2*n.
diff_order : int
order of the derivative to compute (default = 0 means only smoothing)
0 means that filter results in smoothing of function
1 means that filter results in smoothing the first derivative of the
function and so on ...
delta : float, optional
The spacing of the samples to which the filter will be applied.
This is only used if deriv > 0. Default is 1.0.
axis : int, optional
The axis of the array `x` along which the filter is to be applied.
Default is -1.
mode : str, optional
Must be 'mirror', 'constant', 'nearest', 'wrap' or 'interp'. This
determines the type of extension to use for the padded signal to
which the filter is applied. When `mode` is 'constant', the padding
value is given by `cval`. See the Notes for more details on 'mirror',
'constant', 'wrap', and 'nearest'.
When the 'interp' mode is selected (the default), no extension
is used. Instead, a degree `polyorder` polynomial is fit to the
last `window_length` values of the edges, and this polynomial is
used to evaluate the last `window_length // 2` output values.
cval : scalar, optional
Value to fill past the edges of the input if `mode` is 'constant'.
Default is 0.0.
Notes
-----
The Savitzky-Golay is a type of low-pass filter, particularly suited for
smoothing noisy data. The main idea behind this approach is to make for
each point a least-square fit with a polynomial of high order over a
odd-sized window centered at the point.
Details on the `mode` options:
'mirror':
Repeats the values at the edges in reverse order. The value
closest to the edge is not included.
'nearest':
The extension contains the nearest input value.
'constant':
The extension contains the value given by the `cval` argument.
'wrap':
The extension contains the values from the other end of the array.
For example, if the input is [1, 2, 3, 4, 5, 6, 7, 8], and
`window_length` is 7, the following shows the extended data for
the various `mode` options (assuming `cval` is 0)::
mode | Ext | Input | Ext
-----------+---------+------------------------+---------
'mirror' | 4 3 2 | 1 2 3 4 5 6 7 8 | 7 6 5
'nearest' | 1 1 1 | 1 2 3 4 5 6 7 8 | 8 8 8
'constant' | 0 0 0 | 1 2 3 4 5 6 7 8 | 0 0 0
'wrap' | 6 7 8 | 1 2 3 4 5 6 7 8 | 1 2 3
Examples
--------
8 years ago
>>> import wafo.sg_filter as ws
>>> t = np.linspace(-4, 4, 500)
9 years ago
>>> noise = np.random.normal(0, 0.05, t.shape)
>>> noise = np.sqrt(0.05)*np.sin(100*t)
>>> y = np.exp( -t**2 ) + noise
>>> ysg = SavitzkyGolay(n=20, degree=2).smooth(y)
9 years ago
>>> np.allclose(ysg[:3], [ 0.01345312, 0.01164172, 0.00992839])
True
8 years ago
>>> ysm = SavitzkyGolay(n=20, degree=2, mode='mirror').smooth(y)
>>> np.allclose(ysm[:3], [-0.01604804, -0.00592883, 0.0035858 ])
True
>>> ysc = SavitzkyGolay(n=20, degree=2, mode='constant').smooth(y)
>>> np.allclose(ysc[:3], [-0.00279797, 0.00519541, 0.00666146])
True
>>> ysn = SavitzkyGolay(n=20, degree=2, mode='nearest').smooth(y)
>>> np.allclose(ysn[:3], [ 0.08711171, 0.0846945 , 0.07587448])
True
>>> ysw = SavitzkyGolay(n=20, degree=2, mode='wrap').smooth(y)
>>> np.allclose(ysw[:3], [-0.00208422, -0.00201491, 0.00201772])
True
>>> np.allclose(SavitzkyGolay(n=20, degree=2).smooth_last(y),
... 0.004921382626100505)
True
9 years ago
import matplotlib.pyplot as plt
h = plt.plot(t, y, label='Noisy signal')
h1 = plt.plot(t, np.exp(-t**2), 'k', lw=1.5, label='Original signal')
h2 = plt.plot(t, ysg, 'r', label='Filtered signal')
h3 = plt.legend()
h4 = plt.title('Savitzky-Golay')
plt.show()
References
----------
.. [1] A. Savitzky, M. J. E. Golay, Smoothing and Differentiation of
Data by Simplified Least Squares Procedures. Analytical
Chemistry, 1964, 36 (8), pp 1627-1639.
.. [2] Numerical Recipes 3rd Edition: The Art of Scientific Computing
W.H. Press, S.A. Teukolsky, W.T. Vetterling, B.P. Flannery
Cambridge University Press ISBN-13: 9780521880688
"""
def __init__(self, n, degree=1, diff_order=0, delta=1.0, axis=-1,
mode='interp', cval=0.0):
self.n = n
self.degree = degree
self.diff_order = diff_order
self.mode = mode
self.cval = cval
self.axis = axis
self.delta = delta
window_length = 2 * n + 1
self._coeff = _savitzky_golay.savgol_coeffs(window_length,
degree, deriv=diff_order,
delta=delta)
8 years ago
def smooth_last(self, signal, k=1):
coeff = self._coeff
8 years ago
n = (np.size(coeff) - 1) // 2
y = np.squeeze(signal)
if n == 0:
return y
if y.ndim > 1:
coeff.shape = (-1, 1)
8 years ago
first_vals = y[0] - np.abs(y[n:0:-1] - y[0])
last_vals = y[-1] + np.abs(y[-2:-n - 2:-1] - y[-1])
y = concatenate((first_vals, y, last_vals))
return (y[-2 * n - 1 - k:-k] * coeff).sum(axis=0)
def __call__(self, signal):
return self.smooth(signal)
def smooth(self, signal):
8 years ago
dtype = np.result_type(signal, np.float)
x = np.asarray(signal, dtype=dtype)
coeffs = self._coeff
mode, axis = self.mode, self.axis
if mode == "interp":
window_length, polyorder = self.n * 2 + 1, self.degree
deriv, delta = self.diff_order, self.delta
y = convolve1d(x, coeffs, axis=axis, mode="constant")
_savitzky_golay._fit_edges_polyfit(x, window_length, polyorder,
deriv, delta, axis, y)
else:
y = convolve1d(x, coeffs, axis=axis, mode=mode, cval=self.cval)
return y
def evar(y):
"""Noise variance estimation. Assuming that the deterministic function Y
has additive Gaussian noise, EVAR(Y) returns an estimated variance of this
noise.
Note:
----
A thin-plate smoothing spline model is used to smooth Y. It is assumed
that the model whose generalized cross-validation score is minimum can
provide the variance of the additive noise. A few tests showed that
EVAR works very well with "not too irregular" functions.
Examples:
--------
1D signal
>>> n = 1e6
>>> x = np.linspace(0,100,n);
>>> y = np.cos(x/10)+(x/50)
>>> var0 = 0.02 # noise variance
>>> yn = y + sqrt(var0)*np.random.randn(*y.shape)
>>> s = evar(yn) # estimated variance
>>> np.abs(s-var0)/var0 < 3.5/np.sqrt(n)
True
2D function
>>> xp = np.linspace(0,1,50)
>>> x, y = np.meshgrid(xp,xp)
>>> f = np.exp(x+y) + np.sin((x-2*y)*3)
>>> var0 = 0.04 # noise variance
>>> fn = f + sqrt(var0)*np.random.randn(*f.shape)
>>> s = evar(fn) # estimated variance
>>> np.abs(s-var0)/var0 < 3.5/np.sqrt(50)
True
3D function
>>> yp = np.linspace(-2,2,50)
>>> [x,y,z] = np.meshgrid(yp, yp, yp, sparse=True)
9 years ago
>>> f = x*np.exp(-x**2-y**2-z**2)
>>> var0 = 0.5 # noise variance
9 years ago
>>> fn = f + np.sqrt(var0)*np.random.randn(*f.shape)
>>> s = evar(fn) # estimated variance
>>> np.abs(s-var0)/var0 < 3.5/np.sqrt(50)
True
Other example
-------------
http://www.biomecardio.com/matlab/evar.html
Note:
----
EVAR is only adapted to evenly-gridded 1-D to N-D data.
See also
--------
VAR, STD, SMOOTHN
"""
# Damien Garcia -- 2008/04, revised 2009/10
y = np.atleast_1d(y)
d = y.ndim
sh0 = y.shape
S = np.zeros(sh0)
sh1 = np.ones((d,))
cos = np.cos
pi = np.pi
for i in range(d):
ni = sh0[i]
sh1[i] = ni
t = np.arange(ni).reshape(sh1) / ni
S += cos(pi * t)
sh1[i] = 1
S2 = 2 * (d - S).ravel()
# N-D Discrete Cosine Transform of Y
dcty2 = dctn(y).ravel() ** 2
def score_fun(L, S2, dcty2):
# Generalized cross validation score
M = 1 - 1. / (1 + 10 ** L * S2)
noisevar = (dcty2 * M ** 2).mean()
return noisevar / M.mean() ** 2
# fun = lambda x : score_fun(x, S2, dcty2)
Lopt = optimize.fminbound(score_fun, -38, 38, args=(S2, dcty2))
M = 1.0 - 1.0 / (1 + 10 ** Lopt * S2)
noisevar = (dcty2 * M ** 2).mean()
return noisevar
class _Filter(object):
def __init__(self, y, z0, weightstr, weights, s, robust, maxiter, tolz):
self.y = y
self.z0 = z0
self.weightstr = weightstr
self.s = s
self.robust = robust
self.maxiter = maxiter
self.tolz = tolz
self.auto_smooth = s is None
self.is_finite = np.isfinite(y)
self.nof = self.is_finite.sum() # number of finite elements
self.W = self._normalized_weights(weights, self.is_finite)
self.gamma = self._gamma_fun(y)
self.N = self._tensor_rank(y)
self.s_min, self.s_max = self._smoothness_limits(self.N)
# Initialize before iterating
self.Wtot = self.W
self.is_weighted = (self.W < 1).any() # Weighted or missing data?
self.z0 = self._get_start_condition(y, z0)
self.y[~self.is_finite] = 0 # arbitrary values for missing y-data
# Error on p. Smoothness parameter s = 10^p
self.errp = 0.1
# Relaxation factor RF: to speedup convergence
self.RF = 1.75 if self.is_weighted else 1.0
@staticmethod
def _tensor_rank(y):
"""tensor rank of the y-array"""
return (np.array(y.shape) != 1).sum()
@staticmethod
def _smoothness_limits(n):
"""
Return upper and lower bound for the smoothness parameter
The average leverage (h) is by definition in [0 1]. Weak smoothing
occurs if h is close to 1, while over-smoothing appears when h is
near 0. Upper and lower bounds for h are given to avoid under- or
over-smoothing. See equation relating h to the smoothness parameter
(Equation #12 in the referenced CSDA paper).
"""
h_min = 1e-6 ** (2. / n)
h_max = 0.99 ** (2. / n)
s_min = (((1 + sqrt(1 + 8 * h_max)) / 4. / h_max) ** 2 - 1) / 16
s_max = (((1 + sqrt(1 + 8 * h_min)) / 4. / h_min) ** 2 - 1) / 16
return s_min, s_max
@staticmethod
def _lambda_tensor(y):
"""
Return the Lambda tensor
Lambda contains the eigenvalues of the difference matrix used in this
penalized least squares process.
"""
d = y.ndim
Lambda = np.zeros(y.shape)
shape0 = [1, ] * d
for i in range(d):
shape0[i] = y.shape[i]
Lambda = Lambda + \
np.cos(pi * np.arange(y.shape[i]) / y.shape[i]).reshape(shape0)
shape0[i] = 1
Lambda = -2 * (d - Lambda)
return Lambda
def _gamma_fun(self, y):
Lambda = self._lambda_tensor(y)
def gamma(s):
return 1. / (1 + s * Lambda ** 2)
return gamma
@staticmethod
def _initial_guess(y, I):
# Initial Guess with weighted/missing data
# nearest neighbor interpolation (in case of missing values)
z = y
if (1 - I).any():
notI = ~I
z, L = distance_transform_edt(notI, return_indices=True)
z[notI] = y[L.flat[notI]]
# coarse fast smoothing using one-tenth of the DCT coefficients
shape = z.shape
d = z.ndim
z = dctn(z)
for k in range(d):
z[int((shape[k] + 0.5) / 10) + 1::, ...] = 0
z = z.reshape(np.roll(shape, -k))
z = z.transpose(np.roll(range(d), -1))
# z = shiftdim(z,1);
return idctn(z)
def _get_start_condition(self, y, z0):
# Initial conditions for z
if self.is_weighted:
# With weighted/missing data
# An initial guess is provided to ensure faster convergence. For
# that purpose, a nearest neighbor interpolation followed by a
# coarse smoothing are performed.
if z0 is None:
z = self._initial_guess(y, self.is_finite)
else:
z = z0 # an initial guess (z0) has been provided
else:
z = np.zeros(y.shape)
return z
@staticmethod
def _normalized_weights(weight, is_finite):
""" Return normalized weights.
Zero weights are assigned to not finite values (Inf or NaN),
(Inf/NaN values = missing data).
"""
weights = weight * is_finite
_assert(np.all(0 <= weights), 'Weights must all be >=0')
return weights / weights.max()
@staticmethod
def _studentized_residuals(r, I, h):
8 years ago
median_abs_deviation = np.median(np.abs(r[I] - np.median(r[I])))
return np.abs(r / (1.4826 * median_abs_deviation) / sqrt(1 - h))
def robust_weights(self, r, I, h):
"""Return weights for robust smoothing."""
def bisquare(u):
c = 4.685
return (1 - (u / c) ** 2) ** 2 * ((u / c) < 1)
def talworth(u):
c = 2.795
return u < c
def cauchy(u):
c = 2.385
return 1. / (1 + (u / c) ** 2)
u = self._studentized_residuals(r, I, h)
wfun = {'cauchy': cauchy, 'talworth': talworth}.get(self.weightstr,
bisquare)
weights = wfun(u)
weights[np.isnan(weights)] = 0
return weights
@staticmethod
def _average_leverage(s, N):
h = sqrt(1 + 16 * s)
h = sqrt(1 + h) / sqrt(2) / h
return h ** N
def check_smooth_parameter(self, s):
if self.auto_smooth:
8 years ago
if np.abs(np.log10(s) - np.log10(self.s_min)) < self.errp:
8 years ago
warnings.warn("""s = %g: the lower bound for s has been reached.
Put s as an input variable if required.""" % s)
8 years ago
elif np.abs(np.log10(s) - np.log10(self.s_max)) < self.errp:
8 years ago
warnings.warn("""s = %g: the Upper bound for s has been reached.
Put s as an input variable if required.""" % s)
def gcv(self, p, aow, DCTy, y, Wtot):
# Search the smoothing parameter s that minimizes the GCV score
s = 10.0 ** p
Gamma = self.gamma(s)
if aow > 0.9:
# aow = 1 means that all of the data are equally weighted
# very much faster: does not require any inverse DCT
residual = DCTy.ravel() * (Gamma.ravel() - 1)
else:
# take account of the weights to calculate RSS:
is_finite = self.is_finite
yhat = idctn(Gamma * DCTy)
residual = sqrt(Wtot[is_finite]) * (y[is_finite] - yhat[is_finite])
TrH = Gamma.sum()
RSS = linalg.norm(residual)**2 # Residual sum-of-squares
GCVscore = RSS / self.nof / (1.0 - TrH / y.size) ** 2
return GCVscore
def __call__(self, z, s):
auto_smooth = self.auto_smooth
norm = linalg.norm
y = self.y
Wtot = self.Wtot
Gamma = 1
if s is not None:
Gamma = self.gamma(s)
# "amount" of weights (see the function GCVscore)
aow = Wtot.sum() / y.size # 0 < aow <= 1
for nit in range(self.maxiter):
DCTy = dctn(Wtot * (y - z) + z)
if auto_smooth and not np.remainder(np.log2(nit + 1), 1):
# The generalized cross-validation (GCV) method is used.
# We seek the smoothing parameter s that minimizes the GCV
# score i.e. s = Argmin(GCVscore).
# Because this process is time-consuming, it is performed from
# time to time (when nit is a power of 2)
log10s = optimize.fminbound(
self.gcv, np.log10(self.s_min), np.log10(self.s_max),
args=(aow, DCTy, y, Wtot),
xtol=self.errp, full_output=False, disp=False)
s = 10 ** log10s
Gamma = self.gamma(s)
z0 = z
z = self.RF * idctn(Gamma * DCTy) + (1 - self.RF) * z
# if no weighted/missing data => tol=0 (no iteration)
tol = norm(z0.ravel() - z.ravel()) / norm(z.ravel())
converged = tol <= self.tolz or not self.is_weighted
if converged:
break
if self.robust:
# -- Robust Smoothing: iteratively re-weighted process
h = self._average_leverage(s, self.N)
self.Wtot = self.W * self.robust_weights(y - z, self.is_finite, h)
# re-initialize for another iterative weighted process
self.is_weighted = True
return z, s, converged
class SmoothNd(object):
def __init__(self, s=None, weight=None, robust=False, z0=None, tolz=1e-3,
maxiter=100, fulloutput=False):
self.s = s
self.weight = weight
self.robust = robust
self.z0 = z0
self.tolz = tolz
self.maxiter = maxiter
self.fulloutput = fulloutput
@property
def weightstr(self):
if isinstance(self._weight, str):
return self._weight.lower()
return 'bisquare'
@property
def weight(self):
if self._weight is None or isinstance(self._weight, str):
return 1.0
return self._weight
@weight.setter
def weight(self, weight):
self._weight = weight
def _init_filter(self, y):
return _Filter(y, self.z0, self.weightstr, self.weight, self.s,
self.robust, self.maxiter, self.tolz)
@property
def num_steps(self):
return 3 if self.robust else 1
def __call__(self, data):
y = np.atleast_1d(data)
if y.size < 2:
return data
_filter = self._init_filter(y)
z = _filter.z0
s = _filter.s
converged = False
for _i in range(self.num_steps):
z, s, converged = _filter(z, s)
if not converged:
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msg = """Maximum number of iterations (%d) has been exceeded.
Increase MaxIter option or decrease TolZ value.""" % (self.maxiter)
warnings.warn(msg)
_filter.check_smooth_parameter(s)
if self.fulloutput:
return z, s
return z
def smoothn(data, s=None, weight=None, robust=False, z0=None, tolz=1e-3,
maxiter=100, fulloutput=False):
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"""
SMOOTHN fast and robust spline smoothing for 1-D to N-D data.
Parameters
----------
data : array like
uniformly-sampled data array to smooth. Non finite values (NaN or Inf)
are treated as missing values.
s : real positive scalar
smooting parameter. The larger S is, the smoother the output will be.
Default value is automatically determined using the generalized
cross-validation (GCV) method.
weight : string or array weights
weighting array of real positive values, that must have the same size
as DATA. Note that a zero weight corresponds to a missing value.
robust : bool
If true carry out a robust smoothing that minimizes the influence of
outlying data.
tolz : real positive scalar
Termination tolerance on Z (default = 1e-3)
maxiter : scalar integer
Maximum number of iterations allowed (default = 100)
z0 : array-like
Initial value for the iterative process (default = original data)
Returns
-------
z : array like
smoothed data
To be made
----------
Estimate the confidence bands (see Wahba 1983, Nychka 1988).
Reference
---------
Garcia D, Robust smoothing of gridded data in one and higher dimensions
with missing values. Computational Statistics & Data Analysis, 2010.
http://www.biomecardio.com/pageshtm/publi/csda10.pdf
Examples:
--------
1-D example
>>> import matplotlib.pyplot as plt
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>>> import wafo.sg_filter as ws
>>> x = np.linspace(0, 100, 2**8)
>>> noise = np.random.randn(2**8)/10
>>> noise = ws.noise
>>> y = np.cos(x/10)+(x/50)**2 + noise
>>> y[np.r_[70, 75, 80]] = np.array([5.5, 5, 6])
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>>> y[181] = np.nan
>>> z = ws.smoothn(y) # Regular smoothing
>>> np.allclose(z[:3], [ 0.99517904, 0.99372346, 0.99079798])
True
>>> zr = ws.smoothn(y,robust=True) # Robust smoothing
>>> np.allclose(zr[:3], [ 1.01190564, 1.00976197, 1.00513244])
True
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h=plt.subplot(121),
h = plt.plot(x,y,'r.',x,z,'k',linewidth=2)
h=plt.title('Regular smoothing')
h=plt.subplot(122)
h=plt.plot(x,y,'r.',x,zr,'k',linewidth=2)
h=plt.title('Robust smoothing')
2-D example
>>> xp = np.r_[0:1:.02]
>>> [x,y] = np.meshgrid(xp,xp)
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>>> f = np.exp(x+y) + np.sin((x-2*y)*3)
>>> fn = f + np.random.randn(*f.shape)*0.5
>>> fs = smoothn(fn)
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h=plt.subplot(121),
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h=plt.contourf(xp, xp, fn)
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h=plt.subplot(122)
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h=plt.contourf(xp, xp, fs)
2-D example with missing data
>>> import wafo.demos as wd
>>> n = 256
>>> x0, y0, z0 = wd.peaks(n)
z = z0 + rand(size(y0))*2
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I = randperm(n**2)
z[I(1:n^2*0.5)] = np.NaN; # lose 1/2 of data
z[40:90, 140:190] = np.NaN; # create a hole
zs = smoothn(z)
plt.subplot(2,2,1)
plt.imagesc(y) # , axis equal off
plt.title('Noisy corrupt data')
plt.subplot(223)
plt.imagesc(z) # , axis equal off
plt.title('Recovered data ...')
plt.subplot(224)
plt.imagesc(y0) # , axis equal off
plt.title('... compared with original data')
3-D example
[x,y,z] = meshgrid(-2:.2:2);
xslice = [-0.8,1]; yslice = 2; zslice = [-2,0];
vn = x.*exp(-x.^2-y.^2-z.^2) + randn(size(x))*0.06;
subplot(121), slice(x,y,z,vn,xslice,yslice,zslice,'cubic')
title('Noisy data')
v = smoothn(vn);
subplot(122), slice(x,y,z,v,xslice,yslice,zslice,'cubic')
title('Smoothed data')
Cellular vortical flow
[x,y] = meshgrid(linspace(0,1,24));
Vx = cos(2*pi*x+pi/2).*cos(2*pi*y);
Vy = sin(2*pi*x+pi/2).*sin(2*pi*y);
Vx = Vx + sqrt(0.05)*randn(24,24); adding Gaussian noise
Vy = Vy + sqrt(0.05)*randn(24,24); adding Gaussian noise
I = randperm(numel(Vx));
Vx(I(1:30)) = (rand(30,1)-0.5)*5; adding outliers
Vy(I(1:30)) = (rand(30,1)-0.5)*5; adding outliers
Vx(I(31:60)) = NaN; missing values
Vy(I(31:60)) = NaN; missing values
Vs = smoothn(complex(Vx,Vy),'robust'); automatic smoothing
subplot(121), quiver(x,y,Vx,Vy,2.5), axis square
title('Noisy velocity field')
subplot(122), quiver(x,y,real(Vs),imag(Vs)), axis square
title('Smoothed velocity field')
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See also
-------
SmoothNd
-- Damien Garcia -- 2009/03, revised 2010/11
Visit
http://www.biomecardio.com/matlab/smoothn.html
for more details about SMOOTHN
8 years ago
"""
return SmoothNd(s, weight, robust, z0, tolz, maxiter, fulloutput)(data)
class HodrickPrescott(object):
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"""Smooth data with a Hodrick-Prescott filter.
The Hodrick-Prescott filter removes high frequency noise from data.
It has the advantage of preserving the original shape and
features of the signal better than other types of filtering
approaches, such as moving averages techniques.
Parameter
---------
w : real scalar
smooting parameter. Larger w means more smoothing. Values usually
in the [100, 20000] interval. As w approach infinity H-P will approach
a line.
Examples
--------
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>>> import wafo.sg_filter as ws
>>> t = np.linspace(-4, 4, 500)
>>> y = np.exp( -t**2 ) + np.random.normal(0, 0.05, t.shape)
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>>> ysg = ws.HodrickPrescott(w=10000)(y)
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import matplotlib.pyplot as plt
h = plt.plot(t, y, label='Noisy signal')
h1 = plt.plot(t, np.exp(-t**2), 'k', lw=1.5, label='Original signal')
h2 = plt.plot(t, ysg, 'r', label='Filtered signal')
h3 = plt.legend()
h4 = plt.title('Hodrick-Prescott')
plt.show()
References
----------
.. [1] E. T. Whittaker, On a new method of graduation. In proceedings of
the Edinburgh Mathematical association., 1923, 78, pp 88-89.
.. [2] R. Hodrick and E. Prescott, Postwar U.S. business cycles: an
empirical investigation,
Journal of money, credit and banking, 1997, 29 (1), pp 1-16.
.. [3] Kim Hyeongwoo, Hodrick-Prescott filter,
2004, www.auburn.edu/~hzk0001/hpfilter.pdf
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"""
def __init__(self, w=100):
self.w = w
def _get_matrix(self, n):
w = self.w
diag_matrix = np.repeat(
np.atleast_2d([w, -4 * w, 6 * w + 1, -4 * w, w]).T, n, axis=1)
A = spdiags(diag_matrix, np.arange(-2, 2 + 1), n, n).tocsr()
A[0, 0] = A[-1, -1] = 1 + w
A[1, 1] = A[-2, -2] = 1 + 5 * w
A[0, 1] = A[1, 0] = A[-2, -1] = A[-1, -2] = -2 * w
return A
def __call__(self, x):
x = np.atleast_1d(x).flatten()
n = len(x)
if n < 4:
return x.copy()
A = self._get_matrix(n)
return spsolve(A, x)
class Kalman(object):
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"""
Kalman filter object - updates a system state vector estimate based upon an
observation, using a discrete Kalman filter.
The Kalman filter is "optimal" under a variety of
circumstances. An excellent paper on Kalman filtering at
the introductory level, without detailing the mathematical
underpinnings, is:
"An Introduction to the Kalman Filter"
Greg Welch and Gary Bishop, University of North Carolina
http://www.cs.unc.edu/~welch/kalman/kalmanIntro.html
PURPOSE:
The purpose of each iteration of a Kalman filter is to update
the estimate of the state vector of a system (and the covariance
of that vector) based upon the information in a new observation.
The version of the Kalman filter in this function assumes that
observations occur at fixed discrete time intervals. Also, this
function assumes a linear system, meaning that the time evolution
of the state vector can be calculated by means of a state transition
matrix.
USAGE:
filt = Kalman(R, x, P, A, B=0, Q, H)
x = filt(z, u=0)
filt is a "system" object containing various fields used as input
and output. The state estimate "x" and its covariance "P" are
updated by the function. The other fields describe the mechanics
of the system and are left unchanged. A calling routine may change
these other fields as needed if state dynamics are time-dependent;
otherwise, they should be left alone after initial values are set.
The exceptions are the observation vector "z" and the input control
(or forcing function) "u." If there is an input function, then
"u" should be set to some nonzero value by the calling routine.
System dynamics
---------------
The system evolves according to the following difference equations,
where quantities are further defined below:
x = Ax + Bu + w meaning the state vector x evolves during one time
step by premultiplying by the "state transition
matrix" A. There is optionally (if nonzero) an input
vector u which affects the state linearly, and this
linear effect on the state is represented by
premultiplying by the "input matrix" B. There is also
gaussian process noise w.
z = Hx + v meaning the observation vector z is a linear function
of the state vector, and this linear relationship is
represented by premultiplication by "observation
matrix" H. There is also gaussian measurement
noise v.
where w ~ N(0,Q) meaning w is gaussian noise with covariance Q
v ~ N(0,R) meaning v is gaussian noise with covariance R
VECTOR VARIABLES:
s.x = state vector estimate. In the input struct, this is the
"a priori" state estimate (prior to the addition of the
information from the new observation). In the output struct,
this is the "a posteriori" state estimate (after the new
measurement information is included).
z = observation vector
u = input control vector, optional (defaults to zero).
MATRIX VARIABLES:
s.A = state transition matrix (defaults to identity).
s.P = covariance of the state vector estimate. In the input struct,
this is "a priori," and in the output it is "a posteriori."
(required unless autoinitializing as described below).
s.B = input matrix, optional (defaults to zero).
s.Q = process noise covariance (defaults to zero).
s.R = measurement noise covariance (required).
s.H = observation matrix (defaults to identity).
NORMAL OPERATION:
(1) define all state definition fields: A,B,H,Q,R
(2) define intial state estimate: x,P
(3) obtain observation and control vectors: z,u
(4) call the filter to obtain updated state estimate: x,P
(5) return to step (3) and repeat
INITIALIZATION:
If an initial state estimate is unavailable, it can be obtained
from the first observation as follows, provided that there are the
same number of observable variables as state variables. This "auto-
intitialization" is done automatically if s.x is absent or NaN.
x = inv(H)*z
P = inv(H)*R*inv(H')
This is mathematically equivalent to setting the initial state estimate
covariance to infinity.
Example (Automobile Voltimeter):
-------
8 years ago
>>> import wafo.sg_filter as ws
8 years ago
>>> V0 = 12 # Define the system as a constant of 12 volts
>>> h = 1 # voltimeter measure the voltage itself
>>> q = 1e-5 # variance of process noise s the car operates
>>> r = 0.1**2 # variance of measurement error
>>> b = 0 # no system input
>>> u = 0 # no system input
8 years ago
>>> filt = ws.Kalman(R=r, A=1, Q=q, H=h, B=b)
# Generate random voltages and watch the filter operate.
>>> n = 50
>>> truth = np.random.randn(n)*np.sqrt(q) + V0
>>> z = truth + np.random.randn(n)*np.sqrt(r) # measurement
>>> x = np.zeros(n)
>>> for i, zi in enumerate(z):
... x[i] = filt(zi, u) # perform a Kalman filter iteration
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import matplotlib.pyplot as plt
hz = plt.plot(z,'r.', label='observations')
# a-posteriori state estimates:
9 years ago
hx = plt.plot(x,'b-', label='Kalman output')
ht = plt.plot(truth,'g-', label='true voltage')
h = plt.legend()
h1 = plt.title('Automobile Voltimeter Example')
plt.show()
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"""
def __init__(self, R, x=None, P=None, A=None, B=0, Q=None, H=None):
self.R = R # Estimated error in measurements.
self.x = x # Initial state estimate.
self.P = P # Initial covariance estimate.
self.A = A # State transition matrix.
self.B = B # Control matrix.
self.Q = Q # Estimated error in process.
self.H = H # Observation matrix.
self.reset()
def reset(self):
self._filter = self._filter_first
def _set_A(self, n):
if self.A is None:
self.A = np.eye(n)
self.A = np.atleast_2d(self.A)
def _set_Q(self, n):
if self.Q is None:
self.Q = np.zeros((n, n))
self.Q = np.atleast_2d(self.Q)
def _set_H(self, n):
if self.H is None:
self.H = np.eye(n)
self.H = np.atleast_2d(self.H)
def _set_P(self, HI):
if self.P is None:
self.P = np.dot(np.dot(HI, self.R), HI.T)
self.P = np.atleast_2d(self.P)
def _init_first(self, n):
self._set_A(n)
self._set_Q(n)
self._set_H(n)
try:
HI = np.linalg.inv(self.H)
except:
HI = np.eye(n)
self._set_P(HI)
return HI
def _first_state(self, z):
n = np.size(z)
HI = self._init_first(n)
# initialize state estimate from first observation
x = np.dot(HI, z)
return x
def _filter_first(self, z, u):
self._filter = self._filter_main
if self.x is None:
self.x = self._first_state(z)
return self.x
n = np.size(self.x)
self._init_first(n)
return self._filter_main(z, u)
def _predict_state(self, x, u):
return np.dot(self.A, x) + np.dot(self.B, u)
def _predict_covariance(self, P):
A = self.A
return np.dot(np.dot(A, P), A.T) + self.Q
def _compute_gain(self, P):
"""Kalman gain factor."""
H = self.H
PHT = np.dot(P, H.T)
innovation_covariance = np.dot(H, PHT) + self.R
# return np.linalg.solve(PHT, innovation_covariance)
return np.dot(PHT, np.linalg.inv(innovation_covariance))
def _update_state_from_observation(self, x, z, K):
innovation = z - np.dot(self.H, x)
return x + np.dot(K, innovation)
def _update_covariance(self, P, K):
return P - np.dot(K, np.dot(self.H, P))
8 years ago
# return np.dot(np.eye(len(P)) - K * self.H, P)
def _filter_main(self, z, u):
8 years ago
""" This is the code which implements the discrete Kalman filter:
"""
P = self._predict_covariance(self.P)
x = self._predict_state(self.x, u)
K = self._compute_gain(P)
self.P = self._update_covariance(P, K)
self.x = self._update_state_from_observation(x, z, K)
return self.x
def __call__(self, z, u=0):
return self._filter(z, u)
class HampelFilter(object):
"""Hampel Filter.
HAMPEL(X,Y,DX,T,varargin) returns the Hampel filtered values of the
elements in Y. It was developed to detect outliers in a time series,
but it can also be used as an alternative to the standard median
filter.
X,Y are row or column vectors with an equal number of elements.
The elements in Y should be Gaussian distributed.
Parameters
----------
dx : positive scalar (default 3 * median(diff(X))
which defines the half width of the filter window. Dx should be
dimensionally equivalent to the values in X.
t : positive scalar (default 3)
which defines the threshold value used in the equation
|Y - Y0| > T * S0.
adaptive: real scalar
if greater than 0 it uses an experimental adaptive Hampel filter.
If none it uses a standard Hampel filter
fulloutput: bool
if True also the vectors: outliers, Y0,LB,UB,ADX, which corresponds to
the mask of the replaced values, nominal data, lower and upper bounds
on the Hampel filter and the relative half size of the local window,
respectively. outliers.sum() gives the number of outliers detected.
Examples
---------
Hampel filter removal of outliers
>>> import numpy as np
>>> randint = np.random.randint
>>> Y = 5000 + np.random.randn(1000)
>>> outliers = randint(0,1000, size=(10,))
>>> Y[outliers] = Y[outliers] + randint(1000, size=(10,))
>>> YY, res = HampelFilter(fulloutput=True)(Y)
>>> YY1, res1 = HampelFilter(dx=1, t=3, adaptive=0.1, fulloutput=True)(Y)
>>> YY2, res2 = HampelFilter(dx=3, t=0, fulloutput=True)(Y) # Y0 = median
X = np.arange(len(YY))
plt.plot(X, Y, 'b.') # Original Data
plt.plot(X, YY, 'r') # Hampel Filtered Data
plt.plot(X, res['Y0'], 'b--') # Nominal Data
plt.plot(X, res['LB'], 'r--') # Lower Bounds on Hampel Filter
plt.plot(X, res['UB'], 'r--') # Upper Bounds on Hampel Filter
i = res['outliers']
plt.plot(X[i], Y[i], 'ks') # Identified Outliers
plt.show('hold')
References
----------
Chapters 1.4.2, 3.2.2 and 4.3.4 in Mining Imperfect Data: Dealing with
Contamination and Incomplete Records by Ronald K. Pearson.
Acknowledgements
I would like to thank Ronald K. Pearson for the introduction to moving
window filters. Please visit his blog at:
http://exploringdatablog.blogspot.com/2012/01/moving-window-filters-and
-pracma.html
"""
def __init__(self, dx=None, t=3, adaptive=None, fulloutput=False):
self.dx = dx
self.t = t
self.adaptive = adaptive
self.fulloutput = fulloutput
8 years ago
@staticmethod
def _check(dx):
_assert(np.isscalar(dx), 'DX must be a scalar.')
_assert(0 < dx, 'DX must be larger than zero.')
@staticmethod
def localwindow(X, Y, DX, i):
mask = (X[i] - DX <= X) & (X <= X[i] + DX)
Y0 = np.median(Y[mask])
# Calculate Local Scale of Natural Variation
S0 = 1.4826 * np.median(np.abs(Y[mask] - Y0))
return Y0, S0
@staticmethod
def smgauss(X, V, DX):
Xj = X
Xk = np.atleast_2d(X).T
Wjk = np.exp(-((Xj - Xk) / (2 * DX)) ** 2)
G = np.dot(Wjk, V) / np.sum(Wjk, axis=0)
return G
def _adaptive(self, Y, X, dx):
localwindow = self.localwindow
Y0, S0, ADX = self._init(Y, dx)
Y0Tmp = np.nan * np.zeros(Y.shape)
S0Tmp = np.nan * np.zeros(Y.shape)
DXTmp = np.arange(1, len(S0) + 1) * dx
# Integer variation of Window Half Size
# Calculate Initial Guess of Optimal Parameters Y0, S0, ADX
for i in range(len(Y)):
j = 0
S0Rel = np.inf
while S0Rel > self.adaptive:
Y0Tmp[j], S0Tmp[j] = localwindow(X, Y, DXTmp[j], i)
if j > 0:
8 years ago
S0Rel = np.abs((S0Tmp[j - 1] - S0Tmp[j]) /
(S0Tmp[j - 1] + S0Tmp[j]) / 2)
j += 1
Y0[i] = Y0Tmp[j - 2]
S0[i] = S0Tmp[j - 2]
ADX[i] = DXTmp[j - 2] / dx
# Gaussian smoothing of relevant parameters
DX = 2 * np.median(np.diff(X))
ADX = self.smgauss(X, ADX, DX)
S0 = self.smgauss(X, S0, DX)
Y0 = self.smgauss(X, Y0, DX)
return Y0, S0, ADX
def _init(self, Y, dx):
S0 = np.nan * np.zeros(Y.shape)
Y0 = np.nan * np.zeros(Y.shape)
ADX = dx * np.ones(Y.shape)
return Y0, S0, ADX
def _fixed(self, Y, X, dx):
localwindow = self.localwindow
Y0, S0, ADX = self._init(Y, dx)
for i in range(len(Y)):
Y0[i], S0[i] = localwindow(X, Y, dx, i)
return Y0, S0, ADX
def _filter(self, Y, X, dx):
if len(X) <= 1:
Y0, S0, ADX = self._init(Y, dx)
elif self.adaptive is None:
Y0, S0, ADX = self._fixed(Y, X, dx)
else:
Y0, S0, ADX = self._adaptive(Y, X, dx) # 'adaptive'
return Y0, S0, ADX
def __call__(self, y, x=None):
Y = np.atleast_1d(y).ravel()
if x is None:
x = range(len(Y))
X = np.atleast_1d(x).ravel()
dx = 3 * np.median(np.diff(X)) if self.dx is None else self.dx
self._check(dx)
Y0, S0, ADX = self._filter(Y, X, dx)
YY = Y.copy()
T = self.t
# Prepare Output
self.UB = Y0 + T * S0
self.LB = Y0 - T * S0
outliers = np.abs(Y - Y0) > T * S0 # possible outliers
np.putmask(YY, outliers, Y0) # YY[outliers] = Y0[outliers]
self.outliers = outliers
self.num_outliers = outliers.sum()
self.ADX = ADX
self.Y0 = Y0
if self.fulloutput:
return YY, dict(outliers=outliers, Y0=Y0,
LB=self.LB, UB=self.UB, ADX=ADX)
return YY
if __name__ == '__main__':
from wafo.testing import test_docstrings
test_docstrings(__file__)