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lakeator.py
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lakeator.py
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import pickle
import zipfile
import requests
import xml.etree.ElementTree as ET
import numpy as np
import scipy.linalg as la
import scipy.io.wavfile as wav
from matplotlib import (pyplot as plt, image as mpimg)
from scipy.interpolate import interp1d
from itertools import combinations
from scipy.signal import fftconvolve
from scipy.linalg import eigh
from scipy import signal
from numpy import dot, sqrt, argsort, abs
from motionless import DecoratedMap, LatLonMarker
from PIL import Image
from pyproj import Transformer
# """
# This messy code is here because I couldn't get pyfftw installed on my Windows OS, but got it fine on my Linux OS.
# Essentially, I wanted the Locator to use pyfftw when it was available, or numpy's fft module otherwise.
# """
wf = False
pftw = False
try:
raise ImportError
import pyfftw.interfaces.numpy_fft as fft_pack
import pyfftw
pftw = True
pyfftw.interfaces.cache.enable()
try:
with open('pyfftw_wisdom.txt', 'rb') as wizfile:
pyfftw.import_wisdom(pickle.load(wizfile))
wf = True
except:
pass
except ImportError as e:
print(e)
import numpy.fft as fft_pack
class Lakeator:
"""Used to locate the source of a sound in a multi-track .wav file.
The lakeator class may also be used to generate simulated data by means of the shift_sound method, which
takes in a mono wav file and a set of coordinates and produces a multi-track wav simulating the data which
would have been recorded were the signal to have came from the provided location.
Parameters
----------
mic_locations : array
This is an Mx2 array containing the x,y coordinates of the M microphones in the array.
file_path : str
If provided, the file at this filepath will be loaded into the lakeator.
Attributes
----------
sound_speed : float
The speed of sound in air. Defaults to 343.1 m/s.
data : np.array
Numpy array to store the loaded data. Left public for convenience.
sample_rate : int
The sample rate of the currently loaded WAV file.
"""
sample_rate: int = None
"""The sample rate of the currently loaded data."""
data: np.array = None
"""The current data, stored in a numpy array."""
sound_speed: float = 343.1
"""The speed of sound in air to use in the calculations."""
_hm_domain_ = None
_radial_domain_ = None
_cor_fns_ = {}
_mic_pairs_ = None
_GCC_proc_ = ""
def __init__(self, mic_locations=((0.325, 0.000), (-0.160, 0.248), (-0.146, -0.258), (-0.001, 0.002)),
file_path=None):
"""Initialise the Locator. If you pass in a file path "example.wav" here it will call self.load(example.wav).
Parameters
----------
mic_locations : (Mx2 tuple)
Matrix of microphone coordinates, in meters, relative to the center of the array.
file_path : (None/string)
If present, will call self.load() on the given file path with the default load parameters
"""
self.epsg=2193
self.mics = np.array(mic_locations)
self._mic_pairs_ = np.array(
[p for p in combinations(np.arange(0, self.mics.shape[0], dtype="int16"), 2)])
self.maxdist = np.max(np.linalg.norm(self.mics, axis=1))
self.spatial_nyquist_freq = self.sound_speed/(2*self.maxdist)
if file_path:
self.load(file_path)
def load(self, file_path, normalise: bool=True, GCC_processor="p-PHAT", do_FFTs=True, filter_f=(False, False), rho=0.73):
"""Loads the data from the .wav file, and computes the inter-channel correlations.
Correlations are computed, interpolated, and then stored within the lakeator
object for use in the optimisation function or wherever necessary. Pass in a numpy array of data rather than
loading from a file by setting raw_data = True.
Parameters
----------
file_path : str
The file path of the WAV file to be read.
normalise : bool
Normalise the data? This is a good idea, hence the truthy default state.
GCC_processor : str
Which GCC processor to use. Options are: CC, PHAT, Scot, & RIR. See Table 1 of Knapp, C. et. al. (1976) "The Generalised Correlation Method for Estimation of Time Delay"
do_FFTs : bool
Calculate the cross-correlations? Worth turning off to save time if only MUSIC-based algorithms are to be used.
filter_f : (float, float)
Tuple of frequencies (in Hertz) between which to apply a bandpass filter.
"""
self.rho = rho
global wf, pftw
self._GCC_proc_ = GCC_processor
if isinstance(file_path, str):
self.sample_rate, data = wav.read(file_path)
else:
data = file_path[1]
self.sample_rate = file_path[0]
# Convert from integer array to floating point to allow for computation
data = data.astype('float64')
if filter_f[0]:
assert isinstance(filter_f[0], float)
w = filter_f[0]/(self.sample_rate/2)
b, a = signal.butter(5, w, 'highpass')
for i in range(data.shape[1]):
data[:, i] -= signal.filtfilt(b, a, data[:, i], padlen=data.shape[0]-3)
if filter_f[1]:
assert isinstance(filter_f[1], float)
w = filter_f[1]/(self.sample_rate/2)
b, a = signal.butter(5, w, 'lowpass')
for i in range(data.shape[1]):
data[:, i] -= signal.filtfilt(b, a, data[:, i], padlen=data.shape[0]-3)
# Normalise the data
if normalise:
for i in range(data.shape[1]):
data[:, i] -= data[:, i].mean()
# Store appropriately
self.data = data
if do_FFTs:
temp_pad = np.concatenate(
(data, np.zeros(((2**(np.ceil(np.log2(data.shape[0])))-data.shape[0]).astype('int32'), data.shape[1]))),
0)
c = 1
for prdx in np.arange(0, self._mic_pairs_.shape[0]):
pr = self._mic_pairs_[prdx, :]
self._cor_fns_["{}".format(pr)] = self._create_interp_(self.mics[pr[0], :], self.mics[pr[1], :],
temp_pad[:, pr[0]], temp_pad[:, pr[1]])
c += 1
if pftw and not wf:
with open('pyfftw_wisdom.txt', 'wb') as f:
pickle.dump(pyfftw.export_wisdom(), f)
wf = True
def _whiten_signal_(self):
for idx in np.arange(self.mics.shape[0]):
t = np.fft.rfft(self.data[:,idx])
self.data[:, idx] = np.fft.irfft(t/abs(t), n=2*len(t)-1)
def _create_interp_(self, mic1, mic2, mic1data, mic2data, buffer_percent=-10.0, res_scaling=5):
"""This function is to create the cubic interpolants for use in the correlation function. Uses GCC.
Arguments:
mic1 (int): The index of the first microphone of interest.
mic2 (int): The index of the second microphone of interest.
mic1data (np.array): The data corresponding to the first microphone.
mic2data (np.array): The data corresponding to the second microphone.
buffer_percent (float): The percent headroom to give the correlation function to avoid out-of-range exceptions.
res_scaling (float): Scales the resolution
"""
dlen = len(mic1data)
num_samples = la.norm(mic1-mic2)*(1+buffer_percent/100.0)*(1/self.sound_speed)*self.sample_rate
num_samples = int(round(num_samples))
if buffer_percent < 0:
num_samples = dlen-1
n = 2*dlen
X1 = fft_pack.rfft(mic1data, n=n)
X2 = fft_pack.rfft(mic2data, n=n)
X2star = np.conj(X2)
# TODO: Implement more processors (Eckart, ML/HT)
if self._GCC_proc_== "PHAT":
corr = fft_pack.irfft(np.exp(1j*np.angle(X1 * X2star)), n=(res_scaling * n))
elif self._GCC_proc_== "p-CSP" or self._GCC_proc_== "p-PHAT":
proc = 1.0/(abs(X1*X2star)**self.rho)
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
elif self._GCC_proc_== "CC":
proc = 1.0
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
elif self._GCC_proc_== "RIR":
proc = 1.0/(X1*np.conj(X1))
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
elif self._GCC_proc_== "SCOT":
proc = 1.0/sqrt((X1*np.conj(X1))*(X2*X2star))
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
elif self._GCC_proc_== "HB":
proc = abs(X1*np.conj(X2))/(X1*np.conj(X1)*X2*np.conj(X2))
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
elif self._GCC_proc_[:3].lower() == 'bit':
# f_weighting = pickle.load("./bitpsd")
with open("./bitpsd", 'rb') as f:
f_weighting = pickle.load(f)
# print(f_weighting, type(f_weighting))
proc = f_weighting(np.fft.rfftfreq(n)*self.sample_rate)
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
else:
# Defaults to regular CC.
proc = 1.0
corr = fft_pack.irfft(X1 * X2star * proc, n=(res_scaling * n))
corr = np.concatenate((corr[-int(res_scaling*n/2):], corr[:int(res_scaling*n/2)+1]))
corrxs = np.arange(start=(dlen-num_samples)*res_scaling, stop=(dlen+num_samples)*res_scaling, step=1,
dtype='int32')
cInterp = interp1d(x=(corrxs/res_scaling-dlen)+1, y=corr[corrxs], kind='cubic')
return cInterp
def _objective_(self, X, Y):
"""This function takes a matrix/vector of each x and y coordinates, and at each location evaluates the sum of the generalised
cross-correlations between the microphone data as if the signal had come from that location. In this way we can search
for the point with maximum correlation, which should correspond to the most likely actual source position.
Args:
X (np.array): An n by m matrix of x-coordinates of points at which to evaluate the _objective_ function
Y (np.array): An n by m matrix of Y-coordinates of points at which to evaluate the _objective_ function
Returns:
np.array: An n by m matrix of signal correlations corresponding to the source having originated at each point
generated by the input coordinates
"""
# Calculate distances
ds = [sqrt((X-self.mics[i, 0])**2+(Y-self.mics[i, 1])**2) for i in
np.arange(0, self.mics.shape[0], dtype="int16")]
# Calculate times, then pass the times into the correlation functions and sum them
ts = np.array([self._cor_fns_["{}".format(ps)]((ds[ps[0]] - ds[ps[1]]) * self.sample_rate / self.sound_speed) for ps in
self._mic_pairs_])
return np.sum(ts, axis=0)
def estimate_DOA_heatmap(self, method, xrange=(-50, 50), yrange=(-50, 50), xstep=False, ystep=False, colormap="bone", shw=True,
block_run=True, no_fig=False, freq=False, signals=1, AF_freqs=(False, False), f_0=-1, array_GPS=False, save_GIS=False):
"""Displays a heatmap for visual inspection of correlation-based location estimation.
Generates a grid of provided dimension/resolution, and evaluates the selected DOA-estimation at each point on the grid.
Vectorised for fast execution.
Parameters
----------
method : str
One of; "GCC", "MUSIC" or "AF-MUSIC". The method to be used in heatmap generation.
xrange : (float, float)
The lower and upper bound in the x-direction.
yrange : (float, float)
The lower and upper bound in the y-direction.
xstep : float
If given, determines the size of the steps in the x-direction. Otherwise defaults to 1000 steps.
ystep : float
If given, determines the size of the steps in the y-direction. Otherwise defaults to 1000 steps.
colormap : str
The colour map for the heatmap. See https://matplotlib.org/examples/color/colormaps_reference.html
shw : bool
If False, return the axis object rather than display.
block_run : bool
Pause execution of the file while the figure is open? Set to True for running in the command-line.
no_fig : bool
If True, return the heatmap grid rather than plot it.
freq : float
Frequency, in Hz, at which to calculate the MUSIC spectrum.
signals : int
The number of signals to be localised. Only relevant for MUSIC-based methods.
AF_freqs : (float, float)
Lower and upper bounds on the frequencies (in Hz) at which to evaluate the AF-MUSIC algorithm.
f_0 : float
The reference frequency at which to calculate AF-MUSIC. Default of -1 uses the the midway point between AF_freqs.
array_GPS : (float, float)
False, or tuple of GPS lat/long.
save_GIS : bool
Save the image as a tif wth a corresponding .tif.points file for use in GIS software? Requires array_GPS
Returns
-------
np.array
Returns EITHER the current (filled) heatmap domain if no_fig == True, OR a handle to the displayed figure.
"""
if (xstep and ystep):
xdom = np.linspace(start=xrange[0], stop=xrange[1], num=int((xrange[1] - xrange[0])//xstep))
ydom = np.linspace(start=yrange[0], stop=yrange[1], num=int((yrange[1] - yrange[0])//ystep))
else:
xdom = np.linspace(start=xrange[0], stop=xrange[1], num=1000)
ydom = np.linspace(start=yrange[0], stop=yrange[1], num=1000)
self._hm_domain_ = np.zeros((len(ydom), len(xdom)))
xdom, ydom = np.meshgrid(xdom, ydom)
self._hm_corners_ = np.array([[[xrange[0], yrange[1]], [xrange[1], yrange[1]]],[[xrange[0], yrange[0]], [xrange[1], yrange[0]]]])
if method.upper() == "AF-MUSIC" or method.upper() == "AF_MUSIC":
self.dataFFT = fft_pack.rfft(self.data, axis=0, n=2*self.data.shape[0])
self._hm_domain_ = self._AF_MUSIC_subset(xdom, ydom, freqs=AF_freqs, focusing_freq=f_0)
elif method.upper() == "MUSIC":
assert freq, "Frequency must be provided for MUSIC calculation"
pos = fft_pack.rfftfreq(2*self.data.shape[0])*self.sample_rate
actidx = np.argmin(abs(pos-freq))
self.dataFFT = fft_pack.rfft(self.data, axis=0, n=2*self.data.shape[0])
self._hm_domain_ = self._MUSIC2D_((pos[actidx], actidx), xdom, ydom, numsignals=signals)
elif method.upper() == "GCC":
self._hm_domain_ = self._objective_(xdom, ydom)
else:
print("Method not recognised. Defaulting to GCC.")
self._hm_domain_ = self._objective_(xdom, ydom)
if no_fig:
return self._hm_domain_
plt.imshow(self._hm_domain_, cmap=colormap, interpolation='none', origin='lower',
extent=[xrange[0], xrange[1], yrange[0], yrange[1]])
plt.colorbar()
plt.xlabel("Horiz. Dist. from Center of Array [m]")
plt.ylabel("Vert. Dist. from Center of Array [m]")
plt.title("{}-based Source Location Estimate".format(method))
if shw:
plt.show(block=block_run)
return
else:
return plt.imshow(self._hm_domain_, cmap=colormap, interpolation='none', origin='lower',
extent=[xrange[0], xrange[1], yrange[0], yrange[1]])
def heatmap_to_GIS(self, array_coords, EPSG, projected_EPSG=2193, target_EPSG=3857, filepath="./heatmap.tif"):
"""Export the current heatmap domain to ./heatmap.tif, as well as an auxillary CPS file ./heatmap.tif.points
which contains the georeferencing data for QGIS. Converts from `EPSG' to `target_EPSG' (default NZTM2000)
(default WGS84/Pseudo-Mercator; the "Web Mecator Projection")
If changing target_EPSG, must be in cartesian coordinates to allow for addition of array_coords to bounding box dimensions.
Parameters
----------
array_coords : (float, float)
The GPS coordinates of the center of the array (i.e. (0.0, 0.0)) in the order governed by ISO19111 (see https://proj.org/faq.html#why-is-the-axis-ordering-in-proj-not-consistent).
EPSG : int
The EPSG code for the coordinate system which array_coords is in. See https://epsg.io/ for help finding the code.
projected_EPSG : int
A local projected EPSG code. May be the same as the 'EPSG' argument, or may be different. This is used for calculation of the heatmap bounds.
target_EPSG : int
The EPSG of your QGIS project. This will be the coordinate system in which the georeferencing data will be saved.
filepath : str
The filepath for the saved heatmap output.
"""
imdata = self._hm_domain_ - np.min(self._hm_domain_)
imdata = 255.0*imdata/np.max(imdata)
imdata = imdata[::-1,:]
im = Image.fromarray(imdata.astype(np.uint8))
im.save('{}'.format(filepath))
# print("EPSG, projected_EPSG, target_EPSG:", EPSG, projected_EPSG, target_EPSG)
with open("{}.points".format(filepath), 'w') as w:
ts1 = Transformer.from_crs(EPSG, projected_EPSG, always_xy=True)
xt, yt = ts1.transform(array_coords[0], array_coords[1])
# print(xt, yt)
ts2 = Transformer.from_crs(projected_EPSG, target_EPSG, always_xy=True)
test = []
w.write("mapX,mapY,pixelX,pixelY,enable,dX,dY,residual\n")
# print("array_coords", array_coords)
(xs, ys, _) = ts1.transform(array_coords[0], array_coords[1], tt=2020.0)
# print("Array coords in projected EPSG:", xs, ys)
# print("self._hm_corners_:", self._hm_corners_)
xp, yp, _, _ = ts2.transform(xx=xs+self._hm_corners_[1,0,0], yy=ys+self._hm_corners_[1,0,1], zz=0, tt=2020.0)
# print("xs+self._hm_corners_[1,0,0], ys+self._hm_corners_[1,0,1]:", self._hm_corners_[1,0,0], self._hm_corners_[1,0,1])
# print("xp, yp:", xp, yp)
test.append([xp, yp])
w.write("{},{},{},{},1,0,0,0\n".format(xp, yp, 0, -self._hm_domain_.shape[1]+1))
xp, yp, _, _ = ts2.transform(xx=xs+self._hm_corners_[0,0,0], yy=ys+self._hm_corners_[0,0,1], zz=0, tt=2020.0)
# print("xs+self._hm_corners_[0,0,0], ys+self._hm_corners_[0,0,1]:", self._hm_corners_[0,0,0], self._hm_corners_[0,0,1])
# print("xp, yp:", xp, yp)
test.append([xp, yp])
w.write("{},{},{},{},1,0,0,0\n".format(xp, yp, 0, 0))
xp, yp, _, _ = ts2.transform(xx=xs+self._hm_corners_[0,1,0], yy=ys+self._hm_corners_[0,1,1], zz=0, tt=2020.0)
# print("xs+self._hm_corners_[0,1,0], ys+self._hm_corners_[0,1,1]:", self._hm_corners_[0,1,0], self._hm_corners_[0,1,1])
# print("xp, yp:", xp, yp)
test.append([xp, yp])
w.write("{},{},{},{},1,0,0,0\n".format(xp, yp, self._hm_domain_.shape[0]-1, 0))
xp, yp, _, _ = ts2.transform(xx=xs+self._hm_corners_[1,1,0], yy=ys+self._hm_corners_[1,1,1], zz=0, tt=2020.0)
# print("xs+self._hm_corners_[1,1,0], ys+self._hm_corners_[1,1,1]:", self._hm_corners_[1,1,0], self._hm_corners_[1,1,1])
# print("xp, yp:", xp, yp)
test.append([xp, yp])
w.write("{},{},{},{},1,0,0,0".format(xp, yp, self._hm_domain_.shape[0]-1, -self._hm_domain_.shape[1]+1))
def _polynom_steervec(self, samples, max_tau=1500):
"""Takes a vector of M desired delays and a maximum lag parameter max_tau, and returns the (M, 1, 2*max_tau+1)
polynomial steering vector which contains the z-transform of the fractional delay filters necessary to delay each
channel of a M-channel audio file by the corresponding delay parameter from the input vector. For example,
polynom_steervec([1.2, 3, np.pi]) may be used to delay the first channel of a three-channel audio clip by 1.2 samples,
the second channel by 3, and the third channel by approximately pi samples.
Parameters
----------
samples : np.array
A 1D array of the desired delay amounts
max_tau : int
The maximum lag in either direction for the fractional delay filters. A higher number will be more accurate, but take longer to use.
Returns
-------
np.array
A vector containing the desired fractional delay filters.
"""
mics = self.mics
tau = samples
tau.shape = (tau.shape[0], 1)
Az = np.sinc((np.tile(np.arange(-max_tau, max_tau + 1), (mics.shape[0], 1)) - tau))
Az = np.reshape(Az, (mics.shape[0], 1, Az.shape[-1]))
return Az
def shift_sound(self, location, inputfile, output_filename, noisescale=0):
"""Creates a multi-track wav file from a mono one, simulating the array recordings had the sound came from the
provided location and were recorded on the current virtual array's microphone configuration.
Saves the resultant file in the current working directory with the provided filename, at the same sample rate as the input data.
Parameters
----------
location : (float, float)
A tuple (x,y) providing the location in meters relative to the array at which to simulate the sound as having came from.
inputfile : str
File path for the mono wav file to be used.
output_filename : str
The desired file name for the output file.
noisescale : float
Adds Gaussian white noise with standard deviation noisescale*(standard deviation of input file)
"""
[spl, dt] = wav.read(inputfile)
dt = (dt - np.mean(dt))/np.std(dt)
loc_dif = self.mics - np.tile(location, (self.mics.shape[0], 1))
dists = np.linalg.norm(loc_dif, axis=1)
samples = (dists*spl)/self.sound_speed
samples -= min(samples)
fracsamples = samples % 1
intsamples = samples - fracsamples
svs = self._polynom_steervec(fracsamples)
t = np.tile(dt.T, (self.mics.shape[0], 1))
t.shape = (t.shape[0], 1, t.shape[1])
xout = []
for r in np.arange(t.shape[0]):
xout.append(fftconvolve(t[r, 0, :], svs[r, 0, :]))
xout = np.array(xout)
xout = np.hstack((xout, np.zeros((xout.shape[0], int(np.max(intsamples))))))
for idx in np.arange(xout.shape[0]):
xout[idx,:] = np.roll(xout[idx,:], int(intsamples[idx]))
if noisescale != 0:
xout += np.random.normal(0, noisescale*sqrt(np.var(xout)), size=xout.shape)
xout *= (2**15-1)/np.max(abs(xout))
xout = xout.astype('int16')
wav.write(output_filename, spl, xout.T)
def _MUSIC1D_(self, freqtup, theta, numsignals=1, SI=None):
"""Vectorised implementation of the Multiple Signal Classification algorithm for DOA eastimation.
Arguments:
freqtup (float, int): The frequency at which to evaluate the MUSIC algorithm, and the index at where to find it in the FFT of the data.
theta (float/np.array): The angle of arrial at which to evaluate the MUSIC algorithm. May be a 1D numpy array.
numsignals (int): How many signals to localise.
SI (np.array): The covariance matrix S, if known a priori.
"""
freq, idx = freqtup
incidentdir = np.array([-np.cos(theta), -np.sin(theta)])
tau = dot(self.mics, incidentdir) / self.sound_speed
# Populate a(theta)
a = np.exp(-1j * 2 * np.pi * freq * tau)
# Find variance/covariance matrix S=conj(X.X^H)
# Where X = FFT(recieved vector x)
if type(SI) == type(None):
S = dot(self.dataFFT[idx:idx+1, :].T, np.conj(self.dataFFT[idx:idx+1, :]))
else:
S = SI
# Find eigen-stuff of S
lam, v = la.eig(S)
# Should be real as S Hermitian, rounding problems
# mean imaginary part != 0. Take real part.
lam = lam.real
# Find a sorting index list
xs = argsort(lam).astype("int16")
# print(lam[xs])
# Take the Eigenvectors corresponding to the
# 'numsignals' lowest Eigenvalues
EN = v[:, xs[:len(xs)-numsignals]]
# Calculate 1/P_MU
p = dot(dot(np.conj(a.T), EN), dot(np.conj(EN.T), a))
# If more than 1D find relevant entries and flatten
if len(p.shape) > 1:
p = np.ndarray.flatten(np.diag(p))
# Return P_MU
return 1/p.real, lam[xs[-1]]
def _MUSIC2D_(self, freqtup, X, Y, numsignals=1, SI=None):
"""Vectorised 2D implementation of the Multiple Signal Classification algorithm for DOA eastimation.
Arguments:
freqtup (float, int): The frequency at which to evaluate the MUSIC algorithm, and the index at where to find it in the FFT of the data.
X (np.array): An array of x-locations at which to evaluate. Should be the counterpart to Y, as in np.meshgrid
Y (np.array): An array of y-locations at which to evaluate. Should be the counterpart to X, as in np.meshgrid
numsignals (int): How many signals to localise.
SI (np.array): The covariance matrix S, if known a priori.
"""
# print(X.shape, Y.shape)
crds = np.dstack((X, Y))
crds = np.stack([crds for _ in range(self.mics.shape[0])], 3)
delm = np.linalg.norm(crds[:, :]-self.mics.T, axis=2)/self.sound_speed
freq, idx = freqtup
# Populate a(r, theta)
a = np.exp(-1j*2*np.pi*freq*delm)
# Find variance/covariance matrix S=X.X^H
# Where X = FFT(recieved vector x)
if type(SI)==type(None):
S = dot(self.dataFFT[idx:idx+1, :].T, np.conj(self.dataFFT[idx:idx+1, :]))
else:
S = SI
# Find eigen-stuff of S
lam, v = la.eigh(S)
# Should be real as S Hermitian, rounding problems
# mean imaginary part != 0. Take real part.
lam = lam.real
# Find a sorting index list
xs = argsort(lam).astype("int16")
# Take the Eigenvectors corresponding to the
# 'numsignals' lowest Eigenvalues
EN = v[:, xs[:len(xs)-numsignals]]
# Calculate 1/P_MU
p = dot(a, np.conj(EN))*dot(np.conj(a), EN)
p = np.sum(p, axis=-1, keepdims=False)
# print(p.shape)
# Return P_MU
return 1/p.real
def _transpose_(self, mult):
"""
"""
assert self.data is not None, "No data loaded yet."
datatr = np.zeros((self.data.shape[0]*mult, self.data.shape[1]))
tt = self.data.shape[0]/self.sample_rate
fc = self.sample_rate/(2*mult)
w = fc / (self.sample_rate / 2)
b_bl, a_bl = signal.butter(10, w, 'low')
for ch in np.arange(self.data.shape[1]):
sig = interp1d(np.linspace(0, tt, num=self.data.shape[0], endpoint=True),
self.data[:,ch], kind="cubic", assume_sorted=True)
d = sig(np.linspace(0, tt, self.sample_rate*mult*tt, endpoint=True))
datatr[:, ch] = signal.filtfilt(b_bl, a_bl, d, axis=0)
# datatr[:, ch] = d
wav.write(data=datatr.astype('int16'), rate=self.sample_rate, filename="./scarynoise.wav")
_, dnew = wav.read("./scarynoise.wav")
return dnew
def _UfitoRyy_(self, Rxx, f):
"""Returns the covariance matrix of the data at frequency f (Hz), shifted to the focussing frequency f_0. These
should be summed over all frequencies of interest to create the universally focussed sample covariance matrix
R_{yy} for the AF-MUSIC algorithm.
Arguments:
f (int): The frequency index to work with from the FFT of the data
"""
df = self.dataFFT[:, f:f+1]
ta = dot(df, df.conj().T)
ui, Ufi = eigh(Rxx, check_finite=False)
ui = ui.real
sortarg = argsort(abs(ui))[::-1]
Ufi = Ufi[:, sortarg]
Tauto = (dot(self.Uf0, Ufi.conj().T)) / sqrt(self.numbins)
Y = dot(Tauto, df)
Ryy = dot(Y, Y.conj().T)
return Ryy*abs(ui[sortarg[0]])
def _AF_MUSIC_subset(self, xdom, ydom, focusing_freq=-1, npoints=1000, signals=1, shw=True, block_run=True, chunks=10, freqs=(False, False)):
"""Display a polar plot of estimated DOA using the MUSIC algorithm
Arguments:
focusing_freq (float): The frequency (in Hz) at which to perform the calculation. If <0, will default to 0.9*(spatial Nyquist frequency)
npoints (int): The total number of points around the circle at which to evaluate.
signals (int): The numbers of signals to locate.
shw (bool): Show the plot? If False, will return the data that was to be plotted.
block_run (bool): Pause execution of the file while the figure is open? Set to True for running in the command-line.
chunks (int): How many sections to split the data up into. Will split up the data and average the result over the split sections
"""
# print("beggining subset routine")
if focusing_freq < 0:
if freqs[0]:
if freqs[1]:
focusing_freq = (freqs[0]+freqs[1])/2.0
else:
focusing_freq = (self.sample_rate + freqs[0])/2.0
else:
if freqs[1]:
focusing_freq = freqs[1]/2.0
else:
focusing_freq = self.sample_rate/4.0
# print(focusing_freq, freqs)
# Split the data up into "chunks" sections
indices = [int(x) for x in np.linspace(0, self.data.shape[0], num=int(chunks+1), endpoint=True)]
# The frequencies for Tauto and DFT. They all have the same length so this is fine to do outside the loop
pos = fft_pack.rfftfreq(self.data.shape[0]) * self.sample_rate
if freqs[0]:
pos = pos[pos >= freqs[0]]
LHSl = self.data.shape[0]//2+1-len(pos)
else:
LHSl = 0
if freqs[1]:
pos = pos[pos <= freqs[1]]
RHSl = len(pos) + LHSl
else:
RHSl = len(pos)
# print("found lhs1 and rhs1")
# Rxx will go in here
Rxx = np.zeros((self.mics.shape[0], self.mics.shape[0], self.data.shape[0]//2+1) , dtype="complex128")
# Calculate Rxx
for mark in np.arange(len(indices)-1):
dcr = self.data[indices[mark]:indices[mark+1], :]
for chnl in np.arange(dcr.shape[1]):
dcr[:, chnl] *= np.blackman(dcr.shape[0])
# dft is RFFT of current data chunk
dft = fft_pack.rfft(dcr, axis=0, n=self.data.shape[0]).T
dft.shape = (dft.shape[0], 1, dft.shape[1])
# print(dft.shape, self.data.shape, Tauto.shape)
Rxx += np.einsum("jin,iln->jln", dft, np.conj(np.transpose(dft, (1,0,2))))/chunks
# print("calculated Rxx")
# focusing_freq_index is the index along dft and Tauto to find f_0
focusing_freq_index = np.argmin(abs(pos - focusing_freq)) + LHSl
eig_f0, v_f0 = np.linalg.eigh(Rxx[:,:,focusing_freq_index])
Uf0 = v_f0[:, argsort(abs(eig_f0))[::-1]]
# Calculate Tautos
# Tauto will go in here
Tauto = np.zeros((self.mics.shape[0], self.mics.shape[0], len(pos)) , dtype="complex128")
# Ufi will go in here
Ufi = np.zeros((self.mics.shape[0], self.mics.shape[0], self.data.shape[0]//2+1) , dtype="complex128")
for indx, fi in enumerate(pos):
eig_fi, v_fi = np.linalg.eigh(Rxx[:, :, indx+LHSl])
Ufi[:,:,indx] = v_fi[:, argsort(abs(eig_fi))[::-1]]
Tauto[:,:,indx] = dot(Uf0, np.conj(Ufi[:,:,indx].T))/sqrt(pos.shape[0])
# Calculate Ryy
# Ryy will go in here
Ryy = np.zeros((self.mics.shape[0], self.mics.shape[0], len(pos)), dtype="complex128")
# chunks=1.0
indices = [int(x) for x in np.linspace(0, self.data.shape[0], num=int(chunks + 1), endpoint=True)]
for mark in np.arange(len(indices) - 1):
dcr = self.data[indices[mark]:indices[mark + 1], :]
for chnl in np.arange(dcr.shape[1]):
dcr[:, chnl] *= np.blackman(dcr.shape[0])
# dft is RFFT of current data chunk
dft = fft_pack.rfft(dcr, axis=0, n=self.data.shape[0]).T
# print(dft.shape)
dft = dft[:, LHSl:RHSl]
dft.shape = (dft.shape[0], 1, dft.shape[1])
# print(dft.shape, Tauto.shape, LHSl, RHSl)
Yi = np.einsum("abc,bdc->adc", Tauto, dft)
Ryy += np.einsum("jin,iln->jln", Yi, np.conj(np.transpose(Yi, (1, 0, 2)))) / chunks
Rcoh = np.sum(Ryy, axis=-1)/(len(pos))
rest = self._MUSIC2D_((focusing_freq, focusing_freq_index), xdom, ydom, SI=Rcoh)
return rest
def _get_path(self, GEarthFile, array_center, draw=True):
try:
tree = ET.parse('./data/extr/{}.kmz/doc.kml'.format(GEarthFile))
except FileNotFoundError as e:
print("Unzipping .kmz file to ./data/extr/{}.kmz/doc.kml".format(GEarthFile))
with zipfile.ZipFile("./data/{}.kmz".format(GEarthFile), 'r') as zip_ref:
zip_ref.extractall("./data/extr/{}.kmz/".format(GEarthFile))
tree = ET.parse('./data/extr/{}.kmz/doc.kml'.format(GEarthFile))
root = tree.getroot()
coords_str = root[0][-1][-1][-1].text.strip()
coords = list(map(lambda x: x.split(","), coords_str.split(" ")))
coords = np.array(coords).astype(np.float64)
coords *= np.pi/180.0
array_center = np.array(array_center)
array_center *= np.pi/180.0
xy_coords, xy_array = _stereo_proj(coords, array_center)
if False:
plt.scatter(xy_coords[:,0], xy_coords[:,1])
plt.scatter(self.mics[:,0], self.mics[:,1])
plt.xlim([np.min(xy_coords[:,0]), np.max(xy_coords[:,0])])
plt.ylim([np.min(xy_coords[:,1]), np.max(xy_coords[:,1])])
plt.title("{} Stereographic Projection".format(GEarthFile))
plt.xlabel(r"x [m] East/West")
plt.ylabel(r"y [m] North/South")
plt.show()
xfunct = interp1d(x=np.linspace(0, 1, num=xy_coords.shape[0]), y=xy_coords[:,0], kind="linear")
yfunct = interp1d(x=np.linspace(0, 1, num=xy_coords.shape[0]), y=xy_coords[:,1], kind="linear")
pts = lambda x: (xfunct(x), yfunct(x))
return pts
def estimate_DOA_path(self, method, path=lambda x: (np.cos(2*np.pi*x), np.sin(2*np.pi*x)), array_GPS=False, npoints=2500, map_zoom=20, map_scale=2, freq=False, AF_freqs=(False, False)):
"""Gives an estimate of the source DOA along the `path` provided, otherwise along the unit circle if `path` is not present.
Parameters
----------
method : str
One of; "GCC", "MUSIC", or "AF-MUSIC". The method to use for DOA estimation.
path : str/function
A filepath to a saved Google Earth path (in .kmz form), else a function f: [0,1]->R^2 to act as a parametrisation of the path at which to evaluate the DOA estimator.
npoints : int
The number of points along the path to sample.
array_GPS : ()
!! REQUIRES CONVERSION TO PYPROJ !!
map_zoom : int
Zoom level of GEarth imagery. See motionless documentation for more details.
map_scale : int
Map scale of GEarth imagery. See motionless documentation for more details.
freq : float
The frequency at which to evaluate the *narrowband* MUSIC algorithm, if using.
AF_freqs : (float, float)
A lower and upper limit on the frequncies at which to eveluate the AF-MUSIC algorithm, if using.
"""
pathstr = False
if isinstance(path, str):
assert array_GPS
pathstr = path
path = self._get_path(path, array_GPS)
else:
assert callable(path)
dom = np.array(path(np.linspace(0, 1, npoints)))
if method.upper() == "GCC":
eval_dom = self._objective_(dom[0,:], dom[1,:])
elif method.upper() == "MUSIC":
assert freq, "Frequency must be provided for MUSIC calculation"
pos = fft_pack.rfftfreq(2*self.data.shape[0])*self.sample_rate
actidx = np.argmin(abs(pos-freq))
self.dataFFT = fft_pack.rfft(self.data, axis=0, n=2*self.data.shape[0])
eval_dom = self._MUSIC2D_((pos[actidx], actidx), dom[0:1,:].T, dom[1:,:].T).flatten()
elif method.upper() == "AF-MUSIC" or method.upper() == "AF_MUSIC":
self.dataFFT = fft_pack.rfft(self.data, axis=0, n=2*self.data.shape[0])
eval_dom = self._AF_MUSIC_subset(dom[0:1,:].T, dom[1:,:].T, freqs=AF_freqs).flatten()
else:
print("Method not recognised. Defaulting to GCC.")
eval_dom = self._objective_(dom[0,:], dom[1,:])
maxidx = np.argmax(eval_dom)
x_max = dom[0, maxidx]
y_max = dom[1, maxidx]
theta = np.arctan2(y_max, x_max)*180/np.pi
plt.figure(1)
if pathstr:
plt.subplot(121)
else:
pass
p = plt.scatter(dom[0,:], dom[1,:], c=eval_dom)
for m in np.arange(self.mics.shape[0]):
plt.scatter(self.mics[m,0], self.mics[m,1], marker='x')
plt.xlim([np.min(dom[0,:]), np.max(dom[0,:])])
plt.ylim([np.min(dom[1,:]), np.max(dom[1,:])])
plt.title(r"{} DOA Estimate; Max at $({:.2f}, {:.2f})$, $\theta={:.1f}^\circ$".format(pathstr if pathstr else "", x_max, y_max, theta))
plt.xlabel(r"x [m] East/West")
plt.ylabel(r"y [m] North/South")
plt.colorbar(p)
if pathstr:
lat, lon = _inv_proj(dom[:,maxidx:maxidx+1].T, array_GPS)
# print(lat, lon, '\n', array_GPS)
with open("./data/apikey", 'r') as f_ap:
key = f_ap.readline()
dmap = DecoratedMap(maptype='satellite', key=key, zoom=map_zoom, scale=map_scale)
dmap.add_marker(LatLonMarker(lat=array_GPS[1], lon=array_GPS[0], label='A'))
dmap.add_marker(LatLonMarker(lat=lat[0], lon=lon[0], label='B'))
response = requests.get(dmap.generate_url())
with open("{}.png".format(pathstr), 'wb') as outfile:
outfile.write(response.content)
im = mpimg.imread("{}.png".format(pathstr))
plt.subplot(122)
plt.imshow(im)
plt.xticks([])
plt.yticks([])
plt.title("{} Satellite Imagery".format(pathstr))
plt.xlabel("A: Array\nB: Bird")
plt.show()
def UCA(n, r, centerpoint=True, show=False):
"""A helper function to easily set up UCAs (uniform circular arrays).
Parameters
----------
n : int
The number of microphones in the array.
r : float
The radius of the array, in meters.
centerpoint : bool
Include a microphone at (0,0)? This will be one of the n points.
show : bool
If True, shows a scatterplot of the array
Returns
-------
np.array
An (n x 2) numpy array, containing the x and y positions of the n microphones in the UCA.
"""
mics = []
if centerpoint:
n -= 1
mics.append([0,0])
for theta in np.linspace(0, 2*np.pi, n, endpoint=False):
mics.append([r*np.cos(theta), r*np.sin(theta)])
mics = np.array(mics)
if show:
plt.scatter(mics[:,0], mics[:,1])
plt.title("Microphone Locations")
plt.xlabel("Horizontal Distance From Array Center [m]")
plt.ylabel("Vertical Distance From Array Center [m]")
plt.show()
return mics
def UMA8(bearing=0, center=0):
"""Return an array containing the positions of the microphones in a miniDSP UMA-8 USB mic array, if centered at `center` and facing bearing `bearing`.
Parameters
----------
bearing : float
Compass bearing of the USB port on the UMA-8.
center : (float, float)
The coordinates at which to place the UMA-8.
"""
pixel_dist = 90.0/(1171.0-77.0)
pixel_dist /= 1000.0
mics = np.array([[624, 546],
[1147, 546],
[885, 93],
[362, 93],
[101, 546],
[362, 999],
[885, 999]], dtype='float64')
mics -= mics[0,:]
mics *= pixel_dist
# for e, m in enumerate(mics):
# print(e+1, m)
theta = -(bearing+180)*np.pi/180.0
for idx in np.arange(mics.shape[0]):
mics[idx, 0] = mics[idx, 0]*np.cos(theta) - mics[idx, 1]*np.sin(theta)
mics[idx, 1] = mics[idx, 1]*np.cos(theta) + mics[idx, 0]*np.sin(theta)
mics += center
return mics
def _r(phi, r_eq=6378137.0, r_pl=6356752.3):
"""Calculates geocentric radius of Earth at latitude $\phi$.
r_eq is the radius of Earth at the equator
r_pl is the radius of Earth at the poles. Distances are in meters.
Calculated using https://en.wikipedia.org/wiki/Earth_radius#Geocentric_radius
"""
return sqrt(((r_eq**2*np.cos(phi))**2+(r_pl**2*np.sin(phi))**2)/((r_eq*np.cos(phi))**2+(r_pl*np.sin(phi))**2))
def _stereo_proj(points, array_coords):
"""Given a set of points (longitude_i, latitude_i, height_i) on the globe,
calculates their coordinates in the plane under the stereographic projection
centered about the microphone array center.
longitude and latitude here are in (signed) radians.
http://mathworld.wolfram.com/StereographicProjection.html
"""
lam, phi, _ = np.array(array_coords)
points = np.vstack((np.array([lam, phi, 0]), points))
k = 2*_r(phi)/(1+np.sin(phi)*np.sin(points[:,1])+np.cos(phi)*np.cos(points[:,1])*np.cos(points[:,0]-lam))
x = k*np.cos(points[:,1])*np.sin(points[:,0]-lam)
y = k*(np.cos(phi)*np.sin(points[:,1])-np.sin(phi)*np.cos(points[:,1])*np.cos(points[:,0]-lam))
return np.array([x[1:], y[1:]]).T, np.array([x[0], y[0]])
def _inv_proj(points, array_coords):
# points = points[:,::-1]
print("points", points)
lam, phi, _ = np.array(array_coords)*np.pi/180.0
print("lam, phi", lam, phi)
rho = np.linalg.norm(points, axis=1)
print("rho", rho)
c = 2*np.arctan2(rho, 2*_r(phi))
print("c", c)
lat = (np.arcsin(np.cos(c)*np.sin(phi)+(points[:,1]*np.sin(c)*np.cos(phi))/rho))*180.0/np.pi
lon = (lam + np.arctan2(points[:,0]*np.sin(c), rho*np.cos(phi)*np.cos(c)-points[:,1]*np.sin(phi)*np.sin(c)))*180.0/np.pi
print("lat, lon", lat, lon)
return lat, lon