def set_irf( self, irf=None, wraptime=None, dispersion=None ):
"""
The detector response isn't a delta-function, meaning that what
you measure isn't the true time-dependence of the system you are
measuring. It's the time dependence of the system convolved with
the response of the detector. This method sets the measured
trace of the detector response that will be used to convolve
the mult-exponential model before fitting (thereby taking this
convolution into account without doing nearly-impossible
numerical deconvolution).
"""
if isinstance( irf, Trace ):
self.irf = irf
elif type(irf) == str:
self.irf = Trace( irf )
if wraptime is not None:
self.irf.wrapcurves( wraptime )
elif self.wraptime is not None:
self.irf.wrapcurves( self.wraptime )
self.irf_dispersion = dispersion
if dispersion is not None:
# this is meant to address chromatic dispersion within the setup
# (e.g. optical fiber)
# don't bother with normalization b/c it gets normalized to unit area below anyway.
#original = self.irf.curves[0].copy()
#self.irf.curves[0][dispersion:] += original[:-dispersion]
#self.irf.curves[0][:-dispersion] += original[dispersion:]
len1 = len(self.irf.curves[0])
chain_of_three = pylab.zeros( 3*len1 ) # stack three curves end-to-end so cspline1d_eval doesn't have to extrapolate beyond data
chain_of_three[:len1] = self.irf.curves[0][:]
chain_of_three[len1:2*len1] = self.irf.curves[0][:]
chain_of_three[-len1:] = self.irf.curves[0][:]
g = cspline1d(chain_of_three)
smoothed = pylab.zeros( len1 )
std_dev = dispersion/1000.0
for t0 in pylab.linspace(-2*std_dev, 2*std_dev, 50):
weight = pylab.exp( -t0**2/2.0/std_dev**2 )
smoothed += weight * cspline1d_eval( g, self.irf.t[0]-t0, dx=self.irf.t[0][1], x0=-self.irf.t[0][-1] )
self.irf.curves[0] = smoothed
normalized = self.irf.curves[0].astype(numpy.float)/float(sum(self.irf.curves[0])) # normalize integral to 1, just like delta-function!!!
self.irf.curves[0] = normalized.copy()
self.irf_generator = cspline1d(self.irf.curves[0])
self.irf_dt = self.irf.t[0][1]-self.irf.t[0][0]
self.irf_t0 = self.irf.t[0][0]
if False:
"""not sure this matters if we do interpolation
"""
# difference in degree of binning (e.g. 8ps vs. 4ps is bin difference of 2)
bin_difference = pylab.np.int( self.resolution / self.irf.resolution )
if bin_difference != 1:
raise ValueError("Have not yet tested deconvolution with different resolution than detector trace!!!")
d = self.irf.curves[0]
detector_binned = pylab.zeros( len(d)/bin_difference )
for i in range( len(detector_binned ) ):
detector_binned[i] = sum( d[i*bin_difference : i*bin_difference+bin_difference] )
def TransformSpectrum(args):
flux, invvar, c0, c1, newwave = args
smoother = 3.0
fitc = cspline1d(flux, lamb=smoother)
fitc_iv = cspline1d(invvar, lamb=smoother)
newf = cspline1d_eval(fitc, newwave, dx=c1, x0=c0)
newiv = cspline1d_eval(fitc_iv, newwave, dx=c1, x0=c0)
return (newf, newiv)
def TransformSpectrum(args):
flux, invvar, c0, c1, newwave = args
smoother = 3.0
fitc = cspline1d(flux, lamb=smoother)
fitc_iv = cspline1d(invvar, lamb=smoother)
newf = cspline1d_eval(fitc, newwave, dx=c1, x0=c0)
newiv = cspline1d_eval(fitc_iv, newwave, dx=c1, x0=c0)
return (newf, newiv)
def splineIntBig0LittleLog(y,x,xNew,splinecoeff = 0.):
"""
Use the scipy spline interpolation, but linearly extrapolate at the edges,
since scipy.signal.cspline1d assumes periodic boundary conditions
"""
if len(x) < 4:
return interpolateLin(y,x,xNew)
if isinstance(xNew,float):
wasfloat = 1
xNew = N.array([xNew])
else:
wasfloat = 0
whereSpline = N.where((xNew >= x[0]) * (xNew <= x[-1]))[0]
whereLittle = N.where(xNew < x[0])[0]
whereBig = N.where(xNew >= x[-1])[0]
ans = xNew * 0.
if len(whereSpline) > 0:
if isinstance(splinecoeff,float): # not pre-calculated.
splinecoeff = SS.cspline1d(y)
ans[whereSpline] = SS.cspline1d_eval(splinecoeff, xNew[whereSpline], dx=x[1]-x[0], x0 = x[0])
if len(whereLittle) > 0:
xw = xNew[whereLittle]
logx,logy = N.log(x[:2]),N.log(y[:2])
ans[whereLittle] = N.exp(logy[0] + (N.log(xw)-logx[0])/(logx[1]-logx[0])*(logy[1]-logy[0]))
if wasfloat:
return ans[0]
else:
return ans
def splineIntLinExt(y,x,xNew,splinecoeff = 0.):
"""
Use the scipy spline interpolation, but linearly extrapolate at the edges,
since scipy.signal.cspline1d assumes periodic boundary conditions
"""
if len(x) < 4:
return interpolateLin(y,x,xNew)
if isinstance(xNew,float):
wasfloat = 1
xNew = M.array([xNew])
else:
wasfloat = 0
whereSpline = N.where((xNew > x[0]) * (xNew < x[-1]))[0]
whereLin = N.where((xNew <= x[0]) + (xNew >= x[-1]))[0]
ans = xNew * 0.
if len(whereSpline) > 0:
if isinstance(splinecoeff,float): # not pre-calculated.
splinecoeff = SS.cspline1d(y)
ans[whereSpline] = SS.cspline1d_eval(splinecoeff, xNew[whereSpline], dx=x[1]-x[0], x0 = x[0])
if len(whereLin) > 0:
ans[whereLin] = interpolateLin(y,x,xNew[whereLin])
if wasfloat:
return ans[0]
else:
return ans
def interp_T(T, Ts, PPs):
xvals = zeros(1)
xvals[0] = T
Ps = list()
for i in PPs:
cj = cspline1d(i)
Ps.append(cspline1d_eval(cj, xvals, dx=500.0, x0=Ts[0]))
return Ps
def interp_T(T,Ts,PPs):
xvals=zeros(1)
xvals[0]=T
Ps=list()
for i in PPs:
cj=cspline1d(i)
Ps.append(cspline1d_eval(cj,xvals,dx=500.0,x0=Ts[0]))
return Ps
def wiggle(x, origin=0, posFill='black', negFill=None, lineColor='black',
resampleRatio=10, rescale=False, ymin=0, ymax=None, ax=None):
"""Plots a "wiggle" trace
Input:
x: input data (1D numpy array)
origin: (default, 0) value to fill above or below (float)
posFill: (default, black) color to fill positive wiggles with (string
or None)
negFill: (default, None) color to fill negative wiggles with (string
or None)
lineColor: (default, black) color of wiggle trace (string or None)
resampleRatio: (default, 10) factor to resample traces by before
plotting (1 = raw data) (float)
rescale: (default, False) If True, rescale "x" to be between -1 and 1
ymin: (default, 0) The minimum y to use for plotting
ymax: (default, len(x)) The maximum y to use for plotting
ax: (default, current axis) The matplotlib axis to plot onto
Output:
a matplotlib plot on the current axes
"""
from matplotlib import pyplot as plt
from scipy.signal import cspline1d, cspline1d_eval
if ymax is None:
ymax = x.size
# Rescale so that x ranges from -1 to 1
if rescale:
x = x.astype(np.float)
x -= x.min()
x /= x.ptp()
x *= 2
x -= 1
# Interpolate at resampleRatio x the previous density
y = np.linspace(0, x.size, x.size)
interp_y = np.linspace(0, x.size, x.size * resampleRatio)
cj = cspline1d(x)
interpX = cspline1d_eval(cj,interp_y) #,dx=1,x0=0
newy = np.linspace(ymax, ymin, interp_y.size)
if origin == None:
origin = interpX.mean()
# Plot
if ax is None:
ax = plt.gca()
plt.hold(True)
if posFill is not None:
ax.fill_betweenx(newy, interpX, origin,
where=interpX > origin,
facecolor=posFill)
if negFill is not None:
ax.fill_betweenx(newy, interpX, origin,
where=interpX < origin,
facecolor=negFill)
if lineColor is not None:
ax.plot(interpX, newy, color=lineColor)
def spline_interpolate(oldx, oldy, newx, smoothing=0.001, **kw):
"""
newy = spline_interpolate(oldx, oldy, newx)
1-dimensional cubic spline, for cases where oldx and newx are on a uniform grid.
"""
return cspline1d_eval(cspline1d(oldy),
newx,
dx=oldx[1] - oldx[0],
x0=oldx[0])
def wiggle(x, origin=0, posFill='black', negFill=None, lineColor='black',
resampleRatio=10, rescale=False, ymin=0, ymax=None, ax=None):
"""Plots a "wiggle" trace
Input:
x: input data (1D numpy array)
origin: (default, 0) value to fill above or below (float)
posFill: (default, black) color to fill positive wiggles with (string
or None)
negFill: (default, None) color to fill negative wiggles with (string
or None)
lineColor: (default, black) color of wiggle trace (string or None)
resampleRatio: (default, 10) factor to resample traces by before
plotting (1 = raw data) (float)
rescale: (default, False) If True, rescale "x" to be between -1 and 1
ymin: (default, 0) The minimum y to use for plotting
ymax: (default, len(x)) The maximum y to use for plotting
ax: (default, current axis) The matplotlib axis to plot onto
Output:
a matplotlib plot on the current axes
"""
from matplotlib import pyplot as plt
from scipy.signal import cspline1d, cspline1d_eval
if ymax is None:
ymax = x.size
# Rescale so that x ranges from -1 to 1
if rescale:
x = x.astype(np.float)
x -= x.min()
x /= x.ptp()
x *= 2
x -= 1
# Interpolate at resampleRatio x the previous density
y = np.linspace(0, x.size, x.size)
interp_y = np.linspace(0, x.size, x.size * resampleRatio)
cj = cspline1d(x)
interpX = cspline1d_eval(cj,interp_y) #,dx=1,x0=0
newy = np.linspace(ymax, ymin, interp_y.size)
if origin == None:
origin = interpX.mean()
# Plot
if ax is None:
ax = plt.gca()
plt.hold(True)
if posFill is not None:
ax.fill_betweenx(newy, interpX, origin,
where=interpX > origin,
facecolor=posFill)
if negFill is not None:
ax.fill_betweenx(newy, interpX, origin,
where=interpX < origin,
facecolor=negFill)
if lineColor is not None:
ax.plot(interpX, newy, color=lineColor)
def test_basic(self):
y = array([1, 2, 3, 4, 3, 2, 1, 2, 3.0])
x = arange(len(y))
dx = x[1] - x[0]
cj = signal.cspline1d(y)
x2 = arange(len(y) * 10.0) / 10.0
y2 = signal.cspline1d_eval(cj, x2, dx=dx, x0=x[0])
# make sure interpolated values are on knot points
assert_array_almost_equal(y2[::10], y, decimal=5)
def test_basic(self):
y=array([1,2,3,4,3,2,1,2,3.0])
x=arange(len(y))
dx=x[1]-x[0]
cj = signal.cspline1d(y)
x2=arange(len(y)*10.0)/10.0
y2=signal.cspline1d_eval(cj, x2, dx=dx,x0=x[0])
# make sure interpolated values are on knot points
assert_array_almost_equal(y2[::10], y, decimal=5)
def run(self):
"""
create an inifile from the parameters and run camb on it
and store the results in k,pk
"""
self.printIniFile()
os.system(self.cambPath + "/camb " + self.iniName)
self.k, self.pk = utils.readColumns(self.cp.output_root + "_matterpower.dat")
self.logk, self.logpk = M.log(self.k), M.log(self.pk)
self.pkSplineCoeff = SS.cspline1d(self.logpk)
def run(self):
_, fileExtension = os.path.splitext(self.fileName)
if fileExtension == '.gmv':
print('Geomagnetic variation')
with open(self.fileName, 'rt') as csvdata:
date = []
value = []
for row in csv.reader(csvdata):
if ('#' in row[0]):
self.header.append(row)
else:
date.append(row[0])
value.append(row[1])
self.notifyProgress.emit(20)
elif fileExtension == '.ske':
print('Kp estimation')
with open(self.fileName, 'rt') as csvdata:
date = []
value = []
for row in csv.reader(csvdata, delimiter=' '):
if ('#' in row[0]):
self.header.append(row)
else:
print(row)
if int(row[7]) < 2:
date.append(
dt.datetime.strptime(
''.join((row[0], row[1], row[2], row[4])),
'%Y%m%d%H%M')),
value.append(float(row[-1]) -
float(row[-14])) # 4h
# value.append(float(row[-1])-float(row[19])) # 1h
self.notifyProgress.emit(20)
signal_src = np.array((date, value), dtype=np.dtype('a25'))
signal = signal_src[:,
np.logical_not(
np.isnan(signal_src[1, :].astype(np.float)))]
self.notifyProgress.emit(60)
if self.interpolate:
self.time = signal_src[0, :].astype(np.datetime64).astype(
dt.datetime)
dx = dates.date2num(self.time[1]) - dates.date2num(self.time[0])
cj = cspline1d(signal[1, :].astype(float))
self.value = cspline1d_eval(cj,
dates.date2num(self.time),
dx=dx,
x0=dates.date2num(self.time[0]))
else:
self.time = dates.signal[0, :].astype(np.datetime64).astype(
dt.datetime)
self.value = signal[1, :].astype(np.float)
self.notifyProgress.emit(80)
self.loaded.emit()
def runEHuShiftBAO(self, sig8, shiftfact=1.):
#Output EHu file
f = file('ehu.in','w')
f.write((str(self.cp.omega_baryon + self.cp.omega_cdm))+', '+str(self.cp.omega_lambda)+', '+\
str(self.cp.omega_neutrino)+', '+str(self.cp.omega_baryon)+'\n')
f.write(str(self.cp.hubble/100.)+', '+str(self.cp.temp_cmb)+', '+str(self.cp.massless_neutrinos)+'\n')
f.write(str(self.cp.transfer_redshift[0])+'\n')
f.write(str(self.cp.transfer_kmax)+', '+str(self.cp.transfer_k_per_logint)+'\n')
f.write('1\n')
tilt = self.cp.scalar_spectral_index[0]
f.write(str(tilt)+'\n')
f.write('0\n')
f.close()
# run EHu code
os.system('~/ehu/power < ehu.in')
# read into c.k, c.pk
eh = N.loadtxt('trans.dat')
self.k = eh[:,0]*1.
self.logk = M.log(self.k)
if (getnowig):
self.trans = eh[:,3]*1.
else:
self.trans = eh[:,1]*1.
#M.loglog(self.k,self.trans)
#M.show()
if tilt == 1.:
delH = 1.94e-5*(self.cp.omega_cdm + self.cp.omega_baryon)**(-0.785)
delta = delH**2*(3000.0*self.k/(self.cp.hubble/100.))**4*self.trans**2
else:
delH = 1.94e-5*self.cp.omega_cdm**(-0.785 - 0.05*M.log(tilt))\
* M.exp(-0.95*(tilt - 1.) - 0.169*(tilt - 1)**2)
delta = delH**2*(3000.0*self.k/(self.cp.hubble/100.))**(3 + tilt)*self.trans**2
# Just an approximate normalization; really need sig8.
self.pk = (2.*M.pi**2 * delta/self.k**3)*(self.cp.hubble/100.)**3
if self.cp.transfer_redshift[0] > 0.:
ps = PowerSpectrum(self.cp)
sig8use = sig8*ps.d1(self.cp.transfer_redshift[0])/ps.d1(0.)
else:
sig8use = sig8
normalizePk(self,sig8use) # sets c.logpk, too
self.pkSplineCoeff = SS.cspline1d(self.logpk)
return
def doresample(orig_x, orig_y, new_x, method='cubic', padlen=0, antialias=False):
"""
Resample data from one spacing to another. By default, does not apply any antialiasing filter.
Parameters
----------
orig_x
orig_y
new_x
method
padlen
Returns
-------
"""
pad_y = tide_filt.padvec(orig_y, padlen=padlen)
tstep = orig_x[1] - orig_x[0]
if padlen > 0:
pad_x = np.concatenate((np.arange(orig_x[0] - padlen * tstep, orig_x[0], tstep),
orig_x,
np.arange(orig_x[-1] + tstep, orig_x[-1] + tstep * (padlen + 1), tstep)))
else:
pad_x = orig_x
if padlen > 0:
print('padlen=', padlen)
print('tstep=', tstep)
print(pad_x)
# antialias and ringstop filter
init_freq = len(pad_x) / (pad_x[-1] - pad_x[0])
final_freq = len(new_x) / (new_x[-1] - new_x[0])
if antialias and (init_freq > final_freq):
aafilterfreq = final_freq / 2.0
aafilter = tide_filt.noncausalfilter(filtertype='arb', usebutterworth=False)
aafilter.setarb(0.0, 0.0, 0.95 * aafilterfreq, aafilterfreq)
pad_y = aafilter.apply(init_freq, pad_y)
if method == 'cubic':
cj = signal.cspline1d(pad_y)
return tide_filt.unpadvec(
np.float64(signal.cspline1d_eval(cj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])), padlen=padlen)
elif method == 'quadratic':
qj = signal.qspline1d(pad_y)
return tide_filt.unpadvec(
np.float64(signal.qspline1d_eval(qj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])), padlen=padlen)
elif method == 'univariate':
interpolator = sp.interpolate.UnivariateSpline(pad_x, pad_y, k=3, s=0) # s=0 interpolates
return tide_filt.unpadvec(np.float64(interpolator(new_x)), padlen=padlen)
else:
print('invalid interpolation method')
return None
def pkInterp(self, knew, calcsplinecoeff = False):
"""
P(knew) interpolated in log space for arbitrary k.
Call with calcsplinecoeff = True if the power spectrum (self.pk) might have changed recently.
"""
if (calcsplinecoeff):
self.pkSplineCoeff = SS.cspline1d(self.logpk)
w0 = N.where(knew > 0.)[0]
newy = 0.*knew
# will handle the case k = 0
newy[w0] = M.exp(utils.splineIntLinExt(self.logpk, self.logk, M.log(knew[w0]),splinecoeff = self.pkSplineCoeff))
return newy
def run(self):
_, fileExtension = os.path.splitext(self.fileName)
if fileExtension == '.gmv':
print('Geomagnetic variation')
with open(self.fileName, 'rt') as csvdata:
date = []
value = []
for row in csv.reader(csvdata):
if ('#' in row[0]):
self.header.append(row)
else:
date.append(row[0])
value.append(row[1])
self.notifyProgress.emit(20)
elif fileExtension == '.ske':
print('Kp estimation')
with open(self.fileName, 'rt') as csvdata:
date = []
value = []
for row in csv.reader(csvdata, delimiter=' '):
if ('#' in row[0]):
self.header.append(row)
else:
print(row)
if int(row[7]) < 2:
date.append(
dt.datetime.strptime(
''.join((row[0], row[1], row[2],
row[4])),
'%Y%m%d%H%M')),
value.append(float(row[-1])-float(row[-14])) # 4h
# value.append(float(row[-1])-float(row[19])) # 1h
self.notifyProgress.emit(20)
signal_src = np.array((date, value), dtype=np.dtype('a25'))
signal = signal_src[:, np.logical_not(
np.isnan(signal_src[1, :].astype(np.float)))]
self.notifyProgress.emit(60)
if self.interpolate:
self.time = signal_src[0, :].astype(np.datetime64).astype(
dt.datetime)
dx = dates.date2num(self.time[1])-dates.date2num(self.time[0])
cj = cspline1d(signal[1, :].astype(float))
self.value = cspline1d_eval(cj, dates.date2num(self.time),
dx=dx,
x0=dates.date2num(self.time[0]))
else:
self.time = dates.signal[0, :].astype(np.datetime64).astype(
dt.datetime)
self.value = signal[1, :].astype(np.float)
self.notifyProgress.emit(80)
self.loaded.emit()
def interpol(x1, y1, x_out, plot=False):
from scipy.signal import cspline1d, cspline1d_eval
#assumes that data points are evenly spaced
dx = x1[1] - x1[0]
cj = cspline1d(y1)
y_out = cspline1d_eval(cj, x_out, dx=dx, x0=x1[0])
if plot:
from pylab import plot, show, legend
plot(x_out, y_out, 'ob', x1, y1, 'xg', ms=2)
legend(['interpolated', 'original'])
show()
return y_out
def interp_around(X_sc,s_fracpeak,s_before,s_after,kind='cubic'):
n_c = X_sc.shape[1]
n_s = s_before+s_after
Out_sc = np.empty((n_s,n_c),dtype=np.float32)
for i_c in xrange(n_c):
if kind == 'cubic':
coeffs = cspline1d(X_sc[:,i_c])
Out_sc[:,i_c] = cspline1d_eval(coeffs,
newx=np.arange(s_fracpeak - s_before,s_fracpeak+s_after,dtype=np.float32))
elif kind == "linear":
Out_sc[:,i_c] = interp1d(np.arange(X_sc.shape[0]),X_sc[:,i_c],
bounds_error=True,kind=kind)(np.arange(s_fracpeak - s_before,s_fracpeak+s_after,dtype=np.float32))
else: raise Exception("kind must be 'linear' or 'cubic'")
return Out_sc
def interpol(x1,y1,x_out,plot=False): from scipy.signal import cspline1d, cspline1d_eval #assumes that data points are evenly spaced dx=x1[1]-x1[0] cj=cspline1d(y1) y_out=cspline1d_eval(cj,x_out,dx=dx,x0=x1[0]) if plot: from pylab import plot, show,legend plot(x_out,y_out,'ob',x1,y1,'xg',ms=2) legend(['interpolated','original']) show() return y_out
def SplineResample(y, n_x, x_range = None, smoother = 3):
''' Resample a signal y using spline.
y: the signal must be sampled on uniform x
n_x: number of points for the new signal
x_range: tuple (start x, end x) of the signal
smoother: spline smoothing strength
'''
if x_range is None: x_range = (0., 1.)
spcoeffs = cspline1d(y, lamb = smoother)
return cspline1d_eval(
spcoeffs, linspace(x_range[0], x_range[1], n_x),
dx = (x_range[1]-x_range[0])/(len(y)-1.0), x0 = x_range[0])
def SplineResample(y, n_x, x_range=None, smoother=3):
''' Resample a signal y using spline.
y: the signal must be sampled on uniform x
n_x: number of points for the new signal
x_range: tuple (start x, end x) of the signal
smoother: spline smoothing strength
'''
if x_range is None: x_range = (0., 1.)
spcoeffs = cspline1d(y, lamb=smoother)
return cspline1d_eval(spcoeffs,
linspace(x_range[0], x_range[1], n_x),
dx=(x_range[1] - x_range[0]) / (len(y) - 1.0),
x0=x_range[0])
def evalBeams(arrBeams,guessShearLoad,spc,debugFlag = False):
lastBeam = arrBeams[-1]
arrStrainEnergy = np.zeros(np.size(arrBeams))
arrSurfEnergy = np.zeros(np.size(arrBeams))
lastIndex = np.size(arrBeams)
maxSurfEnergy = -gamma * lastBeam.w*(lastBeam.Lt - lastBeam.L)
arrResults = np.array([])
for j,beam in enumerate(arrBeams):
if debugFlag:
print('Beam Length: %f of %f'%(beam.L*scale,beam.Lt*scale))
dispSearch(beam=beam,initLoad = guessShearLoad,goal=spc/2/scale,tol=1e-7,right=0,left=0)
guessShearLoad = beam.shearLoad
if debugFlag:
print('Solved Beam -- TipDisp: %s Goal: %s Force: %s' % (beam.yTipDisplacement()*scale,spc/2,beam.shearLoad))
arrStrainEnergy[j] = beam.calculateStrainEnergy()
arrSurfEnergy[j] = -gamma * beam.w *(beam.Lt - beam.L)
if arrStrainEnergy[j] >= np.abs(maxSurfEnergy):
# since there is more bending energy than surface energy stop computing
print('Super stiff beam')
lastIndex = j
break
if lastIndex > 0: # This ensures that we have more than one data point before trying to interpolate
interpLens = np.linspace(arrBeamLens[0],arrBeamLens[lastIndex-1],num=100,endpoint=True) # Generate x values for which to interpolate
csFit = cspline1d((arrStrainEnergy[0:lastIndex]+arrSurfEnergy[0:lastIndex])) # Generate cubic spline fit to the sub dataset
interpTotalEnergy = cspline1d_eval(csFit,interpLens,dx=(arrBeamLens[1]-arrBeamLens[0]), x0 = arrBeamLens[0]) # Generate the interpolated values from the fit and x points
finalLen = interpLens[interpTotalEnergy.argmin()] # find the minimum of the energy balance and grab index to choose the appropriate length
if debugFlag:
print('beamLens shape: %s arrStrain: %s'%(arrBeamLens[0:lastIndex].shape,arrStrainEnergy[0:lastIndex].shape))
mpl.figure()
mpl.hold(True)
mpl.plot(arrBeamLens[0:lastIndex]*scale,arrStrainEnergy[0:lastIndex]*scale)
mpl.plot(arrBeamLens[0:lastIndex]*scale,arrSurfEnergy[0:lastIndex]*scale)
mpl.plot(interpLens*scale,interpTotalEnergy*scale,arrBeamLens[0:lastIndex]*scale,(arrStrainEnergy+arrSurfEnergy)[0:lastIndex]*scale,'o')
arrResults = np.array([arrBeamLens[0:lastIndex],arrStrainEnergy[0:lastIndex]])
else: # since there is only one datapoint then use that as the value
finalLen = arrBeamLens[lastIndex]
arrResults = np.array([arrBeamLens[lastIndex],arrStrainEnergy[lastIndex]])
return (finalLen,arrResults)
def normalizePk(c, sig8):
"""
renormalize the power spectrum to the given sigma_8
Note: this doesn't take into account the redshift; it just blindly sets c.pk to have
sigma_8 = sig8.
"""
sig2now = sigma2fromPk(c, 8.0)
# print 'sig2now=',sig2now
c.pk *= sig8 ** 2 / sig2now
c.logpk = M.log(c.pk)
c.cp.scalar_amp[0] = c.cp.scalar_amp[0] * sig8 ** 2 / sig2now[0] # inelegant tuple change
# for scipy splines
c.pkSplineCoeff = SS.cspline1d(c.logpk)
return sig2now
def peakdetect_spline(y_axis, x_axis, pad_len=20):
"""
Performs a b-spline interpolation on the data to increase resolution and
send the data to the 'peakdetect_zero_crossing' function for peak
detection.
Omitting the x_axis is forbidden as it would make the resulting x_axis
value silly if it was returned as the index 50.234 or similar.
will find the same amount of peaks as the 'peakdetect_zero_crossing'
function, but might result in a more precise value of the peak.
keyword arguments:
y_axis -- A list containing the signal over which to find peaks
x_axis -- A x-axis whose values correspond to the y_axis list and is used
in the return to specify the position of the peaks.
x-axis must be equally spaced.
pad_len -- By how many times the time resolution should be increased by,
e.g. 1 doubles the resolution.
(default: 20)
return: two lists [max_peaks, min_peaks] containing the positive and
negative peaks respectively. Each cell of the lists contains a tuple
of: (position, peak_value)
to get the average peak value do: np.mean(max_peaks, 0)[1] on the
results to unpack one of the lists into x, y coordinates do:
x, y = zip(*max_peaks)
"""
# check input data
x_axis, y_axis = _datacheck_peakdetect(x_axis, y_axis)
# could perform a check if x_axis is equally spaced
#if np.std(np.diff(x_axis)) > 1e-15: raise ValueError
# perform spline interpolations
dx = x_axis[1] - x_axis[0]
x_interpolated = np.linspace(x_axis.min(), x_axis.max(),
len(x_axis) * (pad_len + 1))
cj = cspline1d(y_axis)
y_interpolated = cspline1d_eval(cj, x_interpolated, dx=dx, x0=x_axis[0])
# get peaks
max_peaks, min_peaks = peakdetect_zero_crossing(y_interpolated,
x_interpolated)
return [max_peaks, min_peaks]
def pkInterp(self, knew, calcsplinecoeff=False):
"""
P(knew) interpolated in log space for arbitrary k.
Call with calcsplinecoeff = True if the power spectrum (self.pk) might have changed recently.
"""
if calcsplinecoeff:
self.pkSplineCoeff = SS.cspline1d(self.logpk)
# newy = M.exp(utils.splineIntLinExt(self.logpk, self.logk, M.log(knew),splinecoeff = self.pkSplineCoeff))
w0 = N.where(knew <= 0.0)
wn0 = N.where(knew > 0.0)
newy = 0.0 * knew
newy[wn0] = M.exp(
utils.splineIntLinExt(self.logpk, self.logk, M.log(knew[wn0]), splinecoeff=self.pkSplineCoeff)
)
# do 0
newy[w0] = 0.0
return newy
def sr_interpol2(x,y,ytarget,doplot=0,factor=10):
dx = x[1]-x[0]
newx = linspace(min(x),max(x),factor*len(x))
cj = cspline1d(y)
newy = cspline1d_eval(cj, newx, dx=dx,x0=x[0])
ysq = (ytarget-newy)**2
index = where(ysq == min(ysq))
if doplot:
clf()
plot(x,y,'o')
plot(newx,newy)
plot(newx[index],newy[index],'o')
show()
return newx[index[0][0]]
def fitSpline(self, degree=2):
"""
**SUMMARY**
A function to generate a spline curve fitting over the points in LineScan with
order of precision given by the parameter degree
**PARAMETERS**
* *degree* - the precision of the generated spline
**RETURNS**
The spline as a LineScan fitting over the initial values of LineScan
**EXAMPLE**
>>> import matplotlib.pyplot as plt
>>> img = Image("lenna")
>>> ls = img.getLineScan(pt1=(10,10)),pt2=(20,20)).normalize()
>>> spline = ls.fitSpline()
>>> plt.plot(ls)
>>> plt.show()
>>> plt.plot(spline)
>>> plt.show()
**NOTES**
Implementation taken from http://www.scipy.org/Cookbook/Interpolation
"""
if degree > 4:
degree = 4 # No significant improvement with respect to time usage
if degree < 1:
warnings.warn('LineScan.fitSpline - degree needs to be >= 1')
return None
retVal = None
y = np.array(self)
x = np.arange(0, len(y), 1)
dx = 1
newx = np.arange(0, len(y) - 1, pow(0.1, degree))
cj = sps.cspline1d(y)
retVal = sps.cspline1d_eval(cj, newx, dx=dx, x0=x[0])
return retVal
def fitSpline(self,degree=2):
"""
**SUMMARY**
A function to generate a spline curve fitting over the points in LineScan with
order of precision given by the parameter degree
**PARAMETERS**
* *degree* - the precision of the generated spline
**RETURNS**
The spline as a LineScan fitting over the initial values of LineScan
**EXAMPLE**
>>> import matplotlib.pyplot as plt
>>> img = Image("lenna")
>>> ls = img.getLineScan(pt1=(10,10)),pt2=(20,20)).normalize()
>>> spline = ls.fitSpline()
>>> plt.plot(ls)
>>> plt.show()
>>> plt.plot(spline)
>>> plt.show()
**NOTES**
Implementation taken from http://www.scipy.org/Cookbook/Interpolation
"""
if degree > 4:
degree = 4 # No significant improvement with respect to time usage
if degree < 1:
warnings.warn('LineScan.fitSpline - degree needs to be >= 1')
return None
retVal = None
y = np.array(self)
x = np.arange(0,len(y),1)
dx = 1
newx = np.arange(0,len(y)-1,pow(0.1,degree))
cj = sps.cspline1d(y)
retVal = sps.cspline1d_eval(cj,newx,dx=dx,x0=x[0])
return retVal
def peakdetect_spline(y_axis, x_axis, pad_len=20):
"""
Performs a b-spline interpolation on the data to increase resolution and
send the data to the 'peakdetect_zero_crossing' function for peak
detection.
Omitting the x_axis is forbidden as it would make the resulting x_axis
value silly if it was returned as the index 50.234 or similar.
will find the same amount of peaks as the 'peakdetect_zero_crossing'
function, but might result in a more precise value of the peak.
keyword arguments:
y_axis -- A list containing the signal over which to find peaks
x_axis -- A x-axis whose values correspond to the y_axis list and is used
in the return to specify the position of the peaks.
x-axis must be equally spaced.
pad_len -- By how many times the time resolution should be increased by,
e.g. 1 doubles the resolution.
(default: 20)
return: two lists [max_peaks, min_peaks] containing the positive and
negative peaks respectively. Each cell of the lists contains a tuple
of: (position, peak_value)
to get the average peak value do: np.mean(max_peaks, 0)[1] on the
results to unpack one of the lists into x, y coordinates do:
x, y = zip(*max_peaks)
"""
# check input data
x_axis, y_axis = _datacheck_peakdetect(x_axis, y_axis)
# could perform a check if x_axis is equally spaced
#if np.std(np.diff(x_axis)) > 1e-15: raise ValueError
# perform spline interpolations
dx = x_axis[1] - x_axis[0]
x_interpolated = np.linspace(x_axis.min(), x_axis.max(), len(x_axis) * (pad_len + 1))
cj = cspline1d(y_axis)
y_interpolated = cspline1d_eval(cj, x_interpolated, dx=dx,x0=x_axis[0])
# get peaks
max_peaks, min_peaks = peakdetect_zero_crossing(y_interpolated, x_interpolated)
return [max_peaks, min_peaks]
def _spline_interpolate(oldx, oldy, newx, smoothing=0.001,fast=True, **kw):
"""
cubic splines for axis alignment using
scipy.signal and/or scipy.interpolate
newy = _spline_interpolate(oldx, oldy, newx, fast=True)
if fast = True
1-dimensional cubic spline for cases where
oldx and newx are on a uniform grid.
else
handles multi-dimensional data, non-uniform x-grids, but is
much slower for 1d cubic splines
"""
from scipy.interpolate import splrep, splev
from scipy.signal import cspline1d, cspline1d_eval
if fast:
return cspline1d_eval(cspline1d(oldy), newx, dx=oldx[1]-oldx[0],x0=oldx[0])
else:
rep = splrep(oldx,oldy,s=smoothing,full_output=False,**kw)
return splev(newx, rep)
def wiggle(self, values):
"""
Plot a trace in VAWT(Variable Area Wiggle Trace)
"""
if self.zmax is None:
self.zmax = values.size
# Rescale so that values ranges from -1 to 1
if self.rescale:
values = values.astype(np.float)
values -= values.min()
values /= values.ptp()
values *= 2
values -= 1
# Interpolate at resampleRatio x the previous density
resample_z = np.linspace(0, values.size,
values.size * self.resampleRatio)
# cubic spline interpolation
cj = cspline1d(values)
resample_v = cspline1d_eval(cj, resample_z)
print(resample_v)
newz = resample_z
if self.origin is None:
self.origin = resample_v.mean()
# Plot
if self.posFill is not None:
self.ax.fill_betweenx(newz,
resample_v,
self.origin,
where=resample_v > self.origin,
facecolor=self.posFill)
if self.negFill is not None:
self.ax.fill_betweenx(newz,
resample_v,
self.origin,
where=resample_v < self.origin,
facecolor=self.negFill)
if self.lineColor is not None:
self.ax.plot(resample_v, newz, color=self.lineColor, linewidth=.1)
def kextend(self, mini, maxi, logkoverk3extrap=0, calcsplinecoeff=False):
"""
Extend range of pk over which k is known, from 10^mini to 10^maxi.
Keeps c.k the same in middle, but extrapolates on both sides.
The logk/k**3 fit (used if last argument = 1) only works reliably if the highest k is around 100
"""
log10interval = M.log10(self.k[-1] / self.k[0]) / (len(self.k) - 1.0)
self.numtomini = M.floor((M.log10(self.k[0]) - mini) / log10interval)
if self.numtomini < 0:
self.numtomini = 0
realmini = M.log10(self.k[0]) - log10interval * self.numtomini
kx = 10.0 ** M.arange(realmini, maxi + log10interval, log10interval)
px = self.pkInterp(kx, calcsplinecoeff=calcsplinecoeff)
self.k = kx
self.logk = M.log(kx)
self.pk = px
kmax = self.k[-1]
# fit logk/k**3 at high end; this is presumably more accurate, but may crash
if logkoverk3extrap == 1:
p0 = (self.pk[-1] * self.k[-1] ** 3 - self.pk[-2] * self.k[-2] ** 3) / (
M.log(self.k[-1]) - M.log(self.k[-2])
)
const = (
self.pk[-1] * self.k[-1] ** 3 * M.log(self.k[-2]) - self.pk[-2] * self.k[-2] ** 3 * M.log(self.k[-1])
) / (self.pk[-1] * self.k[-1] ** 3 - self.pk[-2] * self.k[-2] ** 3)
if (p0 > 0.0) * (maxi > kmax): # if it worked okayly
w = M.where(self.k > kmax)[0][0]
self.pk[w:] = p0 * (self.logk[w:] - const) / self.k[w:] ** 3
self.logpk = M.log(px)
self.pkSplineCoeff = SS.cspline1d(self.logpk)
def interp_around(X_sc, s_fracpeak, s_before, s_after, kind='cubic'):
n_c = X_sc.shape[1]
n_s = s_before + s_after
Out_sc = np.empty((n_s, n_c), dtype=np.float32)
for i_c in xrange(n_c):
if kind == 'cubic':
coeffs = cspline1d(X_sc[:, i_c])
Out_sc[:,
i_c] = cspline1d_eval(coeffs,
newx=np.arange(s_fracpeak - s_before,
s_fracpeak + s_after,
dtype=np.float32))
elif kind == "linear":
Out_sc[:,
i_c] = interp1d(np.arange(X_sc.shape[0]),
X_sc[:, i_c],
bounds_error=True,
kind=kind)(np.arange(s_fracpeak - s_before,
s_fracpeak + s_after,
dtype=np.float32))
else:
raise Exception("kind must be 'linear' or 'cubic'")
return Out_sc
def sr_interpol3(x,y,ytarget,doplot=0,factor=10):
s = numpy.sign(numpy.diff(y)[0])
if s==1:
y[numpy.argmax(y)+1:] = 2*abs(max(y))
else:
y[numpy.argmin(y)+1:] = -2*abs(max(y))
dx = x[1]-x[0]
newx = linspace(min(x),max(x),factor*len(x))
cj = cspline1d(y)
newy = cspline1d_eval(cj, newx, dx=dx,x0=x[0])
ysq = (ytarget-newy)**2
index = where(ysq == min(ysq))
if doplot:
clf()
plot(x,y,'o')
plot(newx,newy)
plot(newx[index],newy[index],'o')
show()
return newx[index[0][0]]
def fit_spline(self, degree=2):
"""
Generates a spline _curve fitting over the points in LineScan with
order of precision given by the parameter degree.
:param degree: the precision of the generated spline.
:return: the spline as a LineScan fitting over the initial values of
LineScan
Notes:
Implementation taken from http://www.scipy.org/Cookbook/Interpolation
"""
if degree > 4:
degree = 4 # No significant improvement with respect to time usage
if degree < 1:
warnings.warn("LineScan.fit_spline - degree needs to be >= 1.")
return None
y = np.array(self)
x = np.arange(0, len(y), 1)
dx = 1
newx = np.arange(0, len(y) - 1, pow(0.1, degree))
cj = signal.cspline1d(y)
ret = signal.cspline1d_eval(cj, newx, dx=dx, x0=x[0])
return ret
def wiggle(self, values):
"""
Plot a trace in VAWT(Variable Area Wiggle Trace)
"""
if self.zmax is None:
self.zmax = values.size
# Rescale so that values ranges from -1 to 1
if self.rescale:
values = values.astype(np.float)
values -= values.min()
values /= values.ptp()
values *= 2
values -= 1
# Interpolate at resampleRatio x the previous density
resample_z = np.linspace(0, values.size, values.size * self.resampleRatio)
# cubic spline interpolation
cj = cspline1d(values)
resample_v = cspline1d_eval(cj, resample_z)
print(resample_v)
newz = resample_z
if self.origin is None:
self.origin = resample_v.mean()
# Plot
if self.posFill is not None:
self.ax.fill_betweenx(newz, resample_v, self.origin,
where=resample_v > self.origin,
facecolor=self.posFill)
if self.negFill is not None:
self.ax.fill_betweenx(newz, resample_v, self.origin,
where=resample_v < self.origin,
facecolor=self.negFill)
if self.lineColor is not None:
self.ax.plot(resample_v, newz, color=self.lineColor, linewidth=.1)
def compute(chifile, Tfil, pressure, lamda):
#####################
#Get lamda and T from the temperature file
try:
Tfil = float(Tfil)
except ValueError:
fndT = False
tlist = open(Tfil, "r")
for line in tlist:
if line[0] == '#':
continue
line = line.rstrip()
vals = line.split(None)
if str(vals[0]) == chifile:
Tfil = int(vals[1])
lamda = float(vals[2])
fndT = True
break
tlist.close()
if fndT == False:
print "Error: Unable to find chi file " + chifile + " in temperature file " + Tfil
print "Please manually enter the temperature or enter the temperature into the temperature list file " + Tfil
exit(0)
else:
if lamda == -1.0:
parser.print_help()
print "\nError: When temperature is given manually, must use -l arguement to set lambda.\n"
exit()
if Tfil != 0 and Tfil != 300 and (Tfil < 500 or Tfil > 3000):
parser.print_help()
print "\nError: Need a valid sample temperature value for analysis"
exit()
#####################
#Read in the chi file
f = open(chifile, 'r')
i = 0
for line in f:
if i < 3:
i += 1
continue
line = line.lstrip().rstrip()
if i == 3:
i += 1
length = int(line)
break
xxs = zeros(length)
yys = zeros(length)
i = 0
for line in f:
line = line.lstrip().rstrip()
[xxs[i], NULL, yys[i]] = line.split(' ')
i += 1
#####################
#Load in the MgO data
mgo_a0 = 4.213
(ARs, Ts, PPs) = loadMgO('mgo_eos.dat')
As = [i * mgo_a0 for i in ARs]
if Tfil == 0.0:
Ps = PPs[:, 0]
elif Tfil == 300.0:
As.insert(0, mgo_a0)
Ps = PPs[:, 1].tolist()
Ps.insert(0, 1.0)
else:
Ps = interp_T(Tfil, Ts[2:], PPs[:, 2:])
#Get the MgO lattice constant for the desired pressure
mgo_s = UnivariateSpline(Ps, As)
mgo_sps = linspace(min(Ps), max(Ps), len(Ps))
mgo_sas = mgo_s(mgo_sps)
coefs = cspline1d(mgo_sas)
latconst = cspline1d_eval(coefs, [pressure],
dx=mgo_sps[1] - mgo_sps[0],
x0=mgo_sps[0])
#Get the intensity factors
mgo_ks = [3, 4, 8, 11, 12] #Valid K vectors
mgo_mp = [8.0, 6.0, 12.0, 24.0, 8.0] #Multiplicity
mgo_sf = [1.0, 3.0, 3.0, 1.0, 3.0] #Structure Factor
mgo_Im = [(mgo_sf[i] * mgo_sf[i]) / mgo_mp[i]
for i in range(len(mgo_sf))] #Intensity multiplicand
#Find the MgO peaks at this pressure
mgo_2th = list()
mgo_I = list()
for (i, K) in enumerate(mgo_ks):
print lamda, K, latconst
theta = asin(lamda * sqrt(K) * 0.5 / latconst)
mgo_2th.append(degrees(theta) * 2)
mgo_I.append(mgo_Im[i] * (1 + cos(theta * 2) * cos(theta * 2)) /
(sin(theta) * sin(theta) * cos(theta)))
mxI = max(mgo_I)
mxA = sum(xxs) / len(xxs)
mgo_I = [(i / mxI + 1) * mxA * mxA for i in mgo_I]
pl.figure()
pl.plot(xxs, yys)
[pl.plot([x, x], [0, y], color='red') for (x, y) in zip(mgo_2th, mgo_I)]
[
pl.text(x, 5, str(z), size='x-small')
for (x, y, z) in zip(mgo_2th, mgo_I, mgo_ks)
]
pl.title(chifile + ", T=" + str(int(Tfil)) + ", P~" + str(pressure))
pl.show()
finalpixel = np.log10(maxwavelength)
deltapix = 1e-4 #10.**(np.min(deredloglambda0))*(10.**1e-4 - 1.)
npix = (finalpixel - initialpixel) / deltapix + 1.
newwave = initialpixel + deltapix * np.arange(npix)
newflux = np.zeros((len(flux), npix + 1))
chisq = np.zeros(len(flux))
#resample spectra at single wavelength spectrum defined above
smoothing_parameter = 3.0
spline_order = 3
number_of_knots = -1
for p in range(len(flux)):
nonzero = np.where(wavevector[p, :] != 0.)
fitcoeff = cspline1d(flux[p], lamb=smoothing_parameter)
newflux[p, :] = cspline1d_eval(fitcoeff,
newwave,
dx=wave1[p],
x0=wavevector[p, 0])
oldfit = cspline1d_eval(fitcoeff,
wavevector[p, nonzero][0],
dx=wave1[p],
x0=wavevector[p, 0])
chisq[p] = np.sum(np.sqrt(
(oldfit - flux[p])**2. * invvar[p])) / np.shape(flux[p])[0]
filename = 'pcaspectra_rest.fits'
pf.writeto(filename, newflux, clobber=True)
pf.append(filename, newwave)
pf.append(filename, z)
# # Example showing how to use B-splines in scipy.signal to do # interpolation. The input points must be equally spaced to use these # routine. # # <codecell> from numpy import r_, sin from scipy.signal import cspline1d, cspline1d_eval x = r_[0:10] dx = x[1]-x[0] newx = r_[-3:13:0.1] # notice outside the original domain y = sin(x) cj = cspline1d(y) newy = cspline1d_eval(cj, newx, dx=dx,x0=x[0]) from pylab import plot, show plot(newx, newy, x, y, 'o') show() # <markdowncell> # *0.6777**2, redshift = 0.,kmax=30.,omk=0.):
"""
possible inputs:
c = Camb instance; contains cosmological parameters, power spectrum
d = configuration-space density field
dk = FFT of a density field
parameters:
sigmaalpt = Gaussian k-space interpolation smoothing scale, as in ALPT
scheme: can be 'zeld'ovich, '2lpt', 'sc' (single-scale spherical collapse), 'muscle' (multiscale)
largescale/smallscale: use for scale interpolation
dopbc: False to preserve distortion of particle lattice, not enforcing periodic boundary conditions
returnpos, returndisp, returnvel: return position, displacement field at particles, velocities [velocities only work for Zeld, 2LPT currently!]
plottest: show a slice of the particles
exactpk: Set each Fourier amplitude exactly to the linear power spectrum,
suppressing fluctuations in Fourier amplitudes
"""
if (returnpos & returndisp):
print 'Choose either position or displacement field to return'
return
if returnvel:
omegam = (ombh2+omch2)/(hubble/100.)**2
omegal = 1.-omk-omegam
hubble_z = 100.*N.sqrt(omegam*(1.+redshift)**3 + omk*(1+redshift)**2 + omegal)
# Valid only for simple dark energy; doesn't allow w != -1
if ((((c == None) | (returnvel & (smallscale != None))) &
((d == None) & (dk == None))) | (justreturnc == True)):
print 'c == None:', (c == None)
print 'returnvel = ', returnvel
c = pt.Camb(hubble=hubble, ombh2 = ombh2, omch2 = omch2,omk=omk,
transfer_kmax=kmax,transfer_redshift=[0.])
if (dk == None):
c.run()
sigma82default_z0 = pt.normalizePk(c,sigma8)
if redshift != 0.:
c = pt.Camb(hubble=hubble, ombh2 = ombh2, omch2 = omch2,omk=omk,
transfer_kmax=kmax,transfer_redshift=[redshift])
c.run()
c.pk *= sigma8**2/sigma82default_z0
c.logpk = N.log(c.pk)
c.pkSplineCoeff = SS.cspline1d(c.logpk)
if justreturnc:
return c
if (returnvel & (smallscale != None)):
print 'Numerically computing velocity'
cplusdeltaz = pt.Camb(hubble=hubble, ombh2 = ombh2, omch2 = omch2, omk=omk,
transfer_kmax=kmax,transfer_redshift=[redshift+deltaz4vel])
cplusdeltaz.run()
cplusdeltaz.pk *= sigma8**2/sigma82default_z0
cplusdeltaz.logpk = N.log(cplusdeltaz.pk)
growthindeltaz=N.mean(c.logpk-cplusdeltaz.logpk)
print 'camb:', growthindeltaz
print 'naive:',2.*N.log(getgrowth(c,z=redshift)/getgrowth(c,z=redshift+deltaz4vel))
noiselevel = N.std(c.logpk-cplusdeltaz.logpk)
print 'std/mean(growth from camb)=',noiselevel/growthindeltaz
if (noiselevel/growthindeltaz > 1./8.):
print "Warning! deltaz so small that it's giving lots of noise."
cplusdeltaz.pk = c.pk * N.exp(growthindeltaz)
cplusdeltaz.logpk = c.logpk + growthindeltaz
cplusdeltaz.pkSplineCoeff = SS.cspline1d(cplusdeltaz.logpk)
#The Hubble parameter at z=redshift
dispplusdeltaz = generate(c=cplusdeltaz,ng=ng,boxsize=boxsize,sigmaalpt = sigmaalpt,
largescale=largescale,smallscale=smallscale, seed = seed,
dopbc=dopbc, fileroot=fileroot, returnpos=False, returndisp=True,
plottest=False, returnvel=False,exactpk=exactpk)
# the Zel'dovich displacement-divergence in Fourier space
if d == None:
if dk == None:
kgrid = getkgrid(ng=ng,boxsize=boxsize,whattoget='k')
dk=makegauss(c,kgrid,boxsize=boxsize,exactpk=exactpk,returnfft=True,seed=seed)
if returnfft:
return dk
else:
#(over)write ng
ng=dk.shape[0]
d = N.fft.irfftn(dk)
else: #shouldn't have both d and dk non-None
print 'd supplied'
ng = d.shape[0]
kgrid = getkgrid(ng=ng,boxsize=boxsize,whattoget='k')
dk = N.fft.rfftn(d)
if ((scheme != None) & ((smallscale != None) | (largescale != None))):
print "Please specify only 'scheme' or ('smallscale' and 'largescale')"
if (smallscale == None) & (largescale == None):
if (scheme != None):
largescale = scheme
else:
print "Please specify either a full 'scheme' or "
print "a 'smallscale' and 'largescale' displacement field scheme."
return
print 'largescale=',largescale
if smallscale == 'sc':
psismall = N.fft.rfftn(sc(-d))
elif smallscale == 'muscle':
psismall = N.fft.rfftn(muscle(-d))
elif smallscale == 'zeld':
psismall = -dk
if largescale == 'zeld':
psilarge = -dk
elif largescale == '2lpt':
psiquadratic = N.fft.rfftn(twolpt(-dk,boxsize=boxsize))
psilarge = psiquadratic - dk
# dk because we didn't add it in twolpt for efficiency reasons
elif largescale == 'sc':
psilarge = N.fft.rfftn(sc(-d))
elif largescale == 'muscle':
psilarge = N.fft.rfftn(muscle(-d))
if (smallscale != None) & (largescale != None):
psik = scalegaussinterp(psilarge,psismall,kgrid,sigma=sigmaalpt)
elif smallscale != None:
psik = psismall
elif largescale != None:
psik = psilarge
disp = invdiv(dk=psik,boxsize=boxsize,dopsi2pos=False).reshape(ng,ng,ng,3)
pos = psi2pos(disp,boxsize=boxsize,dopbc=dopbc)
if returnvel: # only works for Zeld, 2LPT
time = 1./(1.+redshift)
print 'time, hubble_z, f_omega = ',time,hubble_z,f_omega(c,time)
vel = disp * time *hubble_z * f_omega(c,time)
print 'total factor = ',time*hubble_z*f_omega(c,time)
print 'factor in gadget = ',N.sqrt(time)*hubble_z*f_omega(c,time)
if scheme == '2lpt':
vel += 3./7. * time * hubble_z * f2_omega(c,time)* \
invdiv(dk=psiquadratic,boxsize=boxsize,dopsi2pos=False)#.swapaxes(0,2)
if plottest:
if fileroot == None:
fileroot='plottest'
plotslice(pos,filename=fileroot+'.png',boxsize=boxsize)
if returndisp:
return disp
if (returninitdens & (returnpos == False) & (returnvel == False)):
return d
if (returnpos & returnvel & (returninitdens == False)):
return pos,vel
if (returnpos & returninitdens & (returnvel == False)):
return pos,d
if (returnpos & returnvel & returninitdens):
return pos,vel,d
if returnpos:
return pos
if returnvel:
return vel
return
def splinefit(xdata,ydata):
xs=arange(min(xdata),max(xdata),0.1/float(len(xdata)))
cj=cspline1d(array(ydata))
return (xs,cspline1d_eval(cj,xs,dx=xdata[1]-xdata[0],x0=xdata[0]))
def doresample(orig_x, orig_y, new_x, method="cubic", padlen=0, antialias=False, debug=False):
"""
Resample data from one spacing to another. By default, does not apply any antialiasing filter.
Parameters
----------
orig_x
orig_y
new_x
method
padlen
Returns
-------
"""
tstep = orig_x[1] - orig_x[0]
if padlen > 0:
rawxpad = np.linspace(0.0, padlen * tstep, num=padlen, endpoint=False)
frontpad = rawxpad + orig_x[0] - padlen * tstep
backpad = rawxpad + orig_x[-1] + tstep
pad_x = np.concatenate((frontpad, orig_x, backpad))
pad_y = tide_filt.padvec(orig_y, padlen=padlen)
else:
pad_x = orig_x
pad_y = orig_y
if debug:
print("padlen=", padlen)
print("tstep=", tstep)
print("lens:", len(pad_x), len(pad_y))
print(pad_x)
print(pad_y)
fig = pl.figure()
ax = fig.add_subplot(111)
ax.set_title("Original and padded vector")
pl.plot(orig_x, orig_y + 1.0, pad_x, pad_y)
pl.show()
# antialias and ringstop filter
init_freq = len(pad_x) / (pad_x[-1] - pad_x[0])
final_freq = len(new_x) / (new_x[-1] - new_x[0])
if antialias and (init_freq > final_freq):
aafilterfreq = final_freq / 2.0
aafilter = tide_filt.NoncausalFilter(filtertype="arb", transferfunc="trapezoidal")
aafilter.setfreqs(0.0, 0.0, 0.95 * aafilterfreq, aafilterfreq)
pad_y = aafilter.apply(init_freq, pad_y)
if method == "cubic":
cj = signal.cspline1d(pad_y)
# return tide_filt.unpadvec(
# np.float64(signal.cspline1d_eval(cj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])), padlen=padlen)
return signal.cspline1d_eval(cj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])
elif method == "quadratic":
qj = signal.qspline1d(pad_y)
# return tide_filt.unpadvec(
# np.float64(signal.qspline1d_eval(qj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])), padlen=padlen)
return signal.qspline1d_eval(qj, new_x, dx=(orig_x[1] - orig_x[0]), x0=orig_x[0])
elif method == "univariate":
interpolator = sp.interpolate.UnivariateSpline(pad_x, pad_y, k=3, s=0) # s=0 interpolates
# return tide_filt.unpadvec(np.float64(interpolator(new_x)), padlen=padlen)
return np.float64(interpolator(new_x))
else:
print("invalid interpolation method")
return None
def splinefit(xdata, ydata, nx):
xs = arange(min(xdata), max(xdata), 1.0 / float(nx) / len(xdata))
cj = cspline1d(ydata)
return (xs, cspline1d_eval(cj, xs, dx=xdata[1] - xdata[0], x0=xdata[0]))
newwave = initialpixel + deltapix * np.arange(npix)
newflux = np.zeros((len(flux), npix + 1))
newand = np.zeros((len(flux), npix + 1))
newor = np.zeros((len(flux), npix + 1))
chisq = np.zeros(len(flux))
newinvvar = np.zeros((len(flux), npix + 1))
#resample spectra at single wavelength spectrum defined above
smoothing_parameter = 3.0
spline_order = 3
number_of_knots = -1
for p in range(len(flux)):
nonzero = np.where(wavevector[p, :] != 0.)
fitcoeff = cspline1d(flux[p], lamb=smoothing_parameter)
fitcoeff_inv = cspline1d(invvar[p], lamb=smoothing_parameter)
newflux[p, :] = cspline1d_eval(fitcoeff,
newwave,
dx=wave1[p],
x0=wavevector[p, 0])
newinvvar[p, :] = cspline1d_eval(fitcoeff_inv,
newwave,
dx=wave1[p],
x0=wavevector[p, 0])
oldfit = cspline1d_eval(fitcoeff,
wavevector[p, nonzero][0],
dx=wave1[p],
x0=wavevector[p, 0])
chisq[p] = np.sum(np.sqrt(
(oldfit - flux[p])**2. * [p])) / np.shape(flux[p])[0]
def compute():
print ""
#####################
#Read in the chi file
xxs, yys = readchi(chifilename)
s2ti = int(sum([1 for i in xxs
if i < s2t])) #index of the starting location
#####################
#Load in the MgO data
mgo_a0 = 4.213
import os
(ARs, Ts,
PPs) = loadMgO(os.getenv("HOME") + '/Documents/ascwork/EOS/mgo_eos.dat')
As = [i * mgo_a0 for i in ARs]
if Tval == 0.0:
Ps = PPs[:, 0]
elif Tval == 300.0:
As.insert(0, mgo_a0)
Ps = PPs[:, 1].tolist()
Ps.insert(0, 1.0)
else:
Ps = interp_T(Tval, Ts[2:], PPs[:, 2:])
#####################
#Analyze the spectrum: find the peaks
ind = s2ti
inpleft = list()
inpright = list()
while True:
ind = localMax(yys, ind, delta)
if ind == -1:
break
else:
inpleft.append(ind)
rind = s2ti
yreverse = yys[::-1]
while True:
rind = localMax(yreverse, rind, delta)
if rind == -1 or rind < s2ti:
break
else:
ind = len(yys) - rind - 1
inpright.append(ind)
ysmth = windowavg(yys, 15)
ind = s2ti
while True:
ind = localMax(ysmth, ind, delta)
if ind == -1:
break
else:
inpleft.append(ind)
inp = list()
for i in inpright:
possibles = [j for j in inpleft if abs(i - j) < 5]
if len(possibles) > 0:
inp.append(sum(possibles) / len(possibles))
inp = sort(list(set(inp)))
#Write the current peak locations to a file, to be altered by user
towrite = "peak leftbnd rightbnd\n"
towrite += "".join([str(xxs[i]) + " \n" for i in inp])
fname = "peaks_" + chifilename.split("_")[2].split(".")[0] + ".dat"
#Check if the file already exists, if so don't overwrite it!
exists = False
try:
open(fname, "r")
[centerxsold, startxsold, endxsold] = readpeaks(fname)
centers2 = theta2index(xxs, centerxsold)
starts2 = theta2index(xxs, startxsold)
ends2 = theta2index(xxs, endxsold)
exists = True
except IOError as e:
print "%s File doesn't exist creating new one." % fname
open(fname, "w").write(towrite)
except ValueError as e:
pass
#Begin interactive portion
print "List the starting and ending points of the peaks in the file %s." % fname
print "You can add or delete peaks as needed from here."
print "Close the graph when done."
p = Process(target=openemacs, args=fname)
p.start()
#Open up a plot so the user can select the peaks
pl.plot(xxs, yys)
if exists:
for i in centers2:
pl.scatter(xxs[i], yys[i], marker="o")
for i in starts2:
pl.text(xxs[i], yys[i], "S")
for i in ends2:
pl.text(xxs[i], yys[i], "E")
pl.legend(["diff pattern", "center", "start", "end"])
else:
for i in inp:
pl.scatter(xxs[i], yys[i])
pl.show()
p.join()
print "Thanks, got it."
#Read in the newly user generated peaks file
[centerxs, startxs, endxs] = readpeaks(fname)
pcenters = theta2index(xxs, centerxs)
pstarts = theta2index(xxs, startxs)
pends = theta2index(xxs, endxs)
peaks = [[pcenters[i], list(),
list(), list(), list(), 0] for i in range(len(pcenters))]
#Check if there is enough space between the two points.
badgap = False
for i in range(len(pcenters)):
if pends[i] - pstarts[i] < 8:
badgap = True
print ""
print "Error not enough space between start and end points on peak #%d at %g." % (
i + 1, xxs[pcenters[i]])
print "Gap must be at least 7 points wide otherwise fit will be inaccurate."
if badgap: exit()
"""
#####################
#Windowed average to smooth out the plot, useful for multi-peak analysis
yysmth=windowavg(yys,11)
#####################
#Find the groups of peaks from the smooth plot
(pstarts,pends,pgroups)=findclusterbounds(yysmth,inp)
ingroup=list()
for i in inp:
found=False
for group in pgroups:
for j in group:
if i==j:
found=True
break
if found:
break
if not(found):
ingroup.append(False)
else:
ingroup.append(True)
####################
#Transfer the group peaks location from the smooth plot to the original
for g in range(len(pgroups)):
for s in range(len(pgroups[g])):
smthpeak=xxs[pgroups[g][s]]
for i in range(len(inp)):
if abs(smthpeak-xxs[inp[i]]) < 0.05:
pgroups[g][s]=i
break
"""
mpeaks = list()
for i in range(len(peaks)):
print "Fitting peak at %g.\n" % xxs[ind]
ind = peaks[i][0]
start = pstarts[i]
end = pends[i]
[xdata, ydata, coefs] = glinitguess(xxs[start:end], yys[start:end])
peaks[i][4] = coefs
[peaks[i][2], peaks[i][3]] = glfit(xdata, ydata, coefs)
peaks[i][1] = xdata
peaks[i][5] = localMax(peaks[i][2], 0, 1) #new peak
"""
#####################
#Further Refine peaks by seperating out convoluted peaks
for i in range(len(pgroups)):
mpeaks.append(list())
(start,end,group)=(pstarts[i],pends[i],pgroups[i])
groupcoefs=list()
for p in group:
groupcoefs.append(peaks[p][4])
[xdata,ydata,initlsq]=mglinitguess(xxs[start:end],yys[start:end],groupcoefs)
[mgly,lsq]=mglfit(xdata,ydata,initlsq,len(groupcoefs))
mglx=xdata
ilsq=extractpks(lsq,len(group))
for j in range(len(group)):
peaks[group[j]][3]=ilsq[j]
[peaks[group[j]][1],peaks[group[j]][2]]=[xdata,glval(xdata,ilsq[j])]
refpk=localMax(peaks[group[j]][2],0,1)
peaks[group[j]][5]=refpk
mpeaks[i].append(mglx)
mpeaks[i].append(mgly)
"""
#####################
#Plot normal peaks
#Draw the blue peaks first to be overwritten by red peaks
pl.figure()
pl.plot(xxs, yys, ls='dotted')
xx = [xxs[i[0]] for i in peaks]
yy = [yys[i[0]] for i in peaks]
[pl.scatter(xx[i], yy[i], label=str(xx[i])) for i in range(len(peaks))]
#[pl.text(xx[i],yy[i],str(round(xx[i],2)),position=(xx[i],yy[i]),size='x-small') for i in range(len(peaks))]
pl.title(chifilename + ", T=" + str(Tval) + ", Kmag=sqrt(" + str(ksq) +
")")
#Plot fitted peaks
for i in range(len(peaks)):
pl.plot(peaks[i][1], peaks[i][2])
for i in range(len(mpeaks)):
pl.plot(mpeaks[i][0], mpeaks[i][1], ls='dashed')
#Plot initial guesses
#for i in range(len(peaks)):
# pl.plot(peaks[i][1],glval(peaks[i][1],peaks[i][4]))
# print peaks[i][4]
#for i in range(len(mpeaks)):
# pl.plot(mpeaks[i][0],mpeaks[i][1],ls='dashed')
#####################
#Find possible peak matches
s = UnivariateSpline(As, Ps)
sas = linspace(min(As), max(As), len(As))
sps = s(sas)
coefs = cspline1d(sps)
pressure = list()
ks = list()
theas = list()
thetas = list()
i = 0
for (ind, xgf, ygf, lsq, initlsq, npk) in peaks: #for each peak found
theta2 = xgf[npk]
intens = ygf[npk]
i += 1
d = lamda / (2.0 * sin(radians(theta2) / 2.0))
for j in ksq: #for each k value given
a = d * sqrt(float(j))
if (a > min(As) - tol and a < max(As) + tol):
#######################
#Found an MgO peak
ks.append(j)
theas.append(a)
thetas.append(theta2)
pressure.append(
cspline1d_eval(coefs, [a], dx=sas[1] - sas[0], x0=sas[0]))
pl.scatter(theta2, intens, s=30, c='red', marker='o')
pl.text(theta2,
intens - 0.5,
str(round(theta2, 5)),
position=(theta2, intens),
size='x-small')
#ksq.remove(j)
#break
#####################
#Print Results
print "Possible Matches:"
print "kmag\t| theta2(deg)\t| pressure(GPa)\t| a (Angstroms"
for i in range(len(ks)):
print str(ks[i]) + "\t| " + str(round(thetas[i], 5)) + " \t| " + str(
round(pressure[i][0], 2)) + " \t| " + str(round(theas[i], 5))
avgp = sum(pressure) / len(pressure)
print "At temperature " + str(Tval) + "K"
err = max([fabs(i - avgp) for i in pressure])
print "Average Pressure: " + str(round(avgp, 2)) + "GPa, Error: " + str(
round(err, 3)) + "GPa, StdDev: " + str(round(std(pressure), 3))
pl.show()
def compute(chifile, peaksfile, Tfil, delta, ksq, writefile, minp, maxp,
lamda):
xxs, yys = readchi(chifile)
#####################
#Read in the peaks file
found = False
peaksx = list()
peaksy = list()
approx_p = 0.0
if not (peaksfile is None):
f = open(peaksfile, 'r')
for line in f:
if line[0] == '#':
continue
line = line.lstrip().rstrip()
[fname, Ttemp, lamda, approx_p, line] = line.split(None, 4)
if fname == chifile:
lamda = float(lamda)
approx_p = float(approx_p)
if Tfil is None:
Tfil = float(Ttemp)
found = True
break
if found:
val = line.split(None, 2)
if val[0] == '0' or val[0] == '-1': #No information on peaks
startloc = 0
else:
startloc = float(val[0]) #get the new peak info
[peaksx.append(float(i)) for i in val[1].split(',')]
peaksx.sort()
i = 0
px = peaksx[i]
for (j, xx) in enumerate(xxs):
if px < xx:
peaksy.append(((xx - px) * yys[j] +
(px - xxs[j - 1]) * yys[j - 1]) /
(xxs[j] - xxs[j - 1]))
i += 1
if i == len(peaksx):
break
px = peaksx[i]
else:
print "\nError: Unable to find chi file " + chifile + " in peaks file " + peaksfile
print "\nTry calling again without the peaks file arguement."
exit(0)
else:
startloc = xxs[0]
#####################
#Load in the MgO data
mgo_a0 = 4.213
(ARs, Ts, PPs) = loadMgO('/home/acadien/Documents/ascwork/EOS/mgo_eos.dat')
As = [i * mgo_a0 for i in ARs]
if Tfil == 0.0:
Ps = PPs[:, 0]
elif Tfil == 300.0:
As.insert(0, mgo_a0)
Ps = PPs[:, 1].tolist()
Ps.insert(0, 1.0)
else:
Ps = interp_T(Tfil, Ts[2:], PPs[:, 2:])
#####################
#Analyze the spectrum: find the peaks
inp = list()
startloc = max(startloc, 5.0)
for (ind, xx) in enumerate(xxs):
if xx >= startloc:
break
strtind = ind
while True:
ind = localMax(yys, ind, delta)
if ind == -1:
break
else:
mxslp = max(
[fabs(yys[j] - yys[j + 1]) for j in range(ind - 5, ind + 5)])
if mxslp > 0.1:
inp.append(ind)
rind = 50
yreverse = yys[::-1]
while True:
rind = localMax(yreverse, rind, delta)
if len(xxs) - rind >= strtind:
break
if rind == -1:
break
else:
ind = len(yys) - rind
found = False
for pk in inp:
if abs(pk - ind) < 3:
found = True
break
if found == False:
if ind < 50:
continue
mxslp = max([
fabs(yys[j] - yys[j + 1]) for j in range(ind - 5, ind + 5)
])
if mxslp > 0.1:
inp.append(ind)
inp.sort()
#####################
#Plot normal peaks
#Draw the blue peaks first to be overwritten by red peaks
pl.figure()
pl.plot(xxs, yys, ls='dotted')
xx = [xxs[i] for i in inp]
yy = [yys[i] for i in inp]
[pl.scatter(a, b) for (a, b) in zip(xx, yy)]
[pl.scatter(a, b) for (a, b) in zip(peaksx, peaksy)]
pl.title(chifile + ", T=" + str(Tfil) + ", Kmag=sqrt(" + str(ksq) + ")")
#####################
#Calculate the MgO Peaks at this pressure
#Get the MgO lattice constant for the desired pressure
mgo_s = UnivariateSpline(Ps, As)
print Ps
mgo_sps = linspace(min(Ps), max(Ps), len(Ps))
mgo_sas = mgo_s(mgo_sps)
coefs = cspline1d(mgo_sas)
latconst = cspline1d_eval(coefs, [approx_p],
dx=mgo_sps[1] - mgo_sps[0],
x0=mgo_sps[0])[0]
#Get the intensity factors
mgo_ks = [3, 4, 8, 9, 11, 12] #Valid K vectors for MgO
mgo_mp = [8.0, 6.0, 12.0, 6.0, 24.0, 8.0] #Multiplicity
mgo_sf = [1.0, 3.0, 3.0, 1.0, 1.0, 3.0] #Structure Factor
mgo_Im = [(mgo_sf[i] * mgo_sf[i]) / mgo_mp[i]
for i in range(len(mgo_sf))] #Intensity multiplier
#Find the MgO peaks at this pressure
mgo_2th = list()
mgo_I = list()
for (i, K) in enumerate(mgo_ks):
theta = asin(lamda * sqrt(float(K)) * 0.5 / latconst)
mgo_2th.append(degrees(theta) * 2)
mgo_I.append(mgo_Im[i] * (1 + cos(theta * 2) * cos(theta * 2)) /
(sin(theta) * sin(theta) * cos(theta)))
mxI = max(mgo_I)
mxA = sum(xxs) / len(xxs)
mgo_I = [(i / mxI + 1) * mxA * mxA for i in mgo_I]
#####################
#Find possible peak matches
s = UnivariateSpline(As, Ps)
sas = linspace(min(As), max(As), len(As))
sps = s(sas)
coefs = cspline1d(sps)
pressure = list()
ks = list()
theas = list()
thetas = list()
peaksx.extend([xxs[i] for i in inp])
peaksy.extend([yys[i] for i in inp])
for j in ksq: #for each k value given
thepeak = mgo_2th[mgo_ks.index(next(p for p in mgo_ks if int(j) == p))]
i = findnearest(peaksx, thepeak)
#####################
#Refine the peak using a Spline fit
ind = findnearest(xxs, peaksx[i])
lowbnd = ind - 10
upbnd = ind + 10
#[strt,end]=findpeakbounds(yys,findnearest(xxs,peaksx[i]),lowbnd,upbnd)
#[xd,yd]=splinefit(xxs[strt:end],yys[strt:end],10*(end-strt))
#pl.plot(xd,yd)
pl.plot([thepeak, thepeak], [0, peaksy[i]], color='red')
pl.text(thepeak, 5, str(j))
#pkind=posmax(yd)
#(theta2,intens)=(xd[pkind],yd[pkind])
(theta2, intens) = (xxs[ind], yys[ind])
"""if round(theta2,2)==8.84: theta2=8.73"""
d = lamda / (2.0 * sin(radians(theta2) / 2.0))
a = d * sqrt(float(j))
if (a > min(As) - tol and a < max(As) + tol):
#Found a valid MgO peak
pres = cspline1d_eval(coefs, [a], dx=sas[1] - sas[0], x0=sas[0])[0]
if pres < minp or pres > maxp:
continue
ks.append(j)
theas.append(a)
thetas.append(theta2)
pressure.append(pres)
pl.scatter(theta2, intens, s=30, c='red', marker='o')
pl.text(theta2,
intens,
str(round(theta2, 2)),
position=(theta2, intens),
size='x-small')
#####################
#Print Results
print "Possible Matches near approximated pressure " + str(approx_p)
print "kmag\t| theta2(deg)\t| pressure(GPa)\t| a (Angstroms"
for i in range(len(ks)):
print str(ks[i]) + "\t| " + str(round(thetas[i], 5)) + " \t| " + str(
round(pressure[i], 2)) + " \t| " + str(round(theas[i], 5))
avgp = sum(pressure) / len(pressure)
print "At temperature " + str(Tfil) + "K"
err = max([fabs(i - avgp) for i in pressure])
print "Average Pressure: " + str(round(avgp, 2)) + "GPa, Error: " + str(
round(err, 2)) + "GPa, StdDev: " + str(round(std(pressure), 2))
pl.show()
######################
#Write results to file
if writefile is not None:
print "Appending results to file " + writefile + "."
file = open(writefile, 'a')
file.write(chifile + "\t" + str(Tfil) + "\t" + str(round(avgp, 2)) +
"\t" + str(round(err, 2)) + "\t" + str(ks) + "\t" +
str([str(round(i, 2)) for i in pressure]) + "\n")
def getVelocity(self, samplesData:DataFrame, smooth:str, convertToDeg:bool) -> DataFrame:
"""Method for calculating eye velocity, normally pixels converted to degrees first.
:param samplesData: dataframe to operate on, containing appropriate eyetracker columns (Time, X, Y, etc.).
:param smooth: algo to use, normally passed by command line argument.
:param convertToDeg: whether data is passed in raw pixel values or visual angle degrees.
:return: data with added *Velocity columns (and smoothed position columns).
"""
#TODO data column names hard-coded, need refactor to global name dictionary mapper (SMI, Tobii variants)
# mapping goes to multiData metadata property
#TODO B side (binocular) variant not implemented (applicable for SMI ETG)
if all(samplesData['L POR X [px]'] == samplesData['R POR X [px]']) and all(samplesData['L POR Y [px]'] == samplesData['R POR Y [px]']):
self.main.printToOut('Left and right channels detected equivalent. Working with one channel only.')
samplesData.metadata['equivalent'] = True
metadata = samplesData.metadata
self.main.printToOut('WARNING: Dimensions metadata from samples file is considered correct and precise, and used in pixel-to-degree conversions.')
self.main.printToOut('Now calculating velocity, be patient.')
if metadata['equivalent']:
#должен быть ведущий глаз
sides = ['R']
else:
sides = ['L', 'R']
#TODO skipping one channel if same
for side in sides:
for dim in ['X', 'Y']:
# smoothing
dataToSmooth = samplesData['{0} POR {1} [px]'.format(side, dim)]
if smooth == 'savgol':
samplesData['{0}POR{1}PxSmoothed'.format(side, dim)] = savgol_filter(dataToSmooth, 15, 2)
elif smooth == 'spline':
#scipy.interpolate.UnivariateSpline(x,y, k=1).get_coeffs()
samplesData['{0}POR{1}PxSmoothed'.format(side, dim)] = cspline1d(np.array(dataToSmooth), lamb=3)
elif smooth == 'conv':
#width and shape of convolution, equivalent to moving average if all 1
win = np.array([1,1,1,1,1,1])
samplesData['{0}POR{1}PxSmoothed'.format(side, dim)] = convolve(np.array(dataToSmooth), in2=win, mode='same') / win.sum()
else:
self.main.printToOut('ERROR: Invalid smoothing function specified.')
if dim == 'X':
screenDim = metadata['screenWidthPx']
screenRes = metadata['screenHResMm']
multiplier = 1
elif dim == 'Y':
screenDim = metadata['screenHeightPx']
screenRes = metadata['screenVResMm']
multiplier = -1
if not convertToDeg:
self.main.printToOut('ERROR: Raw pixels in data are currently assumed, column names hard-coded.')
raise NotImplementedError
else:
#converting to DEGREES
samplesData['{0}POR{1}Mm'.format(side, dim)] = multiplier * (samplesData['{0} POR {1} [px]'.format(side, dim)] - screenDim / 2) * screenRes
coordsMm = samplesData['{0}POR{1}Mm'.format(side, dim)]
samplesData['{0}POR{1}Deg'.format(side, dim)] = np.sign(coordsMm) * coordsMm.apply(lambda x: Utils.getSeparation(x,0, 0,0, z=metadata['headDistanceMm'], mode='fromCartesian'))
#----
samplesData['{0}POR{1}MmSmoothed'.format(side, dim)] = multiplier * (samplesData['{0}POR{1}PxSmoothed'.format(side, dim)] - screenDim / 2) * screenRes
coordsMm = samplesData['{0}POR{1}MmSmoothed'.format(side, dim)]
samplesData['{0}POR{1}DegSmoothed'.format(side, dim)] = np.sign(coordsMm) * coordsMm.apply(lambda x: Utils.getSeparation(x,0, 0,0, z=metadata['headDistanceMm'], mode='fromCartesian'))
#VELOCITY calculation
x = samplesData['{0}PORXDeg'.format(side)]
y = samplesData['{0}PORYDeg'.format(side)]
row = DataFrame({'x1':x[1:].reset_index(drop=True), 'y1':y[1:].reset_index(drop=True), 'x0':x[:(len(x) - 1)].reset_index(drop=True), 'y0':y[:(len(y) - 1)].reset_index(drop=True)})
seps = row.apply(lambda rowApply: Utils.getSeparation(x1=rowApply['x1'], y1=rowApply['y1'], x2=rowApply['x0'], y2=rowApply['y0'], z=metadata['headDistanceMm'], mode='fromPolar'), axis=1)
separation = np.hstack((1, seps))
timelag = np.hstack((1, np.diff(samplesData['Time'])))
samplesData['{0}Velocity'.format(side)] = separation / timelag
#----
x = samplesData['{0}PORXDegSmoothed'.format(side)]
y = samplesData['{0}PORYDegSmoothed'.format(side)]
row = DataFrame({'x1': x[1:].reset_index(drop=True), 'y1': y[1:].reset_index(drop=True), 'x0': x[:(len(x) - 1)].reset_index(drop=True), 'y0': y[:(len(y) - 1)].reset_index(drop=True)})
seps = row.apply(lambda rowApply: Utils.getSeparation(x1=rowApply['x1'], y1=rowApply['y1'], x2=rowApply['x0'], y2=rowApply['y0'], z=metadata['headDistanceMm'], mode='fromPolar'), axis=1)
separation = np.hstack((1, seps))
timelag = np.hstack(( 1, np.diff(samplesData['Time']) ))
samplesData['{0}VelocitySmoothed'.format(side)] = separation / timelag
self.main.printToOut('Done.', status='ok')
return samplesData
y = np.sin(t) # オブジェクト指向型の FITPACK のラッパー spl1 = interpolate.UnivariateSpline(t, y, s=0) y1 = spl1(tt) # UnivariateSpline で s=0 とした場合と同じ spl2 = interpolate.InterpolatedUnivariateSpline(t, y) y2 = spl2(tt) # 非オブジェクト指向型の FITPACK のラッパー c1 = interpolate.splrep(t, y) y3 = interpolate.splev(tt, c1) # 3 次スプライン曲線 c2 = signal.cspline1d(y) y4 = signal.cspline1d_eval(c2, tt) # 2 次スプライン曲線 c3 = signal.qspline1d(y) y5 = signal.qspline1d_eval(c3, tt) plt.figure() plt.plot(t, y, "o") plt.plot(tt, y1) plt.plot(tt, y2) plt.plot(tt, y3) plt.plot(tt, y4) plt.plot(tt, y5) plt.show()
n_samples = tkinter.simpledialog.askinteger('Number of samples',
'Type in the number of samples you want to be displayed (example: 3000, 6000, 10000 etc.)')
#Define ecg
record = wfdb.rdrecord(file, sampto=n_samples)
ann = wfdb.rdann(file, 'dat', sampto=n_samples)
#Filerecord
file_record = record.__dict__
#print(file_record)
wfdb.plot_items(signal=record.p_signal, title='ECG Signal',ann_samp=[ann.sample, ann.sample], time_units='samples', figsize=(10,4))
#Detect R-Peaks
signal_slice = np.ndarray.flatten(record.p_signal[0:n_samples])
smooth_signal = signal.cspline1d(signal_slice, lamb=1000) #smoothing the signal (filtering)
#r_peak_index = peakutils.indexes(smooth_signal, thres = 0.45, min_dist = 0.1) # first peak detection option
peak_index = signal.find_peaks_cwt(smooth_signal, widths= np.arange(60,80)) # second peak detection option
fig, ax = plt.subplots()
ax.set_title('Detect R peak')
ax.plot(signal_slice)
p_min_distance = -20 # marking for p-wave example
p_max_distance = -60
t_min_distance = 20 # marking for t-wave example
t_max_distance = 100
for peak in peak_index:
def interp(dx, knots, xis):
cspl = cspline1d(knots) #cupic spline coefficients
return cspline1d_eval(cspl, xis, dx=dx, x0=0.0)
def runCosmicEmu(self, sig8):
"""
use the CosmicEmu (Lawrence, Heitmann, Habib et al.) nonlinear power spectrum emulator.
Note that littleh will be (re)set, according to CMB constraint
"""
# first run in camb
#c_lin = copy.copy(self)
#c_lin.
a = 1./(self.cp.transfer_redshift[0] + 1)
if (a < 0.5)|(a > 1.):
print 'Warning! outside range of z accuracy (1 - 0).'
scalefax=N.arange(0.5,1.001,0.1)
coltoreturn = N.where(N.abs(a - scalefax) == min(N.abs(a - scalefax)))[0][0]
print 'returning results at a=',scalefax[coltoreturn]
f = file('emu.in','w')
f.write('emu.out\n')
f.write(str(self.cp.omch2+self.cp.ombh2)+'\n')
f.write(str(self.cp.ombh2)+'\n')
f.write(str(self.cp.scalar_spectral_index[0])+'\n')
f.write(str(sig8)+'\n')
f.write(str(self.cp.w)+'\n')
f.write('2\n')
f.close()
os.system('/Users/neyrinck/CosmicEmu_v1.1/emu.exe < emu.in > emu.err')
# read little h
f = open('emu.out','r')
for i in range(6):
dumb=f.readline()
littleh = float(f.readline().split()[-1])
self.cp.hubble = 100.*littleh
print 'littleh changed to ',littleh
f.close()
emu = N.loadtxt('emu.out')
kemu = emu[:,0]/littleh # should now be in h/Mpc
pemu = emu[:,coltoreturn+1]*littleh**3 # should now be in (Mpc/h)^3
if self.cp.transfer_k_per_logint == 0:
self.cp.transfer_k_per_logint = 512.
#need to get into log-scale k
self.k = kemu[0]*10.**N.arange(0.,N.log10(kemu[-1]/kemu[0]),1./self.cp.transfer_k_per_logint)
interpemu = SI.interp1d(N.log(kemu),N.log(pemu))#,kind='cubic')
#self.pk = interpemu(self.k)
self.pk = N.exp(interpemu(N.log(self.k)))
#self.pk = utils.splineIntLinExt(pemu, kemu, self.k)
self.logk = 1.*N.log(self.k)
self.logpk = 1.*N.log(self.pk)
#self.kextend(-5,3,calcsplinecoeff=True)
self.pkSplineCoeff = SS.cspline1d(self.logpk)
return
def splinefit(xdata, ydata):
xs = arange(min(xdata), max(xdata), 0.1 / float(len(xdata)))
cj = cspline1d(array(ydata))
return (xs, cspline1d_eval(cj, xs, dx=xdata[1] - xdata[0], x0=xdata[0]))
#!/usr/bin/python #coding: utf-8 from numpy import arange, cos, sin #duas funcoes do numpy para processamento de sinais from scipy.signal import cspline1d, cspline1d_eval #duas funcoes do Matplotlib para gerar um grafico from pylab import plot, show x0 = arange(20) y0 = cos(x0) * sin(x0 / 2) #Y a partir de x dx = x0[1] - x0[0] #diferenca original x1 = arange(-1, 21, 0.1) #coeficiente para arranjo de uma dimensao cj = cspline1d(y0) #Avalia o Spline para um novo conjunto de pontos y1 = cspline1d_eval(cj, x1, dx=dx, x0=x0[0]) plot(x1, y1, '-g', x0, y0, '^y') #Desenha show() #Mostra o grafico
def wiggle(values, origin=0, posFill='black', negFill=None, lineColor='black',
resampleRatio=10, rescale=False, zmin=0, zmax=None, ax=None):
"""
Plot a trace in VAWT(Variable Area Wiggle Trace)
Parameters
----------
x: input data (1D numpy array)
origin: (default, 0) value to fill above or below (float)
posFill: (default, black)
color to fill positive wiggles with (string or None)
negFill: (default, None)
color to fill negative wiggles with (string or None)
lineColor: (default, black)
color of wiggle trace (string or None)
resampleRatio: (default, 10)
factor to resample traces by before plotting (1 = raw data) (float)
rescale: (default, False)
If True, rescale "x" to be between -1 and 1
zmin: (default, 0)
The minimum z to use for plotting
zmax: (default, len(x))
The maximum z to use for plotting
ax: (default, current axis)
The matplotlib axis to plot onto
Returns
-------
Plot
"""
if zmax is None:
zmax = values.size
# Rescale so that values ranges from -1 to 1
if rescale:
values = values.astype(np.float)
values -= values.min()
values /= values.ptp()
values *= 2
values -= 1
# Interpolate at resampleRatio x the previous density
resample_z = np.linspace(0, values.size, values.size * resampleRatio)
# cubic spline interpolation
cj = cspline1d(values)
resample_v = cspline1d_eval(cj, resample_z)
# newz = np.linspace(zmax, zmin, resample_z.size)
# newz = np.linspace(zmin, zmax, resample_z.size)
newz = resample_z
if origin is None:
origin = resample_v.mean()
# # Plot
# if ax is None:
# ax = plt.gca()
# # plt.hold(True)
if posFill is not None:
ax.fill_betweenx(newz, resample_v, origin,
where=resample_v > origin,
facecolor=posFill)
if negFill is not None:
ax.fill_betweenx(newz, resample_v, origin,
where=resample_v < origin,
facecolor=negFill)
if lineColor is not None:
ax.plot(resample_v, newz, color=lineColor, linewidth=.1)
def get_errorbar(fv,
fname=None,
trace=None,
frac=0.1,
additional_fixed=None,
plotresult=False,
guess=dict()):
""" Use Lakowicz's f-statistic method to find the 95% confidence interval on a fitting parameter.
fv -- a string/dictionary key identifying the parameter to find a confidence interval on.
fname -- (optional, can use trace instead) fname of data file to fit.
trace -- can use trace instead of fname to pass in info on wraptime and irf fname, etc.
frac -- the fractional change in the parameter to use for the intial 5-point mesh
additional_fixed -- any parameters you want to hold fixed during the fitting
plotresult -- plot the f-statistic curve?
guess -- dictionary of initial parameters for the fit (by default, best-fit values are used)
"""
#bestfit, bestacorr = load_wire( fname )
if fname is not None:
raise ValueError(
'have modified this to prefer working with actual traces to forward wraptime, etc., to do_fit'
)
bestfit = load_wire(fname)
if trace is not None:
assert fname == None
bestfit = trace.fitresults.copy()
bestChi2 = bestfit['ReducedChi2']
irf = bestfit['irf_dispersion']
lkeys = ['l0']
akeys = ['a0']
if bestfit.has_key('l1'):
lkeys.append('l1')
akeys.append('a1')
if bestfit.has_key('l2'):
lkeys.append('l2')
akeys.append('a2')
if bestfit.has_key('l3'):
lkeys.append('l3')
akeys.append('a3')
fixedparams = [fv]
if additional_fixed is not None: fixedparams += additional_fixed
fv_best = bestfit[fv]
# If holding l1-l3 lifetimes fixed, as we did
# for the actual fit, then Fx should equal 1.0 at the 'bestfit' value of the parameter.
# But if l1-l3 are allowed to vary (making a more conservative error bar), then
# Fx may be lower than 1.0, and the minimum may not be at the "bestfit" value.
# This is to say that the bestfit of the constrained fit may not be the bestfit of the unconstrained fit.
#Fx = 1.0038 # Threshold found from F-statistic 1600 deg. freedom (~half trace points, following Fundamentals Of Fluorescence Spectroscopy)
Fx = 1.001858 # Threshold found from F-statistic on all 3282 points. Seems easier to justify
Fx_list = [
] # later we'll sort these in order of increasing parameter value to enable interpolation
val_step = frac * fv_best / 2
argvals = arange(fv_best * (1.0 - frac),
fv_best * (1.0 + frac) + val_step, val_step)
# do a coarse (5-pt) run across the data
for val in argvals:
bestfit[fv] = val
l = [bestfit[key] for key in lkeys]
a = [bestfit[key] for key in akeys]
params = do_fit(trace, l, a, fixedparams, irf, guess)
Fx_list.append([val, params['ReducedChi2'] / bestChi2])
if all(array(Fx_list)[:, 1] > Fx):
Fx_list = []
for val in argvals:
bestfit[fv] = val
cpy = bestfit.copy()
for key in lkeys:
if key not in fixedparams: cpy[key] = 1.25 * bestfit[key]
for key in akeys:
if key not in fixedparams: cpy[key] = 1.5 * bestfit[key]
l = [cpy[key] for key in lkeys]
a = [cpy[key] for key in akeys]
params = do_fit(trace, l, a, fixedparams, irf, guess)
Fx_list.append([val, params['ReducedChi2'] / bestChi2])
if all(array(Fx_list)[:, 1] > Fx):
raise ValueError("Problem fitting: always above Fx. Min: %f" %
(array(Fx_list)[:, 1].min()))
# if the left side (low param value) didn't exceed Fx threshold, extend
val = argvals[0]
while Fx_list[0][1] < Fx:
val -= val_step
if val < 0:
if fv in ['l1', 'l2', 'l3']:
raise ValueError("long-time component just went negative...")
else:
break
bestfit[fv] = val
l = [bestfit[key] for key in lkeys]
a = [bestfit[key] for key in akeys]
params = do_fit(trace, l, a, fixedparams, irf, guess)
Fx_list.append([val, params['ReducedChi2'] / bestChi2])
Fx_list.sort(
key=lambda x: x[0]) # sort by first element (parameter value)
# if the right side (high param value) didn't exceed Fx threshold, extend
val = argvals[-1]
while Fx_list[-1][1] < Fx:
val += val_step
bestfit[fv] = val
l = [bestfit[key] for key in lkeys]
a = [bestfit[key] for key in akeys]
params = do_fit(trace, l, a, fixedparams, irf, guess)
Fx_list.append([val, params['ReducedChi2'] / bestChi2])
Fx_list.sort(
key=lambda x: x[0]) # sort by first element (parameter value)
# interpolate to find values at threshold
Fx_array = array(Fx_list)
splines = cspline1d(Fx_array[:, 1])
interp_val = linspace(Fx_array[0, 0], Fx_array[-1, 0], 500)
interp_Fx = cspline1d_eval(splines,
interp_val,
dx=val_step,
x0=Fx_array[:, 0].min())
error_bar = [
interp_val[find(interp_Fx < Fx)[0]],
interp_val[find(interp_Fx < Fx)[-1]]
]
if plotresult:
fig = figure(1)
#fig.clf()
ax_chi = fig.add_subplot(111)
ax_chi.cla()
ax_chi.plot(interp_val, interp_Fx, '-k')
ax_chi.plot(interp_val, [Fx] * len(interp_val), '--k')
ax_chi.plot(Fx_array[:, 0], Fx_array[:, 1], 'sg')
ax_chi.plot(error_bar, [Fx] * 2, '-b', lw=3.0)
ax_chi.set_ylim([0.99, 1.01])
fig.show()
fig.canvas.draw()
return error_bar