本文整理汇总了Python中numpy.isreal函数的典型用法代码示例。如果您正苦于以下问题:Python isreal函数的具体用法?Python isreal怎么用?Python isreal使用的例子?那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。
在下文中一共展示了isreal函数的20个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于我们的系统推荐出更棒的Python代码示例。
示例1: is_finite
def is_finite(x):
try:
if type(x) == str:
return False
return np.array([np.isreal(e) and np.isfinite(e) for e in x], dtype=bool)
except TypeError:
return np.isreal(x) and np.isfinite(x)
开发者ID:paleolimbot,项目名称:dflite,代码行数:7,代码来源:na.py
示例2: is_nan
def is_nan(x):
try:
if type(x) == str:
raise TypeError()
return np.array([e == NA_character_ or (np.isreal(e) and np.isnan(e)) for e in x], dtype=bool)
except TypeError:
return x == NA_character_ or (np.isreal(x) and np.isnan(x))
开发者ID:paleolimbot,项目名称:dflite,代码行数:7,代码来源:na.py
示例3: test_multib0_dsi
def test_multib0_dsi():
data, gtab = dsi_voxels()
# Create a new data-set with a b0 measurement:
new_data = np.concatenate([data, data[..., 0, None]], -1)
new_bvecs = np.concatenate([gtab.bvecs, np.zeros((1, 3))])
new_bvals = np.concatenate([gtab.bvals, [0]])
new_gtab = gradient_table(new_bvals, new_bvecs)
ds = DiffusionSpectrumModel(new_gtab)
sphere = get_sphere('repulsion724')
dsfit = ds.fit(new_data)
pdf = dsfit.pdf()
dsfit.odf(sphere)
assert_equal(new_data.shape[:-1] + (17, 17, 17), pdf.shape)
assert_equal(np.alltrue(np.isreal(pdf)), True)
# And again, with one more b0 measurement (two in total):
new_data = np.concatenate([data, data[..., 0, None]], -1)
new_bvecs = np.concatenate([gtab.bvecs, np.zeros((1, 3))])
new_bvals = np.concatenate([gtab.bvals, [0]])
new_gtab = gradient_table(new_bvals, new_bvecs)
ds = DiffusionSpectrumModel(new_gtab)
dsfit = ds.fit(new_data)
pdf = dsfit.pdf()
dsfit.odf(sphere)
assert_equal(new_data.shape[:-1] + (17, 17, 17), pdf.shape)
assert_equal(np.alltrue(np.isreal(pdf)), True)
开发者ID:albayenes,项目名称:dipy,代码行数:26,代码来源:test_dsi.py
示例4: findSigT
def findSigT(xIn, yIn):
##
## Added to check their sig test. Yes I know it is paranoid rjel
## regPoints are the number of points going into the
## regression calculation.
## Check that there are some points not masked out first. Else you
## get horrible errors.
if np.any(np.isreal(((xIn <= 1.0) & (np.isreal(yIn))))):
rPoints = int(((xIn <= 1.0) & np.isreal(yIn)).sum())
else:
rPoints = 0
## print( 'There are ', regPoints,' points in the calculation')
##
## Find the value in the ttest table corresponding to n and
## the p value of interest. The table I downloaded had 1-100
## points then more than 100
if (rPoints < 103) & (rPoints > 2):
nIndex = rPoints - 2
##
## if there are less than 2 points don't bother
elif rPoints <= 2:
return 3000.0, rPoints
else:
nIndex = 101
## The first line of the t-table file has the p values in it
## so we can search a split first line for the column
## that contains a given p-value
##
pIndex = tTable[0].index(str(1.0 - p.pVal))
sigLocal = tTable[nIndex][pIndex]
return sigLocal, rPoints
开发者ID:lec8rje,项目名称:SWELTER,代码行数:32,代码来源:xCorrCalcVn3.0.py
示例5: filter_params
def filter_params(io, rsh, rs, ee, isc):
# Function filter_params identifies bad parameter sets. A bad set contains
# Nan, non-positive or imaginary values for parameters; Rs > Rsh; or data
# where effective irradiance Ee differs by more than 5% from a linear fit
# to Isc vs. Ee
badrsh = np.logical_or(rsh < 0., np.isnan(rsh))
negrs = rs < 0.
badrs = np.logical_or(rs > rsh, np.isnan(rs))
imagrs = ~(np.isreal(rs))
badio = np.logical_or(~(np.isreal(rs)), io <= 0)
goodr = np.logical_and(~badrsh, ~imagrs)
goodr = np.logical_and(goodr, ~negrs)
goodr = np.logical_and(goodr, ~badrs)
goodr = np.logical_and(goodr, ~badio)
matrix = np.vstack((ee / 1000., np.zeros(len(ee)))).T
eff = np.linalg.lstsq(matrix, isc)[0][0]
pisc = eff * ee / 1000
pisc_error = np.abs(pisc - isc) / isc
# check for departure from linear relation between Isc and Ee
badiph = pisc_error > .05
u = np.logical_and(goodr, ~badiph)
return u
开发者ID:mattguttenberg,项目名称:pvlib-python,代码行数:25,代码来源:PVsyst_parameter_estimation.py
示例6: bezier_curve_y_out
def bezier_curve_y_out(shift_angle, P0, P1, P2, P3, second_of_day=None):
'''
For a cubic Bezier segment described by the 2-tuples P0, ..., P3, return
the y-value associated with the given x-value.
Ex: getYfromXforBezSegment((10,0), (5,-5), (5,5), (0,0), 3.2)
'''
seconds_per_day = 24*60*60
# Check if the second of the day is provided.
# If provided, calculate y of the Bezier curve with that x
# Otherwise, use the current second of the day
if second_of_day is None:
now = datetime.datetime.now()
dt = datetime.timedelta(hours=now.hour, minutes=now.minute, seconds=now.second)
seconds = dt.total_seconds()
else:
seconds = second_of_day
# Shift the entire graph using 0 - 360 to determine the degree
if shift_angle:
percent_angle = shift_angle/360
angle_seconds = percent_angle*seconds_per_day
if seconds+angle_seconds > seconds_per_day:
seconds_shifted = seconds+angle_seconds-seconds_per_day
else:
seconds_shifted = seconds+angle_seconds
percent_of_day = seconds_shifted/seconds_per_day
else:
percent_of_day = seconds/seconds_per_day
x = percent_of_day*(P0[0]-P3[0])
# First, get the t-value associated with x-value, where t is the
# parameterization of the Bezier curve and ranges from 0 to 1.
# We need the coefficients of the polynomial describing cubic Bezier
# (cubic polynomial in t)
coefficients = [-P0[0] + 3*P1[0] - 3*P2[0] + P3[0],
3*P0[0] - 6*P1[0] + 3*P2[0],
-3*P0[0] + 3*P1[0],
P0[0] - x]
# Find roots of the polynomial to determine the parameter t
roots = np.roots(coefficients)
# Find the root which is between 0 and 1, and is also real
correct_root = None
for root in roots:
if np.isreal(root) and 0 <= root <= 1:
correct_root = root
# Check a valid root was found
if correct_root is None:
print('Error, no valid root found. Are you sure your Bezier curve '
'represents a valid function when projected into the xy-plane?')
param_t = correct_root
# From the value for the t parameter, find the corresponding y-value
# using the formula for cubic Bezier curves
y = (1-param_t)**3*P0[1] + 3*(1-param_t)**2*param_t*P1[1] + 3*(1-param_t)*param_t**2*P2[1] + param_t**3*P3[1]
assert np.isreal(y)
# Typecast y from np.complex128 to float64
y = y.real
return y
开发者ID:zsole2,项目名称:Mycodo,代码行数:60,代码来源:method.py
示例7: kurt
def kurt(x, opt):
if opt=='kurt2':
if np.all(x==0):
K=0
E=0
return K
x = x - np.mean(x)
E = np.mean(np.abs(x)**2)
if E < eps:
K=0
return K
K = np.mean(np.abs(x)**4)/E**2
if np.all(np.isreal(x)):
K = K - 3
else:
K = K - 2
if opt=='kurt1':
if np.all(x==0):
K=0
E=0
return K
x = x - np.mean(x)
E = np.mean(np.abs(x))
if E < eps:
K=0
return K
K = np.mean(np.abs(x)**2)/E**2
if np.all(np.isreal(x)):
K=K-1.57
else:
K=K-1.27
return K
开发者ID:ablkvo,项目名称:waveloc,代码行数:32,代码来源:kurtogram.py
示例8: read_matrix_sparse
def read_matrix_sparse(filename, dtype=float, comments='#'):
coo=np.loadtxt(filename, comments=comments, dtype=dtype)
"""Check if coo is (M, 3) ndarray"""
if len(coo.shape)==2 and coo.shape[1]==3:
row=coo[:, 0]
col=coo[:, 1]
values=coo[:, 2]
"""Check if imaginary part of row and col is zero"""
if np.all(np.isreal(row)) and np.all(np.isreal(col)):
row=row.real
col=col.real
"""Check if first and second column contain only integer entries"""
if np.all(is_integer(row)) and np.all(is_integer(col)):
"""Convert row and col to int"""
row=row.astype(int)
col=col.astype(int)
"""Create coo-matrix"""
A=scipy.sparse.coo_matrix((values,(row, col)))
return A
else:
raise ValueError('File contains non-integer entries for row and col.')
else:
raise ValueError('File contains complex entries for row and col.')
else:
raise ValueError('Given file is not a sparse matrix in coo-format.')
开发者ID:greglever,项目名称:PyEMMA,代码行数:30,代码来源:matrix.py
示例9: idct
def idct(self, X):
'''Compute inverse discrete cosine transform of a 1-d array X'''
N = len(X)
w = np.sqrt(2*N)*np.exp(1j*np.arange(N)*np.pi/(2.*N))
if (N%2==1) or (any(np.isreal(X))== False):
w[0] = w[0] * np.sqrt(2)
yy = np.zeros(2*N)
yy[0:N] = w * X
yy[N+1:2*N] = -1j * w[1:N] * X[1:N][::-1]
y = fftpack.ifft(yy)
x = y[0:N]
else:
w[0] = w[0]/np.sqrt(2)
yy = X *w
y = fftpack.ifft(yy)
x = np.zeros(N)
x[0:N:2] = y[0:N/2]
x[1:N:2] = y[N:(N/2)-1:-1]
if all(np.isreal(x)):
x = np.real(x)
return x
开发者ID:gboyes,项目名称:pydbm,代码行数:25,代码来源:utils.py
示例10: dct
def dct(self, x):
'''Compute discrete cosine transform of 1-d array x'''
#probably don't need this here anymore since it is in fftpack now
N = len(x)
#calculate DCT weights
w = (np.exp(-1j*np.arange(N)*np.pi/(2*N))/np.sqrt(2*N))
w[0] = w[0]/np.sqrt(2)
#test for odd or even function
if (N%2==1) or (any(np.isreal(x)) == False):
y = np.zeros(2*N)
y[0:N] = x
y[N:2*N] = x[::-1]
yy = fftpack.fft(y)
yy = yy[0:N]
else:
y = np.r_[(x[0:N:2], x[N:0:-2])]
yy = fftpack.fft(y)
w = 2*w
#apply weights
X = w * yy
if all(np.isreal(x)):
X = np.real(X)
return X
开发者ID:gboyes,项目名称:pydbm,代码行数:29,代码来源:utils.py
示例11: update_data
def update_data(self, attr, old, new):
mat = matrix(self.a_slider.value, self.b_slider.value,
self.c_slider.value, self.d_slider.value)
evals, evecs = np.linalg.eig(mat)
ev0, ev1 = evals
evec0 = evecs.T[0]
evec1 = evecs.T[1]
trans0 = mat @ evec0
trans1 = mat @ evec1
self.eigen0.text = "eigen0 = " + \
str(ev0) if np.isreal(ev0) else "eigen0 = None"
self.eigen1.text = "eigen1 = " + \
str(ev1) if np.isreal(ev1) else "eigen1 = None"
transXs, transYs = mat @ np.array([self.Xs, self.Ys])
self.source.data = dict(Xs=self.Xs, Ys=self.Ys,
transXs=transXs, transYs=transYs)
data0x = [0, evec0[0]] if np.isreal(ev0) else [0, 0]
data0y = [0, evec0[1]] if np.isreal(ev0) else [0, 0]
data1x = [0, evec1[0]] if np.isreal(ev1) else [0, 0]
data1y = [0, evec1[1]] if np.isreal(ev1) else [0, 0]
trans0x = [0, trans0[0]] if np.isreal(ev0) else [0, 0]
trans0y = [0, trans0[1]] if np.isreal(ev0) else [0, 0]
trans1x = [0, trans1[0]] if np.isreal(ev1) else [0, 0]
trans1y = [0, trans1[1]] if np.isreal(ev1) else [0, 0]
self.evectors.data = dict(ev0x=data0x, ev0y=data0y,
ev1x=data1x, ev1y=data1y,
transev0x=trans0x, transev0y=trans0y,
transev1x=trans1x, transev1y=trans1y)
开发者ID:terasakisatoshi,项目名称:PythonCode,代码行数:28,代码来源:2x2mat.py
示例12: sp_bin_by_space_and_time
def sp_bin_by_space_and_time(data, frameTime, xybin=8, counterTime=40.0e-9):
"""Takes a dataset collected by the SSI photon counting fast camera and bins
the data in time and xy.
arguments:
data - data to bin. This is an (N, 4) array where N is the number of
elements.
frameTime - Amout of time between bins. Measured in seconds
xybin - amount to bin in x and y. defaults to 8, which is a 512x512
output.
counterTime - clock time of the camera. Anton Tremsin says its 40 ns.
returns:
binnedData - a 3-dimension array (frames, y, x) of the binned data.
"""
assert isinstance(data, np.ndarray), "data must be an ndarray"
assert data.shape[1] == 4, "Second dimension must be 4."
assert np.isreal(frameTime), "frameTime (%s) must be real" % repr(frameTime)
assert np.isreal(counterTime), "counterTime (%s) must be real" % repr(counterTime)
# TODO: This could be accelerated if written for a GPU
firsttime = data[:,3].min()
lasttime = data[:, 3].max()
datalen = len(data[:, 0])
nbins = int(np.ceil(float(lasttime - firsttime)*counterTime/frameTime))
xybinnedDim = int(np.ceil(SP_MAX_SIZE/xybin))
binnedData = np.zeros((nbins, xybinnedDim, xybinnedDim), dtype='int')
bin_edges = np.linspace(firsttime, lasttime, nbins+1)
# slightly increase the last bin. For some reason the last bin is slightly too small, and the photons on the edges are not included
bin_edges[-1] = bin_edges[-1]*1.01
# If the frameTime is larger than the total acq time, then sum up everything
if frameTime >= (lasttime-firsttime)*counterTime:
histfn = lambda a,b: (len(a), b)
else:
# this is the default; bin data using histogram
histfn = np.histogram
for i in range(xybinnedDim):
x = data[:, 0]
y = data[:, 1]
xc = np.argwhere( (i*xybin <= x) & (x < (i+1)*xybin) )
idx_to_delete = np.array([])
for j in range(xybinnedDim):
yc = np.argwhere( (j*xybin <= y) & (y < (j+1)*xybin) )
isect, a, b = intersect(xc, yc, assume_unique=True)
if len(isect) != 0:
binned, bin_edges = histfn(data[isect,3]+0.5, bin_edges)
binnedData[:, i, j] = binned
idx_to_delete = np.append(idx_to_delete, isect)
data = np.delete(data, idx_to_delete, axis=0)
if binnedData.sum() != datalen:
print "warning: # of binned data photons (%d) do not match original dataset (%d)" % (binnedData.sum(), datalen)
return binnedData
开发者ID:conkr,项目名称:SCA,代码行数:58,代码来源:xpcs.py
示例13: test_it
def test_it(self):
self.assertTrue(np.isreal(ef.return_real_part(1)))
self.assertTrue(np.isreal(ef.return_real_part(1 + 0j)))
self.assertTrue(np.isreal(ef.return_real_part(1 + 1e-20j)))
self.assertRaises(TypeError, ef.return_real_part, None)
self.assertRaises(TypeError, ef.return_real_part, (1, 2.0, 2 + 2j))
self.assertRaises(TypeError, ef.return_real_part, [None, 2.0, 2 + 2j])
self.assertRaises(ValueError, ef.return_real_part, [1, 2.0, 2 + 2j])
self.assertRaises(ValueError, ef.return_real_part, 1 + 1e-10j)
self.assertRaises(ValueError, ef.return_real_part, 1j)
开发者ID:rihe,项目名称:pyinduct,代码行数:10,代码来源:test_eigenfunctions.py
示例14: symmNormalization
def symmNormalization(MPS, chir, chic):
omega, R = getLargestW(MPS, 'R')
R = fixPhase(R)
if np.isreal(R).all(): omega, R = omega.real, R.real
print "wR", omega, np.isreal(R).all(), "R\n", R
assym = np.linalg.norm(R - R.T.conj())
print "assym R", assym
Rvals, Rvecs = spla.eigh(R)
Rvals_s = np.sqrt(abs(Rvals))
Rvals_si = 1. / Rvals_s
print "Rvals", Rvals
Rs = np.dot(Rvecs, np.dot(np.diag(Rvals_s), Rvecs.T.conj()))
ARs = np.tensordot(MPS, Rs, axes=([1,0]))
Rsi = np.dot(Rvecs, np.dot(np.diag(Rvals_si), Rvecs.T.conj()))
A1 = np.tensordot(Rsi, ARs, axes=([1,0]))
A1 = np.transpose(A1, (0, 2, 1))
omega, L = getLargestW(A1, 'L')
L = fixPhase(L)
if np.isreal(L).all(): omega, L = omega.real, L.real
print "wL", omega, np.isreal(L).all(), "L\n", L
assym = np.linalg.norm(L - L.T.conj())
print "assym L", assym
Lambda2, U = spla.eigh(L)
A1U = np.tensordot(A1, U, axes=([1,0]))
A2 = np.tensordot(U.T.conj(), A1U, axes=([1,0]))
A2 = np.transpose(A2, (0, 2, 1))
print "Lambda**2", Lambda2#, "\n", U
Lambda = np.sqrt(abs(Lambda2))
Lambdas = np.sqrt(Lambda)
Lambdasi = 1. / Lambdas
A2Lsi = np.tensordot(A2, np.diag(Lambdasi), axes=([1,0]))
A3 = np.tensordot(np.diag(Lambdas), A2Lsi, axes=([1,0]))
A3 = np.transpose(A3, (0, 2, 1))
print "Lambda", Lambda
nMPS = A3 / np.sqrt(omega)
RealLambda = fixPhase(np.diag(Lambda))
#print "nMPS", nMPS.shape, "\n", nMPS
print "RealLambda", RealLambda.shape, "\n", RealLambda
######### CHECKING RESULT #########
Trace = np.linalg.norm(RealLambda)
ELambda = linearOpForR(nMPS, RealLambda).reshape(chir, chic)
LambdaE = linearOpForL(nMPS, RealLambda).reshape(chir, chic)
print "Trace(RealLambda)", Trace, "\nE|r)\n", ELambda, "\n(l|E\n", LambdaE
return RealLambda, nMPS
开发者ID:xrincon,项目名称:tdvp,代码行数:54,代码来源:iTdvp.py
示例15: _finalize_limits
def _finalize_limits(self, axis, view, subplots, ranges):
# Extents
extents = self.get_extents(view, ranges)
if extents and not self.overlaid:
coords = [coord if np.isreal(coord) else np.NaN for coord in extents]
if isinstance(view, Element3D) or self.projection == '3d':
l, b, zmin, r, t, zmax = coords
if not np.NaN in (zmin, zmax) and not zmin==zmax: axis.set_zlim((zmin, zmax))
else:
l, b, r, t = [coord if np.isreal(coord) else np.NaN for coord in extents]
if not np.NaN in (l, r) and not l==r: axis.set_xlim((l, r))
if not np.NaN in (b, t) and not b==t: axis.set_ylim((b, t))
开发者ID:gitter-badger,项目名称:holoviews,代码行数:12,代码来源:element.py
示例16: radialUndistort
def radialUndistort(rpp, k, quot=False, der=False):
'''dqD
takes distorted radius and returns the radius undistorted
optioally it returns the undistortion quotient rp = rpp * q
'''
# polynomial coeffs, grade 7
# # (k1,k2,p1,p2[,k3[,k4,k5,k6[,s1,s2,s3,s4[,τx,τy]]]])
# polynomial coeffs, grade 7
# # (k1,k2,p1,p2[,k3[,k4,k5,k6[,s1,s2,s3,s4[,τx,τy]]]])
k.shape = -1
poly = [[k[4], # k3
0,
k[1], # k2
0,
k[0], # k1
0,
1,
-r] for r in rpp]
# calculate roots
rootsPoly = array([roots(p) for p in poly])
# return flag, True if there is a suitable (real AND positive) solution
rPRB = isreal(rootsPoly) & (0 <= real(rootsPoly)) # real Positive Real Bool
retVal = any(rPRB, axis=1)
rp = empty_like(rpp)
if any(~ retVal): # if at least one case of non solution
# calculate extrema of polyniomial
rExtrema = roots([7*k[4], 0, 5*k[1], 0, 3*k[0], 0, 1])
# select real extrema in positive side, keep smallest
rRealPos = min(rExtrema.real[isreal(rExtrema) & (0<=rExtrema.real)])
# assign to problematic values
rp[~retVal] = rRealPos
# choose minimum positive roots
rp[retVal] = [min(rootsPoly[i, rPRB[i]].real)
for i in arange(rpp.shape[0])[retVal]]
if der:
# derivada de la directa
q, dQdP, dQdK = radialDistort(rp, k, der=True)
if quot:
return q, retVal, dQdP, dQdK
else:
return rp, retVal, dQdP, dQdK
else:
if quot:
return rp / rpp, retVal
else:
return rp, retVal
开发者ID:sebalander,项目名称:sebaPhD,代码行数:53,代码来源:PolyCalibration.py
示例17: kurt
def kurt(x, opt):
"""
Calculates kurtosis of a signal according to the option chosen
:param x: signal
:param opt: ['kurt1' | 'kurt2']
* 'kurt1' = variance of the envelope magnitude
* 'kurt2' = kurtosis of the complex envelope
:type x: numpy array
:type opt: string
:rtype: float
:returns: Kurtosis
"""
if opt == 'kurt2':
if np.all(x == 0):
K = 0
E = 0
return K
x = x - np.mean(x)
E = np.mean(np.abs(x)**2)
if E < eps:
K = 0
return K
K = np.mean(np.abs(x)**4)/E**2
if np.all(np.isreal(x)):
K = K - 3
else:
K = K - 2
if opt == 'kurt1':
if np.all(x == 0):
K = 0
E = 0
return K
x = x - np.mean(x)
E = np.mean(np.abs(x))
if E < eps:
K = 0
return K
K = np.mean(np.abs(x)**2)/E**2
if np.all(np.isreal(x)):
K = K-1.57
else:
K = K-1.27
return K
开发者ID:amaggi,项目名称:waveloc,代码行数:52,代码来源:kurtogram.py
示例18: radialUndistort
def radialUndistort(rpp, k, quot=False, der=False):
'''
takes distorted radius and returns the radius undistorted
optionally it returns the distortion quotioent rpp = rp * q
'''
# polynomial coeffs, grade 7
# # (k1,k2,p1,p2[,k3[,k4,k5,k6[,s1,s2,s3,s4[,τx,τy]]]])
# polynomial coeffs, grade 7
# # (k1,k2,p1,p2[,k3[,k4,k5,k6[,s1,s2,s3,s4[,τx,τy]]]])
k.shape = -1
poly = [[k[3], 0, k[2], 0, k[1], 0, k[0], 0, 1, -r] for r in rpp]
# calculate roots
rootsPoly = array([roots(p) for p in poly])
# return flag, True if there is a suitable (real AND positive) solution
rPRB = isreal(rootsPoly) & (0 <= real(rootsPoly)) # real Positive Real Bool
retVal = any(rPRB, axis=1)
thetap = empty_like(rpp)
if any(~retVal): # if at least one case of non solution
# calculate extrema of polyniomial
thExtrema = roots([9*k[3], 0, 7*k[2], 0, 5*k[1], 0, 3*k[0], 0, 1])
# select real extrema in positive side, keep smallest
thRealPos = min(thExtrema.real[isreal(thExtrema) & (0<=thExtrema.real)])
# assign to problematic values
thetap[~retVal] = thRealPos
# choose minimum positive roots
thetap[retVal] = [min(rootsPoly[i, rPRB[i]].real)
for i in arange(rpp.shape[0])[retVal]]
rp = abs(tan(thetap)) # correct negative values
# if theta angle is greater than pi/2, retVal=False
retVal[thetap >= pi/2] = False
if der:
# derivada de la directa
q, dQdP, dQdK = radialDistort(rp, k, quot, der)
if quot:
return q, retVal, dQdP, dQdK
else:
return rp, retVal, dQdP, dQdK
else:
if quot:
# returns q
return rpp / rp, retVal
else:
return rp, retVal
开发者ID:sebalander,项目名称:sebaPhD,代码行数:52,代码来源:FisheyeCalibration.py
示例19: computeStationaryCovariance
def computeStationaryCovariance(self, ls):
'''Compute the asymptotic covariance for a given linear system.
(Eq. 104-106)
'''
A, H, G, Q, M, R = map(np.mat, [ls.getA(), ls.getH(), ls.getG(),
ls.getQ(), ls.getM(), ls.getR()])
try:
Pprd = np.mat(dare(A.T, H.T, G * Q * G.T, M * R * M.T))
except:
raise AssertionError("Dare Unsolvable: "
+ "The given system state is not stable/observable.")
assert np.all(np.isreal(Pprd)) and np.all(Pprd == Pprd.T)
Pest = Pprd - (Pprd * H.T) * (H * Pprd * H.T + M * R * M.T).I * (Pprd * H.T).T
assert np.all(np.isreal(Pest)) and np.all(Pest == Pest.T)
return Pest
开发者ID:wasserfeder,项目名称:gdtl-firm,代码行数:15,代码来源:filter.py
示例20: multiply
def multiply(self,x,mode):
op1 = self.children[0]
if np.isreal(x).all():
# Purely real
y = np.real(op1.applyMultiply(x,mode))
elif np.isreal(1j*x).all():
# Purely imaginary
y = np.real(op1.applyMultiply(np.imag(x),mode)) * 1j
else:
# Mixed
y = np.real(op1.applyMultiply(np.real(x),mode)) + np.real(op1.applyMultiply(np.imag(x),mode)) * 1j
return y
开发者ID:mingwy,项目名称:spotboxpy,代码行数:13,代码来源:opReal.py
注:本文中的numpy.isreal函数示例由纯净天空整理自Github/MSDocs等源码及文档管理平台,相关代码片段筛选自各路编程大神贡献的开源项目,源码版权归原作者所有,传播和使用请参考对应项目的License;未经允许,请勿转载。 |
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