def buildSection(self, xo = None, yo = None, xm = None, ym = None,
pts = 100, gfilter = 5):
"""
Extract a slice from the 3D data set and compute the stratigraphic layers.
Parameters
----------
variable: xo, yo
Lower X,Y coordinates of the cross-section.
variable: xm, ym
Upper X,Y coordinates of the cross-section.
variable: pts
Number of points to discretise the cross-section.
variable: gfilter
Gaussian smoothing filter.
"""
if xm > self.x.max():
xm = self.x.max()
if ym > self.y.max():
ym = self.y.max()
if xo < self.x.min():
xo = self.x.min()
if yo < self.y.min():
yo = self.y.min()
xsec, ysec = self._cross_section(xo, yo, xm, ym, pts)
self.dist = np.sqrt(( xsec - xo )**2 + ( ysec - yo )**2)
self.xsec = xsec
self.ysec = ysec
for k in range(self.nz):
# Thick
rect_B_spline = RectBivariateSpline(self.yi, self.xi, self.th[:,:,k])
data = rect_B_spline.ev(ysec, xsec)
secTh = filters.gaussian_filter1d(data,sigma=gfilter)
secTh[secTh < 0] = 0
self.secTh.append(secTh)
# Elev
rect_B_spline1 = RectBivariateSpline(self.yi, self.xi, self.elev[:,:,k])
data1 = rect_B_spline1.ev(ysec, xsec)
secElev = filters.gaussian_filter1d(data1,sigma=gfilter)
self.secElev.append(secElev)
# Depth
rect_B_spline2 = RectBivariateSpline(self.yi, self.xi, self.dep[:,:,k])
data2 = rect_B_spline2.ev(ysec, xsec)
secDep = filters.gaussian_filter1d(data2,sigma=gfilter)
self.secDep.append(secDep)
# Ensure the spline interpolation does not create underlying layers above upper ones
topsec = self.secDep[self.nz-1]
for k in range(self.nz-2,-1,-1):
secDep = self.secDep[k]
self.secDep[k] = np.minimum(secDep, topsec)
topsec = self.secDep[k]
return
def __init__(self, periods):
"""
Create an instance of LB13.
Args:
periods (numpy.array): An array of periods that will be requested
from the function. Values must be [0.01 -> 10.0], and must me
sorted from smallest to largest.
Returns:
An instance of :class:`LothBaker2013`.
"""
if np.any(periods < 0.01):
raise ValueError('The periods must be greater or equal to 0.01s')
if np.any(periods > 10):
raise ValueError('The periods must be less or equal to 10s')
rbs1 = RectBivariateSpline(Tlist, Tlist, B1, kx=1, ky=1)
rbs2 = RectBivariateSpline(Tlist, Tlist, B2, kx=1, ky=1)
rbs3 = RectBivariateSpline(Tlist, Tlist, B3, kx=1, ky=1)
#
# Build new tables with entries at the periods we will use
#
tlist = list(zip(*it.product(periods, periods)))
nper = np.size(periods)
self.b1 = rbs1.ev(tlist[0], tlist[1]).reshape((nper, nper))
self.b2 = rbs2.ev(tlist[0], tlist[1]).reshape((nper, nper))
self.b3 = rbs3.ev(tlist[0], tlist[1]).reshape((nper, nper))
def main():
filenameEffArea='aeff_P7REP_ULTRACLEAN_V15_back.fits'
directoryEffectiveArea='/Users/dspolyar/Documents/IRF/EffectiveArea/'
print pyfits.info( directoryEffectiveArea+filenameEffArea)
CTHETA_LO, CTHETA_HI, energyLow, energyHigh, EFFAREA = importEffectiveArea(directoryEffectiveArea+filenameEffArea)
energylog, Ctheta=centeringDataAndConvertingToLog(energyHigh,energyLow,CTHETA_HI,CTHETA_LO)
SplineEffectiveArea=RectBivariateSpline(Ctheta,energylog,EFFAREA)
plotofEffectiveArea(SplineEffectiveArea,EFFAREA,energylog,Ctheta)
print SplineEffectiveArea.ev(1.,5.)
def LucasKanadeAffine(It, It1):
# Input:
# It: template image
# It1: Current image
# Output:
# M: the Affine warp matrix [2x3 numpy array]
# put your implementation here
M = np.array([[1.0, 0.0, 0.0], [0.0, 1.0, 0.0]])
p = M.flatten()
x1, y1, x2, y2 = 0, 0, It.shape[1] - 1, It.shape[0] - 1
threshold = 1e-3
dp = np.array([float("inf")] * 6)
interpolated_It1 = RectBivariateSpline(
x=np.array([i for i in range(int(It1.shape[0]))]),
y=np.array([i for i in range(int(It1.shape[1]))]),
z=It1)
while np.sum(np.square(dp)) >= threshold:
x = np.arange(x1, x2 + .5)
y = np.arange(y1, y2 + .5)
X = np.array([x for i in range(len(y))])
Y = np.array([y for i in range(len(x))]).T
warp_X = p[0] * X + p[1] * Y + p[2]
warp_Y = p[3] * X + p[4] * Y + p[5]
valid_points = (warp_X >= x1) & (warp_X <= x2) & (warp_Y >=
y1) & (warp_Y <= y2)
X, Y = X[valid_points], Y[valid_points]
warp_X, warp_Y = warp_X[valid_points], warp_Y[valid_points]
warp_It1x = interpolated_It1.ev(warp_Y, warp_X)
dx = interpolated_It1.ev(warp_Y, warp_X, dx=0, dy=1).flatten()
dy = interpolated_It1.ev(warp_Y, warp_X, dx=1, dy=0).flatten()
A = np.array([
dx * X.flatten(),
dx * Y.flatten(),
dx,
dy * X.flatten(),
dy * Y.flatten(),
dy,
]).T
b = (It[valid_points] - warp_It1x).flatten()
dp = np.dot(np.linalg.inv(np.dot(A.T, A)), np.dot(A.T, b))
p += dp.flatten()
M = np.copy(p).reshape(2, 3)
M = np.vstack((M, np.array([[0, 0, 1]])))
return M
def LucasKanade(It, It1, rect, threshold, num_iters, p0=np.zeros(2)):
"""
:param It: template image
:param It1: Current image
:param rect: Current position of the car (top left, bot right coordinates)
:param threshold: if the length of dp is smaller than the threshold, terminate the optimization
:param num_iters: number of iterations of the optimization
:param p0: Initial movement vector [dp_x0, dp_y0]
:return: p: movement vector [dp_x, dp_y]
"""
# Put your implementation here
p = p0
x1, y1, x2, y2 = rect[0], rect[1], rect[2], rect[3]
It_spline = RectBivariateSpline(np.arange(It.shape[0]),
np.arange(It.shape[1]), It)
It1_spline = RectBivariateSpline(np.arange(It1.shape[0]),
np.arange(It1.shape[1]), It1)
dp = np.array([float("inf"), float("inf")])
count = 0
x = np.arange(x1, x2 + 1)
y = np.arange(y1, y2 + 1)
x, y = np.meshgrid(x, y)
while np.linalg.norm(dp) >= threshold and count <= num_iters:
count += 1
Itx = It_spline.ev(y, x).flatten()
It1x_warp = It1_spline.ev(y + p[1], x + p[0]).flatten()
A = np.array([
It1_spline.ev(y + p[1], x + p[0], dx=0, dy=1).flatten(),
It1_spline.ev(y + p[1], x + p[0], dx=1, dy=0).flatten()
]).T
# print(np.shape(A))
b = (Itx - It1x_warp).flatten()
# print(np.shape(b))
dp = (np.linalg.inv(A.T @ A)) @ (A.T @ b)
p += dp
return p
def getEroDep(self,
xo=None,
yo=None,
xm=None,
ym=None,
pts=100,
gfilter=5):
"""
Extract a slice from the 3D data set and compute its deposition thicknesses.
Parameters
----------
variable: xo, yo
Lower X,Y coordinates of the cross-section
variable: xm, ym
Upper X,Y coordinates of the cross-section
variable: pts
Number of points to discretise the cross-section
variable: gfilter
Gaussian smoothing filter
"""
if xm > self.x.max():
xm = self.x.max()
if ym > self.y.max():
ym = self.y.max()
if xo < self.x.min():
xo = self.x.min()
if yo < self.y.min():
yo = self.y.min()
xsec, ysec = self._cross_section(xo, yo, xm, ym, pts)
self.dist = np.sqrt((xsec - xo)**2 + (ysec - yo)**2)
# Surface
rect_B_spline = RectBivariateSpline(self.y[:, 0], self.x[0, :], self.z)
datatop = rect_B_spline.ev(ysec, xsec)
self.top = filters.gaussian_filter1d(datatop, sigma=gfilter)
# Cumchange
rect_B_spline = RectBivariateSpline(self.y[:, 0], self.x[0, :],
self.cumchange)
cumdat = rect_B_spline.ev(ysec, xsec)
gcum = filters.gaussian_filter1d(cumdat, sigma=gfilter)
self.depo = gcum.clip(min=0)
return
class GridSag(ExplicitShape):
"""
Class for gridsag
"""
def __init__(self, lc, xxx_todo_changeme, name="", *args, **kwargs):
(xlinspace, ylinspace, Zgrid) = xxx_todo_changeme
kwargs_dict = kwargs
name = kwargs_dict.pop('name', '')
self.interpolant = RectBivariateSpline(xlinspace, ylinspace, Zgrid)
#self.interpolant = interp2d(xlinspace, ylinspace, Zgrid, kind=kind, *args, **kwargs_dict)
def gsf(x, y):
res = self.interpolant.ev(x, y)
return res
def gradgsf(x, y,
z): # gradient for implicit function z - af(x, y) = 0
res = np.zeros((3, len(x)))
res[0, :] = -self.interpolant.ev(x, y, dx=1)
res[1, :] = -self.interpolant.ev(x, y, dy=1)
res[2, :] = 1.
return res
def hessgsf(x, y, z):
res = np.zeros((3, 3, len(x)))
res[0, 0, :] = -self.interpolant.ev(x, y, dx=2)
res[0, 1, :] = res[1,
0, :] = -self.interpolant.ev(x, y, dx=1, dy=1)
res[1, 1, :] = -self.interpolant.ev(x, y, dy=2)
return res
super(GridSag, self).__init__(lc,
gsf,
gradgsf,
hessgsf,
eps=1e-4,
iterations=10,
name=name)
def setKind(self):
self.kind = "shape_GridSag"
def SubtractDominantMotion(image1, image2):
# Input:
# Images at time t and t+1
# Output:
# mask: [nxm]
# put your implementation here
mask = np.zeros(image1.shape, dtype=bool)
# M = LucasKanadeAffine.LucasKanadeAffine(image1, image2)
# use efficient method
M = InverseCompositionAffine.InverseCompositionAffine(image1, image2)
if M.shape[0] < 3:
M = np.vstack((M, np.array([[0, 0, 1]])))
M = np.linalg.inv(M)
interp_spline_image1 = RectBivariateSpline(np.arange(image1.shape[0]),
np.arange(image1.shape[1]),
image1)
interp_spline_image2 = RectBivariateSpline(np.arange(image2.shape[0]),
np.arange(image2.shape[1]),
image2)
# project coordinates to interpolate the values
x = np.arange(0, image2.shape[1])
y = np.arange(0, image2.shape[0])
X, Y = np.meshgrid(x, y)
X_ = M[0, 0] * X + M[0, 1] * Y + M[0, 2]
Y_ = M[1, 0] * X + M[1, 1] * Y + M[1, 2]
# get the invalid positions that are not common ares in two images
invalid = (X_ < 0) | (X_ >=
image1.shape[1]) | (Y_ < 0) & (Y_ >= image1.shape[0])
interped_I1 = interp_spline_image1.ev(Y_, X_)
interped_I2 = interp_spline_image2.ev(Y, X)
interped_I1[invalid] = 0
interped_I2[invalid] = 0
# calculate the difference
diff = abs(interped_I2 - interped_I1)
th = 0.1
ind = (diff > th) & (interped_I2 != 0)
mask[ind] = 1
ker = np.array(([0, 0, 1, 0, 0], [0, 1, 1, 1,
0], [1, 1, 1, 1,
1], [0, 1, 1, 1,
0], [0, 0, 1, 0, 0]))
mask = mp.binary_dilation(mask, structure=ker).astype(mask.dtype)
return mask
def InverseCompositionAffine(It, It1, threshold, num_iters):
"""
:param It: template image
:param It1: Current image
:param threshold: if the length of dp is smaller than the threshold, terminate the optimization
:param num_iters: number of iterations of the optimization
:return: M: the Affine warp matrix [2x3 numpy array]
"""
# put your implementation here
p = np.zeros(6)
M = np.array([[1.0 + p[0], p[1], p[2]], [p[3], 1.0 + p[4], p[5]]])
template_height, template_width = It.shape[0], It.shape[1]
image_height, image_width = It1.shape[0], It1.shape[1]
x_range = np.arange(0, template_width, 1)
y_range = np.arange(0, template_height, 1)
# get rectangular splines
interpolated_template_spline = RectBivariateSpline(y_range, x_range, It)
interpolated_current_image_spline = RectBivariateSpline(np.arange(0, image_height, 1),
np.arange(0, image_width, 1), It1)
# get template grid
xv, yv = np.meshgrid(x_range, y_range)
xv, yv = xv.reshape(1, -1), yv.reshape(1, -1)
template = np.vstack((xv, yv, np.ones((1, template_height * template_width))))
grad_x = interpolated_current_image_spline.ev(yv, xv, dy=1).flatten()
grad_y = interpolated_current_image_spline.ev(yv, xv, dx=1).flatten()
jacobian_gd = np.vstack((xv * grad_x,
yv * grad_x,
grad_x,
xv * grad_y,
yv * grad_y,
grad_y))
h = np.linalg.pinv(jacobian_gd)
for i in range(num_iters):
warped_image = np.dot(M, template)
interpolated_template = interpolated_template_spline.ev(yv, xv).flatten()
interpolated_current_image = interpolated_current_image_spline.ev(warped_image[1, :],
warped_image[0, :]).flatten()
difference = interpolated_template - interpolated_current_image
dp = np.dot(h.T, difference)
p += dp
M = np.array([[1.0 + p[0], p[1], p[2]], [p[3], 1.0 + p[4], p[5]]])
if np.linalg.norm(dp) <= threshold:
break
return M
def setModel(self,model,dx,think_positive=False):
'''
Set new model for the source.
:param model: ``(n, n)``
Numpy image array.
:param dx: scalar
Pixel size in microarcseconds.
:param think_positive: (optional) bool
Should we enforce that the source image has no negative pixel values?
'''
self.nx = int(ceil(model.shape[-1] * dx / self.dx)) # number of image pixels
self.model = model # source model
self.model_dx = dx # source model resolution
# load source image that has size and resolution compatible with the screen.
self.isrc = np.empty(2*(self.nx,))
self.think_positive = think_positive
M = self.model.shape[1] # size of original image array
f_img = RectBivariateSpline(self.model_dx/self.dx*(np.arange(M) - 0.5*(M-1)),\
self.model_dx/self.dx*(np.arange(M) - 0.5*(M-1)),\
self.model)
xx_,yy_ = np.meshgrid((np.arange(self.nx) - 0.5*(self.nx-1)),\
(np.arange(self.nx) - 0.5*(self.nx-1)),indexing='xy')
m = f_img.ev(yy_.flatten(),xx_.flatten()).reshape(2*(self.nx,))
self.isrc = m * (self.dx/self.model_dx)**2 # rescale for change in pixel size
if self.think_positive:
self.isrc[self.isrc < 0] = 0
if not self.live_dangerously: self._checkSanity()
def transform(self, sourceImage, destinationImage):
# - Verify that both input arguments are numpy arrays,
if not isinstance(sourceImage, np.ndarray) or not isinstance(
destinationImage, np.ndarray):
raise TypeError('One or more images not np arrays')
# - affine transformation from the triangle in the source image to its corresponding triangle
# 1st step: create mask
length, width = destinationImage.shape
img = Image.new('L', (width, length), 0)
vertices = [(x, y) for [x, y] in self.destination]
ImageDraw.Draw(img).polygon(vertices, outline=255, fill=255)
mask = np.array(img)
# 2nd step: create H inverse and get bivariate spline approximation
H_inv = np.linalg.inv(self.matrix)
x = np.arange(length)
y = np.arange(width)
approx = RectBivariateSpline(x, y, sourceImage, kx=1, ky=1)
#get each point in mask whose value is greater than 0
for yp, xp in np.transpose(np.nonzero(mask)):
#H^-1 * [x' y' 1] = [x y 1]
P = H_inv.dot([xp, yp, 1])[0:2]
#2d interpolation to obtain a value if x y are floats
shade = np.round(approx.ev(P[1], P[0]))
#assign that value to x' y'
destinationImage[yp][xp] = shade
def calcAnker(IS, inputPoints, rasterdata, gp):
"""
"""
dhm = rasterdata['subraster']
[Xa, Ya, Xe, Ye] = inputPoints
# Letzte Koordinate in xi/yi entspricht nicht exakt den Endkoordinaten
Xe_ = gp['xi'][-1]
Ye_ = gp['yi'][-1]
AnkA_dist = IS['d_Anker_A'][0]
AnkE_dist = IS['d_Anker_E'][0]
stueA_H = IS['HM_Anfang'][0]
stueE_H = IS['HM_Ende_max'][0]
# X- und Y-Koordinate der Geodaten im Projektionssystem berechnen
dx = float(Xe - Xa)
dy = float(Ye - Ya)
if dx == 0:
dx = 0.0001
azimut = math.atan(dy/dx)
if dx > 0:
azimut += 2 * math.pi
else:
azimut += math.pi
# X- und Y-Koordinaten der beiden Ankerpunkte am Boden
AnkXa = Xa - AnkA_dist * math.cos(azimut)
AnkYa = Ya - AnkA_dist * math.sin(azimut)
AnkXe = Xe_ + AnkE_dist * math.cos(azimut)
AnkYe = Ye_ + AnkE_dist * math.sin(azimut)
# Linear Interpolation
# Koordinatenarrays des DHMs
coordX = gp['linspaces'][0]
coordY = gp['linspaces'][1]
# kx, ky bezeichnen grad der interpolation, 1=linear
spline = RectBivariateSpline(-coordY, coordX, dhm, kx=1, ky=1)
xi = np.array([AnkXa, Xa, Xe_, AnkXe])
yi = np.array([AnkYa, Ya, Ye_, AnkYe])
# Z-Koordinate der Anker für Anfangs- und Endpunkte
zAnker = spline.ev(-yi, xi) # Höhenangaben am Boden
AnkA_z = stueA_H + 0.1*(zAnker[1] - zAnker[0])
AnkE_z = stueE_H + 0.1*(zAnker[2] - zAnker[3])
if AnkA_dist == 0:
AnkA_z = 0.0
if AnkE_dist == 0:
AnkE_z = 0.0
Ank = [AnkA_dist, AnkA_z, AnkE_dist, AnkE_z]
# Ausdehnungen der Anker Felder, alles in [m]
#Ank = [d_Anker_A, z_Anker_A * 0.1, d_Anker_E, z_Anker_E * 0.1]
Laenge_Ankerseil = (AnkA_dist**2 + AnkA_z**2)**0.5 + \
(AnkE_dist**2 + AnkE_z**2)**0.5
# Eventuell nicht nötig
#IS['z_Anker_A'][0] = z_Anker_A
#IS['z_Anker_E'][0] = z_Anker_E
return [Ank, Laenge_Ankerseil, zAnker]
def skybg_phot(x0, y0, data, r=25, dr=5, samp=3, debug=False):
# determine img indexes for aperture region
xv, yv = mesh_box([x0, y0], (r + dr) + 2)
# derive indexs on a higher resolution grid and create aperture mask
px, py, mask = sky_annulus(x0, y0, r=r, samp=xv.shape[0] * samp)
# interpolate original data onto higher resolution grid
subdata = data[yv, xv]
model = RectBivariateSpline(np.unique(xv), np.unique(yv), subdata)
# evaluate data on highres grid
pz = model.ev(px, py)
# zero out pixels larger than radius
pz[~mask] = 0
pz[pz < 0] = 0
# scale area back to original grid, total flux in sky annulus
parea = pz.sum() * np.diff(px).mean() * np.diff(py[:, 0]).mean()
if debug:
print('mask area=',
mask.sum() * np.diff(px).mean() * np.diff(py[:, 0]).mean())
print('true area=', 2 * np.pi * r * dr)
print('subdata flux=', subdata.sum())
print('bg phot flux=', parea)
import pdb
pdb.set_trace()
# return bg value per pixel
return pz.sum() / mask.sum()
def plot(self, ax, V=None, **kwargs):
'''Plot the contours into matplotlib axis.
Parameters
----------
ax : matplotlib.Axes
Axes to plot into
V : array-like
A list of contour values to plot. If not None, the internal contour
values will be overriden during plotting, but not inside the
object.
kwargs : dict
Keyword arguments to pass on to the ax.contour() method.
'''
if V is None:
V = self.V
d, X, Y = self.data.getData()
# hack - add zero value to close contours
d = np.hstack((d, np.zeros((d.shape[0], 1))))
d = np.vstack((d, np.zeros((1, d.shape[1]))))
dx = X[0, 1] - X[0, 0]
dy = Y[1, 0] - Y[0, 0]
x_longer = X[0, :].tolist()
x_longer.append(X[0, -1] + dx)
y_longer = Y[:, 0].tolist()
y_longer.append(Y[-1, 0] + dy)
x_interp, y_interp = np.meshgrid(
np.linspace(x_longer[0], x_longer[-1],
len(x_longer) * self.upsample_factor),
np.linspace(x_longer[0], y_longer[-1],
len(y_longer) * self.upsample_factor))
spl = RectBivariateSpline(x_longer, y_longer, d.T)
d_interp = spl.ev(x_interp, y_interp)
ax.contour(x_interp, y_interp, d_interp, V, **kwargs)
def interpolate_individual(self, image):
# unpacking
ogridx, ogridy = self.ogrid
ngridx, ngridy = self.ngrid
f = RectBivariateSpline(ogridy, ogridx, image, kx=1, ky=1)
return f.ev(ngridy.flatten(), ngridx.flatten()).reshape(ngridx.shape)
def _mesh_interpolate_worker(args):
coords, raster, crs, chunk_size = args
raster = Raster(raster)
raster.warp(crs)
results = []
for window in raster.iter_windows(chunk_size=chunk_size, overlap=2):
xi = raster.get_x(window)
yi = raster.get_y(window)
zi = raster.get_values(window=window)
f = RectBivariateSpline(
xi,
np.flip(yi),
np.fliplr(zi).T,
bbox=[np.min(xi), np.max(xi),
np.min(yi), np.max(yi)],
kx=3,
ky=3,
s=0)
idxs = np.where(
np.logical_and(
np.logical_and(
np.min(xi) < coords[:, 0],
np.max(xi) > coords[:, 0]),
np.logical_and(
np.min(yi) < coords[:, 1],
np.max(yi) > coords[:, 1])))[0]
values = f.ev(coords[idxs, 0], coords[idxs, 1])
results.append((idxs, values))
return results
def _get_above_cloud_r_and_dr(self,
P_profile,
T_profile,
abundances,
planet_mass,
planet_radius,
star_radius,
above_cloud_cond,
T_star=None):
assert (len(P_profile) == len(T_profile))
# First, get atmospheric weight profile
mu_profile = np.zeros(len(P_profile))
for species_name in abundances:
interpolator = RectBivariateSpline(self.P_grid,
self.T_grid,
abundances[species_name],
kx=1,
ky=1)
atm_abundances = interpolator.ev(P_profile, T_profile)
mu_profile += atm_abundances * self.mass_data[species_name]
return _hydrostatic_solver._solve(P_profile, T_profile,
self.ref_pressure, mu_profile,
planet_mass, planet_radius,
star_radius, above_cloud_cond,
T_star)
def regrid_imagery(image,
x_image,
y_image,
x_regrid,
y_regrid,
image_proj,
regrid_proj,
spline_kws=None):
"""
For a given image, regrid it to another projection using spline interpolation.
Args:
image:
x_image:
y_image:
x_regrid:
y_regrid:
image_proj:
regrid_proj:
spline_kws:
Returns:
"""
if spline_kws is None:
spline_kws = dict()
x_regrid_image, y_regrid_image = transform(image_proj, regrid_proj,
x_regrid.ravel(),
y_regrid.ravel())
rbs = RectBivariateSpline(x_image, y_image, image, **spline_kws)
regridded_image = rbs.ev(x_regrid_image,
y_regrid_image).reshape(x_regrid.shape)
return regridded_image
def get_pixels(self, DU, DV, image):
"""Return pixel values for each xyz point from the image
Arguments:
DU (np.ndarray): Pixel location in camera orientation and coordinate system
DV (np.ndarray): Pixel location in cmaera orientation and coorindate system
Returns:
K (np.ndarray): Pixel intensity for each point in the image
"""
K = np.zeros((self.target_grid.X.shape[0], self.target_grid.X.shape[1],
self.ncolors))
for c, _ in enumerate(['r', 'b', 'g']):
rbs = RectBivariateSpline(
# use this range to match matlab exactly
np.arange(1, image.shape[0] + 1),
np.arange(1, image.shape[1] + 1),
image[:, :, c],
kx=1,
ky=1)
K[:, :, c] = rbs.ev(DV, DU)
# mask out values out of range like matlab
# avoid runtime nan comparison warning (UV, DV already have nans)
with np.errstate(invalid='ignore'):
mask_u = np.logical_or(DU <= 1, DU >= image.shape[1])
mask_v = np.logical_or(DV <= 1, DV >= image.shape[0])
mask = np.logical_or(mask_u, mask_v)
K[mask] = np.nan
return K
def get_elevations(subpaths, ufnames, flagsmissing):
interpvalues = np.empty(0, dtype=int)
for i in range(len(subpaths)):
# open srtmdata filename according to subpath
path = Path.joinpath(hgtpath, ufnames[i])
if not flagsmissing[i]:
with open(path, 'rb') as data:
# data is stored in srtmdata files in big-endian format:
# SRTM1 (1-arc sampling) is used, so each file contains 3601x3601 individual elevations
# after reading all elevatin ins file, we reshape it into a rectangular numpy array
elevationdata = np.fromfile(data, np.dtype('>i2'),
3601**2).reshape(3601, 3601)
# interpolate elevation values with scipy.interpolate.griddata
f1 = RectBivariateSpline(x, x, elevationdata, kx=1, ky=1)
latcorr = int(ufnames[i][1:3]) + 1
loncorr = int(ufnames[i][4:7])
interpvalues = np.hstack((interpvalues,
f1.ev(latcorr - subpaths[i][0],
subpaths[i][1] - loncorr)))
else:
interpvalues = np.hstack(
(interpvalues, np.zeros_like(subpaths[i][0])))
return interpvalues
def put_psf_on_subarray(psf, y, frame_height=256):
"""Make a 2D SOSS trace from a sequence of psfs and trace center locations
Parameters
----------
psf: sequence
The 2D psf
y: float
The grid y value to place the center of the psf
grid: sequence
The [x, y] grid ranges
Returns
-------
np.ndarray
The 2D frame with the interpolated psf
"""
# Create spline generator
dim = psf.shape[0]
mid = (dim - 1.0) / 2.0
arr = np.arange(dim, dtype=np.float)
spline = RectBivariateSpline(arr, arr, psf.T, kx=3, ky=3, s=0)
# Create output frame, shifted as necessary
yg, xg = np.indices((frame_height, dim), dtype=np.float64)
yg += mid - y
# Resample onto the subarray
frame = spline.ev(xg, yg)
# Fill resampled points with zeros
extrapol = (((xg < -0.5) | (xg >= dim - 0.5)) | ((yg < -0.5) | (yg >= dim - 0.5)))
frame[extrapol] = 0
return frame
def Transformation(self, originalImage, targetImage, Target,
original): # this is image
# print(targetimage)
# print(xp,yp)
#NbyTwo[:, [0, 1]] = NbyTwo[:, [1, 0]]
NbyTwo = Target.getPoints()
#getCoord = np.vectorize(lambda x, y, a: self.inverseMatrix[a, 0] * y + self.inverseMatrix[a, 1] * x + self.inverseMatrix[a, 2], otypes=[np.float64])
#NbyTwo[:, [1, 0]] = NbyTwo[:, [0, 1]]
xp, yp = np.transpose(
NbyTwo
) ## this will return the points reside in one triangle, in morpher
x = self.calcXPoints(xp, yp)
y = self.calcYPoints(xp, yp)
# xdim = np.array([a for a in range(int(min(original.vertices[:, 1])), int(max(original.vertices[:, 1])))])
# # print(len(xdim))
# ydim = np.array([a for a in range(int(min(original.vertices[:, 0])), int(max(original.vertices[:, 0])))])
#
# xyVal = originalImage[xdim[0]:xdim[len(xdim) - 1]+1, ydim[0]:ydim[len(ydim) - 1]+1]
xdim = np.arange(np.amin(original.vertices[:, 1]),
np.amax(original.vertices[:, 1]), 1)
ydim = np.arange(np.amin(original.vertices[:, 0]),
np.amax(original.vertices[:, 0]), 1)
xyVal = originalImage[int(xdim[0]):int(xdim[-1] + 1),
int(ydim[0]):int(ydim[-1] + 1)]
bilinear = RectBivariateSpline(xdim, ydim, xyVal, kx=1, ky=1)
targetImage[xp, yp] = bilinear.ev(x, y)
def _get_above_cloud_profiles(self, P_profile, T_profile, abundances,
planet_mass, planet_radius, star_radius,
above_cloud_cond, T_star=None):
assert(len(P_profile) == len(T_profile))
# First, get atmospheric weight profile
mu_profile = np.zeros(len(P_profile))
atm_abundances = {}
for species_name in abundances:
interpolator = RectBivariateSpline(
np.log10(self.P_grid), self.T_grid,
np.log10(abundances[species_name]), kx=1, ky=1)
abund = 10**interpolator.ev(np.log10(P_profile), T_profile)
atm_abundances[species_name] = abund
mu_profile += abund * self.mass_data[species_name]
radii, dr = _hydrostatic_solver._solve(
P_profile, T_profile, self.ref_pressure, mu_profile, planet_mass,
planet_radius, star_radius, above_cloud_cond, T_star)
for key in atm_abundances:
atm_abundances[key] = atm_abundances[key][above_cloud_cond]
return radii, dr, atm_abundances, mu_profile
def get_subpixel(res):
mgx, mgy = np.meshgrid(np.arange(-1, 1.01, 0.1),
np.arange(-1, 1.01, 0.1),
indexing='xy') # sub-pixel mesh
minval, _, minloc, _ = cv2.minMaxLoc(res)
rbs_halfsize = 3 # size of peak area used for spline for subpixel peak loc
rbs_order = 4 # polynomial order for subpixel rbs interpolation of peak location
if ((np.array([n - rbs_halfsize
for n in minloc]) >= np.array([0, 0])).all()
& (np.array([(n + rbs_halfsize)
for n in minloc]) < np.array(list(res.shape))).all()):
rbs_p = RBS(
range(-rbs_halfsize, rbs_halfsize + 1),
range(-rbs_halfsize, rbs_halfsize + 1),
res[(minloc[1] - rbs_halfsize):(minloc[1] + rbs_halfsize + 1),
(minloc[0] - rbs_halfsize):(minloc[0] + rbs_halfsize + 1)],
kx=rbs_order,
ky=rbs_order)
b = rbs_p.ev(mgx.flatten(), mgy.flatten())
mml = cv2.minMaxLoc(b.reshape(21, 21))
# mgx,mgy: meshgrid x,y of common area
# sp_delx,sp_dely: subpixel delx,dely
sp_delx = mgx[mml[3][0], mml[3][1]]
sp_dely = mgy[mml[3][0], mml[3][1]]
else:
sp_delx = 0.0
sp_dely = 0.0
return sp_delx, sp_dely
def imresize2D(im0, h0, dim):
h0 = h0[0:2]
dim = dim[0:2]
# Image size
dim0 = im0.shape
# Create a regular grid
x0, y0, x0lin, y0lin = gengrid.centered2D(dim0, h0)
# Require the same FOV
fov0 = dim0 * h0
# New voxelsize
h = fov0 / dim
# Create a regular grid where we want the new values
x, y, xlin, ylin = gengrid.centered2D(dim, h)
# Interpolation
f = RectBivariateSpline(x0lin, y0lin, im0)
x = x.flatten()
y = y.flatten()
# Must revert the order of x and y, otherwise its rotated
im = f.ev(y, x).reshape(dim[0], dim[1])
return im
def _p(self, K, c):
if self.params['use_interp']:
data_path = os.path.join(os.path.dirname(__file__), 'data')
data = np.load(os.path.join(data_path, "uKc_einasto.npz"))
pk = data['pk']
_k = data['K']
_c = data['c']
c = np.atleast_1d(c)
if np.isscalar(K):
K = np.atleast_2d(K)
if K.ndim < 2:
if len(K) != len(c):
K = np.atleast_2d(K).T # should be len(rs) x len(k)
else:
K = np.atleast_2d(K)
pk[pk <= 0] = 1e-8
spl = RectBivariateSpline(np.log(_k), np.log(_c), np.log(pk))
cc = np.repeat(c, K.shape[0])
return np.exp(
self._reduce(
spl.ev(np.log(K.flatten()), np.log(cc)).reshape(K.shape)))
else: #Numerical version.
return super(Einasto, self)._p(K, c)
def test_spline_2d_outofbounds(self):
x = np.array([.5, 2., 3., 4., 5.5])
y = np.array([.5, 2., 3., 4., 5.5])
z = np.array([[1, 2, 1, 2, 1], [1, 2, 1, 2, 1], [1, 2, 3, 2, 1],
[1, 2, 2, 2, 1], [1, 2, 1, 2, 1]])
lut = RectBivariateSpline(x, y, z)
xi = np.array([[1, 2.3, 6.3, 0.5, 3.3, 1.2, 3],
[1, 3.3, 1.2, -4.0, 5.0, 1.0, 3]]).T
actual = interpn((x, y),
z,
xi,
method="splinef2d",
bounds_error=False,
fill_value=999.99)
expected = lut.ev(xi[:, 0], xi[:, 1])
expected[2:4] = 999.99
assert_array_almost_equal(actual, expected)
# no extrapolation for splinef2d
assert_raises(ValueError,
interpn, (x, y),
z,
xi,
method="splinef2d",
bounds_error=False,
fill_value=None)
def correlate(image,
pattern,
include_direct_beam=False,
sim_threshold=1e-5,
interpolate=False,
**kwargs):
"""The correlation between a diffraction pattern and a simulation.
Calculated using
.. math::
\frac{\sum_{j=1}^m P(x_j, y_j) T(x_j, y_j)}{\sqrt{\sum_{j=1}^m P^2(x_j, y_j)} \sqrt{\sum_{j=1}^m T^2(x_j, y_j)}}
Parameters
----------
image : :class:`np.ndarray`
A single electron diffraction signal. Should be appropriately scaled
and centered.
pattern : :class:`DiffractionSimulation`
The pattern to compare to.
sim_threshold : float
The threshold simulation intensity to consider for correlation
interpolate : bool
If True, perform sub-pixel interpolation of the image.
**kwargs
Arguments to pass to scipy.interpolate.RectBivariateSpline
Returns
-------
float
The correlation coefficient.
References
----------
E. F. Rauch and L. Dupuy, “Rapid Diffraction Patterns identification through
template matching,” vol. 50, no. 1, pp. 87–99, 2005.
"""
shape = image.shape
half_shape = tuple(i // 2 for i in shape)
pixel_coordinates = pattern.calibrated_coordinates.astype(
int)[:, :2] + half_shape
in_bounds = np.product(
(pixel_coordinates > 0) * (pixel_coordinates < shape[0]),
axis=1).astype(bool)
pattern_intensities = pattern.intensities
large_intensities = pattern_intensities > sim_threshold
mask = np.logical_and(in_bounds, large_intensities)
if interpolate:
x = np.arange(shape[0], dtype='float') - half_shape[0]
y = np.arange(shape[1], dtype='float') - half_shape[1]
for ar, i in zip([x, y], shape):
if not i % 2:
ar += 0.5
x = x * pattern.calibration[0]
y = y * pattern.calibration[1]
ip = RectBivariateSpline(x, y, image.T, **kwargs)
image_intensities = ip.ev(pattern.coordinates[:, 0][mask],
pattern.coordinates[:, 1][mask])
else:
image_intensities = image.T[pixel_coordinates[:, 0][in_bounds],
pixel_coordinates[:, 1][in_bounds]]
pattern_intensities = pattern_intensities[mask]
return np.nan_to_num(_correlate(image_intensities, pattern_intensities))
def SubtractDominantMotion(image1, image2):
# Input:
# Images at time t and t+1
# Output:
# mask: [nxm]
# put your implementation here
M = InverseCompositionAffine(image1, image2)
tol = 0.35
h, w = image1.shape
x = np.arange(w)
y = np.arange(h)
mask = np.ones((h, w), dtype=bool)
x_temp = np.arange(0, w)
y_temp = np.arange(0, h)
xi, yi = np.meshgrid(x_temp, y_temp)
ones = np.ones(w * h)
xy1 = np.array([yi.flatten(), xi.flatten(), ones])
xy1_new = np.matmul(np.vstack((M, np.array([0, 0, 1]))), xy1)
y_new = xy1_new[0, :]
x_new = xy1_new[1, :]
image2_spline = RectBivariateSpline(y, x, image2)
temp = np.array(image2_spline.ev(y_new, x_new).tolist())
image1_new = np.reshape(temp, (h, w))
abs_diff = np.absolute(image1_new, image1)
ind = (abs_diff >= tol)
abs_diff[ind] = 1
abs_diff[~ind] = 0
mask = abs_diff
return mask
def distort(image, center, angle, lengths):
"""Takes an image and distorts the image based on an elliptical distortion
Parameters
---------------
image: array-like
The image to apply the elliptical distortion to
center: list
The center of the ellipse
angle: float
The angle of the major axis in radians
lengths: The lengths of the major and minor axis of the ellipse
Returns
------------
distorted:array-like
The elliptically distorted image
"""
img_shape = np.shape(image)
initial_y, initial_x = range(-center[1], img_shape[-2] - center[1]), range(
-center[0], img_shape[-1] - center[0])
spline = RectBivariateSpline(initial_x, initial_y, image, kx=1, ky=1)
xInd, yInd = cartesian_to_ellipse(center=center,
angle=angle,
lengths=lengths)
distorted = np.array(spline.ev(yInd, xInd))
return distorted
def interpolate_grid(self, in_lon, in_lat):
"""
Interpolates MRMS data to a different grid using cubic bivariate splines
"""
out_data = np.zeros(
(self.data.shape[0], in_lon.shape[0], in_lon.shape[1]))
for d in range(self.data.shape[0]):
print("Loading ", d, self.variable, self.start_date)
if self.data[d].max() > -999:
step = self.data[d]
step[step < 0] = 0
if self.lat[-1] < self.lat[0]:
spline = RectBivariateSpline(self.lat[::-1],
self.lon,
step[::-1],
kx=3,
ky=3)
else:
spline = RectBivariateSpline(self.lat,
self.lon,
step,
kx=3,
ky=3)
print("Evaluating", d, self.variable, self.start_date)
flat_data = spline.ev(in_lat.ravel(), in_lon.ravel())
out_data[d] = flat_data.reshape(in_lon.shape)
del spline
else:
print(d, " is missing")
out_data[d] = -9999
return out_data
def main():
basis = fits.open('basis.fits')[0].data
aperture = fits.open('aperture.fits')[0].data
name = sys.argv[1]
size = basis.shape[1]
size_ = int(sys.argv[2])
x_old_res = np.linspace(-size / 2, size / 2, size)
y_old_res = np.linspace(-size / 2, size / 2, size)
x_new_res = np.linspace(-size / 2, size / 2, size_)
y_new_res = np.linspace(-size / 2, size / 2, size_)
abscissae_lr, ordinates_lr = np.meshgrid(x_old_res, y_old_res)
abscissae_nr, ordinates_nr = np.meshgrid(x_new_res, y_new_res)
basis_new = np.zeros((basis.shape[0], size_, size_))
for i in range(basis.shape[0]):
spline_basis_functions = RectBivariateSpline(x_old_res, y_old_res,
basis[i])
basis_new[i] = spline_basis_functions.ev(ordinates_nr,
abscissae_nr) * aperture
writefits(basis_new, name)
def resample2d(i_data, i_s, i_e, i_i, o_s, o_e, o_i, kx=3, ky=3, s=0,
gauss_sig=0, median_boxcar_size=0, clip=True):
'''
Resample a square 2D input grid with extents defined by [i_s] and [i_e] with
increment [i_i] to a new 2D grid with extents defined by [o_s] and [o_e]
with increment [o_i].
Returns a 2D resampled array, with options for smoothing (gaussian and
median) and clipping.
'''
# calculate bivariate spline, G, using input grid and data
grid_pre_rebin = np.arange(i_s, i_e, i_i)
G = RectBivariateSpline(grid_pre_rebin, grid_pre_rebin, i_data, kx=kx, ky=ky)
# evaluate this spline at new points on output grid
grid_x, grid_y = np.mgrid[o_s:o_e:o_i, o_s:o_e:o_i]
data = G.ev(grid_x, grid_y)
if gauss_sig != 0:
data = gaussian_filter(data, gauss_sig)
if median_boxcar_size != 0:
data = median_filter(data, median_boxcar_size)
if clip:
input_max = np.max(i_data)
input_min = np.min(i_data)
data[np.where(data>input_max)] = input_max
data[np.where(data<input_min)] = input_min
return data
def _interpolate_array(self, target) -> np.array:
"""
Interpolates SLSTR data arrays based on cartesian information
contained within the sensor product using the RectBivariateSpline
approach.
Args:
target: the product to be interpolated
Returns:
The interpolated data
"""
sat_zn = self.product['geometry_tn'][target][:]
tx_x_var = self.product['cartesian_tx']['x_tx'][0, :]
tx_y_var = self.product['cartesian_tx']['y_tx'][:, 0]
an_x_var = self.product['cartesian_an']['x_an'][:]
an_y_var = self.product['cartesian_an']['y_an'][:]
spl = RectBivariateSpline(tx_y_var, tx_x_var[::-1],
sat_zn[:, ::-1].filled(0))
interpolated = spl.ev(an_y_var.compressed(), an_x_var.compressed())
interpolated = np.ma.masked_invalid(interpolated, copy=False)
sat = np.ma.empty(an_y_var.shape, dtype=sat_zn.dtype)
sat[np.logical_not(np.ma.getmaskarray(an_y_var))] = interpolated
sat.mask = an_y_var.mask
return sat
def interpolate_individual(self, image):
# unpacking
ogridx, ogridy = self.ogrid
ngridx, ngridy = self.ngrid
f = RectBivariateSpline(ogridy, ogridx, image, kx=1, ky=1)
return f.ev(ngridy.flatten(), ngridx.flatten()).reshape(ngridx.shape)
def LucasKanade(It, It1, rect, p0=np.zeros(2)):
# Input:
# It: template image
# It1: Current image
# rect: Current position of the car
# (top left, bot right coordinates)
# p0: Initial movement vector [dp_x0, dp_y0]
# Output:
# p: movement vector [dp_x, dp_y]
# Put your implementation here
p = p0
x1, y1, x2, y2 = rect[0], rect[1], rect[2], rect[3]
threshold = 1e-3
dp = np.array([float("inf"), float("inf")])
interpolated_It = RectBivariateSpline(
x=np.array([i for i in range(int(It.shape[0]))]),
y=np.array([i for i in range(int(It.shape[1]))]),
z=It)
interpolated_It1 = RectBivariateSpline(
x=np.array([i for i in range(int(It1.shape[0]))]),
y=np.array([i for i in range(int(It1.shape[1]))]),
z=It1)
while np.sum(np.square(dp)) >= threshold:
warp_x = np.arange(x1 + p[0], x2 + p[0] + .5)
warp_y = np.arange(y1 + p[1], y2 + p[1] + .5)
warp_X = np.array([warp_x for i in range(len(warp_y))])
warp_Y = np.array([warp_y for i in range(len(warp_x))]).T
warp_It1x = interpolated_It1.ev(warp_Y, warp_X)
x = np.arange(x1, x2 + .5)
y = np.arange(y1, y2 + .5)
X = np.array([x for i in range(len(y))])
Y = np.array([y for i in range(len(x))]).T
Itx = interpolated_It.ev(Y, X)
A = np.array([
interpolated_It1.ev(warp_Y, warp_X, dx=0, dy=1).flatten(),
interpolated_It1.ev(warp_Y, warp_X, dx=1, dy=0).flatten()
]).T
b = (Itx - warp_It1x).flatten()
dp = np.dot(np.linalg.inv(np.dot(A.T, A)), np.dot(A.T, b))
p += dp
return p
def InverseCompositionAffine(It, It1, threshold, num_iters):
"""
:param It: template image
:param It1: Current image
:param threshold: if the length of dp is smaller than the threshold, terminate the optimization
:param num_iters: number of iterations of the optimization
:return: M: the Affine warp matrix [3x3 numpy array]
"""
# put your implementation here
M = np.eye(3)
H0, W0 = It.shape
H1, W1 = It1.shape
It_interpolate = RectBivariateSpline(np.arange(0, H0, 1), np.arange(0, W0, 1), It)
It1_interpolate = RectBivariateSpline(np.arange(0, H1, 1), np.arange(0, W1, 1), It1)
# Gradient of warpped It
x_warp, y_warp = np.meshgrid(np.arange(0, W0, 1), np.arange(0, H0, 1))
delta_I = np.array([It_interpolate.ev(y_warp, x_warp, dx=0, dy=1).flatten(),
It_interpolate.ev(y_warp, x_warp, dx=1, dy=0).flatten()]).T
A_origin = np.array([delta_I[:, 0] * x_warp.flatten(), delta_I[:, 0] * y_warp.flatten(), delta_I[:, 0], delta_I[:, 1] * x_warp.flatten(), delta_I[:, 1] * y_warp.flatten(), delta_I[:, 1]]).T
for _ in range(int(num_iters)):
# Warp It+1
x1, y1 = np.meshgrid(np.arange(0, W1, 1), np.arange(0, H1, 1))
x1_warp = M[0, 0] * x1 + M[0, 1] * y1 + M[0, 2]
y1_warp = M[1, 0] * x1 + M[1, 1] * y1 + M[1, 2]
# Only get common region for It and warpped It+1
overlap = (0 <= x1_warp) & (x1_warp < W1) & (0 <= y1_warp) & (y1_warp < H1)
x1_warp = x1_warp[overlap]
y1_warp = y1_warp[overlap]
It1_warp = It1_interpolate.ev(y1_warp, x1_warp)
A = A_origin[overlap.flatten()]
b = It1_warp - It[overlap]
delta_p = np.dot(np.dot(np.linalg.inv(np.dot(A.T, A)), A.T), b.flatten())
delta_M = np.concatenate((delta_p, np.array([0, 0, 1]))).reshape((3, 3))
delta_M[0, 0] += 1
delta_M[1, 1] += 1
M = np.dot(M, np.linalg.inv(delta_M))
if np.linalg.norm(delta_p) < threshold:
break
return M
def getStraightenWormInt(worm_img, skeleton, half_width = -1, cnt_widths = np.zeros(0), width_resampling = 7, ang_smooth_win = 12, length_resampling = 49):
'''
Code to straighten the worm worms.
worm_image - image containing the worm
skeleton - worm skeleton
half_width - half width of the worm, if it is -1 it would try to calculated from cnt_widths
cnt_widths - contour widths used in case the half width is not given
width_resampling - number of data points used in the intensity map along the worm width
length_resampling - number of data points used in the intensity map along the worm length
ang_smooth_win - window used to calculate the skeleton angles.
A small value will introduce noise, therefore obtaining bad perpendicular segments.
A large value will over smooth the skeleton, therefore not capturing the correct shape.
'''
#if np.all(np.isnan(skeleton)):
# buff = np.empty((skeleton.shape[0], width_resampling))
# buff.fill(np.nan)
# return buff
assert half_width>0 or cnt_widths.size>0
assert not np.any(np.isnan(skeleton))
if ang_smooth_win%2 == 1:
ang_smooth_win += 1;
if skeleton.shape[0] != length_resampling:
skeleton, _ = curvspace(np.ascontiguousarray(skeleton), length_resampling)
skelX = skeleton[:,0];
skelY = skeleton[:,1];
assert np.max(skelX) < worm_img.shape[0]
assert np.max(skelY) < worm_img.shape[1]
assert np.min(skelY) >= 0
assert np.min(skelY) >= 0
#calculate smoothed angles
skel_angles = angleSmoothed(skelX, skelY, ang_smooth_win)
#%get the perpendicular angles to define line scans (orientation doesn't
#%matter here so subtracting pi/2 should always work)
perp_angles = skel_angles - np.pi/2;
#%for each skeleton point get the coordinates for two line scans: one in the
#%positive direction along perpAngles and one in the negative direction (use
#%two that both start on skeleton so that the intensities are the same in
#%the line scan)
#resample the points along the worm width
if half_width <= 0:
half_width = (np.median(cnt_widths[10:-10])/2.) #add half a pixel to get part of the contour
r_ind = np.linspace(-half_width, half_width, width_resampling)
#create the grid of points to be interpolated (make use of numpy implicit broadcasting Nx1 + 1xM = NxM)
grid_x = skelX + r_ind[:, np.newaxis]*np.cos(perp_angles);
grid_y = skelY + r_ind[:, np.newaxis]*np.sin(perp_angles);
f = RectBivariateSpline(np.arange(worm_img.shape[0]), np.arange(worm_img.shape[1]), worm_img)
return f.ev(grid_y, grid_x) #return interpolated intensity map
class SplineEstimator(object):
def fit(self, x, y):
self.lut = RectBivariateSpline(x[1], x[0], y)
return self
def predict(self, X):
return self.lut.ev(X[:, 1], X[:, 0])
def getEroDep(self, xo = None, yo = None, xm = None, ym = None,
pts = 100, gfilter = 5):
"""
Extract a slice from the 3D data set and compute its deposition thicknesses.
Parameters
----------
variable: xo, yo
Lower X,Y coordinates of the cross-section
variable: xm, ym
Upper X,Y coordinates of the cross-section
variable: pts
Number of points to discretise the cross-section
variable: gfilter
Gaussian smoothing filter
"""
if xm > self.x.max():
xm = self.x.max()
if ym > self.y.max():
ym = self.y.max()
if xo < self.x.min():
xo = self.x.min()
if yo < self.y.min():
yo = self.y.min()
xsec, ysec = self._cross_section(xo, yo, xm, ym, pts)
self.dist = np.sqrt(( xsec - xo )**2 + ( ysec - yo )**2)
# Surface
rect_B_spline = RectBivariateSpline(self.y[:,0], self.x[0,:], self.z)
datatop = rect_B_spline.ev(ysec, xsec)
self.top = filters.gaussian_filter1d(datatop,sigma=gfilter)
# Cumchange
rect_B_spline = RectBivariateSpline(self.y[:,0], self.x[0,:], self.cumchange)
cumdat = rect_B_spline.ev(ysec, xsec)
gcum = filters.gaussian_filter1d(cumdat,sigma=gfilter)
self.depo = gcum.clip(min=0)
return
def __init__(self, R_in, z_in, Raxis, zaxis, psi_in, R_out, z_out, psi_sep=0):
print('2d interp')
self.error = 0
# Check input dimensions, R_out z_out must be flat
if len(R_out) != len(z_out):
print('R and z must have the same dimensions')
self.error = 1
return
if np.array(R_out).ndim > 1:
print('R_out must be flat')
self.error = 2
return
if np.array(z_out).ndim > 1:
print('z_out must be flat')
self.error = 3
return
nz_psi, nR_psi = psi_in.shape
if len(R_in) != nR_psi:
print('Inconsistent R axis for psi_in')
self.error = 5
return
if len(z_in) != nz_psi:
print('Inconsistent z axis for psi_in')
self.error = 6
return
nRz = len(R_out)
self.psi_red = np.zeros(nRz)
# Bilinear interpolation
bisp = RectBivariateSpline(z_in, R_in, psi_in)
self.psi_axis = bisp.ev(zaxis, Raxis)
for jRz, R in enumerate(R_out):
z = z_out[jRz]
self.psi_red[jRz] = bisp.ev(z, R)
self.psi_norm = (self.psi_red - self.psi_axis)/(psi_sep - self.psi_axis)
self.rho_pol = np.sqrt(self.psi_norm)
def assign_phases_to_antennas(ant1,ant2,antX,antY,PhaseGrid,phase_x,phase_y,velocity,time):
'''
Given antenna IDs, coordinates, and the phase grid and its coordinates: Translate
the antennas across the grid and record the phase for each antenna. Returns a 1D array
of antenna phases (uncalibrated) for the 1st and 2nd antenna in each observation
'''
f_interp = RectBivariateSpline(phase_y,phase_x,PhaseGrid,kx=1,ky=1)
antenna1_phase = f_interp.ev(antY[ant1],antX[ant1]+velocity*time)
antenna2_phase = f_interp.ev(antY[ant2],antX[ant2]+velocity*time)
# Also want to get a 2d array of the phase of each antenna with time, to ease with calibration
Ntsteps = len(time)/(len(antX)*(len(antX)-1)/2)
antennaphases = np.zeros([len(antX),Ntsteps],float)
tstepsize = np.unique(time)[1]-np.unique(time[0])
for i in range(len(antX)):
antennaphases[i,:] = f_interp.ev(antY[i]*np.ones(Ntsteps),antX[i]+tstepsize*velocity*np.arange(Ntsteps))
return antenna1_phase,antenna2_phase,antennaphases
def scatter(self,move_pix=0,scale=1):
'''
Generate the scattered image which is stored in the ``iss`` member.
:param move_pix: (optional) int
Number of pixels to roll the screen (for time evolution).
:param scale: (optional) scalar
Scale factor for gradient. To simulate the scattering effect at another
wavelength this is (lambda_new/lambda_old)**2
'''
M = self.model.shape[-1] # size of original image array
N = self.nx # size of output image array
#if not self.live_dangerously: self._checkSanity()
# calculate phase gradient
dphi_x,dphi_y = self._calculate_dphi(move_pix=move_pix)
if scale != 1:
dphi_x *= scale/sqrt(2.)
dphi_y *= scale/sqrt(2.)
xx_,yy = np.meshgrid((np.arange(N) - 0.5*(N-1)),\
(np.arange(N) - 0.5*(N-1)),indexing='xy')
# check whether we care about PA of scattering kernel
if self.pa != None:
f_model = RectBivariateSpline(self.model_dx/self.dx*(np.arange(M) - 0.5*(M-1)),\
self.model_dx/self.dx*(np.arange(M) - 0.5*(M-1)),\
self.model)
# apply rotation
theta = -(90 * pi / 180) + np.radians(self.pa) # rotate CW 90 deg, then CCW by PA
xx_ += dphi_x
yy += dphi_y
xx = cos(theta)*xx_ - sin(theta)*yy
yy = sin(theta)*xx_ + cos(theta)*yy
self.iss = f_model.ev(yy.flatten(),xx.flatten()).reshape((self.nx,self.nx))
# rotate back and clip for positive values for I
if self.think_positive:
self.iss = clip(rotate(self.iss,-1*theta/np.pi*180,reshape=False),a_min=0,a_max=1e30) * (self.dx/self.model_dx)**2
else:
self.iss = rotate(self.iss,-1*theta/np.pi*180,reshape=False) * (self.dx/self.model_dx)**2
# otherwise do a faster lookup rather than the expensive interpolation.
else:
yyi = np.rint((yy+dphi_y+self.nx/2)).astype(np.int) % self.nx
xxi = np.rint((xx_+dphi_x+self.nx/2)).astype(np.int) % self.nx
if self.think_positive:
self.iss = clip(self.isrc[yyi,xxi],a_min=0,a_max=1e30)
else:
self.iss = self.isrc[yyi,xxi]
def x_sig( self, x, sigma ):
eps_list, mu_q = self.spirrid_response
eps_sig = InterpolatedUnivariateSpline( mu_q[0, :], eps_list[1] )
if max( mu_q ) > sigma:
pass
else:
raise ValueError( 'applied stress higher than the maximum in micromechanical evaluation of a CB' )
eps = eps_sig( sigma )
spline = RectBivariateSpline( eps_list[0], eps_list[1], mu_q )
sigma_f = spline.ev( x, ones( len( x ) ) * eps ) / self.V_f
sigma_m = ( sigma - sigma_f * self.V_f ) / self.V_m
return sigma_m
def kde_histogram(events_x, events_y, xout=None, yout=None, bins=None):
""" Histogram-based Kernel Density Estimation
Parameters
----------
events_x, events_y: 1D ndarray
The input points for kernel density estimation. Input
is flattened automatically.
xout, yout: ndarray
The coordinates at which the KDE should be computed.
If set to none, input coordinates are used.
bins: tuple (binsx, binsy)
The number of bins to use for the histogram.
Returns
-------
density: ndarray, same shape as `xout`
The KDE for the points in (xout, yout)
See Also
--------
`numpy.histogram2d`
`scipy.interpolate.RectBivariateSpline`
"""
valid_combi = ((xout is None and yout is None) or
(xout is not None and yout is not None)
)
if not valid_combi:
raise ValueError("Both `xout` and `yout` must be (un)set.")
if yout is None and yout is None:
xout = events_x
yout = events_y
if bins is None:
bins = (max(5, bin_num_doane(events_x)),
max(5, bin_num_doane(events_y)))
# Compute the histogram
hist2d, xedges, yedges = np.histogram2d(x=events_x,
y=events_y,
bins=bins,
normed=True)
xip = xedges[1:]-(xedges[1]-xedges[0])/2
yip = yedges[1:]-(yedges[1]-yedges[0])/2
estimator = RectBivariateSpline(x=xip, y=yip, z=hist2d)
density = estimator.ev(xout, yout)
density[density < 0] = 0
return density.reshape(xout.shape)
def add_dem_2D(self, x, dem, y0=0., y1=np.infty, yref=None, kx=3, ky=1,
s=None):
'''
Add topography by vertically stretching the domain in the region [y0,
y1] - points below y0 are kept fixed, points above y1 are moved as
the DEM, points in between are interpolated.
Usage: first call add_dem_2D for each boundary that is to be perturbed
and finally call apply_dem to add the perturbation to the mesh
coordinates.
:param x: x coordinates of the DEM
:type x: numpy array
:param dem: the DEM
:type dem: numpy array
:param y0: vertical coordinate, at which the stretching begins
:type y0: float
:param y1: vertical coordinate, at which the stretching ends, can be
infinity
:type y1: float
:param yref: vertical coordinate, at which the stretching ends
:type yref: float
:param kx: horizontal degree of the spline interpolation
:type kx: integer
:param ky: vertical degree of the spline interpolation
:type ky: integer
:param s: smoothing factor
:type s: float
'''
if not self.ndim == 2: # pragma: no cover
raise ValueError('apply_dem_2D works on 2D meshes only')
if yref is None:
yref = self.points[:, 1].max()
if y1 < np.infty:
y = np.array([y0, yref, y1])
d = np.c_[np.zeros(len(dem)), dem, np.zeros(len(dem))]
else:
y = np.array([y0, yref])
d = np.c_[np.zeros(len(dem)), dem]
xx, yy = np.meshgrid(x, y, indexing='ij')
rbs = RectBivariateSpline(x, y, d, kx=kx, ky=ky, s=s)
# add to topography
if self.topography is None:
self.topography = np.zeros_like(self.points[:, -1])
self.points[:, 1] += rbs.ev(self.points[:, 0], self.points[:, 1])
def fft_interpolate(visdata,immap,xmap,ymap,ug=None,scaleamp=1.,shiftphase=[0.,0.]):
"""
Take a dataset and a map of a field, fft the image,
and interpolate onto the uv-coordinates of the dataset.
Returns:
interpdata: Visdata object
A dataset which samples the given immap
"""
# Correct for PB attenuation
if visdata.PBfwhm is not None:
PBs = visdata.PBfwhm / (2.*np.sqrt(2.*np.log(2)))
immap *= np.exp(-(xmap**2./(2.*PBs**2.)) - (ymap**2./(2.*PBs**2.)))
#immap = immap[::-1,:] # Fixes issue of origin in tlc vs blc to match sky coords
imfft = fftshift(fft2(fftshift(immap)))
# Calculate the uv points we need, if we don't already have them
if ug is None:
kmax = 0.5/((xmap[0,1]-xmap[0,0])*arcsec2rad)
ug = np.linspace(-kmax,kmax,xmap.shape[0])
# Interpolate the FFT'd image onto the data's uv points
# Using RBS, much faster since ug is gridded
spliner = RectBivariateSpline(ug,ug,imfft.real,kx=1,ky=1)
splinei = RectBivariateSpline(ug,ug,imfft.imag,kx=1,ky=1)
interpr = spliner.ev(visdata.v,visdata.u)
interpi = splinei.ev(visdata.v,visdata.u)
interpdata = Visdata(visdata.u,visdata.v,interpr,interpi,visdata.sigma,\
visdata.ant1,visdata.ant2,visdata.PBfwhm,'interpolated_data')
# Apply scaling, phase shifts; wrap phases to +/- pi.
interpdata.amp *= scaleamp
interpdata.phase += 2.*np.pi*arcsec2rad*(shiftphase[0]*interpdata.u + shiftphase[1]*interpdata.v)
interpdata.phase = (interpdata.phase + np.pi) % (2*np.pi) - np.pi
return interpdata
def _interp(self):
"""Interpolate the cartesian coordinates.
"""
if np.all(self.hrow_indices == self.row_indices):
return self._interp1d()
xpoints, ypoints = np.meshgrid(self.hrow_indices,
self.hcol_indices)
spl = RectBivariateSpline(self.row_indices,
self.col_indices,
self.x__,
s=0,
kx=self.kx_,
ky=self.ky_)
self.newx = spl.ev(xpoints.ravel(), ypoints.ravel())
self.newx = self.newx.reshape(xpoints.shape).T
spl = RectBivariateSpline(self.row_indices,
self.col_indices,
self.y__,
s=0,
kx=self.kx_,
ky=self.ky_)
self.newy = spl.ev(xpoints.ravel(), ypoints.ravel())
self.newy = self.newy.reshape(xpoints.shape).T
spl = RectBivariateSpline(self.row_indices,
self.col_indices,
self.z__,
s=0,
kx=self.kx_,
ky=self.ky_)
self.newz = spl.ev(xpoints.ravel(), ypoints.ravel())
self.newz = self.newz.reshape(xpoints.shape).T
def run_slimscat(isrc,idx,screenfile='screen.bin'):
'''
Scatter source image.
:param isrc: source image
:param idx: source pixel scale
:param screenfile: screen file
'''
# read in screen parameters
f = open(screenfile,'rb')
hdrsize = struct.unpack('i',f.read(4))[0]
nphi = int(np.sqrt(struct.unpack('i',f.read(4))[0]))
dx = struct.unpack('d',f.read(8))[0]
f.seek(hdrsize)
# filter image
# check fov
iny,inx = isrc.shape
ny = int(np.floor(iny*idx/dx))
nx = int(np.floor(inx*idx/dx))
assert idx*max([iny,inx]) < nphi*dx
# read in screen
dphi_x = np.empty((ny,nx),dtype=np.float64)
dphi_y = np.empty((ny,nx),dtype=np.float64)
for i in range(ny):
f.seek(hdrsize + i*8*1*nphi,0)
dphi_x[i,:] = struct.unpack('{0:d}d'.format(nx),f.read(nx*8))
for i in range(ny):
f.seek(hdrsize + 8*nphi*nphi + i*8*1*nphi,0)
dphi_y[i,:] = struct.unpack('{0:d}d'.format(nx),f.read(nx*8))
f.close()
# construct spline fit to source image
f_isrc = RectBivariateSpline(idx/dx*(np.arange(iny) - 0.5*(iny-1)),\
idx/dx*(np.arange(inx) - 0.5*(inx-1)),\
isrc)
# scatter pixel coordinates
yy,_xx = np.meshgrid((np.arange(ny) - 0.5*(ny-1)),\
(np.arange(nx) - 0.5*(nx-1)),indexing='ij')
_xx += dphi_x
yy += dphi_y
return f_isrc.ev(yy.flatten(),_xx.flatten()).reshape((ny,nx))
def get_interpolated_pixel_color_rbspline(pts, s_im, size):
"""given pts in floats, linear interpolate pixel values nearby to get a good colour"""
pts = clamp(pts, size)
s_im = np.atleast_3d(s_im)
ys,xs = size
ycoords, xcoords = np.arange(ys), np.arange(xs)
out = np.empty(pts.shape[1:] + (s_im.shape[-1],),dtype=s_im.dtype)
pts_vec = pts.reshape((2,-1))
out_vec = out.reshape((-1,s_im.shape[-1])) #flatten for easier vectorization
for i in range(s_im.shape[-1]): #loop over color channels
rbspline = RectBivariateSpline(ycoords, xcoords, s_im[...,i])
out_vec[:,i] = rbspline.ev(pts_vec[0],pts_vec[1])
return out
def interp3d_emergence(uplift, data, out_times, verbose=False):
"""Interpolate uplift surfaces (xyz data at a specific t) to data locations
(non-grid) and data times (between times calculated).
Uses progressive linear interpolations: first the uplift at each outputted
time is interpolated to the data locations in data.locs, then they are
interpolated to the data times in each location.
Parameters
----------
uplift (array-like) - size (times, lon, lat) array of uplift surfaces
data - data whose data.locs are the locations to interpolate to.
out_times - the times for the first index of the uplift array (should be
of uplift eventually, yes?)
"""
time_start = time.clock()
##########################################
# STUFF TO FIX HEEEEEEERE!!!!!!!!!!!!!
N = uplift[0].shape
# TODO These should be gotten from somewhere, right? uplift.grid??
X = np.linspace(0, 4900000, num=N[1], endpoint=True)
Y = np.linspace(0, 4700000, num=N[0], endpoint=True)
##########################################
# interp_data will be an array of size (N_output_times, N_locations)
# for use in interpolating the calculated emergence to the locations and
# times at which there are data in data
interp_data = []
# Interpolate the calculated uplift at each time on the Lat-Lon grid
# to the data locations.
for uplift_at_a_time in uplift:
interp_func = RectBivariateSpline(X, Y, uplift_at_a_time.T)
interp_data.append(interp_func.ev(data.locs[:,0], data.locs[:,1]))
interp_data = np.array(interp_data).T
calc_vector = []
# Interpolate the calculated uplifted at each time and data location
# to the times of the data location.
for interp, loc in zip(interp_data, data):
calc_vector.append(np.interp(loc['data_dict']['times'],
out_times[::-1], interp[::-1]))
# flatten the array
calc_vector = np.array([item for l in calc_vector for item in l])
if verbose: print 'Interpolation time: {0}s'.format(time.clock()-time_start)
return calc_vector
def project_interp(self,to_file=None,sys_a8=False,bok=True,clobber=False,**kwd):
# projected image x,y
to_nx,to_ny=self.to_size
print('get XY in image for pixels in new WCS ...')
xx,yy=np.meshgrid(np.arange(to_nx),np.arange(to_ny))
# projected image ra dec
ra,dec=self.to_wcs.all_pix2world(xx,yy,0)
# image XY
if sys_a8:
imxx,imyy=a8.a8_ad2xy(self.head,ra,dec,bok=bok)
imxx-=1.0
imyy-=1.0
else:
imxx,imyy=self.wcs.all_world2pix(ra,dec,0)
data=self.data.copy()
ny,nx=self.data.shape
inmask=(imyy > -0.5) & (imyy < ny-0.5) & (imxx > -0.5) & (imxx < nx-0.5)
if not inmask.any(): return None,None
int_data=np.zeros((to_ny,to_nx))
if self.mask is not None:
int_mask=np.zeros((to_ny,to_nx),dtype='bool')
indr,indc=np.where(inmask)
tmpyy=np.round(imyy[inmask]).astype('int')
tmpxx=np.round(imxx[inmask]).astype('int')
tmpmask=self.mask[tmpyy,tmpxx]
int_mask[indr,indc]=tmpmask
int_mask[np.logical_not(inmask)]=True
print('project image to new WCS by interpolating ...')
ff=RectBivariateSpline(np.arange(ny),np.arange(nx),data,**kwd)
inmaskval=ff.ev(imyy[inmask],imxx[inmask])
#int_data[np.logical_not(inmask)]=np.nan
int_data[inmask]=inmaskval
if to_file is not None:
hdu=self.to_wcs.to_fits()[0]
hdu.data=int_data
hdu.writeto(to_file,clobber=clobber)
if self.mask is not None:
f,ext=os.path.splitext(to_file)
hdu.data=int_mask.astype('uint8')
hdu.writeto(f+'-mask.fits',clobber=clobber)
if self.mask is not None:
return int_data,int_mask
else:
return int_data,None
def generate_score_map(structure):
if structure == 'BackG':
return None
score_matrix = np.zeros((n_sample_x, n_sample_y))
score_matrix[sample_location_indices[:,0], sample_location_indices[:,1]] = probs_allClasses[structure]
spline = RectBivariateSpline(sample_locations_unique_xs/shrink_factor,
sample_locations_unique_ys/shrink_factor,
score_matrix,
bbox=[interpolation_xmin/shrink_factor,
interpolation_xmax/shrink_factor,
interpolation_ymin/shrink_factor,
interpolation_ymax/shrink_factor])
t1 = time.time()
dense_score_map = spline.ev(sample_locations_interpolatedArea_xs_matrix,
sample_locations_interpolatedArea_ys_matrix)
sys.stderr.write('evaluate spline: %.2f seconds\n' % (time.time() - t1)) # 5s for shrink_factor=4; doubling results in quadratic time reduction
t1 = time.time()
dense_score_map = resize(dense_score_map, (interpolation_h, interpolation_w)) # similar speed as rescale
# dense_score_map = rescale(dense_score_map, shrink_factor)
sys.stderr.write('scale up: %.2f seconds\n' % (time.time() - t1)) # 10s, very high penalty when multiprocessing
# t = time.time()
dense_score_map[dense_score_map < 1e-1] = 0
dense_score_map[dense_score_map > 1.] = 1.
# sys.stderr.write('threshold: %.2f seconds\n' % (time.time() - t))
if np.count_nonzero(dense_score_map) < 1e5:
sys.stderr.write('No %s is detected on section %d\n' % (structure, sec))
return None
t1 = time.time()
scoremap_bp_filepath, scoremap_interpBox_filepath = \
DataManager.get_scoremap_filepath(stack=stack, fn=fn, anchor_fn=anchor_fn, structure=structure,
return_bbox_fp=True, setting=actual_setting)
save_hdf(dense_score_map.astype(np.float16), scoremap_bp_filepath, complevel=5)
np.savetxt(scoremap_interpBox_filepath,
np.array((interpolation_xmin, interpolation_xmax, interpolation_ymin, interpolation_ymax))[None],
fmt='%d')
sys.stderr.write('save: %.2f seconds\n' % (time.time() - t1)) # 4s, very high penalty when multiprocessing
def getStraightenWormIntT(worm_img, skeleton, half_width = -1, cnt_widths = np.zeros(0), width_resampling = 7, ang_smooth_win = 12, length_resampling = 49):
#if np.all(np.isnan(skeleton)):
# buff = np.empty((skeleton.shape[0], width_resampling))
# buff.fill(np.nan)
# return buff
assert half_width>0 or cnt_widths.size>0
assert not np.any(np.isnan(skeleton))
if ang_smooth_win%2 == 1:
ang_smooth_win += 1;
if skeleton.shape[0] != length_resampling:
skeleton, _ = curvspace(np.ascontiguousarray(skeleton), length_resampling)
skelX = skeleton[:,0];
skelY = skeleton[:,1];
assert np.max(skelX) < worm_img.shape[0]
assert np.max(skelY) < worm_img.shape[1]
assert np.min(skelY) >= 0
assert np.min(skelY) >= 0
#calculate smoothed angles
skel_angles = angleSmoothed(skelX, skelY, ang_smooth_win)
#%get the perpendicular angles to define line scans (orientation doesn't
#%matter here so subtracting pi/2 should always work)
perp_angles = skel_angles - np.pi/2;
#%for each skeleton point get the coordinates for two line scans: one in the
#%positive direction along perpAngles and one in the negative direction (use
#%two that both start on skeleton so that the intensities are the same in
#%the line scan)
#resample the points along the worm width
if half_width <= 0:
half_width = (np.median(cnt_widths[10:-10])/2.) #add half a pixel to get part of the contour
r_ind = np.linspace(-half_width, half_width, width_resampling)
#create the grid of points to be interpolated (make use of numpy implicit broadcasting Nx1 + 1xM = NxM)
grid_x = skelX + r_ind[:, np.newaxis]*np.cos(perp_angles);
grid_y = skelY + r_ind[:, np.newaxis]*np.sin(perp_angles);
f = RectBivariateSpline(np.arange(worm_img.shape[0]), np.arange(worm_img.shape[1]), worm_img)
return f.ev(grid_y, grid_x), grid_x, grid_y #return interpolated intensity map
def find_stop_power(**kwargs):
data = TRS398_table7()
stop_power_interp = RectBivariateSpline(
np.array(data["depth/R50"]), np.array(data["R50"]), np.array(data["contents"])
)
energy = kwargs["energy"]
depth_mm = np.array(kwargs["depth"])
depth_cm = depth_mm / 10
R50_mm = energy_to_R50(energy)
R50_cm = R50_mm / 10
depth_over_R50 = depth_cm / R50_cm
stop_power = np.ravel(stop_power_interp.ev(depth_over_R50, R50_cm))
return stop_power
def getStraightenWormInt(worm_img, skeleton, half_width, width_resampling):
'''
Code to straighten the worm worms.
worm_image - image containing the worm
skeleton - worm skeleton
half_width - half width of the worm, if it is -1 it would try to calculated from cnt_widths
cnt_widths - contour widths used in case the half width is not given
width_resampling - number of data points used in the intensity map along the worm width
length_resampling - number of data points used in the intensity map along the worm length
ang_smooth_win - window used to calculate the skeleton angles.
A small value will introduce noise, therefore obtaining bad perpendicular segments.
A large value will over smooth the skeleton, therefore not capturing the correct shape.
'''
assert half_width>0 or cnt_widths.size>0
assert not np.any(np.isnan(skeleton))
dX = np.diff(skeleton[:,0])
dY = np.diff(skeleton[:,1])
skel_angles = np.arctan2(dY, dX)
skel_angles = np.hstack((skel_angles[0], skel_angles))
#%get the perpendicular angles to define line scans (orientation doesn't
#%matter here so subtracting pi/2 should always work)
perp_angles = skel_angles - np.pi/2;
#%for each skeleton point get the coordinates for two line scans: one in the
#%positive direction along perpAngles and one in the negative direction (use
#%two that both start on skeleton so that the intensities are the same in
#%the line scan)
r_ind = np.linspace(-half_width, half_width, width_resampling)
#create the grid of points to be interpolated (make use of numpy implicit broadcasting Nx1 + 1xM = NxM)
grid_x = skeleton[:,0] + r_ind[:, np.newaxis]*np.cos(perp_angles);
grid_y = skeleton[:,1] + r_ind[:, np.newaxis]*np.sin(perp_angles);
#interpolated the intensity map
f = RectBivariateSpline(np.arange(worm_img.shape[0]), np.arange(worm_img.shape[1]), worm_img)
straighten_worm = f.ev(grid_y, grid_x)
return straighten_worm, grid_x, grid_y
def _interp(self):
"""Interpolate the cartesian coordinates.
"""
if np.all(self.hrow_indices == self.row_indices):
return self._interp1d()
xpoints, ypoints = np.meshgrid(self.hrow_indices,
self.hcol_indices)
for num, data in enumerate(self.tie_data):
spl = RectBivariateSpline(self.row_indices,
self.col_indices,
data,
s=0,
kx=self.kx_,
ky=self.ky_)
self.new_data[num] = spl.ev(xpoints.ravel(), ypoints.ravel())
self.new_data[num] = self.new_data[num].reshape(xpoints.shape).T
def interp_tilt(uplift, data, out_times, basemap, verbose=False):
time_start = time.clock()
##########################################
# STUFF TO FIX HEEEEEEERE!!!!!!!!!!!!!
N = uplift[0].shape
# TODO These should be gotten from somewhere, right? uplift.grid??
X = np.linspace(0, 4900000, num=N[1], endpoint=True)
Y = np.linspace(0, 4700000, num=N[0], endpoint=True)
##########################################
Lon, Lat = basemap(*np.meshgrid(X, Y), inverse=True)
tilt = calc_tilts(uplift[np.where(out_times==13)[0][0]], Lon, Lat)
interp_func = RectBivariateSpline(X, Y, tilt.T)
calc_vector = interp_func.ev(data.locs[:,0], data.locs[:,1])
return calc_vector
def optpath_scipyode(xs, ys, tt, phi, startpoint):
# setting up interpolation
tt_interp=RectBivariateSpline(xs,ys,tt.T)
phi_interp=RectBivariateSpline(xs,ys,phi.T)
# initial condition
t0 = 0.0
y0 = startpoint
signorigphi=np.asscalar(phi_interp.ev(y0[0],y0[1]))
# trajectory
ts = []
ys = []
# for trajectory and aborting condition
def solout(t, y):
# time of the solver is not time in the problem...
ts.append(tt_interp.ev(y[0],y[1]))
ys.append(y.copy())
if not signorigphi*np.asscalar(phi_interp.ev(y0[0],y0[1]))>0:
return -1
else:
return 0
# rhs of ODE
def rhs(t, y):
gradx=tt_interp.ev(y[0],y[1],dx=1,dy=0)
grady=tt_interp.ev(y[0],y[1],dx=0,dy=1)
auxgrad=math.sqrt(gradx*gradx+grady*grady)
return [-gradx/auxgrad, -grady/auxgrad]
# the actual integration
ig = ode(rhs).set_integrator('dopri5')
ig.set_initial_value(y0, t0)
ig.set_solout(solout)
# throws a warning at the moment...
ret = ig.integrate(1.0e8)
# what an ugly hack to make a proper np array...
npts=np.asarray(ts)
npts.resize((len(ts),1))
npys=np.asarray(ys)
return np.concatenate((npts,npys),axis=1)
