def test_distance():
# First, let's test some distances that are easy to figure out
# without any spherical trig.
eq1 = galsim.CelestialCoord(0. * galsim.radians, 0. * galsim.radians) # point on the equator
eq2 = galsim.CelestialCoord(1. * galsim.radians, 0. * galsim.radians) # 1 radian along equator
eq3 = galsim.CelestialCoord(pi * galsim.radians, 0. * galsim.radians) # antipode of eq1
north_pole = galsim.CelestialCoord(0. * galsim.radians, pi/2. * galsim.radians) # north pole
south_pole = galsim.CelestialCoord(0. * galsim.radians, -pi/2. * galsim.radians) # south pole
numpy.testing.assert_almost_equal(eq1.distanceTo(eq2).rad(), 1.)
numpy.testing.assert_almost_equal(eq2.distanceTo(eq1).rad(), 1.)
numpy.testing.assert_almost_equal(eq1.distanceTo(eq3).rad(), pi)
numpy.testing.assert_almost_equal(eq2.distanceTo(eq3).rad(), pi-1.)
numpy.testing.assert_almost_equal(north_pole.distanceTo(south_pole).rad(), pi)
numpy.testing.assert_almost_equal(eq1.distanceTo(north_pole).rad(), pi/2.)
numpy.testing.assert_almost_equal(eq2.distanceTo(north_pole).rad(), pi/2.)
numpy.testing.assert_almost_equal(eq3.distanceTo(north_pole).rad(), pi/2.)
numpy.testing.assert_almost_equal(eq1.distanceTo(south_pole).rad(), pi/2.)
numpy.testing.assert_almost_equal(eq2.distanceTo(south_pole).rad(), pi/2.)
numpy.testing.assert_almost_equal(eq3.distanceTo(south_pole).rad(), pi/2.)
c1 = galsim.CelestialCoord(0.234 * galsim.radians, 0.342 * galsim.radians) # Some random point
c2 = galsim.CelestialCoord(0.234 * galsim.radians, -1.093 * galsim.radians) # Same meridian
c3 = galsim.CelestialCoord((pi + 0.234) * galsim.radians, -0.342 * galsim.radians) # Antipode
c4 = galsim.CelestialCoord((pi + 0.234) * galsim.radians, 0.832 * galsim.radians) # Different point on opposide meridian
numpy.testing.assert_almost_equal(c1.distanceTo(c1).rad(), 0.)
numpy.testing.assert_almost_equal(c1.distanceTo(c2).rad(), 1.435)
numpy.testing.assert_almost_equal(c1.distanceTo(c3).rad(), pi)
numpy.testing.assert_almost_equal(c1.distanceTo(c4).rad(), pi-1.174)
# Now some that require spherical trig calculations.
# Importantly, this uses the more straightforward spherical trig formula, the cosine rule.
# The CelestialCoord class uses a different formula that is more stable for very small
# distances, which are typical in the correlation function calculation.
c5 = galsim.CelestialCoord(1.832 * galsim.radians, -0.723 * galsim.radians) # Some other random point
# The standard formula is:
# cos(d) = sin(dec1) sin(dec2) + cos(dec1) cos(dec2) cos(delta ra)
d = arccos(sin(0.342) * sin(-0.723) + cos(0.342) * cos(-0.723) * cos(1.832 - 0.234))
numpy.testing.assert_almost_equal(c1.distanceTo(c5).rad(), d)
# Tiny displacements should have dsq = (dra^2 cos^2 dec) + (ddec^2)
c6 = galsim.CelestialCoord((0.234 + 1.7e-9) * galsim.radians, 0.342 * galsim.radians)
c7 = galsim.CelestialCoord(0.234 * galsim.radians, (0.342 + 1.9e-9) * galsim.radians)
c8 = galsim.CelestialCoord((0.234 + 2.3e-9) * galsim.radians, (0.342 + 1.2e-9) * galsim.radians)
# Note that the standard formula gets thsse wrong. d comes back as 0.
d = arccos(sin(0.342) * sin(0.342) + cos(0.342) * cos(0.342) * cos(1.7e-9))
print 'd(c6) = ',1.7e-9 * cos(0.342), c1.distanceTo(c6), d
d = arccos(sin(0.342) * sin(0.342+1.9e-9) + cos(0.342) * cos(0.342+1.9e-9) * cos(0.))
print 'd(c7) = ',1.9e-9, c1.distanceTo(c7), d
d = arccos(sin(0.342) * sin(0.342) + cos(0.342) * cos(0.342) * cos(1.2e-9))
true_d = sqrt( (2.3e-9 * cos(0.342))**2 + 1.2e-9**2)
print 'd(c7) = ',true_d, c1.distanceTo(c8), d
numpy.testing.assert_almost_equal(c1.distanceTo(c6).rad()/(1.7e-9 * cos(0.342)), 1.0)
numpy.testing.assert_almost_equal(c1.distanceTo(c7).rad()/1.9e-9, 1.0)
numpy.testing.assert_almost_equal(c1.distanceTo(c8).rad()/true_d, 1.0)
def match(self):
""" 第1の画像の各記述子について、第2の画像の対応点を求める。
入力：desc1（第1の画像の記述子）、desc2（第2の画像の記述子）"""
if self._image_1.get_sift_descriptors() is None:
self._image_1.make_sift_feature()
desc1 = numpy.array([d / numpy.linalg.norm(d) for d in self._image_1.get_sift_descriptors()])
if self._image_2.get_sift_descriptors() is None:
self._image_2.make_sift_feature()
desc2 = numpy.array([d / numpy.linalg.norm(d) for d in self._image_2.get_sift_descriptors()])
dist_ratio = 0.6
desc1_size = desc1.shape
matchscores = numpy.zeros(desc1_size[0], 'int')
desc2t = desc2.T # あらかじめ転置行列を計算しておく
for i in range(desc1_size[0]):
dotprods = numpy.dot(desc1[i,:],desc2t) # 内積ベクトル
dotprods = 0.9999 * dotprods
# 第2の画像の特徴点の逆余弦を求め、ソートし、番号を返す
indx = numpy.argsort(numpy.arccos(dotprods))
# 最も近い近接点との角度が、2番目に近いもののdist_rasio倍以下か？
if numpy.arccos(dotprods)[indx[0]] < dist_ratio * numpy.arccos(dotprods)[indx[1]]:
matchscores[i] = int(indx[0])
self._match_score = matchscores
def rotation_matrix(a1, a2, b1, b2):
"""Returns a rotation matrix that rotates the vectors *a1* in the
direction of *a2* and *b1* in the direction of *b2*.
In the case that the angle between *a2* and *b2* is not the same
as between *a1* and *b1*, a proper rotation matrix will anyway be
constructed by first rotate *b2* in the *b1*, *b2* plane.
"""
a1 = np.asarray(a1, dtype=float) / np.linalg.norm(a1)
b1 = np.asarray(b1, dtype=float) / np.linalg.norm(b1)
c1 = np.cross(a1, b1)
c1 /= np.linalg.norm(c1) # clean out rounding errors...
a2 = np.asarray(a2, dtype=float) / np.linalg.norm(a2)
b2 = np.asarray(b2, dtype=float) / np.linalg.norm(b2)
c2 = np.cross(a2, b2)
c2 /= np.linalg.norm(c2) # clean out rounding errors...
# Calculate rotated *b2*
theta = np.arccos(np.dot(a2, b2)) - np.arccos(np.dot(a1, b1))
b3 = np.sin(theta) * a2 + np.cos(theta) * b2
b3 /= np.linalg.norm(b3) # clean out rounding errors...
A1 = np.array([a1, b1, c1])
A2 = np.array([a2, b3, c2])
R = np.linalg.solve(A1, A2).T
return R
def clockwise_angle(x,y,r=None,r0=None):
# angle between two vectors defined by three points,
#(x0,y0),(x1,y1),(x2,y2)
x1=x[0]-x[1]
x2=x[2]-x[1]
y1=y[0]-y[1]
y2=y[2]-y[1]
dot = x1*x2 + y1*y2
det = x1*y2 - y1*x2
angle = np.arctan2(det, dot)
if angle<0: angle=-angle
else: angle=2*np.pi-angle
if r and r==r0: # may not make sense if r~=r0
L=np.sqrt(x2**2+y2**2)
a=np.arccos(L/r)
angle=angle-a
L0=np.sqrt(x1**2+y1**2)
if L0<r0:
a0=np.arccos(L0/r0)
angle=angle-a0
return angle
def get_new_cell(self):
"""Returns new basis vectors"""
a = np.sqrt(self.a)
b = np.sqrt(self.b)
c = np.sqrt(self.c)
ad = self.atoms.cell[0] / np.linalg.norm(self.atoms.cell[0])
Z = np.cross(self.atoms.cell[0], self.atoms.cell[1])
Z /= np.linalg.norm(Z)
X = ad - np.dot(ad, Z) * Z
X /= np.linalg.norm(X)
Y = np.cross(Z, X)
alpha = np.arccos(self.x / (2 * b * c))
beta = np.arccos(self.y / (2 * a * c))
gamma = np.arccos(self.z / (2 * a * b))
va = a * np.array([1, 0, 0])
vb = b * np.array([np.cos(gamma), np.sin(gamma), 0])
cx = np.cos(beta)
cy = (np.cos(alpha) - np.cos(beta) * np.cos(gamma)) \
/ np.sin(gamma)
cz = np.sqrt(1. - cx * cx - cy * cy)
vc = c * np.array([cx, cy, cz])
abc = np.vstack((va, vb, vc))
T = np.vstack((X, Y, Z))
return np.dot(abc, T)
def rotation_params(r0, r1, r2):
r10 = [a - b for a, b in zip(r1, r0)]
r21 = [a - b for a, b in zip(r2, r1)]
# print('r10 is ' +str(r10) )
# print('r21 is ' +str(r21) )
# angle between r10 and r21
# print('arg to arcos is ' +str(dot(r21,r10)/(norm(r21)*norm(r10))) )
arg = dot(r21, r10) / (norm(r21) * norm(r10))
if (norm(r21) * norm(r10) > 1e-16):
if arg < 0:
theta = 180 * arccos(max(-1, arg)) / pi
else:
theta = 180 * arccos(min(1, arg)) / pi
else:
theta = 0.0
# get normal vector to plane r0 r1 r2
u = cross(r21, r10)
# check for collinear case
if norm(u) < 1e-16:
# pick random perpendicular vector
if (abs(r21[0]) > 1e-16):
u = [(-r21[1] - r21[2]) / r21[0], 1, 1]
elif (abs(r21[1]) > 1e-16):
u = [1, (-r21[0] - r21[2]) / r21[1], 1]
elif (abs(r21[2]) > 1e-16):
u = [1, 1, (-r21[0] - r21[1]) / r21[2]]
return theta, u
def solve_nonlinear(self, params, unknowns, resids): x = params['xr'] y = params['yr'] z = params['z'] r = params['r'] alpha = params['alpha'] nTurbs = len(x) overlap_fraction = np.eye(nTurbs) for i in range(nTurbs): for j in range(nTurbs): #overlap_fraction[i][j] is the fraction of the area of turbine i in the wake from turbine j dx = x[i]-x[j] dy = abs(y[i]-y[j]) dz = abs(z[i]-z[j]) d = np.sqrt(dy**2+dz**2) R = r[j]+dx*alpha A = r[i]**2*np.pi overlap_area = 0 if dx <= 0: #if turbine i is in front of turbine j overlap_fraction[i][j] = 0.0 else: if d <= R-r[i]: #if turbine i is completely in the wake of turbine j if A <= np.pi*R**2: #if the area of turbine i is smaller than the wake from turbine j overlap_fraction[i][j] = 1.0 else: #if the area of turbine i is larger than tha wake from turbine j overlap_fraction[i][j] = np.pi*R**2/A elif d >= R+r[i]: #if turbine i is completely out of the wake overlap_fraction[i][j] = 0.0 else: #if turbine i overlaps partially with the wake overlap_area = r[i]**2.*np.arccos((d**2.+r[i]**2.-R**2.)/(2.0*d*r[i]))+R**2.*np.arccos((d**2.+R**2.-r[i]**2.)/(2.0*d*R))-0.5*np.sqrt((-d+r[i]+R)*(d+r[i]-R)*(d-r[i]+R)*(d+r[i]+R)) overlap_fraction[i][j] = overlap_area/A print "Overlap Fraction Matrix: ", overlap_fraction unknowns['overlap'] = overlap_fraction
def _compute_static_prob(tri, com):
"""
For an object with the given center of mass, compute
the probability that the given tri would be the first to hit the
ground if the object were dropped with a pose chosen uniformly at random.
Parameters
----------
tri: (3,3) float, the vertices of a triangle
cm: (3,) float, the center of mass of the object
Returns
-------
prob: float, the probability in [0,1] for the given triangle
"""
sv = [(v - com) / np.linalg.norm(v - com) for v in tri]
# Use L'Huilier's Formula to compute spherical area
a = np.arccos(min(1, max(-1, np.dot(sv[0], sv[1]))))
b = np.arccos(min(1, max(-1, np.dot(sv[1], sv[2]))))
c = np.arccos(min(1, max(-1, np.dot(sv[2], sv[0]))))
s = (a + b + c) / 2.0
# Prevents weirdness with arctan
try:
return 1.0 / np.pi * np.arctan(np.sqrt(np.tan(s / 2) * np.tan(
(s - a) / 2) * np.tan((s - b) / 2) * np.tan((s - c) / 2)))
except BaseException:
s = s + 1e-8
return 1.0 / np.pi * np.arctan(np.sqrt(np.tan(s / 2) * np.tan(
(s - a) / 2) * np.tan((s - b) / 2) * np.tan((s - c) / 2)))
def star(a,b,c,alpha,beta,gamma):
"Calculate unit cell volume, reciprocal cell volume, reciprocal lattice parameters"
alpha=np.radians(alpha)
beta=np.radians(beta)
gamma=np.radians(gamma)
V=2*a*b*c*\
np.sqrt(np.sin((alpha+beta+gamma)/2)*\
np.sin((-alpha+beta+gamma)/2)*\
np.sin((alpha-beta+gamma)/2)*\
np.sin((alpha+beta-gamma)/2))
Vstar=(2*np.pi)**3/V;
astar=2*np.pi*b*c*np.sin(alpha)/V
bstar=2*np.pi*a*c*np.sin(beta)/V
cstar=2*np.pi*b*a*np.sin(gamma)/V
alphastar=np.arccos((np.cos(beta)*np.cos(gamma)-\
np.cos(alpha))/ \
(np.sin(beta)*np.sin(gamma)))
betastar= np.arccos((np.cos(alpha)*np.cos(gamma)-\
np.cos(beta))/ \
(np.sin(alpha)*np.sin(gamma)))
gammastar=np.arccos((np.cos(alpha)*np.cos(beta)-\
np.cos(gamma))/ \
(np.sin(alpha)*np.sin(beta)))
V=V
alphastar=np.degrees(alphastar)
betastar=np.degrees(betastar)
gammastar=np.degrees(gammastar)
return astar,bstar,cstar,alphastar,betastar,gammastar
def calculate_couplings_levine(dt: float, w_jk: Matrix,
w_kj: Matrix) -> Matrix:
"""
Compute the non-adiabatic coupling according to:
`Evaluation of the Time-Derivative Coupling for Accurate Electronic
State Transition Probabilities from Numerical Simulations`.
Garrett A. Meek and Benjamin G. Levine.
dx.doi.org/10.1021/jz5009449 | J. Phys. Chem. Lett. 2014, 5, 2351−2356
"""
# Orthonormalize the Overlap matrices
w_jk = np.linalg.qr(w_jk)[0]
w_kj = np.linalg.qr(w_kj)[0]
# Diagonal matrix
w_jj = np.diag(np.diag(w_jk))
w_kk = np.diag(np.diag(w_kj))
# remove the values from the diagonal
np.fill_diagonal(w_jk, 0)
np.fill_diagonal(w_kj, 0)
# Components A + B
acos_w_jj = np.arccos(w_jj)
asin_w_jk = np.arcsin(w_jk)
a = acos_w_jj - asin_w_jk
b = acos_w_jj + asin_w_jk
A = - np.sin(np.sinc(a))
B = np.sin(np.sinc(b))
# Components C + D
acos_w_kk = np.arccos(w_kk)
asin_w_kj = np.arcsin(w_kj)
c = acos_w_kk - asin_w_kj
d = acos_w_kk + asin_w_kj
C = np.sin(np.sinc(c))
D = np.sin(np.sinc(d))
# Components E
w_lj = np.sqrt(1 - (w_jj ** 2) - (w_kj ** 2))
w_lk = -(w_jk * w_jj + w_kk * w_kj) / w_lj
asin_w_lj = np.arcsin(w_lj)
asin_w_lk = np.arcsin(w_lk)
asin_w_lj2 = asin_w_lj ** 2
asin_w_lk2 = asin_w_lk ** 2
t1 = w_lj * w_lk * asin_w_lj
x1 = np.sqrt((1 - w_lj ** 2) * (1 - w_lk ** 2)) - 1
t2 = x1 * asin_w_lk
t = t1 + t2
E_nonzero = 2 * asin_w_lj * t / (asin_w_lj2 - asin_w_lk2)
# Check whether w_lj is different of zero
E1 = np.where(np.abs(w_lj) > 1e-8, E_nonzero, np.zeros(A.shape))
E = np.where(np.isclose(asin_w_lj2, asin_w_lk2), w_lj ** 2, E1)
cte = 1 / (2 * dt)
return cte * (np.arccos(w_jj) * (A + B) + np.arcsin(w_kj) * (C + D) + E)
def test_02_08_three(self):
'''Test the angles between three objects'''
labels = np.zeros((10,10),int)
labels[2,2] = 1 # x=3,y=4,5 triangle
labels[2,5] = 2
labels[6,2] = 3
workspace, module = self.make_workspace(labels,
M.D_WITHIN, 5)
module.run(workspace)
m = workspace.measurements
fo = m.get_current_measurement(OBJECTS_NAME,
"Neighbors_FirstClosestObjectNumber_5")
self.assertEqual(len(fo),3)
self.assertEqual(fo[0],2)
self.assertEqual(fo[1],1)
self.assertEqual(fo[2],1)
so = m.get_current_measurement(OBJECTS_NAME,
"Neighbors_SecondClosestObjectNumber_5")
self.assertEqual(len(so),3)
self.assertEqual(so[0],3)
self.assertEqual(so[1],3)
self.assertEqual(so[2],2)
d = m.get_current_measurement(OBJECTS_NAME,
"Neighbors_SecondClosestDistance_5")
self.assertEqual(len(d),3)
self.assertAlmostEqual(d[0],4)
self.assertAlmostEqual(d[1],5)
self.assertAlmostEqual(d[2],5)
angle = m.get_current_measurement(OBJECTS_NAME,
"Neighbors_AngleBetweenNeighbors_5")
self.assertEqual(len(angle),3)
self.assertAlmostEqual(angle[0],90)
self.assertAlmostEqual(angle[1],np.arccos(3.0/5.0) * 180.0 / np.pi)
self.assertAlmostEqual(angle[2],np.arccos(4.0/5.0) * 180.0 / np.pi)
def make_cluster(n):
''' Make n particles in sphere with distribution given by Plummer
model. '''
particles = []
for i in range(n):
mass = 1.0 / n # total mass of system normalised to 1
radius = 1.0 / N.sqrt( R.random() ** (-2.0/3.0) - 1.0 )
theta = R.uniform(0, 2*N.pi)
phi = N.arccos(R.uniform(-1, 1))
x = radius * N.cos(theta) * N.sin(phi)
y = radius * N.sin(theta) * N.sin(phi)
z = radius * N.cos(phi)
pos = N.array((x, y, z))
# von Newmann's rejection technique
a = 0.0
b = 0.1
while b > a*a * (1.0 - a*a)**3.5:
a = R.uniform(0, 1)
b = R.uniform(0, 0.1)
velocity = a * N.sqrt(2.0) * (1.0 + radius*radius)**(-0.25)
theta = R.uniform(0, 2*N.pi)
phi = N.arccos(R.uniform(-1, 1))
vx = velocity * N.cos(theta) * N.sin(phi)
vy = velocity * N.sin(theta) * N.sin(phi)
vz = velocity * N.cos(phi)
vel = N.array((vx, vy, vz))
p = Particle(mass, pos, vel)
particles.append(p)
return particles
def spherical_excess(a, b, c):
"spherical excess of the triangle."
A = arccos((cos(a) - cos(b) * cos(c)) / sin(b) / sin(c))
B = arccos((cos(b) - cos(c) * cos(a)) / sin(c) / sin(a))
C = arccos((cos(c) - cos(a) * cos(b)) / sin(a) / sin(b))
E = A + B + C - pi
return(E)
def draw_cell_2d(axis, cell_output, total_radius=True, zorder=0, y_limits=None, alpha=1.0):
"""
"""
(x, y, z) = cell_output.get_location()
rad = cell_output.get_radius(total_radius=total_radius)
if cell_output.color == None:
print 'Cell has no defined color!'
col = (0, 1, 0)
else:
col = cell_output.color
#col = (0, 1, 0) if cell_output.color == None else cell_output.color
#col = cell_output.color
if (y_limits != None) and (y - rad < y_limits[0]):
segment = toolbox_schematic.CircleSegment()
segment.set_defaults(alpha=alpha, edgecolor='none', facecolor=col, zorder=zorder)
angle = pi - numpy.arccos((y - y_limits[0])/rad)
segment.set_points((y, x), rad, [angle, -angle])
segment.draw(axis)
segment.set_points((y - y_limits[0] + y_limits[1], x), rad, [angle, 2*pi-angle])
segment.draw(axis)
elif (y_limits != None) and (y + rad > y_limits[1]):
segment = toolbox_schematic.CircleSegment()
segment.set_defaults(alpha=alpha, edgecolor='none', facecolor=col, zorder=zorder)
angle = numpy.arccos((y_limits[1] - y)/rad)
segment.set_points((y, x), rad, [angle, 2*pi-angle])
segment.draw(axis)
segment.set_points((y + y_limits[0] - y_limits[1], x), rad, [-angle, angle])
segment.draw(axis)
else:
circle = toolbox_schematic.Circle()
circle.set_defaults(alpha=alpha, edgecolor='none', facecolor=col, zorder=zorder)
circle.set_points((y, x), rad)
circle.draw(axis)
def Jacobsen(h1, Xm_1, h2, Xm_2):
alp = np.degrees(np.arccos(np.dot(h1, h2) /
(np.linalg.norm(h1) * np.linalg.norm(h2))))
bet = np.degrees(np.arccos(np.dot(Xm_1, Xm_2) /
(np.linalg.norm(Xm_1) * np.linalg.norm(Xm_2))))
if ((alp - bet)**2) > 1:
print('check your indexing!')
a = 3.567 # diamond lattice parameter
# recip lattice par(note this is the mantid convention: no 2 pi)
ast = (2 * np.pi) / a
B = np.array([[ast, 0, 0], [0, ast, 0], [0, 0, ast]])
Xm_g = np.cross(Xm_1, Xm_2)
Xm = np.column_stack([Xm_1, Xm_2, Xm_g])
# Vector Q1 is described in reciprocal space by its coordinate matrix h1
Xa_1 = B.dot(h1)
Xa_2 = B.dot(h2)
Xa_g = np.cross(Xa_1, Xa_2)
Xa = np.column_stack((Xa_1, Xa_2, Xa_g))
R = Xa.dot(np.linalg.inv(Xm))
U = np.linalg.inv(R)
UB = U.dot(B)
return UB
def forward(self, lons, lats, az, dist, radians=False):
""" Forward geodetic problem from a point """
if not radians:
lons = np.array(lons) * pi / 180.0
lats = np.array(lats) * pi / 180.0
az = np.array(az) * pi / 180.0
d_ = dist / self.radius
lats2 = np.arcsin(np.sin(lats) * np.cos(d_) +
np.cos(lats) * np.sin(d_) * np.cos(az))
dlons = np.arccos((np.cos(d_) - np.sin(lats2) * np.sin(lats)) /
(np.cos(lats) * np.cos(lats2)))
baz = np.arccos((np.sin(lats) - np.cos(d_) * np.sin(lats2)) /
(np.sin(d_) * np.cos(lats2)))
if 0 <= az < pi:
lons2 = lons + dlons
baz = -baz
elif pi <= az < 2*pi:
lons2 = lons - dlons
else:
raise ValueError("azimuth should be [0, 2pi)")
baz = geodesy.unroll_rad(baz)
if not radians:
lons2 = np.array(lons2) * 180 / pi
lats2 = np.array(lats2) * 180 / pi
baz = np.array(baz) * 180 / pi
return lons2, lats2, baz
def main():
map_obstacles = np.loadtxt('obstacles_map.txt')
laser_obstacles = np.loadtxt('obstacles_laser.txt')
true_rotation = np.pi / 10
true_translation = np.array([5, 5])
laser_rot = rotate(laser_obstacles, true_rotation)
laser_trans = translate(laser_rot, true_translation)
t, r = relocalize(map_obstacles, laser_rot)
theta = np.arccos(r.item(0, 1))
print "True Rotation:", true_rotation
print "True Translation:", true_translation
print "-------------------------------------"
print "Estimated Rotation:", theta
print "Estimated Translation:", t
print "-------------------------------------"
print "Rotation Error:", np.abs(true_rotation - theta)
print "Translation Error:", np.abs(true_translation - t)
laser_reloc = rotate(laser_rot, -np.arccos(r.item(0, 1)))
plot_super(map_obstacles, laser_obstacles, "Original")
plot_super(map_obstacles, laser_trans, "Measure misaligned with map")
plot_super(map_obstacles, laser_reloc, "Measure realigned with map")
plt.show()
def uniform_random_ellipsoid5d(Npts, r1, r2, r3, r4, r5):
"""
5D case of uniform_random_ellipsoid
"""
r = np.random.rand(Npts)
ph = np.random.rand(Npts) * 2.*np.pi
costh1 = np.random.rand(Npts)*2.-1.
costh2 = np.random.rand(Npts)*2.-1.
costh3 = np.random.rand(Npts)*2.-1.
sinth1 = np.sqrt(1.-costh1*costh1)
sinth2 = np.sqrt(1.-costh2*costh2)
sinth3 = np.sqrt(1.-costh3*costh3)
th1 = np.arccos(costh1)
th2 = np.arccos(costh2)
th3 = np.arccos(costh3)
rrt = r**(1./5.)
x1 = r1 * rrt * sinth1 * sinth2 * sinth3 * np.cos(ph)
x2 = r2 * rrt * sinth1 * sinth2 * sinth3 * np.sin(ph)
x3 = r3 * rrt * sinth1 * sinth2 * costh3
x4 = r4 * rrt * sinth1 * costh2
x5 = r5 * rrt * costh1
cart_pts = np.transpose((x1,x2,x3,x4,x5))
sph_pts = np.transpose((rrt,th1,th2,th3,ph))
origin = np.array([[0.,0.,0.,0.,0.]]) # Always put a pt at ellipse center
cart_pts = np.append(origin, cart_pts, axis=0)
sph_pts = np.append(origin, sph_pts, axis=0)
return cart_pts, sph_pts
def qea(im):
H = ss.hilbert(im,axis = 2)
H = im+1j*H
ia = np.abs(H)
ip = np.angle(H)
h1col = H[1:-1,:,:]
h0col = H[:-2,:,:]
h2col = H[2:,:,:]
ifColSign = np.sign(np.real((h0col-h2col)/(2j*h1col)))
ifCol = np.arccos((h2col+h0col)/(2*h1col))
ifCol = (np.abs(ifCol)*ifColSign)/np.pi/2
ifCol = np.pad(ifCol,((1,1),(0,0),(0,0)), mode='reflect')
h0row = H[:,:-2,:]
h1row = H[:,1:-1,:]
h2row = H[:,2:,:]
#ifxSign = np.sign(np.real((h2x-h0x)/(2j*h1x)))
ifRow = np.arccos((h2row+h0row)/(2*h1row))
ifRow = (np.abs(ifRow))/np.pi/2
ifRow = np.pad(ifRow,((0,0),(1,1),(0,0)), mode='reflect')
h0time = H[:,:,:-2]
h1time = H[:,:,1:-1]
h2time = H[:,:,2:]
#ifxSign = np.sign(np.real((h2x-h0x)/(2j*h1x)))
ifTime = np.arccos((h2time+h0time)/(2*h1time))
ifTime = (np.abs(ifTime))/np.pi/2
ifTime = np.pad(ifTime,((0,0),(0,0),(1,1)), mode='reflect')
return(ia,ip,ifRow,ifCol,ifTime)
def _get_lw(box):
p0 = box[0]
p1 = box[1]
vec1 = np.array(box[2] - p0)
vec1 = vec1 / np.linalg.norm(vec1)
vec2 = np.array(p1 - p0)
vec2 = vec2 / np.linalg.norm(vec2)
vec3 = np.array(box[3] - p0)
vec3 = vec3 / np.linalg.norm(vec3)
ang1 = np.arccos((vec1).dot(vec2))
ang2 = np.arccos((vec3).dot(vec2))
dif1 = 1.5708 - ang1
dif2 = 1.5708 - ang2
if dif1 < dif2:
p2 = box[2]
else:
p2 = box[3]
l, lp = np.linalg.norm(abs(p1 - p0)), p1
w, wp = np.linalg.norm(abs(p2 - p0)), p2
if l < w:
temp = w
templ = wp
w = l
wp = lp
l = temp
lp = templ
direc = (wp - p0) / np.linalg.norm(wp - p0)
dot = direc.dot(np.array([0, 1]))
vcost = abs(dot)
return l, w, vcost
def cart2sph(x, y, z):
"""
Cartesian coordinates to spherical polar coordinates
Returns r,fi (azimuth),teta (inclination, not elevation, ie,
not latitude)
"""
if not isarray(x):
x = np.array([x])
y = np.array([y])
z = np.array([z])
r = 0.0 * x
teta = 0.0 * x
fi = 0.0 * x
r = np.sqrt(x ** 2 + y ** 2 + z ** 2)
teta[r != 0] = np.arccos(z[r != 0] / r[r != 0])
rr = np.sqrt(x ** 2 + y ** 2)
c1 = (y >= 0) & (rr != 0)
c2 = (y < 0) & (rr != 0)
fi[c1] = np.arccos(x[c1] / rr[c1]) # y>=0 & rr!=0
fi[c2] = 2 * np.pi - np.arccos(x[c2] / rr[c2]) # y<0 & rr!=0
return r, fi, teta
def PlotEccOrbit_aRs(par,t):
"""Function to plot planet orbit in 3D"""
#read in parameters
T0,P,a_Rstar,p,b,c1,c2,e,w,foot,Tgrad,Sec_depth = par
#ensure b and p >= 0
if b<0.: b=-b
if p<0.: p=-p
w *= np.pi / 180.
i = np.arccos(b/a_Rstar)
#make w lie in range 0-2pi
if w >= 2*np.pi:
w -= 2*np.pi #make f lie in range 0-2pi
elif w < 0:
w += 2*np.pi #make f lie in range 0-2pi
#true anomaly of central transit time
f = 1.*np.pi/2. + w
if f >= 2*np.pi:
f -= 2*np.pi #make f lie in range 0-2pi
elif f < 0:
f += 2*np.pi #make f lie in range 0-2pi
if f < np.pi:
E = np.arccos( (np.cos(f) + e) / (e*np.cos(f)+1.) )
M_tr = E - e*np.sin(E)
T_peri = T0 + M_tr * P/(2*np.pi)
if f >= np.pi:
#f = np.pi - f #correct for acos calc
E = np.arccos( (np.cos(f) + e) / (e*np.cos(f)+1.) )
M_tr = E - e*np.sin(E)
#M_tr = 2*np.pi - M_tr
T_peri = T0 - M_tr * P/(2*np.pi)
#calculate mean anomaly
M = (2*np.pi/P) * (t - T_peri)
#get coords
x = PlanetOrbit.get_x(M,a_Rstar,e,w)
y = PlanetOrbit.get_y(M,a_Rstar,e,w,i)
z = PlanetOrbit.get_z(M,a_Rstar,e,w,i)
#make plot
ax = Axes3D(pylab.gcf())
ax.plot(x, y, z, c='k')
ax.scatter(x, y, z, c='r', s=50)
ax.scatter([0],[0],[0],c='y', s=500) #plot star position
ax.scatter([x[0],],[y[0],],[z[0],],c='g', s=100) #plot initial planet position
ax.scatter([x[1],],[y[1],],[z[1],],c='y', s=100) #plot initial planet position
ax.set_xlabel('X')
ax.set_ylabel('Y')
ax.set_zlabel('Z')
range = abs(np.array([x,y,z])).max()
ax.set_xlim3d(-range,range)
ax.set_ylim3d(-range,range)
ax.set_zlim3d(-range,range)
def compute_cd(self):
# DA is the measured sensor value
# 1) compute diagonal E (using A, D + angle DA)
# E = sqrt(A * A + D * D - 2 * A * D * cos(DA))
e = numpy.sqrt(
self.a * self.a +
self.d * self.d -
2 * self.a * self.d * cos(radians(self.da)))
# 2) compute angle ED of triangle 1 (using A, D, E)
# ED = acos((E * E + D * D - A * A) / (2 * E * D))
ed = numpy.arccos(
(e * e + self.d * self.d - self.a * self.a) /
(2 * e * self.d))
# 3) compute angle of CE of triangle 2 (using B, C, E)
# CE = acos((E * E + C * C - B * B) / (2 * E * C))
ce = numpy.arccos(
(e * e + self.c * self.c - self.b * self.b) /
(2 * e * self.c))
# 4) add angles #2 and #3
# CD = CE + ED
cd = ce + ed # radians
#e = numpy.degrees(cd) - self.cd
#print("calf link angle error: %s" % e)
# 5) compute excursion of spring using angle #4
# sqrt(F * F + G * G - 2 * F * G * cos(CD))
return cd
def circle_intersection_area(r, R, d):
'''
Formula from: http://mathworld.wolfram.com/Circle-CircleIntersection.html
Does not make sense for negative r, R or d
>>> circle_intersection_area(0.0, 0.0, 0.0)
0.0
>>> circle_intersection_area(1.0, 1.0, 0.0)
3.1415...
>>> circle_intersection_area(1.0, 1.0, 1.0)
1.2283...
'''
if np.abs(d) < tol:
minR = np.min([r, R])
return np.pi * minR**2
if np.abs(r - 0) < tol or np.abs(R - 0) < tol:
return 0.0
d2, r2, R2 = float(d**2), float(r**2), float(R**2)
arg = (d2 + r2 - R2) / 2 / d / r
arg = np.max([np.min([arg, 1.0]), -1.0]) # Even with valid arguments, the above computation may result in things like -1.001
A = r2 * np.arccos(arg)
arg = (d2 + R2 - r2) / 2 / d / R
arg = np.max([np.min([arg, 1.0]), -1.0])
B = R2 * np.arccos(arg)
arg = (-d + r + R) * (d + r - R) * (d - r + R) * (d + r + R)
arg = np.max([arg, 0])
C = -0.5 * np.sqrt(arg)
return A + B + C
def calculateDiffuseRay(self, intersectionPoint, firstGeometry):
pointNormal = firstGeometry.getNormal(intersectionPoint)
r1 = rand.random()
r2 = rand.random()
phi = 2 * np.pi * r1
theta = np.arccos(np.sqrt(r2))
# To cartesian coordinates
x = np.cos(phi) * np.sin(theta)
y = np.sin(phi) * np.sin(theta)
z = np.cos(theta)
newDirection = [x, y, z]
# Rotate new direction to distribution of normal vector
el = -1 * np.arccos(pointNormal[2])
az = -1 * np.arctan2(pointNormal[1], pointNormal[0])
rotationRay = [np.cos(el) * newDirection[0] - np.sin(el) * newDirection[2], newDirection[1], np.sin(el) * newDirection[0] + np.cos(el) * newDirection[2]]
rotationRay = [np.cos(az) * rotationRay[0] + np.sin(az) * rotationRay[1], -1 * np.sin(az) * rotationRay[0] + np.cos(az) * rotationRay[1], rotationRay[2]]
newDirectionCorrect = rotationRay / np.linalg.norm(rotationRay)
randomRay = Ray(newDirectionCorrect, intersectionPoint + (0.00001 * newDirectionCorrect))
return randomRay
def overlap(self, blob):
"""Overlap between two blobs.
Defined by the overlap area.
"""
# For now it is just the overlap area of two containment circles
# It could be replaced by the Q or C factor, which also defines
# a certain neighborhood.
d = sqrt((self.x_pos - blob.x_pos) ** 2 + (self.y_pos - blob.y_pos) ** 2)
# One circle lies inside the other
if d < abs(self.radius - blob.radius):
area = pi * min(self.radius, blob.radius) ** 2
# Circles don't overlap
elif d > (self.radius + blob.radius):
area = 0
# Compute overlap area.
# Reference: http://mathworld.wolfram.com/Circle-CircleIntersection.html (04.04.2013)
else:
term_a = blob.radius ** 2 * arccos((d ** 2 + blob.radius ** 2 - self.radius ** 2) / (2 * d * blob.radius))
term_b = self.radius ** 2 * arccos((d ** 2 + self.radius ** 2 - blob.radius ** 2) / (2 * d * self.radius))
term_c = 0.5 * sqrt(
abs(
(-d + self.radius + blob.radius)
* (d + self.radius - blob.radius)
* (d - self.radius + blob.radius)
* (d + self.radius + blob.radius)
)
)
area = term_a + term_b - term_c
return max(area / self.area(), area / blob.area())
def miso((q1, q2)):
q1 = quaternion.Quaternion(numpy.array(q1) / numpy.linalg.norm(q1)).conjugate()
q2 = quaternion.Quaternion(numpy.array(q2) / numpy.linalg.norm(q2)).conjugate()
misot = 180.0
misoa = None
for i in range(len(cubicSym)):
for ii in range(len(orthoSym)):
qa = orthoSym[ii] * q1 * cubicSym[i]
for j in range(len(cubicSym)):
#for jj in range(len(orthoSym)):
qb = q2 * cubicSym[j]
qasb1 = qa.conjugate() * qb
qasb2 = qb * qa.conjugate()
t1 = qasb1.wxyz / numpy.linalg.norm(qasb1.wxyz)
t2 = qasb2.wxyz / numpy.linalg.norm(qasb2.wxyz)
a1 = 2 * numpy.arccos(t1[0]) * 180 / numpy.pi
a2 = 2 * numpy.arccos(t2[0]) * 180 / numpy.pi
if a1 < misot:
misot = a1
misoa = qasb1
if a2 < misot:
misot = a2
misoa = qasb2
return misot
def GetOrientTransmat(self, biounit=False, target=False):
cen = np.zeros((3,1))
cenlist = self.Centroid(biounit, target)
cen[0:3] = [[cenlist[0]],[cenlist[1]],[cenlist[2]]]
tmat = translation_matrix(-self.Centroid(biounit, target))
max = 0
farthestxyz = None
for atom in self.IterAtoms(biounit, target):
dist = np.sum((atom.xyz[0:3] - cen)**2)
if dist > max:
farthestxyz = atom.xyz[0:3] - cen
max = dist
firstrotax = np.cross(farthestxyz.transpose().tolist()[0], np.array([1,0,0]))
firstrotang = np.arccos(np.dot(farthestxyz.transpose().tolist()[0], np.array([1,0,0]))/(np.sqrt(np.dot(farthestxyz.transpose().tolist()[0], farthestxyz.transpose().tolist()[0]))))
firstrotmat = rotation_matrix(firstrotang, firstrotax, self.Centroid(biounit, target))
max = 0
firsttransmat = tmat.dot(firstrotmat)
for atom in self.IterAtoms(biounit, target):
dist = sum(firsttransmat.dot(atom.xyz)[1:3]**2)
if dist > max:
secfarthestyz = firsttransmat.dot(atom.xyz)[0:3]
max = dist
secfarthestyz[0] = 0
secondrotax = np.array([1,0,0])
secondrotang = np.arccos(np.dot(secfarthestyz.transpose().tolist()[0], np.array([0,1,0]))/np.sqrt(np.dot(secfarthestyz.transpose().tolist()[0],secfarthestyz.transpose().tolist()[0])))
secondrotmat = rotation_matrix(secondrotang, secondrotax, self.Centroid(biounit, target))
return secondrotmat.dot(firsttransmat)
def get_sunset_ele(d):
if (-np.tan(get_declination_angle(d)) * np.tan(np.deg2rad(lat))) > 1.0:
return np.arccos(1.0)
elif (-np.tan(get_declination_angle(d)) * np.tan(np.deg2rad(lat))) < -1.0:
return np.arccos(-1.0)
else:
return np.arccos(-np.tan(get_declination_angle(d)) * np.tan(np.deg2rad(lat)))
def test_water_cost_angle_ic():
fn_xyz = context.get_fn('test/water_trajectory.xyz')
system = System.from_file(fn_xyz, ffatypes=['O', 'H', 'H'])
system.detect_bonds()
fn_pars = context.get_fn('test/parameters_water.txt')
parameters = Parameters.from_file(fn_pars)
del parameters.sections['FIXQ']
del parameters.sections['DAMPDISP']
del parameters.sections['EXPREP']
refpos = np.array([
[0.0, 0.0, 0.0],
[0.0, 0.0, 1.1],
[0.0, 1.1, 0.0],
])*angstrom
rules = [ScaleRule('BENDCHARM', 'PARS', 'H\s*O\s*H', 4)]
mods = [ParameterModifier(rules)]
pt = ParameterTransform(parameters, mods)
simulations = [GeoOptSimulation('only', system)]
tests = [ICTest(5*deg, refpos, simulations[0], BendGroup(system))]
assert tests[0].icgroup.cases == [[2, 0, 1]]
cost = CostFunction(pt, {'all': tests})
x = np.array([1.0])
assert abs(cost(x) - np.log(0.5*((np.arccos(2.7892000007e-02) - 1.5707963267948966)/(5*deg))**2)) < 1e-4
x = np.array([1.1])
assert abs(cost(x) - np.log(0.5*((np.arccos(1.1*2.7892000007e-02) - 1.5707963267948966)/(5*deg))**2)) < 1e-4
x = np.array([0.8])
assert abs(cost(x) - np.log(0.5*((np.arccos(0.8*2.7892000007e-02) - 1.5707963267948966)/(5*deg))**2)) < 1e-4
def findAnglesBetweenTwoVectors1(v1, v2):
v1_u = unitVector(v1)
v2_u = unitVector(v2)
return np.arccos(np.clip(np.dot(v1_u, v2_u), -1.0, 1.0))
for j in range(ny):
Bot[i, j] = [bx[i, j], by[i, j]] #only note (useless)
av = np.array([bx[i, j], by[i, j]])
Bot_mag[i, j] = np.linalg.norm(av)
Bpt[i, j] = [bxp[i, j], byp[i, j]] #only note (useless)
bv = np.array([bxp[i, j], byp[i, j]])
Bpt_mag[i, j] = np.linalg.norm(bv)
cv = np.subtract(av, bv)
Bnt_mag[i, j] = np.linalg.norm(cv)
Brt_mag[i, j] = np.sqrt((Bot_mag[i, j]**2) + (bz[i, j]**2))
#Calculate shear angle between observed and potential field
denum[i, j] = (Bot_mag[i, j] * Bpt_mag[i, j])
if denum[i, j] != 0:
cos_shear[i, j] = (av @ bv) / denum[i, j]
shear_ang[i, j] = np.arccos(cos_shear[i, j])
shear_deg[i, j] = np.math.degrees(shear_ang[i, j])
#Calculate proxy of the photospheric magnetic energy
exc_erg[i, j] = (Bnt_mag[i, j]**2) * dAr / (8 * np.math.pi)
exc_ergn = np.zeros((nx, ny), float)
for i in range(nx):
for j in range(ny - 1):
if abs(bzn[i, j]) >= 0.1:
exc_ergn[i, j] = exc_erg[i, j]
else:
exc_ergn[i, j] = 0.0
pot_erg = np.zeros((nx, ny), float)
tot_erg = np.zeros((nx, ny), float)
}
# Query user for desired number of streams:
print "2, 4, 6, 8, or 16 streams are available in the CRTM."
n_streams = raw_input("Select the number of streams: ")
selector = int(switcher.get(int(n_streams), "Invalid number of streams!"))
streams = [2,4,6,8,16]
low = selector
high = low + int(n_streams)
coeff = coeff[low:high]
reso = 1800
p = np.zeros(reso)
x = np.arange(-1,1,2./reso)
for ii in range(0,reso):
# Reconstruction of the phase function:
p[ii] = np.polynomial.legendre.legval(x[ii],coeff)
plt.figure(1)
plt.plot(180./np.pi*np.arccos(x),p)
np.savetxt("phasefunction.txt",p,newline='\n')
plt.xlabel('polar angle [$^{\circ}$ deg]', fontsize=22)
plt.ylabel('$P_{11}$', fontsize=22)
plt.grid('on')
plt.figure(2)
plt.semilogy(abs(coeff),'o-')
plt.ylabel('$|C_n|$', fontsize=22)
plt.xlabel('n', fontsize=22)
plt.show()
def get_ang_norm(self):
"""Return the angular norm, i.e. the angular rotation, of
this orientation."""
return 2 * np.arccos(self._s)
def main():
progname = os.path.basename(sys.argv[0])
usage = """prog [options] <crystal image>
Orient crystals imaged via electron microscopy.
"""
parser = EMArgumentParser(usage=usage, version=EMANVERSION)
parser.add_argument("--apix",
required=True,
type=float,
default=False,
help="Specify the Apix of your input images")
parser.add_argument(
"--params",
required=True,
type=str,
help=
"Lattice parameters separated by commas, i.e. '70.3,70.3,32.0,90.0,90.0,90.0'",
default="",
guitype='intbox',
row=11,
col=0,
rowspan=1,
colspan=1,
mode="align")
parser.add_argument(
"--slab",
type=float,
help="Specify the thickness of the central slab. Default is 10.0",
default=10.0)
parser.add_argument(
"--mindeg",
type=float,
help=
"Specify the minimum angle for initial orientation search. Default is -180.0",
default=-180.0)
parser.add_argument(
"--maxdeg",
type=float,
help=
"Specify the maximum angle for initial orientation search. Default is 180.0",
default=180.0)
parser.add_argument(
"--diameter",
type=float,
help="Specify the minimum spot diameter. Default is 5.0",
default=5.0)
parser.add_argument(
"--maxshift",
type=float,
help=
"Specify the maximum pixel shift when optimizing peak locations. Default is 32.0 pixels.",
default=32.0)
parser.add_argument(
"--exper_weight",
type=float,
help=
"Weight of penalty for spots in experimental data not found in the reference lattice. Default is 10.0.",
default=10.0)
parser.add_argument(
"--data_weight",
type=float,
help=
"Weight of penalty for points in reference lattice not found in the experimental data. Default is 1.0.",
default=1.0)
parser.add_argument(
"--plot",
default=False,
help=
"Show plot of reciprocal reference lattice points overlayed on input image and detected reflections.",
action="store_true")
parser.add_argument(
"--threads",
type=int,
help=
"Number of cores over which parallel optimization will be performed. Default is to use 1 core.",
default=1)
parser.add_argument(
"--ppid",
type=int,
help="Set the PID of the parent process, used for cross platform PPID",
default=-2)
parser.add_argument(
"--verbose",
"-v",
dest="verbose",
action="store",
metavar="n",
type=int,
default=0,
help=
"verbose level [0-9], higner number means higher level of verboseness")
(options, args) = parser.parse_args()
apix = float(options.apix)
close = options.slab
try:
params = [float(p) for p in options.params.split(",")]
a, b, c, alpha, beta, gamma = params
except:
print(
"Could not read lattice parameters. Please specify as a comma separated list containing 'a,b,c,alpha,beta,gamma'."
)
for fn in args:
try:
print(("READING {}".format(fn)))
orig = EMData(fn)
except:
print(("Could not find {}".format(fn)))
sys.exit(1)
# PREPROCESSING
nx = orig["nx"]
orig.process_inplace("normalize.edgemean")
#orig.process_inplace("filter.highpass.gauss",{"cutoff_pixels":2})
#orig.process_inplace("filter.lowpass.gauss",{"cutoff_abs":0.34})
nx = min(orig["nx"],
orig["ny"]) # clip to min x,y to obtain square image
reg = Region(0, 0, nx, nx)
orig = orig.get_clip(reg)
#orig.process_inplace("filter.highpass.gauss",{"cutoff_freq":0.01}) # remove strong signal at origin for improved peak finding
orig.process_inplace("filter.xyaxes0", {"neighbornorm": 2})
#orig.process_inplace("mask.gaussian",{"outer_radius":orig["nx"]/8}) # overly stringent apodization
#orig.process_inplace("mask.decayedge2d",{"width":nx/4}) # simple apodization
orig.process_inplace("mask.gaussian", {
"outer_radius": old_div(orig["nx"], 8),
"exponent": 3.0
})
norig = orig.numpy().copy()
fnorig = np.fft.fftshift(np.fft.fft2(np.fft.fftshift(norig)))
img = orig.process("math.realtofft") # obtain an amplitude image
img.process_inplace("normalize")
img.process_inplace("filter.lowpass.gauss",
{"cutoff_abs": 0.1}) # strong lowpass
ra = img.process("math.rotationalaverage")
img -= ra
img.process_inplace("threshold.belowtozero",
{"minval": img["mean"] + 3.0 * img["sigma"]})
#img.process_inplace("threshold.notzero")
nimg = img.numpy().copy()
print("\nDETECTING SPOTS")
# dilation of nimg with a size*size structuring element
image_max = ndi.maximum_filter(
nimg, size=np.min([a, b, c]).astype(int),
mode='constant') # measured size of spot (rough) # 30
# compare image_max and nimg to find the coordinates of local maxima
tmp = peak_local_max(
nimg, min_distance=np.max([a, b, c]).astype(int)
) # measured minimum distance from origin to first point (rough) # 50
coords = []
for coord in tmp:
if np.abs(np.linalg.norm(c - old_div(nimg.shape[0], 2.))) <= (
old_div(nx, 2.)):
coords.append(coord)
coords = np.asarray(coords)
refined_coords = refine_peaks(coords, img, options.maxshift,
options.maxshift * 2.)
ds = old_div(1, (apix * nx)) # angstroms per fourier pixel
exper_max_radius = np.linalg.norm(refined_coords - old_div(nx, 2),
axis=1).max()
print(("Highest resolution reflection: {:.2f}A ({} pix)\n".format(
old_div(1, (ds * exper_max_radius)),
int(round(exper_max_radius, 0)))))
print("DETERMINING ORIENTATION")
resolutions = np.asarray([
1000., 100., 50., 25., 20., 18., 16., 10., 8., 5., 4., 3., 2.9,
2.8, 2.7, 2.6, 2.5, 2.4, 2.3, 2.2, 2.1, 2.0, 1.9, 1.8
])
radii = [
float(r) for r in old_div(1, (resolutions * ds))
if r <= old_div(nx, 2.)
]
# initial search range
a_mindeg = options.mindeg
a_maxdeg = options.maxdeg
b_mindeg = options.mindeg
b_maxdeg = options.maxdeg
g_mindeg = options.mindeg
g_maxdeg = options.maxdeg
old_nrefs = 0.0
count = 0
for r in radii:
ang = np.arccos(np.sqrt(old_div(
(r**2 - options.diameter), r**2))) * 180. / np.pi
#max_radius = r#1/np.sin(ang)**2
#if r > nx/2: continue
max_resol = old_div(1, (r * ds))
hkl_exper = np.vstack([refined_coords[:, 1], refined_coords[:,
0]]).T
hkl_exper = (hkl_exper - np.mean(hkl_exper, axis=0))
all_exper_radii = np.linalg.norm(hkl_exper, axis=1)
hkl_exper = hkl_exper[all_exper_radii <= r]
exper_radii = np.linalg.norm(hkl_exper, axis=1)
hkl_exper = np.c_[hkl_exper, exper_radii]
if len(hkl_exper) < 2: continue
if len(hkl_exper) == old_nrefs:
continue
else:
old_nrefs = len(hkl_exper)
print((
"\nAngular step: {:.2f} degrees\tRadius: {:.2f} pixels ({:.2f} Angstroms)\t{} Reflections"
.format(ang, r, max_resol, len(hkl_exper))))
hkl_ref = generate_lattice(nx, apix, r, a, b, c, alpha, beta,
gamma)
dist_exper, idx_exper = scipy.spatial.cKDTree(
hkl_exper[:, :2]).query([0, 0], k=9)
min_distance = np.min(
[dist_exper[1], dist_exper[3], dist_exper[5], dist_exper[7]])
if count == 0:
rngs = list(
itertools.product(np.arange(a_mindeg, a_maxdeg + ang, ang),
np.arange(b_mindeg, b_maxdeg + ang, ang),
np.arange(g_mindeg, g_maxdeg + ang,
ang)))
else:
rngs = []
for s in solns:
print(s)
a_mindeg = s[0] - ang
a_maxdeg = s[0] + ang
b_mindeg = s[1] - ang
b_maxdeg = s[1] + ang
c_mindeg = s[2] - ang
c_maxdeg = s[2] + ang
rngs.extend(
list(
itertools.product(
np.arange(a_mindeg, a_maxdeg + ang, ang),
np.arange(b_mindeg, b_maxdeg + ang, ang),
np.arange(g_mindeg, g_maxdeg + ang, ang))))
count += 1
start = time.time()
resq = queue.Queue(0)
res = [0] * len(rngs)
thds = []
if options.verbose:
sys.stdout.write("\rCreating {} threads".format(len(rngs)))
for i in range(len(rngs)):
if options.verbose and i % 100 == 0:
sys.stdout.write("\rCreating {}/{} threads".format(
i + 1, len(rngs)))
thd = threading.Thread(target=cost_async,
args=(rngs[i], hkl_exper, hkl_ref,
close, old_div(min_distance, 10.),
options.exper_weight,
options.data_weight, i, resq))
thds.append(thd)
t0 = time.time()
if options.verbose: sys.stdout.flush()
minval = np.inf
thrtolaunch = 0
while thrtolaunch < len(thds) or threading.active_count() > 1:
if thrtolaunch < len(thds):
while (threading.active_count() == options.threads):
time.sleep(.1)
if options.verbose and (thrtolaunch % 100 == 0
or len(thds) - thrtolaunch < 5):
sys.stdout.write(
"\rSearched {}/{} orientations".format(
thrtolaunch + 1, len(thds)))
thds[thrtolaunch].start()
thrtolaunch += 1
else:
time.sleep(0.5)
while not resq.empty():
i, cx = resq.get()
if cx < minval: minval = cx
res[i] = cx
for th in thds:
th.join()
solns = [rngs[i] for i, v in enumerate(res) if v == minval]
sys.stdout.write("\t\t\tFound {} solutions:".format(len(solns)))
print(solns)
sys.stdout.flush()
print("\n\nREFINING PARAMETERS")
best_cost = np.inf
scost = best_cost
best_orient = None
hkl_exper = np.vstack([refined_coords[:, 1], refined_coords[:, 0]]).T
hkl_exper = (hkl_exper - np.mean(hkl_exper, axis=0))
all_exper_radii = np.linalg.norm(hkl_exper, axis=1)
hkl_exper = hkl_exper[all_exper_radii <= exper_max_radius]
exper_radii = np.linalg.norm(hkl_exper, axis=1)
hkl_exper = np.c_[hkl_exper, exper_radii]
hkl_ref = generate_lattice(nx, apix, exper_max_radius, a, b, c, alpha,
beta, gamma)
for ii, soln in enumerate(solns):
hkl_ref = generate_lattice(nx, apix, exper_max_radius, a, b, c,
alpha, beta, gamma)
refine1 = optimize.fmin(cost,
soln,
args=(
hkl_exper,
hkl_ref,
close,
old_div(min_distance, 10.0),
options.data_weight,
options.exper_weight,
),
disp=False)
az, alt, phi = refine1[0], refine1[1], refine1[2]
refine_apix = optimize.fmin(apix_cost, [apix],
args=(
az,
alt,
phi,
hkl_exper,
hkl_ref,
close,
16.,
nx,
exper_max_radius,
options.data_weight,
options.exper_weight,
a,
b,
c,
alpha,
beta,
gamma,
),
disp=False)
refine_apix = float(refine_apix[0]) #float(refine_apix.x)
hkl_ref = generate_lattice(nx, refine_apix, exper_max_radius, a, b,
c, alpha, beta, gamma)
ds = old_div(1, (refine_apix * nx)) # angstroms per fourier pixel
refine_close = optimize.fmin(close_cost, [close],
args=(
az,
alt,
phi,
hkl_exper,
hkl_ref,
8.,
5.0,
options.data_weight,
options.exper_weight,
),
disp=False)
refine_close = refine_close[0]
if refine_close <= 1.0: refine_close = close
refine2 = optimize.fmin(cost,
refine1,
args=(
hkl_exper,
hkl_ref,
refine_close,
old_div(min_distance, 10.0),
options.data_weight,
options.exper_weight,
),
disp=False) # re-refine orientation
scost = cost(refine2, hkl_exper, hkl_ref, refine_close,
min_distance, options.data_weight,
options.exper_weight)
if scost < best_cost:
best_cost = scost
best_orient = refine2
best_refine_apix = refine_apix
best_refine_close = refine_close
sys.stdout.flush()
ds = old_div(1, (best_refine_apix * nx)) # angstroms per fourier pixel
print(("Refined Apix: {:.2f} -> {:.2f}".format(apix,
best_refine_apix)))
print(("Refined thickness: {:.2f} -> {:.2f}".format(
close, best_refine_close)))
print(("Refined orientation: ({:.2f},{:.2f},{:.2f})\n".format(
*best_orient)))
hkl_ref = generate_lattice(nx, refine_apix, exper_max_radius, a, b, c,
alpha, beta, gamma)
pln = get_plane(best_orient, hkl_ref, close=best_refine_close)
pln = pln[np.argsort(pln[:, 3])] # sort by radius
if options.plot:
plt.imshow(nimg, origin="lower", cmap=plt.cm.Greys_r)
plt.scatter(hkl_exper[:, 1] + old_div(nx, 2),
hkl_exper[:, 0] + old_div(nx, 2),
c='b',
marker='x')
plt.scatter(pln[:, 1] + old_div(nx, 2),
pln[:, 0] + old_div(nx, 2),
c='r',
marker='x')
plt.axis("off")
plt.title("(Az, Alt, Phi) -> ({:.2f},{:.2f},{:.2f})".format(
*best_orient))
plt.show()
print(
" xc yc zc r resol h k l raw_F raw_p"
)
with open("{}.sf".format(fn.split(".")[0]),
"w") as sf: # create a quasi.sf file for this image
for nrow, row in enumerate(pln):
xc, yc, zc, r, h, k, l = row[:7]
if r > 0: resol = old_div(1, (r * ds))
else: resol = "inf"
if nrow in range(9):
raw_F, raw_p = get_sf(fnorig,
int(xc) + old_div(nx, 2),
int(yc) + old_div(nx, 2),
2) #,show=True)
else:
raw_F, raw_p = get_sf(fnorig,
int(xc) + old_div(nx, 2),
int(yc) + old_div(nx, 2),
2) #,show=False)
try:
print((
"{:8.1f},{:8.1f},{:8.1f} {:6.1f} {:6.1f} {:4d} {:4d} {:4d} {:8.2f} {:8.2f}"
.format(xc, yc, zc, r, resol, int(h), int(k), int(l),
raw_F, raw_p)))
except:
print((
"{:8.1f},{:8.1f},{:8.1f} {:6.1f} inf {:4d} {:4d} {:4d} {:.2f} {:.2f}"
.format(xc, yc, zc, r, int(h), int(k), int(l), raw_F,
raw_p)))
sf.write("{}\t{}\t{}\t{}\t{}\t{}\t{}\n".format(
h, k, l, raw_F, raw_p, r, resol))
def perturb(self, params):
"""
Unlike in C++, this takes a numpy array of parameters as input,
and modifies it in-place. The return value is still logH.
"""
logH = 0.0
reps = 1;
if(rng.rand() < 0.5):
reps += np.int(np.power(100.0, rng.rand()));
# print "going to perturb %d reps" % reps
for i in range(reps):
# print " rep iteration %d" % i
which = rng.randint(len(params))
if which == 0:
rad_idx = 0
theta_idx = 2
theta = params[theta_idx]
#FIND THE MAXIMUM RADIUS STILL INSIDE THE DETECTOR
theta_eq = np.arctan(detector.detector_length/detector.detector_radius)
theta_taper = np.arctan(detector.taper_length/detector.detector_radius)
# print "theta: %f pi" % (theta / np.pi)
if theta <= theta_taper:
z = np.tan(theta)*(detector.detector_radius - detector.taper_length) / (1-np.tan(theta))
max_rad = z / np.sin(theta)
elif theta <= theta_eq:
max_rad = detector.detector_radius / np.cos(theta)
# print "max rad radius: %f" % max_rad
else:
theta_comp = np.pi/2 - theta
max_rad = detector.detector_length / np.cos(theta_comp)
# print "max rad length: %f" % max_rad
#AND THE MINIMUM (from PC dimple)
#min_rad = 1./ ( np.cos(theta)**2/detector.pcRad**2 + np.sin(theta)**2/detector.pcLen**2 )
min_rad = np.amax([detector.pcRad, detector.pcLen])
total_max_rad = np.sqrt(detector.detector_length**2 + detector.detector_radius**2 )
params[which] += total_max_rad*dnest4.randh()
params[which] = dnest4.wrap(params[which] , min_rad, max_rad)
elif which ==2: #theta
rad_idx = 0
rad = params[rad_idx]
# print "rad: %f" % rad
if rad < np.amin([detector.detector_radius - detector.taper_length, detector.detector_length]):
max_val = np.pi/2
min_val = 0
# print "theta: min %f pi, max %f pi" % (min_val, max_val)
else:
if rad < detector.detector_radius - detector.taper_length:
#can't possibly hit the taper
# print "less than taper adjustment"
min_val = 0
elif rad < np.sqrt(detector.detector_radius**2 + detector.taper_length**2):
#low enough that it could hit the taper region
# print "taper adjustment"
a = detector.detector_radius - detector.taper_length
z = 0.5 * (np.sqrt(2*rad**2-a**2) - a)
min_val = np.arcsin(z/rad)
else:
#longer than could hit the taper
# print " longer thantaper adjustment"
min_val = np.arccos(detector.detector_radius/rad)
if rad < detector.detector_length:
max_val = np.pi/2
else:
max_val = np.pi/2 - np.arccos(detector.detector_length/rad)
# print "theta: min %f pi, max %f pi" % (min_val, max_val)
params[which] += np.pi/2*dnest4.randh()
params[which] = dnest4.wrap(params[which], min_val, max_val)
# if which == 0:
# params[which] += (detector.detector_radius)*dnest4.randh()
# params[which] = dnest4.wrap(params[which] , 0, detector.detector_radius)
elif which == 1:
max_val = np.pi/4
params[which] += np.pi/4*dnest4.randh()
params[which] = dnest4.wrap(params[which], 0, max_val)
if params[which] < 0 or params[which] > np.pi/4:
print "wtf phi"
#params[which] = np.clip(params[which], 0, max_val)
# elif which == 2:
# params[which] += (detector.detector_length)*dnest4.randh()
# params[which] = dnest4.wrap(params[which] , 0, detector.detector_length)
elif which == 3: #scale
min_scale = wf.wfMax - 0.01*wf.wfMax
max_scale = wf.wfMax + 0.005*wf.wfMax
params[which] += (max_scale-min_scale)*dnest4.randh()
params[which] = dnest4.wrap(params[which], min_scale, max_scale)
# print " adjusted scale to %f" % ( params[which])
elif which == 4: #t0
params[which] += 1*dnest4.randh()
params[which] = dnest4.wrap(params[which], min_maxt, max_maxt)
elif which == 5: #smooth
params[which] += 0.1*dnest4.randh()
params[which] = dnest4.wrap(params[which], 0, 25)
# print " adjusted smooth to %f" % ( params[which])
# elif which == 6: #wf baseline slope (m)
# logH -= -0.5*(params[which]/1E-4)**2
# params[which] += 1E-4*dnest4.randh()
# logH += -0.5*(params[which]/1E-4)**2
# elif which == 7: #wf baseline incercept (b)
# logH -= -0.5*(params[which]/1E-2)**2
# params[which] += 1E-2*dnest4.randh()
# logH += -0.5*(params[which]/1E-2)**2
# params[which] += 0.01*dnest4.randh()
# params[which]=dnest4.wrap(params[which], -1, 1)
# print " adjusted b to %f" % ( params[which])
else: #velocity or rc params: cant be below 0, can be arb. large
print "which value %d not supported" % which
exit(0)
return logH
return (-np.sort(-input, axis=-1)[..., :k], (n - (np.argsort(
input[..., ::-1], kind='stable', axis=-1)[..., ::-1]))[..., :k])
# --- Begin Public Functions --------------------------------------------------
abs = utils.copy_docstring( # pylint: disable=redefined-builtin
tf.math.abs,
lambda x, name=None: np.abs(x))
accumulate_n = utils.copy_docstring(
tf.math.accumulate_n,
lambda inputs, shape=None, tensor_dtype=None, name=None: ( # pylint: disable=g-long-lambda
sum(map(np.array, inputs)).astype(utils.numpy_dtype(tensor_dtype))))
acos = utils.copy_docstring(tf.math.acos, lambda x, name=None: np.arccos(x))
acosh = utils.copy_docstring(tf.math.acosh, lambda x, name=None: np.arccosh(x))
add = utils.copy_docstring(tf.math.add, lambda x, y, name=None: np.add(x, y))
add_n = utils.copy_docstring(
tf.math.add_n, lambda inputs, name=None: sum(map(np.array, inputs)))
angle = utils.copy_docstring(tf.math.angle,
lambda input, name=None: np.angle(input))
argmax = utils.copy_docstring(
tf.math.argmax,
lambda input, axis=None, output_type=tf.int64, name=None: ( # pylint: disable=g-long-lambda
np.argmax(input, axis=0 if axis is None else _astuple(axis)).astype(
def three_point_correlation_function(coord0,
coord1,
coord2,
nbins=(100, 100, 100),
histrange=[(0, 200), (0, 200), (0, 200)],
triplet_to_calculate="DDD"):
# For debugging
#hist = np.histogram(coord0.transpose()[0], bins=nbins, range=histrange)
#hist_tot = hist[0]
#bin_edges = hist[1]
#return hist_tot,bin_edges
# Assume the data is coming in ngals x 3 arrays
# x, y, z (all in Mpc)
# For example,
# [ [ 1253.0, 2384.4, 3425.24],
# [ 1987.5, 2564.7, 2439.42],
# ......................... ]
#print("Ngals: %d %d" % (len(coord0), len(coord1)))
nc0 = len(coord0)
nc1 = len(coord1)
nc2 = len(coord2)
print("sizes: ", nc0, nc1, nc2)
hist_tot = np.zeros(nbins, dtype=int)
bin_edges = None
triangles = []
for i in range(nc0):
c0 = coord0[i]
if i % 10 == 0:
print("Outermost loop {0} of {1}".format(i, nc0))
lo1 = 0
if triplet_to_calculate=="DDD" or \
triplet_to_calculate=="DDR" or \
triplet_to_calculate=="RRR":
lo1 = i + 1
for j in range(lo1, nc1):
c1 = coord1[j]
lo2 = 0
if triplet_to_calculate=="DDD" or \
triplet_to_calculate=="DRR" or \
triplet_to_calculate=="RRR":
lo2 = j + 1
for k in range(lo2, nc2):
c2 = coord2[k]
#print(i,j,k)
#print(c0,c1,c2)
r01 = distance(c0, c1)
r02 = distance(c0, c2)
r12 = distance(c1, c2)
# From Fig. 6
# https://arxiv.org/pdf/astro-ph/0403638.pdf
sides = np.sort([r01, r02, r12])
r01 = sides[0]
r02 = sides[1]
r12 = sides[2]
#print("sides")
#print(sides)
s = r01
q = r02 / r01
theta = np.arccos(
(r01 * r01 + r02 * r02 - r12 * r12) / (2 * r01 * r02))
theta /= PI
#print([s,q,theta])
triangles.append([s, q, theta])
triangles = np.array(triangles)
print(len(triangles))
H, edges = np.histogramdd(triangles, bins=nbins, range=histrange)
return H, edges
def d2z(d):
phi = np.arccos(d2z_p_2 - d2z_p_3 * h_0 * d / 1.0e6)
return d2z_p_0 * np.cos((phi + 4.0 * np.pi) / 3.0) + d2z_p_1
F = np.array(fList)
N = pList
Ttotal = np.sum(T, 0)
Ttotal[0] = Ttotal[2] = 0
Ftotal = np.sum(F, 0)
Ftotal[2] -= G
Ftotal[1] = 0
print(beta)
if(i == 0.06) :
plt.scatter(N[:, 0], N[:, 1])
plt.scatter(N[4, 0], N[4, 1])
plt.grid()
plt.show()
sita = np.arccos(n[2])
print(sita * 180 / np.pi)
def SO3LogUp(rotation):
psi = np.arccos((np.trace(rotation) - 1) / 2)
return psi * np.array(rotation - rotation.T) / (2 * np.sin(psi))
def angular_distance(coord0,
coord1,
nbins=100,
histrange=(0, 200),
log_scale=False,
same_coords=False,
verbose=False):
# Data is coming in as [ [xxx, xxx, xxx], ...]
# and is in degrees
coord0_T = coord0.transpose()
ra0 = np.deg2rad(coord0_T[0])
dec0 = np.deg2rad(coord0_T[1])
coord1_T = coord1.transpose()
ra1 = np.deg2rad(coord1_T[0])
dec1 = np.deg2rad(coord1_T[1])
cosdec0 = np.cos(dec0)
cosdec1 = np.cos(dec1)
sindec0 = np.sin(dec0)
sindec1 = np.sin(dec1)
#hist_bins_log = []
#hist_bins_log += np.linspace(0.001,0.009,9).tolist()
#hist_bins_log += np.linspace(0.01,0.09,9).tolist()
#hist_bins_log += np.linspace(0.1,0.9,9).tolist()
#hist_bins_log += np.linspace(1.,10,10).tolist()
hist_bins_log = np.logspace(np.log10(0.005), np.log10(10.0), 31)
if log_scale == True:
nbins = len(hist_bins_log) - 1
#nbins = len(hist_bins_log)
hist_tot = np.zeros(nbins, dtype=int)
bin_edges = None
#print("HEREREERE")
#print(hist_bins_log)
#exit()
ngals0 = len(ra0)
for i in range(0, ngals0):
#for i,(s,c,r) in enumerate(zip(sindec0,cosdec0,ra0)):
#print(i,s,c,r)
s = sindec0[i]
c = cosdec0[i]
r = ra0[i]
if verbose:
if i % 1000 == 0:
print(i)
cos_ang_dist = None
if same_coords == False:
cos_ang_dist = s * sindec1 + c * cosdec1 * np.cos(r - ra1)
else:
cos_ang_dist = s * sindec1[i + 1:] + c * cosdec1[i + 1:] * np.cos(
r - ra1[i + 1:])
ang_dist = np.rad2deg(np.arccos(cos_ang_dist)) # Convert to degrees
if log_scale == False:
hist = np.histogram(ang_dist, bins=nbins, range=histrange)
else:
hist = np.histogram(ang_dist, bins=hist_bins_log)
hist_tot += hist[0]
bin_edges = hist[1]
return hist_tot, bin_edges
def compute_angle(phi1, phi2): dot = np.sum(phi1*phi2) / (np.linalg.norm(phi1) * np.linalg.norm(phi2)) angle = np.arccos(dot) * 180 / np.pi return 0 if np.isnan(angle) else angle
def SO3Log(rotation):
psi = np.arccos((np.trace(rotation) - 1) / 2)
return psi * np.array([rotation[2,1] - rotation[1,2], rotation[0,2] - rotation[2,0], rotation[1,0] - rotation[0,1]]) / (2 * np.sin(psi))
def evaluatePlanes(planes,
filename=None,
depths=None,
normals=None,
invalidMask=None,
outputFolder=None,
outputIndex=0,
colorMap=None):
if filename != None:
if 'mlt' not in filename:
filename = filename.replace('color', 'mlt')
pass
normalFilename = filename.replace('mlt', 'norm_camera')
normals = np.array(PIL.Image.open(normalFilename)).astype(
np.float) / 255 * 2 - 1
norm = np.linalg.norm(normals, 2, 2)
for c in range(3):
normals[:, :, c] /= norm
continue
depthFilename = filename.replace('mlt', 'depth')
depths = np.array(PIL.Image.open(depthFilename)).astype(
np.float) / 1000
# if len(depths.shape) == 3:
# depths = depths.mean(2)
# pass
maskFilename = filename.replace('mlt', 'valid')
invalidMask = np.array(PIL.Image.open(maskFilename))
invalidMask = invalidMask < 128
invalidMask += depths > 10
pass
height = normals.shape[0]
width = normals.shape[1]
focalLength = 517.97
urange = np.arange(width).reshape(1, -1).repeat(height, 0) - width * 0.5
vrange = np.arange(height).reshape(-1, 1).repeat(width, 1) - height * 0.5
ranges = np.array(
[urange / focalLength,
np.ones(urange.shape), -vrange / focalLength]).transpose([1, 2, 0])
X = depths / focalLength * urange
Y = depths
Z = -depths / focalLength * vrange
d = -(normals[:, :, 0] * X + normals[:, :, 1] * Y + normals[:, :, 2] * Z)
normalDotThreshold = np.cos(np.deg2rad(30))
distanceThreshold = 50000
reconstructedNormals = np.zeros(normals.shape)
reconstructedDepths = np.zeros(depths.shape)
segmentationImage = np.zeros((height, width, 3))
distanceMap = np.ones((height, width)) * distanceThreshold
occupancyMask = np.zeros((height, width)).astype(np.bool)
segmentationTest = np.zeros((height, width))
y = 297
x = 540
for planeIndex, plane in enumerate(planes):
planeD = np.linalg.norm(plane)
planeNormal = -plane / planeD
normalXYZ = np.dot(ranges, planeNormal)
normalXYZ = np.reciprocal(normalXYZ)
planeY = -normalXYZ * planeD
distance = np.abs(planeNormal[0] * X + planeNormal[1] * Y +
planeNormal[2] * Z + planeD) / np.abs(
np.dot(normals, planeNormal))
#distance = np.abs(planeY - depths)
mask = (distance < distanceMap) * (planeY > 0) * (np.abs(
np.dot(normals, planeNormal)) > normalDotThreshold) * (
np.abs(planeY - depths) < 0.5)
occupancyMask += mask
reconstructedNormals[mask] = planeNormal
#if planeNormal[2] > 0.9:
#print(planeD)
#print(planeNormal)
# minDepth = depths.min()
# maxDepth = depths.max()
# print(depths[300][300])
# print(planeY[300][300])
# print(depths[350][350])
# print(planeY[350][350])
# PIL.Image.fromarray((np.maximum(np.minimum((planeY - minDepth) / (maxDepth - minDepth), 1), 0) * 255).astype(np.uint8)).save(outputFolder + '/plane.png')
# exit(1)
#pass
reconstructedDepths[mask] = planeY[mask]
if colorMap != None and planeIndex in colorMap:
segmentationImage[mask] = colorMap[planeIndex]
else:
segmentationImage[mask] = np.random.randint(255, size=(3, ))
pass
distanceMap[mask] = distance[mask]
segmentationTest[mask] = planeIndex + 1
#print((planeIndex, planeY[y][x], distance[y][x], np.abs(np.dot(normals, planeNormal))[y][x]))
continue
# print(distanceMap.mean())
# print(distanceMap.max())
# print(np.abs(reconstructedDepths - depths)[occupancyMask].max())
# print(pow(reconstructedDepths - depths, 2)[True - invalidMask].mean())
# exit(1)
# planeIndex = segmentationTest[y][x]
# print(normals[y][x])
# plane = planes[int(planeIndex)]
# planeD = np.linalg.norm(plane)
# planeNormal = -plane / planeD
# print((planeNormal, planeD))
# print(depths[y][x])
# print(reconstructedDepths[y][x])
# print(segmentationTest[y][x])
if outputFolder != None:
depths[invalidMask] = 0
normals[invalidMask] = 0
reconstructedDepths[invalidMask] = 0
reconstructedNormals[invalidMask] = 0
minDepth = depths.min()
maxDepth = depths.max()
#print(minDepth)
#print(maxDepth)
PIL.Image.fromarray(
((depths - minDepth) / (maxDepth - minDepth) * 255).astype(
np.uint8)).save(outputFolder + '/' + str(outputIndex) +
'_depth.png')
PIL.Image.fromarray((np.maximum(
np.minimum(
(reconstructedDepths - minDepth) /
(maxDepth - minDepth), 1), 0) * 255).astype(
np.uint8)).save(outputFolder + '/' + str(outputIndex) +
'_depth_reconstructed.png')
#PIL.Image.fromarray((np.maximum(np.minimum((reconstructedDepths - depths) / (distanceThreshold), 1), 0) * 255).astype(np.uint8)).save(outputFolder + '/depth_' + str(outputIndex) + '_diff.png')
PIL.Image.fromarray(((normals + 1) / 2 * 255).astype(
np.uint8)).save(outputFolder + '/' + str(outputIndex) +
'_normal_.png')
PIL.Image.fromarray(((reconstructedNormals + 1) / 2 * 255).astype(
np.uint8)).save(outputFolder + '/' + str(outputIndex) +
'_normal_reconstructed.png')
PIL.Image.fromarray(segmentationImage.astype(
np.uint8)).save(outputFolder + '/' + str(outputIndex) +
'_plane_segmentation.png')
#depthImage = ((depths - minDepth) / (maxDepth - minDepth) * 255).astype(np.uint8)
#PIL.Image.fromarray((invalidMask * 255).astype(np.uint8)).save(outputFolder + '/mask.png')
#exit(1)
else:
occupancy = (occupancyMask > 0.5).astype(
np.float32).sum() / (1 - invalidMask).sum()
invalidMask += np.invert(occupancyMask)
#PIL.Image.fromarray(invalidMask.astype(np.uint8) * 255).save(outputFolder + '/mask.png')
reconstructedDepths = np.maximum(np.minimum(reconstructedDepths, 10),
0)
depthError = pow(reconstructedDepths - depths,
2)[np.invert(invalidMask)].mean()
#depthError = distanceMap.mean()
normalError = np.arccos(
np.maximum(
np.minimum(np.sum(reconstructedNormals * normals, 2), 1),
-1))[np.invert(invalidMask)].mean()
#normalError = pow(np.linalg.norm(reconstructedNormals - normals, 2, 2), 2)[True - invalidMask].mean()
#print((depthError, normalError, occupancy))
# print(depths.max())
# print(depths.min())
# print(reconstructedDepths.max())
# print(reconstructedDepths.min())
# print(occupancy)
# exit(1)
#reconstructedDepths[np.invert(occupancyMask)] = depths[np.invert(occupancyMask)]
return depthError, normalError, occupancy, segmentationTest, reconstructedDepths, occupancyMask
return
R_p = D_p / 2 # [m]. Propeller disk radius
S_p = np.pi * R_p**2 # [m^2]. Propeller disk area
T_cruise = 10 # [N]. Propeller thrust during cruise
T_VTOL = 10 # [N]. Propeller thrust during VTOL
N_p = 4 # [-]. Amount of propellers
omega_cruise = 60 # [rad/s]. Propeller angular velocity during cruise
omega_VTOL = 60 # [rad/s]. Propeller angular velocity during VTOL
# Wing discretization
N = 1000 # [-]. Number of spanwise wing stations.
K = 100 # [-]. Number of Fourier modes used. N>K for a solvable system
alpha_fly = 2 # [deg]. Geometric angle of attack.
dy = b / N # [m]. Width of panels
y = np.linspace(-b / 2 + dy / 2, b / 2 - dy / 2,
N) # [-]. Control point locations on mid-panel
theta = np.arccos(-2 * y / b) # [-]. Coordinate transformation
# Defining and computing the axial velocity induced by the propeller.
def v_axial_propeller(V_0, T, rho, S_p):
v_a = 0.5 * (-V_0 + np.sqrt(V_0**2 + 2 * T /
(rho * S_p))) #Equation A.29 PhD Veldhuis
return v_a
v_a_cruise = v_axial_propeller(V_cruise, T_cruise, rho_cruise, S_p)
v_a_stall = v_axial_propeller(V_stall, T_VTOL, rho_stall, S_p)
v_a_VTOL = v_axial_propeller(V_VTOL, T_VTOL, rho_VTOL, S_p)
# Defining and computing the radial/swirl velocity induced by the propellers
x2Sum = x2Sum + (x*x)
y2Sum = y2Sum + (y*y)
xySum = xySum + (x*y)
volume = volume + area
radius = math.sqrt(area/pi)
if area > 0:
xCom = xSum / area
yCom = ySum / area
x2Com = x2Sum / area
y2Com = y2Sum / area
xyCom = xySum / area
arr = scipy.array([[ x2Com - (xCom * xCom), xyCom - (xCom * yCom)],[ xyCom - (xCom * yCom) , y2Com - (yCom * yCom) ]])
vals, vecs = scipy.linalg.eigh(arr)
#print vecs.shape
#print vecs
#print vecs[0,1]
semimajor = math.sqrt(abs(vals[0])) * 2.0
semiminor = math.sqrt(abs(vals[1])) * 2.0
orientation = numpy.arccos(vecs[0,1]) * (180 / pi)
file.write('%i, %i, %i, %.3f, %i, %i, %.3f, %.3f, %.2f' % (slices, area, volume, radius, xCom, yCom, semimajor, semiminor, orientation))
file.write('\n')
file.close
print slices, area, volume, radius, xCom, yCom, semimajor, semiminor, orientation
# TO Do
# im.getbox()
# Multiprocessing
#
def angleToVector(self, vector):
v0 = numpy.array(self._data, dtype=numpy.float64, copy=False)
v1 = numpy.array(vector.getData(), dtype=numpy.float64, copy=False)
dot = numpy.sum(v0 * v1)
dot /= self._normalizeVector(v0) * self._normalizeVector(v1)
return numpy.arccos(numpy.fabs(dot))
def calc_ik(self, tcp_pose, current_joint_pos):
a1 = self.link_param[0]
a2 = self.link_param[1]
b = self.link_param[2]
c1 = self.link_param[3]
c2 = self.link_param[4]
c3 = self.link_param[5]
c4 = self.link_param[6]
# 把持しているワークの座標を被Work座標からRobot座標への変換もやってる
wrist_pos, wrist_orn_m = self._calc_wrist_pose(tcp_pose=tcp_pose)
# A.
c0 = np.array(wrist_pos)
nx1 = np.sqrt(c0[0] ** 2 + c0[1] ** 2) - a1
s1_sq = nx1 ** 2 + (c0[2] - c1) ** 2
s2_sq = (nx1 + 2 * a1) ** 2 + (c0[2] - c1) ** 2
k_sq = a2 ** 2 + c3 ** 2
# B.1(J1)
q1_ = []
q1_.append(np.arctan2(c0[1], c0[0]))
if (q1_[0] < 0):
q1_.append(np.arctan2(c0[1], c0[0]) + np.pi)
else:
q1_.append(np.arctan2(c0[1], c0[0]) - np.pi)
q1_idx = self.getNearestValue(q1_, current_joint_pos[0])
q1 = q1_[q1_idx]
# B.2(J2)
q2_ = []
if q1_idx == 0:
tmp = (s1_sq + c2 ** 2 - k_sq) / (2 * np.sqrt(s1_sq) * c2)
if abs(tmp) > 1:
return current_joint_pos, False
q2_.append(- np.arccos(tmp) + np.arctan2(nx1, c0[2] - c1) - np.pi / 2)
q2_.append(np.arccos(tmp) + np.arctan2(nx1, c0[2] - c1) - np.pi / 2)
else:
tmp = (s2_sq + c2 ** 2 - k_sq) / (2 * np.sqrt(s2_sq) * c2)
if abs(tmp) > 1:
return current_joint_pos, False
q2_.append(- np.arccos(tmp) - np.arctan2(nx1 + 2 * a1, c0[2] - c1) - np.pi / 2)
q2_.append(np.arccos(tmp) - np.arctan2(nx1 + 2 * a1, c0[2] - c1) - np.pi / 2)
q2_idx = self.getNearestValue(q2_, current_joint_pos[1])
q2 = q2_[q2_idx]
# B.3(J3)
q3_ = []
if q1_idx == 0:
tmp = (s1_sq - c2 ** 2 - k_sq) / (2 * c2 * np.sqrt(k_sq))
if abs(tmp) > 1:
return current_joint_pos, False
q3_.append(np.arccos(tmp) - np.arctan2(a2, c3) + np.pi / 2)
q3_.append(- np.arccos(tmp) - np.arctan2(a2, c3) + np.pi / 2)
else:
tmp = (s2_sq - c2 ** 2 - k_sq) / (2 * c2 * np.sqrt(k_sq))
if abs(tmp) > 1:
return current_joint_pos, False
q3_.append(np.arccos(tmp) - np.arctan2(a2, c3) + np.pi / 2)
q3_.append(- np.arccos(tmp) - np.arctan2(a2, c3) + np.pi / 2)
q3 = q3_[q2_idx]
# C.
e11 = wrist_orn_m[0][0]
e12 = wrist_orn_m[0][1]
e13 = wrist_orn_m[0][2]
e21 = wrist_orn_m[1][0]
e22 = wrist_orn_m[1][1]
e23 = wrist_orn_m[1][2]
e31 = wrist_orn_m[2][0]
e32 = wrist_orn_m[2][1]
e33 = wrist_orn_m[2][2]
s1p = np.sin(q1)
s23p = np.sin(q2 + q3)
c1p = np.cos(q1)
c23p = np.cos(q2 + q3)
mp = e13 * s23p * c1p + e23 * s23p * s1p + e33 * c23p
# D.1(J4)
q4_p = np.arctan2(e23 * c1p - e13 * s1p, e13 * c23p * c1p + e23 * c23p * s1p - e33 * s23p)
if abs(current_joint_pos[3] - q4_p) > np.pi * 1.9:
if q4_p > 0:
q4_p = -np.pi * 2.0 + q4_p
else:
q4_p = np.pi * 2.0 + q4_p
if q4_p > 0:
q4_q = q4_p - np.pi
elif q4_p <= 0:
q4_q = q4_p + np.pi
# D.2(J5)
q5_p = np.arctan2(np.sqrt(1 - mp ** 2), mp)
q5_q = - q5_p
# D.3(J6)
q6_p = np.arctan2(e12 * s23p * c1p + e22 * s23p * s1p + e32 * c23p,
-e11 * s23p * c1p - e21 * s23p * s1p - e31 * c23p)
if abs(current_joint_pos[5] - q6_p) > np.pi * 1.9:
if q6_p > 0:
q6_p = -np.pi * 2.0 + q6_p
else:
q6_p = np.pi * 2.0 + q6_p
if q6_p > 0:
q6_q = q6_p - np.pi
elif q6_p <= 0:
q6_q = q6_p + np.pi
# E.
if abs(current_joint_pos[3] - q4_p) + abs(current_joint_pos[5] - q6_p) <= \
abs(current_joint_pos[3] - q4_q) + abs(current_joint_pos[5] - q6_p):
q4 = q4_p
q5 = q5_p
q6 = q6_p
q4_idx = 0
else:
q4 = q4_q
q5 = q5_q
q6 = q6_q
q4_idx = 1
if abs(q4) > np.pi * (190.0/180.0):
return current_joint_pos, False
return [q1, q2, q3, q4, q5, q6], True
def angle_between_vectors(v1, v2):
""" Compute the angle (in rad) between the two vectors v1 and v2. """
v1_u = v1 / np.linalg.norm(v1)
v2_u = v2 / np.linalg.norm(v2)
return np.arccos(np.clip(np.dot(v1_u, v2_u), -1.0, 1.0))
def specific_atom_centric(structure, atom1, atom2, atom3, radius):
point = args.point
if not point == None:
site_search = struct.get_sites_in_sphere(point,
include_image=True,
r=args.radius)
sites_init = [
i[0].coords for i in site_search
if i[0].as_dict()['species'][0]['element'] == atom1
]
sites_init_frac = [
i[0].frac_coords for i in site_search
if i[0].as_dict()['species'][0]['element'] == atom1
]
else:
sites_init = [
np.array(x['xyz']) for x in struct.as_dict()['sites']
if x['species'][0]['element'] == atom1
]
sites_init_frac = [
np.array(x['abc']) for x in struct.as_dict()['sites']
if x['species'][0]['element'] == atom1
]
total_data = []
for i, site in enumerate(sites_init):
def second_site_search(site1, new_radius):
second_sites = struct.get_sites_in_sphere(site1,
include_image=True,
r=new_radius)
new_second_sites = []
new_second_sites_frac = []
for x in second_sites:
if x[0].as_dict()['species'][0]['element'] == atom2:
if not np.array_equal(x[0].coords, site1):
new_second_sites.append(x[0].coords)
new_second_sites_frac.append(x[0].frac_coords)
return (new_second_sites, new_second_sites_frac)
new_second_sites, new_second_sites_frac = second_site_search(
site, radius)
if new_second_sites == []:
for new_radius in np.linspace(float(radius + 0.1), radius + 5,
100):
new_second_sites, new_second_sites_frac = second_site_search(
site, new_radius)
if not new_second_sites == []:
break
for j, second_site in enumerate(new_second_sites):
def third_site_search(site1, site2, new_radius):
third_sites = struct.get_sites_in_sphere(
site2, include_image=True, r=new_radius)
new_third_sites = []
new_third_sites_frac = []
for x in third_sites:
if x[0].as_dict()['species'][0]['element'] == atom3:
if not np.array_equal(x[0].coords, site1):
if not np.array_equal(x[0].coords, site2):
new_third_sites.append(x[0].coords)
new_third_sites_frac.append(
x[0].frac_coords)
return (new_third_sites, new_third_sites_frac)
new_third_sites, new_third_sites_frac = third_site_search(
site, second_site, radius)
if new_third_sites == []:
for new_radius in np.linspace(float(radius + 0.1),
radius + 5, 100):
new_third_sites, new_third_sites_frac = third_site_search(
site, second_site, new_radius)
if not new_third_sites == []:
break
for k, third_site in enumerate(new_third_sites):
ba = site - second_site
bc = third_site - second_site
cosine_angle = np.dot(
ba, bc) / (np.linalg.norm(ba) * np.linalg.norm(bc))
angle = np.around(np.degrees(np.arccos(cosine_angle)),
decimals=args.decimal)
total_data.append([
sites_init_frac[i], new_second_sites_frac[j],
new_third_sites_frac[k], angle
])
np.set_printoptions(
formatter={'float': lambda x: "{0:0.3f}".format(x)})
df = pd.DataFrame(total_data, columns=[atom1, atom2, atom3, 'angle'])
df = df.sort_values(by=['angle'])
df = df.reset_index(drop=True)
if args.verbose == False:
df = df.drop_duplicates(subset='angle', keep='first')
df = df.reset_index(drop=True)
return (df)
else:
return (df)
def get_fluxmap(self, eners, local_coords, resolution):
if resolution == None:
resolution = 30
else:
resolution = int(N.ceil(resolution / 3.) * 3)
flux = N.zeros(resolution**2)
if len(eners) == 0:
return flux
local_rads = N.sqrt(N.sum(local_coords[:2]**2, axis=0))
local_angs = N.arctan2(local_coords[1], local_coords[0])
local_angs[local_angs < 0.] = local_angs[local_angs < 0.] + 2. * N.pi
dangcut = N.arccos(self.x_cut / self._Re)
if dangcut < (N.pi / 2.):
angcut1 = N.arange(0., dangcut, dangcut / (resolution / 3))
angdisk = N.arange(dangcut, 2. * N.pi - dangcut,
2. * (N.pi - dangcut) / (resolution / 3))
angcut2 = N.linspace(2. * N.pi - dangcut, 2. * N.pi,
(resolution / 3) + 1)
angs = N.hstack((angcut1, angdisk, angcut2))
rs = N.linspace(0., self._Re, resolution + 1)
xs = N.linspace(0., self.x_cut, resolution + 1)
# Treat differently the disk region and the cut region
# Disk region: bin according to radii and angle
disk = angs[resolution / 3:2 * resolution / 3 + 1]
enersdisk = N.histogram2d(local_rads,
local_angs,
bins=[rs, disk],
weights=eners)[0]
drs = N.tile(rs[1:] - rs[:-1], (len(disk) - 1, 1)).T
ravgs = N.tile((rs[1:] + rs[:-1]) / 2., (len(disk) - 1, 1)).T
dangs = N.tile(N.abs(disk[1:] - disk[:-1]), (len(rs) - 1, 1))
areas = drs * ravgs * dangs
fluxdisk = N.hstack(enersdisk / areas)
# Cut region: bin according to x coord and angle
cut1 = angs <= dangcut
enerscut1 = N.histogram2d(local_coords[0],
local_angs,
bins=[xs, angs[cut1]],
weights=eners)[0]
dxs = N.tile(xs[1:] - xs[:-1], (len(angs[cut1]) - 1, 1))
dys = (xs[:-1] * N.vstack(N.tan(angs[cut1][:-1])) +
xs[1:] * N.vstack(N.tan(angs[cut1][1:]) / 2.))
areas = N.abs(dxs * dys)
fluxcut1 = N.hstack(enerscut1 / areas.T)
cut2 = angs >= (2. * N.pi - dangcut)
enerscut2 = N.histogram2d(local_coords[0],
local_angs,
bins=[xs, angs[cut2]],
weights=eners)[0]
dxs = N.tile(xs[1:] - xs[:-1], (len(angs[cut2]) - 1, 1))
dys = (xs[:-1] * N.vstack(N.tan(angs[cut2][:-1])) +
xs[1:] * N.vstack(N.tan(angs[cut2][1:]) / 2.))
areas = N.abs(dxs * dys)
fluxcut2 = N.hstack(enerscut2 / areas.T)
for i in xrange(len(flux) / 3):
idx = resolution / 3
flux[resolution * i:resolution * i +
idx] = fluxcut1[idx * i:idx * (i + 1)]
flux[resolution * i + idx:resolution * i +
2 * idx] = fluxdisk[idx * i:idx * (i + 1)]
flux[resolution * i + 2 * idx:resolution * i +
3 * idx] = fluxcut2[idx * i:idx * (i + 1)]
else:
flux = N.zeros(resolution**2)
angs = N.linspace(dangcut, 2. * N.pi - dangcut, resolution + 1)
x, y, z = self.mesh(resolution)
xA = x[:-1, :-1]
xB = x[:-1, 1:]
xC = x[1:, 1:]
xD = x[1:, :-1]
yA = y[:-1, :-1]
yB = y[:-1, 1:]
yC = y[1:, 1:]
yD = y[1:, :-1]
a = N.sqrt((xB - xA)**2 + (yB - yA)**2)
b = N.sqrt((xC - xB)**2 + (yC - yB)**2)
c = N.sqrt((xD - xC)**2 + (yD - yC)**2)
d = N.sqrt((xA - xD)**2 + (yA - yD)**2)
p = N.sqrt((xC - xA)**2 + (yC - yA)**2)
q = N.sqrt((xD - xB)**2 + (yD - yB)**2)
# Quadrilateral area:
areas = 0.25 * N.sqrt(4. * p**2 * q**2 -
(b**2 + d**2 - a**2 - c**2)**2)
# Add the disk cap that is unaccounted for to the last element
areas[:, -1] += (
angs[1:] - angs[:-1]
) / 2. * self._Re**2 - b[:, -1] / 2. * self._Re * N.cos(
N.arcsin(b[:, -1] / (2. * self._Re)))
# Binning:
for i in xrange(int(resolution)):
# Separations lines equation coefficients:
a_seps = N.tile((y[i + 1] - y[i]) / (x[i + 1] - x[i]),
(local_coords.shape[1], 1))
b_seps = y[i] - a_seps * x[i]
# Equation of the line from the origin goping through the hit coordinate:
local_a = local_coords[1] / local_coords[0]
# Intersection with the "radial" separations:
local_inters_x = b_seps / (N.vstack(local_a) - a_seps)
local_inters_x[N.isnan(local_inters_x)] = self.x_cut
local_inters_y = N.vstack(local_a) * local_inters_x
inter_rads = N.vstack(
N.sqrt(local_inters_x**2 + local_inters_y**2))
in_wedge = N.logical_and((local_angs >= angs[i]),
(local_angs < angs[i + 1]))
if in_wedge.any():
inter_rads[:,
-1] = self._Re # to grab the hits that are beyond the last separation but before the end of the disk.
in_bins = N.logical_and(
(N.vstack(local_rads) >= inter_rads[:, :-1]),
(N.vstack(local_rads) < inter_rads[:, 1:]))
#flux[i*resolution:(i+1)*resolution] = N.sum(N.vstack(eners)*in_bins, axis=0)/areas[i]
flux[i:resolution**2:resolution] = N.sum(
N.vstack(eners) * in_bins, axis=0) / areas[i]
return flux
def minimum_curvature(md, inc, azi):
"""Minimum curvature
Calculate TVD, northing, easting, and dogleg, using the minimum curvature
method.
This is the inner workhorse of the min_curve_method, and only implement the
pure mathematics. As a user, you should probably use the min_curve_method
function.
This function considers md unitless, and assumes inc and azi are in
radians.
Parameters
----------
md : array_like of float
measured depth
inc : array_like of float
inclination in radians
azi : array_like of float
azimuth in radians
Returns
-------
tvd : array_like of float
true vertical depth
northing : array_like of float
easting : array_like of float
dogleg : array_like of float
Notes
-----
This function does not insert surface location
"""
md, inc, azi = checkarrays(md, inc, azi)
# extract upper and lower survey stations
md_upper, md_lower = md[:-1], md[1:]
inc_upper, inc_lower = inc[:-1], inc[1:]
azi_upper, azi_lower = azi[:-1], azi[1:]
cos_inc = np.cos(inc_lower - inc_upper)
sin_inc = np.sin(inc_upper) * np.sin(inc_lower)
cos_azi = 1 - np.cos(azi_lower - azi_upper)
dogleg = np.arccos(cos_inc - (sin_inc * cos_azi))
# ratio factor, correct for dogleg == 0 values
rf = 2 / dogleg * np.tan(dogleg / 2)
rf = np.where(dogleg == 0., 1, rf)
md_diff = md_lower - md_upper
upper = np.sin(inc_upper) * np.cos(azi_upper)
lower = np.sin(inc_lower) * np.cos(azi_lower) * rf
northing = np.cumsum(md_diff / 2 * (upper + lower))
upper = np.sin(inc_upper) * np.sin(azi_upper)
lower = np.sin(inc_lower) * np.sin(azi_lower) * rf
easting = np.cumsum(md_diff / 2 * (upper + lower))
tvd = np.cumsum(md_diff / 2 * (np.cos(inc_upper) + np.cos(inc_lower)) * rf)
return tvd, northing, easting, dogleg
dir_create("./temp/percept")
sig = get_param_sig(tau_relative, fixed_tau, use_prior, update_only_on_error)
pdfpath = "./temp/percept/percept_%s.pdf" % sig
dp = DataPlotter(pdfpath=pdfpath, rows=1, cols=1)
plot_initial_only = False
# logger.debug("Oracle: %s" % str(oracle.y))
u = np.array([np.cos(u_theta), np.sin(u_theta)])
if plot_initial_only:
budget = 0
title = None
else:
budget = 30
title = r"initial (${\theta}$: %1.2f)" % (np.arccos(u.dot(aad.w)) * 180. / np.pi)
plot_learning(x, y, None, queried, aad, u_theta, dp,
title=title,
plot_xtau=False, plot_theta=plot_initial_only, plot_legends=plot_initial_only
)
for iter in range(budget):
# active learning step
q = aad.get_query(x, queried)
queried[q] = oracle.get_label(q)
# logger.debug(queried)
# logger.debug("q: %d, label: %d" % (q, queried[q]))
if (not update_only_on_error) or queried[q] != 1:
if update_only_on_error:
logger.debug("updating on error...")
aad.update(x, queried)
def verify_triangle_binding(self, distance, first_bond, angle_res):
# Gather pairs
n = len(self.s.part)
angle_res = angle_res - 1
expected_pairs = []
for i in range(n):
for j in range(i + 1, n, 1):
if self.s.distance(self.s.part[i], self.s.part[j]) <= distance:
expected_pairs.append((i, j))
# Find triangles
# Each element is a particle id, a bond id and two bond partners in
# ascending order
expected_angle_bonds = []
for i in range(n):
for j in range(i + 1, n, 1):
for k in range(j + 1, n, 1):
# Ref to particles
p_i = self.s.part[i]
p_j = self.s.part[j]
p_k = self.s.part[k]
# Normalized distance vectors
d_ij = np.copy(p_j.pos - p_i.pos)
d_ik = np.copy(p_k.pos - p_i.pos)
d_jk = np.copy(p_k.pos - p_j.pos)
d_ij /= np.sqrt(np.sum(d_ij**2))
d_ik /= np.sqrt(np.sum(d_ik**2))
d_jk /= np.sqrt(np.sum(d_jk**2))
if self.s.distance(p_i,
p_j) <= distance and self.s.distance(
p_i, p_k) <= distance:
id_i = first_bond._bond_id + \
int(np.round(
np.arccos(np.dot(d_ij, d_ik)) * angle_res / np.pi))
expected_angle_bonds.append((i, id_i, j, k))
if self.s.distance(p_i,
p_j) <= distance and self.s.distance(
p_j, p_k) <= distance:
id_j = first_bond._bond_id + \
int(np.round(
np.arccos(np.dot(-d_ij, d_jk)) * angle_res / np.pi))
expected_angle_bonds.append((j, id_j, i, k))
if self.s.distance(p_i,
p_k) <= distance and self.s.distance(
p_j, p_k) <= distance:
id_k = first_bond._bond_id + \
int(np.round(
np.arccos(np.dot(-d_ik, -d_jk)) * angle_res / np.pi))
expected_angle_bonds.append((k, id_k, i, j))
# Gather actual pairs and actual triangles
found_pairs = []
found_angle_bonds = []
for i in range(n):
for b in self.s.part[i].bonds:
if len(b) == 2:
self.assertEqual(b[0]._bond_id, self.H._bond_id)
found_pairs.append(tuple(sorted((i, b[1]))))
elif len(b) == 3:
partners = sorted(b[1:])
found_angle_bonds.append(
(i, b[0]._bond_id, partners[0], partners[1]))
else:
raise Exception(
"There should be only 2 and three particle bonds")
# The order between expected and found bonds does not always match
# because collisions occur in random order. Sort stuff
found_pairs = sorted(found_pairs)
found_angle_bonds = sorted(found_angle_bonds)
expected_angle_bonds = sorted(expected_angle_bonds)
self.assertEqual(expected_pairs, found_pairs)
if not expected_angle_bonds == found_angle_bonds:
# Verbose info
print("expected:", expected_angle_bonds)
missing = []
for b in expected_angle_bonds:
if b in found_angle_bonds:
found_angle_bonds.remove(b)
else:
missing.append(b)
print("missing", missing)
print("extra:", found_angle_bonds)
print()
self.assertEqual(expected_angle_bonds, found_angle_bonds)
omega = -B0 * gamma
ms = IntBloch(m0, lambda t: Bcirc(t, localB0, B1, omega), times, gamma)
print("vector")
print(ms)
finalMs.append(ms)
#print("M")
#print(ms)
#mTnorm=np.linalg.norm(ms[0:2])
#phase=np.degrees(np.arctan2(ms[1],ms[0]))
#print("phase")
#print(phase)
#phase=phase-phi0
#phase=np.tan(np.radians(phase))
#print(phase)
theta = np.degrees(np.arccos(ms[2])) #np.arctan2(mTnorm,ms[2]))
thetas.append(theta)
#phases.append(phase)
dOmega = (G * x * gamma)
omegaMag = np.power((G * x * gamma)**2 + (gamma * B1)**2, 0.5)
#sinAngle2=(2./(1.+(G*x/B1)**2))
#expTheta=1.-sinAngle2*(np.sin(0.5*times[-1]*omegaMag))**2
#expThetas.append(np.degrees(np.arccos(expTheta)))
#expThetas.append(-(expTheta-1))
sinterm = np.abs((gamma * B1 * times[-1] / 2) *
np.sinc(omegaMag * times[-1] / (np.pi * 2.)))
expThetas.append(2 * np.degrees(np.arcsin(sinterm)))
#expThetas3.append(np.degrees(2*sinterm))
import os
from numpy import arccos
#Load unit conversion
sys.path.append(os.path.abspath("./pyprop/pyprop/utilities"))
import units
from units import ElectricFieldAtomicFromIntensitySI as field_from_intensity
from units import AngularFrequencyAtomicFromWavelengthSI as freq_from_wavelength
from units import IntensitySIFromElectricFieldAtomic as intensity_from_field
#Unit conversion factors
femtosec_to_au = 1e-15 / units.constantsAU.time
#Pulse duration from intensity full with half maximum
#for a cos**2 pulse
fwhm_intensity = pi / arccos(0.5**0.25) / 2.0
#Converts wavelength in nm -> time of one cycle a.u.
cycletime_from_wavelength = lambda l: 2 * pi / freq_from_wavelength(l)
#Converts frequency in a.u. -> time of one cycle a.u.
cycletime_from_frequency = lambda f: 2 * pi / f
#Ponderomotive energy
#ponderomotive_energy = lambda I, omega: I / (4.0 * omega**2)
ponderomotive_energy = lambda E0, omega: E0**2 / (4.0 * omega**2)
#eV -> au
eV_to_au = 3.674932540e-2
def get_metrics(endmembersPredicted,
image,
exec_id,
abundancesPredicted=None,
path_abundances_GT=None,
show_images=False):
import matplotlib
if show_images == False:
matplotlib.use('Agg')
K = endmembersPredicted.shape[1]
endmembersGT = scipy.io.loadmat(path_abundances_GT)['M']
if image == 'cuprite':
bands = scipy.io.loadmat(path_abundances_GT)['slctBnds'][0, :]
endmembersGT = endmembersGT[bands]
softmaxed = softmax(endmembersGT.T)
endmembersGT = softmaxed.T
rmse = 0.0
sad = 0.0
if (path_abundances_GT != None):
# Pair predicted/true equal endmembers before SAD
endm_s1 = endmembersPredicted
endm_gt = endmembersGT
dists = []
for col in range(endm_s1.shape[1]):
act_sim = []
row = endm_s1[:, col]
for col2 in range(endm_gt.shape[1]):
row2 = endm_gt[:, col2]
act_sim.append(sp_dist.cosine(row, row2))
dists.append(act_sim)
dists = np.array(dists)
new_classes = [0] * K
en2 = copy.deepcopy(endmembersPredicted)
for i in range(K):
(fil, col) = np.unravel_index(dists.argmin(), dists.shape)
endmembersPredicted[:, col] = en2[:, fil]
new_classes[fil] = col
dists[:, col] = 100000
dists[fil, :] = 100000
del en2, new_classes, dists, endm_gt, endm_s1
from numpy.linalg import norm
cos_sim = 0
for i in range(K):
b = endmembersGT[:, i]
a = endmembersPredicted[:, i]
cos_sim += np.arccos(np.dot(a, b) / (norm(a) * norm(b)))
sad = cos_sim / float(K)
if ('A' in scipy.io.loadmat(path_abundances_GT).keys()):
abundancesGT = scipy.io.loadmat(path_abundances_GT)['A'].T
abundancesGT = \
np.transpose(\
abundancesGT.reshape(abundancesPredicted.shape[1], abundancesPredicted.shape[0], abundancesGT.shape[1]), (1,0,2))
# Pair predicted/true equal abundances before RMSE
image_s1 = abundancesPredicted.reshape(-1, K)
image_gt = abundancesGT.reshape(-1, K)
dists = []
for col in range(image_s1.shape[1]):
act_sim = []
row = image_s1[:, col]
for col2 in range(image_gt.shape[1]):
row2 = image_gt[:, col2]
act_sim.append(sp_dist.cosine(row, row2))
dists.append(act_sim)
dists = np.array(dists)
new_classes = [0] * K
ab2 = copy.deepcopy(abundancesPredicted)
for i in range(K):
(fil, col) = np.unravel_index(dists.argmin(), dists.shape)
abundancesPredicted[:, :, col] = ab2[:, :, fil]
new_classes[fil] = col
dists[:, col] = 100000
dists[fil, :] = 100000
del ab2, new_classes, dists, image_gt, image_s1
rmse = np.sqrt(
mean_squared_error(abundancesGT.reshape(-1, K),
abundancesPredicted.reshape(-1, K)))
mosaicPred = abundancesPredicted[:, :, 0]
mosaicGT = abundancesGT[:, :, 0]
for i in range(1, K):
mosaicPred = np.hstack((mosaicPred, abundancesPredicted[:, :,
i]))
mosaicGT = np.hstack((mosaicGT, abundancesGT[:, :, i]))
mosaicFinal = np.vstack((mosaicPred, mosaicGT))
if show_images:
plt.imshow(mosaicFinal)
plt.show()
plt.clf()
else:
plt.imsave(('outputs/images/abundances_' + image + '_' +
exec_id + '.png'), mosaicFinal)
else:
mosaicPred = abundancesPredicted[:, :, 0]
for i in range(1, K):
mosaicPred = np.hstack((mosaicPred, abundancesPredicted[:, :,
i]))
if show_images:
plt.imshow(mosaicPred)
plt.show()
plt.clf()
else:
plt.imsave(('outputs/images/abundances_' + image + '_' +
exec_id + '.png'), mosaicPred)
if image == 'cuprite':
endmembersPredicted = endmembersPredicted[3:, :]
plt.plot(endmembersPredicted)
if show_images:
plt.show()
else:
plt.savefig(
('outputs/images/endmembers_' + image + '_' + exec_id + '.png'),
bbox_inches='tight',
pad_inches=0.2,
dpi=200)
return rmse, sad # -*- coding: utf-8 -*-
def eucl2deg(eucl):
raw = (180 / np.pi) * np.arccos(np.clip(1 - 0.5 * eucl**2, -1, 1))
return np.minimum(raw, 180 - raw)
def get_wavefront_parallel(data,aim,i,t,side,PAAM_ang,ret,mode='opposite',precision=0,ksi=[0,0],angles=False):
[i_self,i_left,i_right] = utils.i_slr(i)
if mode=='opposite':
if side=='l':
tdel = data.L_sl_func_tot(i_self,t)
if data.calc_method=='Waluschka':
tdel0=tdel
elif data.calc_method=='Abram':
tdel0=0
if angles==False:
tele_ang = aim.tele_l_ang(i_self,t+tdel0)
else:
tele_ang=angles
coor_start = beam_coor_out(data,i_self,t,tele_ang,PAAM_ang,aim.offset_tele['l'])
coor_end = aim.tele_r_coor(i_left,t+tdel)
start=aim.tele_l_start(i_self,t+tdel0)
end=aim.tele_r_start(i_left,t+tdel)+coor_end[1]*ksi[1]+coor_end[2]*ksi[0]
elif side=='r':
tdel=data.L_sr_func_tot(i_self,t)
if data.calc_method=='Waluschka':
tdel0=tdel
elif data.calc_method=='Abram':
tdel0=0
if angles==False:
tele_ang = aim.tele_r_ang(i_self,t+tdel0)
else:
tele_ang=angles
coor_start = beam_coor_out(data,i_self,t,tele_ang,PAAM_ang,aim.offset_tele['r'])
coor_end = aim.tele_l_coor(i_right,t+tdel)
start = aim.tele_r_start(i_self,t+tdel0)
end=aim.tele_l_start(i_right,t+tdel)+coor_end[1]*ksi[1]+coor_end[2]*ksi[0]
[zoff,yoff,xoff]=LA.matmul(coor_start,end-start)
if precision==0:
R = zoff # Not precise
elif precision==1:
try:
[piston,z_extra] = wfe.z_solve(xoff,yoff,zoff,ret='all')
except:
[piston,z_extra] = [np.nan,np.nan]
R = wfe.R(piston)
R_vec = np.array([(R**2-xoff**2-yoff**2)**0.5,yoff,xoff])
tele_vec = LA.matmul(coor_start,-coor_end[0])
angx_R = np.sign(R_vec[2])*abs(np.arctan(R_vec[2]/R_vec[0]))
angy_R = np.sign(R_vec[1])*abs(np.arctan(R_vec[1]/R_vec[0]))
angx_tele = np.sign(tele_vec[2])*abs(np.arctan(tele_vec[2]/tele_vec[0]))
angy_tele = np.sign(tele_vec[1])*abs(np.arctan(tele_vec[1]/tele_vec[0]))
angx = (angx_tele-angx_R)
angy = (angy_tele-angy_R)
elif mode=='self':
if side=='l':
tdel = data.L_rl_func_tot(i_self,t)
if data.calc_method=='Waluschka':
tdel0=tdel
elif data.calc_method=='Abram':
tdel0=0
if angles==False:
tele_ang = aim.tele_r_ang(i_left,t-tdel)
tele_ang_end = aim.tele_l_ang(i_self,t-tdel0)
PAAM_ang = aim.beam_r_ang(i_left,t-tdel)
elif len(angles)>=2:
tele_ang_end = angles[0]
tele_ang = angles[2]
PAAM_ang = aim.beam_r_ang(i_left,t-tdel)
coor_start = beam_coor_out(data,i_left,t-tdel,tele_ang,PAAM_ang,aim.offset_tele['r'])
coor_end = coor_tele(data,i_self,t,tele_ang_end)
start = LA.unit(coor_start[0])*data.L_tele+data.putp(i_left,t-tdel)
end = LA.unit(coor_end[0])*data.L_tele+data.putp(i_self,t-tdel0)+coor_end[1]*ksi[1]+coor_end[2]*ksi[0]
elif side=='r':
tdel = data.L_rr_func_tot(i_self,t)
if data.calc_method=='Waluschka':
tdel0=tdel
elif data.calc_method=='Abram':
tdel0=0
if angles==False:
tele_ang = aim.tele_l_ang(i_right,t-tdel)
tele_ang_end = aim.tele_r_ang(i_self,t-tdel0)
PAAM_ang = aim.beam_l_ang(i_right,t-tdel)
elif len(angles)>=2:
tele_ang_end = angles[0]
tele_ang = angles[2]
PAAM_ang = aim.beam_l_ang(i_right,t-tdel)
coor_start = beam_coor_out(data,i_right,t-tdel,tele_ang,PAAM_ang,aim.offset_tele['l'])
coor_end = coor_tele(data,i_self,t,tele_ang_end)
start = LA.unit(coor_start[0])*data.L_tele+data.putp(i_right,t-tdel)
end = LA.unit(coor_end[0])*data.L_tele+data.putp(i_self,t-tdel0)+coor_end[1]*ksi[1]+coor_end[2]*ksi[0]
[zoff,yoff,xoff]=LA.matmul(coor_start,end-start)
out=OUTPUT(aim)
if precision==0:
R = zoff # Not precise
elif precision==1:
try:
[piston,z_extra] = out.z_solve(xoff,yoff,zoff,ret='all')
except:
[piston,z_extra] = [np.nan,np.nan]
R = out.R(piston)
R_vec = np.array([(R**2-xoff**2-yoff**2)**0.5,yoff,xoff])
R_vec_origin = LA.matmul(np.linalg.inv(coor_start),R_vec)
R_vec_tele_rec = LA.matmul(coor_end,-R_vec_origin)
angx = np.arctan(abs(R_vec_tele_rec[2]/R_vec_tele_rec[0]))*np.sign(R_vec_tele_rec[2])
angy = np.arctan(abs(R_vec_tele_rec[1]/R_vec_tele_rec[0]))*np.sign(R_vec_tele_rec[1])
if ret=='angy':
return angy
elif ret=='angx':
return angx
elif ret=='tilt':
return (angx**2+angy**2)**0.5
elif ret=='xoff':
return xoff
elif ret=='yoff':
return yoff
elif ret=='r':
return (xoff**2 +yoff**2)**0.5
elif ret=='all':
ret_val={}
ret_val['start']=start
ret_val['end']=end
ret_val['zoff']=zoff
ret_val['yoff']=yoff
ret_val['xoff']=xoff
ret_val['coor_start']=coor_start
ret_val['coor_end']=coor_end
ret_val['bd_original_frame'] = np.array(coor_start[0])
ret_val['bd_receiving_frame'] = LA.matmul(coor_end,ret_val['bd_original_frame'])
ret_val['angx_func_rec'] = angx
ret_val['angy_func_rec'] = angy
ret_val['R_vec_tele_rec']=R_vec_tele_rec
#ret_val['tilt'] = np.arccos(R_vec_tele_rec[0]/np.linalg.norm(R_vec_tele))
#ret_val['tilt']=(angx**2+angy**2)**0.5
#ret_val['tilt']=LA.angle(R_vec_tele,(angx**2+angy**2)**0.5
if precision==1:
ret_val['piston']=piston
ret_val['z_extra'] = z_extra
ret_val['R']=R
ret_val["R_vec_beam_send"] = R_vec
ret_val['R_vec_origin'] = R_vec_origin
ret_val['r']=(xoff**2+yoff**2)**0.5
FOV_beamline = np.arccos(-ret_val['bd_receiving_frame'][0]/np.linalg.norm(ret_val['bd_receiving_frame']))
FOV_wavefront = LA.angle(-R_vec_origin,coor_end[0])
FOV_position = LA.angle(start-end,coor_end[0])
ret_val['tilt']=FOV_wavefront
ret_val['FOV_beamline']=FOV_beamline
ret_val['FOV_wavefront']=FOV_wavefront
ret_val['FOV_position']=FOV_position
return ret_val