def write_ubi(param):
# Save the generated UBI's
#
# INPUT: The parameter set from the input file and the grain generator
# OUTPUT: for each grain the 3x3 UBI matrix
#
# Jette Oddershede, Risoe DTU, April 4 2008
#
filename = '%s/%s.ubi' % (param['direc'], param['stem'])
f = open(filename, 'w')
format = "%f " * 3 + "\n"
for i in range(param['no_grains']):
U = param['U_grains_%s' % (param['grain_list'][i])]
gr_eps = n.array(param['eps_grains_%s' % (param['grain_list'][i])])
if param['no_phases'] == 1:
phase = param['phase_list'][0]
else:
phase = param['phase_grains_%s' % (param['grain_list'][i])]
# Calculate the B-matrix based on the strain tensor for each grain
B = tools.epsilon_to_b(
gr_eps, param['unit_cell_phase_%i' % phase]) / (2 * n.pi)
UBI = n.linalg.inv(n.dot(U, B))
for j in range(3):
out = format % (UBI[j, 0], UBI[j, 1], UBI[j, 2])
f.write(out)
out = "\n"
f.write(out)
f.close()
def run_asr(self, topology, ystep, number_y_scans, ymin, g, flt):
origin = np.array([topology.shape[0] // 2, topology.shape[0] // 2])
mesh = mesher.create_pixel_mesh(topology, ystep, origin)
distance = self.params.get('distance')
pixelsize = (self.params.get('y_size') +
self.params.get('z_size')) / 2.0
wavelength = self.params.get('wavelength')
cell_original = [
self.params.get('cell__a'),
self.params.get('cell__b'),
self.params.get('cell__c'),
self.params.get('cell_alpha'),
self.params.get('cell_beta'),
self.params.get('cell_gamma')
]
strains, directions, omegas, dtys, weights, tths, etas, intensity, sc, G_omegas, hkl = mc.extract_strain_and_directions(
cell_original, wavelength, distance, pixelsize, g, flt, ymin,
ystep, self.omegastep, number_y_scans)
# #With orient
# UBs = asr.solve_with_orient( g, hkl, G_omegas, omegas, weights, mesh, dtys, ystep, cell_original )
# voxels = []
# coordinates = mesher.get_elm_centres( mesh )
# #print("UBs.shape",UBs.shape)
# for i in range(UBs.shape[0]):
# #print(UBs[i,:,:])
# UBI = np.linalg.inv(UBs[i,:,:])
# voxels.append( grain.grain( UBI ) )
# return voxels, coordinates
# only strain
# tikhonov_solve
#eps_xx, eps_yy, eps_zz, eps_yz, eps_xz, eps_xy = asr.tikhonov_solve( mesh, directions, strains , omegas, dtys, weights, ystep, self.gradient_constraint )
#trust region
eps_xx, eps_yy, eps_zz, eps_yz, eps_xz, eps_xy = asr.trust_constr_solve(
mesh, etas, hkl, tths, intensity, directions, strains, omegas,
dtys, weights, ystep, self.gradient_constraint, self.maxiter)
voxels = []
coordinates = mesher.get_elm_centres(mesh)
for i, elm in enumerate(mesh):
# [e11, e12, e13, e22, e23, e33]
epsilon_sample = np.array([[eps_xx[i], eps_xy[i], eps_xz[i]],
[eps_xy[i], eps_yy[i], eps_yz[i]],
[eps_xz[i], eps_yz[i], eps_zz[i]]])
eps_cry = np.dot(np.dot(np.transpose(g.u), epsilon_sample), g.u)
eps_cry_flat = [
eps_cry[0, 0], eps_cry[0, 1], eps_cry[0, 2], eps_cry[1, 1],
eps_cry[1, 2], eps_cry[2, 2]
]
B = tools.epsilon_to_b(eps_cry_flat, cell_original)
UBI = np.linalg.inv(np.dot(g.u, B)) * (2 * np.pi)
voxels.append(grain.grain(UBI))
return voxels, coordinates
def strain_and_euler_to_ub(self,strain,euler):
'''
cell = [a,b,c,alpha,beta,gamma]
euler= [phi1,PHI,phi2]
'''
U = tools.euler_to_u(euler[0],euler[1],euler[2])
B = tools.epsilon_to_b(strain, self.unit_cell)
return np.dot(U,B)
def test_epsilon2B2epsilon(self):
ucell = n.array([
3.5 + n.random.rand(), 3.5 + n.random.rand(),
3.5 + n.random.rand(), 89.5 + n.random.rand(),
89.5 + n.random.rand(), 89.5 + n.random.rand()
])
eps = (n.random.rand(6) - .5) / 1000.
B = tools.epsilon_to_b(eps, ucell)
eps2 = tools.b_to_epsilon(B, ucell)
def test_UdotBtoUandB(self):
ucell = n.array([
3.5 + n.random.rand(), 3.5 + n.random.rand(),
3.5 + n.random.rand(), 89.5 + n.random.rand(),
89.5 + n.random.rand(), 89.5 + n.random.rand()
])
eps = (n.random.rand(6) - .5) / 1000.
B = tools.epsilon_to_b(eps, ucell)
U = tools.euler_to_u(n.random.rand() * 2. * n.pi,
n.random.rand() * 2. * n.pi,
n.random.rand() * n.pi)
UB = n.dot(U, B)
(U1, B1) = tools.ub_to_u_b(UB)
diffU = n.abs(U - U1).sum()
diffB = n.abs(B - B1).sum()
self.assertAlmostEqual(diffU, 0, 9)
self.assertAlmostEqual(diffB, 0, 9)
def run(self, start_voxel, end_voxel, log=True, parallel=None):
'''
This is the main algorithmic loop that will calculate the diffraction pattern
based on a per-voxel definition of the sample. The algorithm deals with one voxel at the
time, computing all reflections that would be generated for that voxel in a single go.
Therefore, the run time is linear with voxel number regardless of the number of y-scans.
Input: start_voxel: Used for running in parrallel, equal to 0 for 1 cpu
end_voxel: Used for running in parrallel, equal to number of voxels for 1 cpu
log: used to determine of this process should print to stdout or be quiet.
parallel: Flag to indicate parallel mode. Such a mode requires that we pass the result
of the run to the calling process.
'''
self.param['lorentz_apply']=1
tth_lower_bound = self.param['two_theta_lower_bound']*np.pi/180.
tth_upper_bound = self.param['two_theta_upper_bound']*np.pi/180.
spot_id = 0
# Compute used quanteties once for speed
#--------------------------------------------
# Don't make static dictonary calls in loop, slower..
no_voxels = self.param['no_voxels']
beam_width = self.param['beam_width']
omega_start = self.param['omega_start']*np.pi/180
omega_end = self.param['omega_end']*np.pi/180
wavelength = self.param['wavelength']
scale_Gw = wavelength/(4.*np.pi)
detz_center = self.param['detz_center']
dety_center = self.param['dety_center']
z_size = self.param['z_size']
y_size = self.param['y_size']
distance = self.param['distance']
wavelength = self.param['wavelength']
if log==True:
print('no of voxels ',no_voxels)
# print(start_voxel, end_voxel)
# with open('solution','w') as f:
# for voxel_nbr in range(start_voxel, end_voxel):
# if len(self.param['phase_list']) == 1:
# phase = self.param['phase_list'][0]
# else:
# phase = self.param['phase_voxels_%s' %(self.param['voxel_list'][voxel_nbr])]
# unit_cell = self.param['unit_cell_phase_%i' %phase]
# U = self.param['U_voxels_%s' %(self.param['voxel_list'][voxel_nbr])]
# voxel_eps = np.array(self.param['eps_voxels_%s' %(self.param['voxel_list'][voxel_nbr])])
# B = tools.epsilon_to_b(voxel_eps,unit_cell)
# UB = np.dot(U,B)
# ub = UB.ravel()
# f.write("np.array([")
# for val in ub:
# f.write(str(val)+", ")
# f.write("])\n")
# raise
for voxel_nbr in range(start_voxel, end_voxel):
A = []
U = self.param['U_voxels_%s' %(self.param['voxel_list'][voxel_nbr])]
if len(self.param['phase_list']) == 1:
phase = self.param['phase_list'][0]
else:
phase = self.param['phase_voxels_%s' %(self.param['voxel_list'][voxel_nbr])]
unit_cell = self.param['unit_cell_phase_%i' %phase]
self.voxel[voxel_nbr] = variables.voxel_cont(U)
voxel_pos = np.array(self.param['pos_voxels_%s' %(self.param['voxel_list'][voxel_nbr])])
voxel_eps = np.array(self.param['eps_voxels_%s' %(self.param['voxel_list'][voxel_nbr])])
# Calculate the B-matrix based on the strain tensor for each voxel
B = tools.epsilon_to_b(voxel_eps,unit_cell)
# add B matrix to voxel container
self.voxel[voxel_nbr].B = B
V = tools.cell_volume(unit_cell)
voxel_vol = np.pi/6 * self.param['size_voxels_%s' %self.param['voxel_list'][voxel_nbr]]**3
nrefl = 0
for hkl in self.hkl[self.param['phase_list'].index(phase)]:
check_input.interrupt(self.killfile)
Gc = np.dot(B,hkl[0:3])
Gw = np.dot(self.S,np.dot(U,Gc))
# if hkl[0]==0 and hkl[1]==-2 and hkl[2]==0:
# print(np.dot(U,B))
# print(hkl[0:3])
# print(Gw)
# raise
tth = tools.tth2(Gw,wavelength)
# If specified in input file do not compute for two
# thetaoutside range [tth_lower_bound, tth_upper_bound]
# if tth_upper_bound<tth or tth<tth_lower_bound :
# continue
costth = np.cos(tth)
(Omega, Eta, Omega_mat, Gts) = self.find_omega_general(Gw*scale_Gw,scale_Gw,tth)
for omega,eta,Om,Gt in zip(Omega, Eta, Omega_mat, Gts):
if omega_start < omega and omega < omega_end:
#print(np.degrees(omega))
# Calc crystal position at present omega
[tx,ty,tz]= np.dot(Om,voxel_pos)
#The 3 beam y positions that could illuminate the voxel
beam_centre_1 = np.round(ty/beam_width)*beam_width
beam_centre_0 = beam_centre_1+beam_width
beam_centre_2 = beam_centre_1-beam_width
#Compute precentual voxel beam overlap for the three regions
overlaps_info = convexPolygon.compute_voxel_beam_overlap(tx,ty,omega,beam_centre_1, beam_width)
regions = [ beam_centre_0, beam_centre_1,beam_centre_2]
for beam_centre_y,info in zip(regions,overlaps_info):
# perhaps we should have a less restrictive
# comparision here, like: if intensity_modifier<0.0001,
# there is some possibilty to simulate nosie here
intensity_modifier = info[0]
if intensity_modifier==0:
continue
#Lorentz factor
if self.param['lorentz_apply'] == 1:
if eta != 0:
L=1/(np.sin(tth)*abs(np.sin(eta)))
else:
L=np.inf;
else:
L = 1.0
intensity = L*intensity_modifier*hkl[3]
# If no unit cells where activated we continue
dty = beam_centre_y*1000. # beam cetre in microns
cx = info[1]
cy = info[2]
# Compute peak based on cms of illuminated voxel fraction
tx = cx
ty = cy - beam_centre_y # The sample moves not the beam!
# print("tx",tx)
# print("ty",ty)
# print("")
tz = 0
(dety, detz) = self.det_coor(Gt,
costth,
wavelength,
distance,
y_size,
z_size,
dety_center,
detz_center,
self.R,
tx,ty,tz)
#If shoebox extends outside detector exclude it
if (-0.5 > dety) or\
(dety > self.param['dety_size']-0.5) or\
(-0.5 > detz) or\
(detz > self.param['detz_size']-0.5):
continue
if self.param['spatial'] != None :
# To match the coordinate system of the spline file
(x,y) = detector.detyz_to_xy([dety,detz],
self.param['o11'],
self.param['o12'],
self.param['o21'],
self.param['o22'],
self.param['dety_size'],
self.param['detz_size'])
# Do the spatial distortion
(xd,yd) = self.spatial.distort(x,y)
# transform coordinates back to dety,detz
(detyd,detzd) = detector.xy_to_detyz([xd,yd],
self.param['o11'],
self.param['o12'],
self.param['o21'],
self.param['o22'],
self.param['dety_size'],
self.param['detz_size'])
else:
detyd = dety
detzd = detz
if self.param['beampol_apply'] == 1:
#Polarization factor (Kahn, J. Appl. Cryst. (1982) 15, 330-337.)
rho = np.pi/2.0 + eta + self.param['beampol_direct']*np.pi/180.0
P = 0.5 * (1 + costth*costth -\
self.param['beampol_factor']*np.cos(2*rho)*np.sin(tth)**2)
else:
P = 1.0
overlaps = 0 # set the number overlaps to zero
# if self.param['intensity_const'] != 1:
# intensity = intensity_modifier*int_intensity(hkl[3],
# L,
# P,
# self.param['beamflux'],
# self.param['wavelength'],
# V,
# voxel_vol)
# else:
# intensity = intensity_modifier*hkl[3]
#TODO: try and build up the images as we go
# Mapp reflection to the correct image
self.peak_merger.add_reflection_to_images([self.param['voxel_list'][voxel_nbr],
nrefl,spot_id,
hkl[0],hkl[1],hkl[2],
tth,omega,eta,
dety,detz,
detyd,detzd,
Gw[0],Gw[1],Gw[2],
L,P,hkl[3],intensity,overlaps,dty,1])
A.append([self.param['voxel_list'][voxel_nbr],
nrefl,spot_id,
hkl[0],hkl[1],hkl[2],
tth,omega,eta,
dety,detz,
detyd,detzd,
Gw[0],Gw[1],Gw[2],
L,P,hkl[3],intensity,overlaps,dty,1])
nrefl = nrefl+1
#TODO: When run in parallel the spot id might be duplicated..
#but who cares about spot id anyways huh..
spot_id = spot_id+1
# A = np.array(A)
# if len(A) > 0:
# # sort rows according to omega
# A = A[np.argsort(A,0)[:,A_id['omega']],:]
# # Renumber the reflections
# A[:,A_id['ref_id']] = np.arange(nrefl)
# # Renumber the spot_id
# A[:,A_id['spot_id']] = np.arange(np.min(A[:,A_id['spot_id']]),
# np.max(A[:,A_id['spot_id']])+1)
# else:
# A = np.zeros((0,len(A_id)))
# save reflection info in voxel container, if we are not in parallel mode this
# will be the same object that we ran the run() method upon. Otherwise it is by
# defualt a copy of that object and we will need to pass the result to the calling
# process at the end of the algorithm
self.voxel[voxel_nbr].refs = A
if parallel and log==True:
progress = int(100*(voxel_nbr+1-start_voxel)/float(end_voxel-start_voxel))
print('\rDone approximately %3i percent' %progress, end=' ')
sys.stdout.flush()
elif log==True:
print('\rDone approximately %3i voxel(s) of %3i' %(voxel_nbr+1,self.param['no_voxels']), end=' ')
sys.stdout.flush()
if log==True:
print('\n')
# if we are running in parrallel the memory cannot be shared (easily)
# so wee return our result in order to merge all results
# into a single find_refl.py Object.
if parallel:
result = {"start_voxel": start_voxel,
"end_voxel": end_voxel,
"refl_list": self.voxel}
return result
else:
# if not in parallel we may merge here
# this allows us to include analyse_images_as_clusters()
# easy in profiling
self.peak_merger.analyse_images_as_clusters()
def write_grains(param):
# Save the generated grain parameters, pos, U and eps
#
# INPUT: The parameter set from the input file and the grain generator
# OUTPUT: grainno x y z phi1 PHI phi2 U11 U12 U13 U21 U22 U23 U31 U32 U33 eps11 eps12 eps13 eps22 eps23 eps33
#
# Jette Oddershede, Risoe DTU, March 31 2008
#
filename = '%s/%s.gff' % (param['direc'], param['stem'])
f = open(filename, 'w')
# format = "%d "*1 + "%f "*1 + "%e"*1 + "%f"*18 + "\n"
format = "%d " * 1 + "%d " * 1 + "%f " * 1 + "%e " * 1 + "%f " * 6 + "%0.12f " * 9 + "%0.12f " * 9 + "%e " * 6 + "\n"
out = "# grain_id phase_id grainsize grainvolume x y z phi1 PHI phi2 U11 U12 U13 U21 U22 U23 U31 U32 U33 UBI11 UBI12 UBI13 UBI21 UBI22 UBI23 UBI31 UBI32 UBI33 eps11 eps12 eps13 eps22 eps23 eps33 \n"
f.write(out)
for i in range(param['no_grains']):
euler = 180 / n.pi * tools.u_to_euler(param['U_grains_%s' %
(param['grain_list'][i])])
if len(param['phase_list']) == 1:
phase = param['phase_list'][0]
else:
phase = param['phase_grains_%s' % (param['grain_list'][i])]
b = tools.epsilon_to_b(
param['eps_grains_%s' % (param['grain_list'][i])],
param['unit_cell_phase_%i' % phase])
u = param['U_grains_%s' % (param['grain_list'][i])]
ubi = n.linalg.inv(n.dot(u, b)) * 2 * n.pi
out = format % (
param['grain_list'][i],
phase,
param['size_grains_%s' % (param['grain_list'][i])],
n.pi / 6 * (param['size_grains_%s' %
(param['grain_list'][i])])**3.,
param['pos_grains_%s' % (param['grain_list'][i])][0],
param['pos_grains_%s' % (param['grain_list'][i])][1],
param['pos_grains_%s' % (param['grain_list'][i])][2],
euler[0],
euler[1],
euler[2],
param['U_grains_%s' % (param['grain_list'][i])][0, 0],
param['U_grains_%s' % (param['grain_list'][i])][0, 1],
param['U_grains_%s' % (param['grain_list'][i])][0, 2],
param['U_grains_%s' % (param['grain_list'][i])][1, 0],
param['U_grains_%s' % (param['grain_list'][i])][1, 1],
param['U_grains_%s' % (param['grain_list'][i])][1, 2],
param['U_grains_%s' % (param['grain_list'][i])][2, 0],
param['U_grains_%s' % (param['grain_list'][i])][2, 1],
param['U_grains_%s' % (param['grain_list'][i])][2, 2],
ubi[0, 0],
ubi[0, 1],
ubi[0, 2],
ubi[1, 0],
ubi[1, 1],
ubi[1, 2],
ubi[2, 0],
ubi[2, 1],
ubi[2, 2],
param['eps_grains_%s' % (param['grain_list'][i])][0],
param['eps_grains_%s' % (param['grain_list'][i])][1],
param['eps_grains_%s' % (param['grain_list'][i])][2],
param['eps_grains_%s' % (param['grain_list'][i])][3],
param['eps_grains_%s' % (param['grain_list'][i])][4],
param['eps_grains_%s' % (param['grain_list'][i])][5],
)
f.write(out)
f.close()
def find_refl(inp):
"""
From U, (x,y,z) and B determined for the far-field case
calculate the possible reflection on the near-field detector
output[grainno][reflno]=[h,k,l,omega,dety,detz,tth,eta]
"""
S = n.array([[1, 0, 0],[0, 1, 0],[0, 0, 1]])
R = tools.detect_tilt(inp.param['tilt_x'],
inp.param['tilt_y'],
inp.param['tilt_z'])
inp.possible = []
# if structure info is given use this
if inp.files['structure_file'] != None:
inp.param['structure_phase_0'] = inp.files['structure_file']
xtal_structure = reflections.open_structure(inp.param,0)
HKL = reflections.gen_miller(inp.param,0)
else:
inp.param['unit_cell_phase_0'] = inp.unit_cell
inp.param['sgno_phase_0'] = inp.fit['sgno']
HKL = reflections.gen_miller(inp.param,0)
for grainno in range(inp.no_grains):
inp.possible.append([])
if grainno+1 not in inp.fit['skip']:
B = tools.epsilon_to_b(n.array([inp.values['epsaa%s' %grainno],
inp.values['epsab%s' %grainno],
inp.values['epsac%s' %grainno],
inp.values['epsbb%s' %grainno],
inp.values['epsbc%s' %grainno],
inp.values['epscc%s' %grainno]]),
inp.unit_cell)
U = tools.rod_to_u([inp.rod[grainno][0]+inp.values['rodx%s' %grainno],
inp.rod[grainno][1]+inp.values['rody%s' %grainno],
inp.rod[grainno][2]+inp.values['rodz%s' %grainno]])
gr_pos = n.array([inp.values['x%s' %grainno],
inp.values['y%s' %grainno],
inp.values['z%s' %grainno]])
for hkl in HKL:
Gc = n.dot(B,hkl[0:3])
Gw = n.dot(S,n.dot(U,Gc))
tth = tools.tth2(Gw,inp.param['wavelength'])
# print hkl[0:3],tth*180./n.pi
costth = n.cos(tth)
(Omega, Eta) = tools.find_omega_general(inp.param['wavelength']/(4.*n.pi)*Gw,
tth,
inp.values['wx']*n.pi/180,
inp.values['wy']*n.pi/180)
if len(Omega) > 0:
for solution in range(len(Omega)):
omega = Omega[solution]
eta = Eta[solution]
for i in range(len(inp.fit['w_limit'])//2):
if (inp.fit['w_limit'][2*i]*n.pi/180) < omega and\
omega < (inp.fit['w_limit'][2*i+1]*n.pi/180):
# form Omega rotation matrix
Om = tools.form_omega_mat_general(omega,inp.values['wx']*n.pi/180,inp.values['wy']*n.pi/180)
Gt = n.dot(Om,Gw)
# Calc crystal position at present omega
[tx,ty,tz]= n.dot(Om,gr_pos)
# Calc detector coordinate for peak
(dety, detz) = detector.det_coor(Gt,costth,
inp.param['wavelength'],
inp.param['distance'],
inp.param['y_size'],
inp.param['z_size'],
inp.param['y_center'],
inp.param['z_center'],
R,tx,ty,tz)
#If peak within detector frame store it in possible
if (-0.5 < dety) and\
(dety < inp.fit['dety_size']-0.5) and\
(-0.5 < detz) and\
(detz < inp.fit['detz_size']-0.5):
inp.possible[grainno].append([hkl[0],
hkl[1],
hkl[2],
omega*180/n.pi,
dety,
detz,
tth,
eta])
def write_ubi(param):
'''
Construct UBI matrices for each voxel and save them to file.
If the voxels have been mapped to grains we also output the grain average
UBI matrices.
'''
# If we specified which voxels belong to which grains
# we also get a per voxel average UBI file
if param['voxel_grain_map'] is not None:
m = param['voxel_grain_map']
grain_U = {}
grain_eps = {}
#Loop over grain id:s (val = grain number)
for val in m.values():
if (val not in grain_U.keys()) and (val not in grain_eps.keys()) :
#construct dictionary where the key is grain number and the value is the
#list of properties of the voxels populating that grain
grain_U[val] = []
grain_eps[val] = []
#loop over all voxels and fill up the dictionaries
for voxel in range(param['no_voxels']):
voxelId = param['voxel_list'][voxel]
U = param['U_voxels_%s' % voxelId]
gr_eps = n.array(param['eps_voxels_%s' % voxelId])
voxel_grain_id = m[voxelId]
grain_U[voxel_grain_id].append(U)
grain_eps[voxel_grain_id].append(gr_eps)
filename = '%s/grain_average_%s.ubi' %(param['direc'],param['stem'])
with open(filename,'w') as f:
format = "%f "*3 + "\n"
for voxel in grain_U.keys():
avg_U = n.zeros((3,3))
avg_eps = n.array([0.,0.,0.,0.,0.,0.])
for U,eps in zip(grain_U[voxel],grain_eps[voxel]):
avg_U += U
avg_eps += eps
avg_U[:,0] = avg_U[:,0]/n.linalg.norm(avg_U[:,0])
avg_U[:,1] = avg_U[:,1]/n.linalg.norm(avg_U[:,1])
avg_U[:,2] = avg_U[:,2]/n.linalg.norm(avg_U[:,2])
avg_eps = avg_eps/len(grain_eps[voxel])
#TODO: implement several phases!
if len(param['phase_list'])>1:
raise ValueError('Currently only single phase simulations are supported')
phase = param['phase_list'][0]
avg_B = tools.epsilon_to_b(avg_eps,param['unit_cell_phase_%i' %phase])/(2*n.pi)
avg_UBI = n.linalg.inv(n.dot(avg_U,avg_B))
for j in range(3):
out = format %(avg_UBI[j,0],avg_UBI[j,1],avg_UBI[j,2])
f.write(out)
out = "\n"
f.write(out)
filename = '%s/voxel_%s.ubi' %(param['direc'],param['stem'])
with open(filename,'w') as f:
format = "%f "*3 + "\n"
for i in range(param['no_voxels']):
U = param['U_voxels_%s' %(param['voxel_list'][i])]
gr_eps = n.array(param['eps_voxels_%s' %(param['voxel_list'][i])])
if param['no_phases'] == 1:
phase = param['phase_list'][0]
else:
phase = param['phase_voxels_%s' %(param['voxel_list'][i])]
# Clculate the B-matrix based on the strain tensor for each voxel
B = tools.epsilon_to_b(gr_eps,param['unit_cell_phase_%i' %phase])/(2*n.pi)
UBI = n.linalg.inv(n.dot(U,B))
for j in range(3):
out = format %(UBI[j,0],UBI[j,1],UBI[j,2])
f.write(out)
out = "\n"
f.write(out)
def write_voxels(param):
'''
Save the generated voxel parameters, pos, U and eps
INPUT: The parameter set from the input file and the voxel generator
OUTPUT: voxelno x y z phi1 PHI phi2 U11 U12 U13 U21 U22 U23 U31 U32 U33 eps11 eps12 eps13 eps22 eps23 eps33
'''
filename = '%s/%s.gff' %(param['direc'],param['stem'])
with open(filename,'w') as f:
# format = "%d "*1 + "%f "*1 + "%e"*1 + "%f"*18 + "\n"
format = "%d "*1 + "%d "*1 + "%f "*1 + "%e "*1 + "%f "*6 + "%0.12f "*9 + "%0.12f "*9 + "%e "*6 +"\n"
out = "# voxel_id phase_id voxelsize voxelvolume x y z phi1 PHI phi2 U11 U12 U13 U21 U22 U23 U31 U32 U33 UBI11 UBI12 UBI13 UBI21 UBI22 UBI23 UBI31 UBI32 UBI33 eps11 eps12 eps13 eps22 eps23 eps33 \n"
f.write(out)
for i in range(param['no_voxels']):
euler = 180/n.pi*tools.u_to_euler(param['U_voxels_%s' %(param['voxel_list'][i])])
if len(param['phase_list']) == 1:
phase = param['phase_list'][0]
else:
phase = param['phase_voxels_%s' %(param['voxel_list'][i])]
b = tools.epsilon_to_b(param['eps_voxels_%s' %(param['voxel_list'][i])],
param['unit_cell_phase_%i' %phase ])
u = param['U_voxels_%s' %(param['voxel_list'][i])]
ubi = n.linalg.inv(n.dot(u,b))*2*n.pi
out = format %(param['voxel_list'][i],
phase,
param['size_voxels_%s' %(param['voxel_list'][i])],
n.pi/6*(param['size_voxels_%s' %(param['voxel_list'][i])])**3.,
param['pos_voxels_%s' %(param['voxel_list'][i])][0],
param['pos_voxels_%s' %(param['voxel_list'][i])][1],
param['pos_voxels_%s' %(param['voxel_list'][i])][2],
euler[0],
euler[1],
euler[2],
param['U_voxels_%s' %(param['voxel_list'][i])][0,0],
param['U_voxels_%s' %(param['voxel_list'][i])][0,1],
param['U_voxels_%s' %(param['voxel_list'][i])][0,2],
param['U_voxels_%s' %(param['voxel_list'][i])][1,0],
param['U_voxels_%s' %(param['voxel_list'][i])][1,1],
param['U_voxels_%s' %(param['voxel_list'][i])][1,2],
param['U_voxels_%s' %(param['voxel_list'][i])][2,0],
param['U_voxels_%s' %(param['voxel_list'][i])][2,1],
param['U_voxels_%s' %(param['voxel_list'][i])][2,2],
ubi[0,0],
ubi[0,1],
ubi[0,2],
ubi[1,0],
ubi[1,1],
ubi[1,2],
ubi[2,0],
ubi[2,1],
ubi[2,2],
param['eps_voxels_%s' %(param['voxel_list'][i])][0],
param['eps_voxels_%s' %(param['voxel_list'][i])][1],
param['eps_voxels_%s' %(param['voxel_list'][i])][2],
param['eps_voxels_%s' %(param['voxel_list'][i])][3],
param['eps_voxels_%s' %(param['voxel_list'][i])][4],
param['eps_voxels_%s' %(param['voxel_list'][i])][5],
)
f.write(out)
def run(self):
spot_id = 0
# Generate orientations of the grains and loop over all grains
print('no of grains ', self.param['no_grains'])
for grainno in range(self.param['no_grains']):
A = []
U = self.param['U_grains_%s' % (self.param['grain_list'][grainno])]
if len(self.param['phase_list']) == 1:
phase = self.param['phase_list'][0]
else:
phase = self.param['phase_grains_%s' %
(self.param['grain_list'][grainno])]
unit_cell = self.param['unit_cell_phase_%i' % phase]
self.grain.append(variables.grain_cont(U))
gr_pos = n.array(self.param['pos_grains_%s' %
(self.param['grain_list'][grainno])])
gr_eps = n.array(self.param['eps_grains_%s' %
(self.param['grain_list'][grainno])])
# Calculate the B-matrix based on the strain tensor for each grain
B = tools.epsilon_to_b(gr_eps, unit_cell)
# add B matrix to grain container
self.grain[grainno].B = B
V = tools.cell_volume(unit_cell)
grain_vol = n.pi / 6 * self.param[
'size_grains_%s' % self.param['grain_list'][grainno]]**3
# print 'GRAIN NO: ',self.param['grain_list'][grainno]
# print 'GRAIN POSITION of grain ',self.param['grain_list'][grainno],': ',gr_pos
# print 'STRAIN TENSOR COMPONENTS (e11 e12 e13 e22 e23 e33) of grain ',self.param['grain_list'][grainno],':\n',gr_eps
# print 'U of grain ',self.param['grain_list'][grainno],':\n',U
nrefl = 0
# Calculate these values:
# totalnr, grainno, refno, hkl, omega, 2theta, eta, dety, detz
# For all reflections in Ahkl that fulfill omega_start < omega < omega_end.
# All angles in Grain are in degrees
for hkl in self.hkl[self.param['phase_list'].index(phase)]:
check_input.interrupt(self.killfile)
Gc = n.dot(B, hkl[0:3])
Gw = n.dot(self.S, n.dot(U, Gc))
tth = tools.tth2(Gw, self.param['wavelength'])
costth = n.cos(tth)
(Omega, Eta) = tools.find_omega_general(
Gw * self.param['wavelength'] / (4. * n.pi), tth, self.wx,
self.wy)
if len(Omega) > 0:
for solution in range(len(Omega)):
omega = Omega[solution]
eta = Eta[solution]
if (self.param['omega_start']*n.pi/180) < omega and\
omega < (self.param['omega_end']*n.pi/180):
# form Omega rotation matrix
Om = tools.form_omega_mat_general(
omega, self.wx, self.wy)
Gt = n.dot(Om, Gw)
# Calc crystal position at present omega and continue if this is outside the illuminated volume
[tx, ty, tz] = n.dot(Om, gr_pos)
if self.param['beam_width'] != None:
if n.abs(ty) > self.param['beam_width'] / 2.:
continue
# Calc detector coordinate for peak
(dety, detz) = detector.det_coor(
Gt, costth, self.param['wavelength'],
self.param['distance'], self.param['y_size'],
self.param['z_size'],
self.param['dety_center'],
self.param['detz_center'], self.R, tx, ty, tz)
#If shoebox extends outside detector exclude it
if (-0.5 > dety) or\
(dety > self.param['dety_size']-0.5) or\
(-0.5 > detz) or\
(detz > self.param['detz_size']-0.5):
continue
if self.param['spatial'] != None:
# To match the coordinate system of the spline file
(x, y) = detector.detyz_to_xy(
[dety, detz], self.param['o11'],
self.param['o12'], self.param['o21'],
self.param['o22'], self.param['dety_size'],
self.param['detz_size'])
# Do the spatial distortion
(xd, yd) = self.spatial.distort(x, y)
# transform coordinates back to dety,detz
(detyd, detzd) = detector.xy_to_detyz(
[xd, yd], self.param['o11'],
self.param['o12'], self.param['o21'],
self.param['o22'], self.param['dety_size'],
self.param['detz_size'])
else:
detyd = dety
detzd = detz
if self.param['beampol_apply'] == 1:
#Polarization factor (Kahn, J. Appl. Cryst. (1982) 15, 330-337.)
rho = n.pi / 2.0 + eta + self.param[
'beampol_direct'] * n.pi / 180.0
P = 0.5 * (1 + costth*costth -\
self.param['beampol_factor']*n.cos(2*rho)*n.sin(tth)**2)
else:
P = 1.0
#Lorentz factor
if self.param['lorentz_apply'] == 1:
if eta != 0:
L = 1 / (n.sin(tth) * abs(n.sin(eta)))
else:
L = n.inf
else:
L = 1.0
overlaps = 0 # set the number overlaps to zero
if self.param['intensity_const'] != 1:
intensity = int_intensity(
hkl[3], L, P, self.param['beamflux'],
self.param['wavelength'], V, grain_vol)
else:
intensity = hkl[3]
A.append([
self.param['grain_list'][grainno], nrefl,
spot_id, hkl[0], hkl[1], hkl[2], tth, omega,
eta, dety, detz, detyd, detzd, Gw[0], Gw[1],
Gw[2], L, P, hkl[3], intensity, overlaps
])
nrefl = nrefl + 1
spot_id = spot_id + 1
# print 'Length of Grain', len(self.grain[0].refl)
A = n.array(A)
if len(A) > 0:
# sort rows according to omega
A = A[n.argsort(A, 0)[:, A_id['omega']], :]
# Renumber the reflections
A[:, A_id['ref_id']] = n.arange(nrefl)
# Renumber the spot_id
A[:,
A_id['spot_id']] = n.arange(n.min(A[:, A_id['spot_id']]),
n.max(A[:, A_id['spot_id']]) + 1)
else:
A = n.zeros((0, len(A_id)))
# save reflection info in grain container
self.grain[grainno].refs = A
print('\rDone %3i grain(s) of %3i' %
(grainno + 1, self.param['no_grains']),
end=' ')
sys.stdout.flush()
print('\n')
