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authorepapoutsellis <epapoutsellis@gmail.com>2019-04-25 11:22:14 +0100
committerepapoutsellis <epapoutsellis@gmail.com>2019-04-25 11:22:14 +0100
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TV, TGV Tomo
Diffstat (limited to 'Wrappers/Python')
-rw-r--r--Wrappers/Python/wip/Demos/PDHG_TGV_Tomo2D.py124
-rw-r--r--Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D.py211
2 files changed, 335 insertions, 0 deletions
diff --git a/Wrappers/Python/wip/Demos/PDHG_TGV_Tomo2D.py b/Wrappers/Python/wip/Demos/PDHG_TGV_Tomo2D.py
new file mode 100644
index 0000000..26578bb
--- /dev/null
+++ b/Wrappers/Python/wip/Demos/PDHG_TGV_Tomo2D.py
@@ -0,0 +1,124 @@
+# -*- coding: utf-8 -*-
+# This work is part of the Core Imaging Library developed by
+# Visual Analytics and Imaging System Group of the Science Technology
+# Facilities Council, STFC
+
+# Copyright 2018-2019 Evangelos Papoutsellis and Edoardo Pasca
+
+# Licensed under the Apache License, Version 2.0 (the "License");
+# you may not use this file except in compliance with the License.
+# You may obtain a copy of the License at
+
+# http://www.apache.org/licenses/LICENSE-2.0
+
+# Unless required by applicable law or agreed to in writing, software
+# distributed under the License is distributed on an "AS IS" BASIS,
+# WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+# See the License for the specific language governing permissions and
+# limitations under the License.
+
+from ccpi.framework import ImageData, ImageGeometry, AcquisitionGeometry, AcquisitionData
+
+import numpy as np
+import numpy
+import matplotlib.pyplot as plt
+
+from ccpi.optimisation.algorithms import PDHG
+
+from ccpi.optimisation.operators import BlockOperator, Gradient, Identity, \
+ SymmetrizedGradient, ZeroOperator
+from ccpi.optimisation.functions import ZeroFunction, KullbackLeibler, \
+ MixedL21Norm, BlockFunction
+
+from ccpi.astra.ops import AstraProjectorSimple
+
+# Create phantom for TV 2D tomography
+N = 75
+
+data = np.zeros((N,N))
+
+x1 = np.linspace(0, int(N/2), N)
+x2 = np.linspace(int(N/2), 0., N)
+xv, yv = np.meshgrid(x1, x2)
+
+xv[int(N/4):int(3*N/4)-1, int(N/4):int(3*N/4)-1] = yv[int(N/4):int(3*N/4)-1, int(N/4):int(3*N/4)-1].T
+data = xv
+data = ImageData(data/data.max())
+
+ig = ImageGeometry(voxel_num_x = N, voxel_num_y = N)
+
+detectors = N
+angles = np.linspace(0, np.pi, N, dtype=np.float32)
+
+ag = AcquisitionGeometry('parallel','2D',angles, detectors)
+Aop = AstraProjectorSimple(ig, ag, 'cpu')
+sin = Aop.direct(data)
+
+# Create noisy data. Apply Poisson noise
+scale = 0.1
+np.random.seed(5)
+n1 = scale * np.random.poisson(sin.as_array()/scale)
+noisy_data = AcquisitionData(n1, ag)
+
+
+plt.imshow(noisy_data.as_array())
+plt.show()
+#%%
+# Regularisation Parameters
+alpha = 0.7
+beta = 2
+
+# Create Operators
+op11 = Gradient(ig)
+op12 = Identity(op11.range_geometry())
+
+op22 = SymmetrizedGradient(op11.domain_geometry())
+op21 = ZeroOperator(ig, op22.range_geometry())
+
+op31 = Aop
+op32 = ZeroOperator(op22.domain_geometry(), ag)
+
+operator = BlockOperator(op11, -1*op12, op21, op22, op31, op32, shape=(3,2) )
+
+f1 = alpha * MixedL21Norm()
+f2 = beta * MixedL21Norm()
+f3 = KullbackLeibler(noisy_data)
+f = BlockFunction(f1, f2, f3)
+g = ZeroFunction()
+
+# Compute operator Norm
+normK = operator.norm()
+
+# Primal & dual stepsizes
+sigma = 1
+tau = 1/(sigma*normK**2)
+
+
+# Setup and run the PDHG algorithm
+pdhg = PDHG(f=f,g=g,operator=operator, tau=tau, sigma=sigma, memopt=True)
+pdhg.max_iteration = 2000
+pdhg.update_objective_interval = 50
+pdhg.run(2000)
+
+plt.figure(figsize=(15,15))
+plt.subplot(3,1,1)
+plt.imshow(data.as_array())
+plt.title('Ground Truth')
+plt.colorbar()
+plt.subplot(3,1,2)
+plt.imshow(noisy_data.as_array())
+plt.title('Noisy Data')
+plt.colorbar()
+plt.subplot(3,1,3)
+plt.imshow(pdhg.get_output()[0].as_array())
+plt.title('TGV Reconstruction')
+plt.colorbar()
+plt.show()
+##
+plt.plot(np.linspace(0,N,N), data.as_array()[int(N/2),:], label = 'GTruth')
+plt.plot(np.linspace(0,N,N), pdhg.get_output()[0].as_array()[int(N/2),:], label = 'TGV reconstruction')
+plt.legend()
+plt.title('Middle Line Profiles')
+plt.show()
+
+
diff --git a/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D.py b/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D.py
new file mode 100644
index 0000000..0711e91
--- /dev/null
+++ b/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D.py
@@ -0,0 +1,211 @@
+# -*- coding: utf-8 -*-
+# This work is part of the Core Imaging Library developed by
+# Visual Analytics and Imaging System Group of the Science Technology
+# Facilities Council, STFC
+
+# Copyright 2018-2019 Evangelos Papoutsellis and Edoardo Pasca
+
+# Licensed under the Apache License, Version 2.0 (the "License");
+# you may not use this file except in compliance with the License.
+# You may obtain a copy of the License at
+
+# http://www.apache.org/licenses/LICENSE-2.0
+
+# Unless required by applicable law or agreed to in writing, software
+# distributed under the License is distributed on an "AS IS" BASIS,
+# WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+# See the License for the specific language governing permissions and
+# limitations under the License.
+
+from ccpi.framework import ImageData, ImageGeometry, AcquisitionGeometry, AcquisitionData
+
+import numpy as np
+import numpy
+import matplotlib.pyplot as plt
+
+from ccpi.optimisation.algorithms import PDHG
+
+from ccpi.optimisation.operators import BlockOperator, Identity, Gradient
+from ccpi.optimisation.functions import ZeroFunction, KullbackLeibler, \
+ MixedL21Norm, BlockFunction
+
+from ccpi.astra.ops import AstraProjectorSimple
+
+# Create phantom for TV 2D tomography
+N = 75
+x = np.zeros((N,N))
+x[round(N/4):round(3*N/4),round(N/4):round(3*N/4)] = 0.5
+x[round(N/8):round(7*N/8),round(3*N/8):round(5*N/8)] = 1
+
+data = ImageData(x)
+ig = ImageGeometry(voxel_num_x = N, voxel_num_y = N)
+
+detectors = N
+angles = np.linspace(0, np.pi, N, dtype=np.float32)
+
+ag = AcquisitionGeometry('parallel','2D',angles, detectors)
+Aop = AstraProjectorSimple(ig, ag, 'cpu')
+sin = Aop.direct(data)
+
+# Create noisy data. Apply Poisson noise
+scale = 2
+n1 = scale * np.random.poisson(sin.as_array()/scale)
+noisy_data = AcquisitionData(n1, ag)
+
+# Regularisation Parameter
+alpha = 5
+
+# Create operators
+op1 = Gradient(ig)
+op2 = Aop
+
+# Create BlockOperator
+operator = BlockOperator(op1, op2, shape=(2,1) )
+
+# Create functions
+
+f1 = alpha * MixedL21Norm()
+f2 = KullbackLeibler(noisy_data)
+f = BlockFunction(f1, f2)
+
+g = ZeroFunction()
+
+# Compute operator Norm
+normK = operator.norm()
+
+# Primal & dual stepsizes
+sigma = 1
+tau = 1/(sigma*normK**2)
+
+
+# Setup and run the PDHG algorithm
+pdhg = PDHG(f=f,g=g,operator=operator, tau=tau, sigma=sigma, memopt=True)
+pdhg.max_iteration = 2000
+pdhg.update_objective_interval = 50
+pdhg.run(2000)
+
+plt.figure(figsize=(15,15))
+plt.subplot(3,1,1)
+plt.imshow(data.as_array())
+plt.title('Ground Truth')
+plt.colorbar()
+plt.subplot(3,1,2)
+plt.imshow(noisy_data.as_array())
+plt.title('Noisy Data')
+plt.colorbar()
+plt.subplot(3,1,3)
+plt.imshow(pdhg.get_output().as_array())
+plt.title('TV Reconstruction')
+plt.colorbar()
+plt.show()
+##
+plt.plot(np.linspace(0,N,N), data.as_array()[int(N/2),:], label = 'GTruth')
+plt.plot(np.linspace(0,N,N), pdhg.get_output().as_array()[int(N/2),:], label = 'TV reconstruction')
+plt.legend()
+plt.title('Middle Line Profiles')
+plt.show()
+
+
+#%% Check with CVX solution
+
+from ccpi.optimisation.operators import SparseFiniteDiff
+import astra
+import numpy
+
+try:
+ from cvxpy import *
+ cvx_not_installable = True
+except ImportError:
+ cvx_not_installable = False
+
+
+if cvx_not_installable:
+
+
+ ##Construct problem
+ u = Variable(N*N)
+ #q = Variable()
+
+ DY = SparseFiniteDiff(ig, direction=0, bnd_cond='Neumann')
+ DX = SparseFiniteDiff(ig, direction=1, bnd_cond='Neumann')
+
+ regulariser = alpha * sum(norm(vstack([DX.matrix() * vec(u), DY.matrix() * vec(u)]), 2, axis = 0))
+
+ # create matrix representation for Astra operator
+
+ vol_geom = astra.create_vol_geom(N, N)
+ proj_geom = astra.create_proj_geom('parallel', 1.0, detectors, angles)
+
+ proj_id = astra.create_projector('strip', proj_geom, vol_geom)
+
+ matrix_id = astra.projector.matrix(proj_id)
+
+ ProjMat = astra.matrix.get(matrix_id)
+
+ fidelity = sum( ProjMat * u - noisy_data.as_array().ravel() * log(ProjMat * u))
+ #constraints = [q>= fidelity, u>=0]
+ constraints = [u>=0]
+
+ solver = SCS
+ obj = Minimize( regulariser + fidelity)
+ prob = Problem(obj, constraints)
+ result = prob.solve(verbose = True, solver = solver)
+
+
+##%% Check with CVX solution
+
+from ccpi.optimisation.operators import SparseFiniteDiff
+
+try:
+ from cvxpy import *
+ cvx_not_installable = True
+except ImportError:
+ cvx_not_installable = False
+
+
+if cvx_not_installable:
+
+ ##Construct problem
+ u = Variable(ig.shape)
+
+ DY = SparseFiniteDiff(ig, direction=0, bnd_cond='Neumann')
+ DX = SparseFiniteDiff(ig, direction=1, bnd_cond='Neumann')
+
+ # Define Total Variation as a regulariser
+ regulariser = alpha * sum(norm(vstack([DX.matrix() * vec(u), DY.matrix() * vec(u)]), 2, axis = 0))
+ fidelity = pnorm( u - noisy_data.as_array(),1)
+
+ # choose solver
+ if 'MOSEK' in installed_solvers():
+ solver = MOSEK
+ else:
+ solver = SCS
+
+ obj = Minimize( regulariser + fidelity)
+ prob = Problem(obj)
+ result = prob.solve(verbose = True, solver = solver)
+
+
+ plt.figure(figsize=(15,15))
+ plt.subplot(3,1,1)
+ plt.imshow(pdhg.get_output().as_array())
+ plt.title('PDHG solution')
+ plt.colorbar()
+ plt.subplot(3,1,2)
+ plt.imshow(np.reshape(u.value, (N, N)))
+ plt.title('CVX solution')
+ plt.colorbar()
+ plt.subplot(3,1,3)
+ plt.imshow(diff_cvx)
+ plt.title('Difference')
+ plt.colorbar()
+ plt.show()
+
+ plt.plot(np.linspace(0,N,N), pdhg.get_output().as_array()[int(N/2),:], label = 'PDHG')
+ plt.plot(np.linspace(0,N,N), u.value[int(N/2),:], label = 'CVX')
+ plt.legend()
+ plt.title('Middle Line Profiles')
+ plt.show()
+
+ print('Primal Objective (CVX) {} '.format(obj.value))
+ print('Primal Objective (PDHG) {} '.format(pdhg.objective[-1][0])) \ No newline at end of file