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authorepapoutsellis <epapoutsellis@gmail.com>2019-04-25 17:43:16 +0100
committerepapoutsellis <epapoutsellis@gmail.com>2019-04-25 17:43:16 +0100
commitfb6f44dff00c194e4936f39e4be8d0f22e8fe4da (patch)
tree3cd868266414506b5cb8f491bd9b35cfec6559db
parent36c36aa4395eb7625b28180bdd6bd376ae2017a7 (diff)
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TV dynamic tomo
-rw-r--r--Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D_time.py169
-rw-r--r--Wrappers/Python/wip/pdhg_TV_tomography2D_time.py4
2 files changed, 171 insertions, 2 deletions
diff --git a/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D_time.py b/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D_time.py
new file mode 100644
index 0000000..045458a
--- /dev/null
+++ b/Wrappers/Python/wip/Demos/PDHG_TV_Tomo2D_time.py
@@ -0,0 +1,169 @@
+# -*- 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
+from ccpi.optimisation.functions import ZeroFunction, KullbackLeibler, \
+ MixedL21Norm, BlockFunction
+
+from ccpi.astra.ops import AstraProjectorMC
+
+import os
+import tomophantom
+from tomophantom import TomoP2D
+
+# Create phantom for TV 2D dynamic tomography
+
+model = 102 # note that the selected model is temporal (2D + time)
+N = 50 # set dimension of the phantom
+# one can specify an exact path to the parameters file
+# path_library2D = '../../../PhantomLibrary/models/Phantom2DLibrary.dat'
+path = os.path.dirname(tomophantom.__file__)
+path_library2D = os.path.join(path, "Phantom2DLibrary.dat")
+#This will generate a N_size x N_size x Time frames phantom (2D + time)
+phantom_2Dt = TomoP2D.ModelTemporal(model, N, path_library2D)
+
+plt.close('all')
+plt.figure(1)
+plt.rcParams.update({'font.size': 21})
+plt.title('{}''{}'.format('2D+t phantom using model no.',model))
+for sl in range(0,np.shape(phantom_2Dt)[0]):
+ im = phantom_2Dt[sl,:,:]
+ plt.imshow(im, vmin=0, vmax=1)
+ plt.pause(.1)
+ plt.draw
+
+
+ig = ImageGeometry(voxel_num_x = N, voxel_num_y = N, channels = np.shape(phantom_2Dt)[0])
+data = ImageData(phantom_2Dt, geometry=ig)
+
+detectors = N
+angles = np.linspace(0,np.pi,N)
+
+ag = AcquisitionGeometry('parallel','2D', angles, detectors, channels = np.shape(phantom_2Dt)[0])
+Aop = AstraProjectorMC(ig, ag, 'gpu')
+sin = Aop.direct(data)
+
+scale = 2
+n1 = scale * np.random.poisson(sin.as_array()/scale)
+noisy_data = AcquisitionData(n1, ag)
+
+tindex = [3, 6, 10]
+
+fig, axes = plt.subplots(nrows=1, ncols=3, figsize=(10, 10))
+plt.subplot(1,3,1)
+plt.imshow(noisy_data.as_array()[tindex[0],:,:])
+plt.axis('off')
+plt.title('Time {}'.format(tindex[0]))
+plt.subplot(1,3,2)
+plt.imshow(noisy_data.as_array()[tindex[1],:,:])
+plt.axis('off')
+plt.title('Time {}'.format(tindex[1]))
+plt.subplot(1,3,3)
+plt.imshow(noisy_data.as_array()[tindex[2],:,:])
+plt.axis('off')
+plt.title('Time {}'.format(tindex[2]))
+
+fig.subplots_adjust(bottom=0.1, top=0.9, left=0.1, right=0.8,
+ wspace=0.02, hspace=0.02)
+
+plt.show()
+
+#%%
+# Regularisation Parameter
+alpha = 5
+
+# Create operators
+#op1 = Gradient(ig)
+op1 = Gradient(ig, correlation='SpaceChannels')
+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 = 200
+pdhg.run(2000)
+
+
+#%%
+fig, axes = plt.subplots(nrows=2, ncols=3, figsize=(10, 8))
+
+plt.subplot(2,3,1)
+plt.imshow(phantom_2Dt[tindex[0],:,:],vmin=0, vmax=1)
+plt.axis('off')
+plt.title('Time {}'.format(tindex[0]))
+
+plt.subplot(2,3,2)
+plt.imshow(phantom_2Dt[tindex[1],:,:],vmin=0, vmax=1)
+plt.axis('off')
+plt.title('Time {}'.format(tindex[1]))
+
+plt.subplot(2,3,3)
+plt.imshow(phantom_2Dt[tindex[2],:,:],vmin=0, vmax=1)
+plt.axis('off')
+plt.title('Time {}'.format(tindex[2]))
+
+
+plt.subplot(2,3,4)
+plt.imshow(pdhg.get_output().as_array()[tindex[0],:,:])
+plt.axis('off')
+plt.subplot(2,3,5)
+plt.imshow(pdhg.get_output().as_array()[tindex[1],:,:])
+plt.axis('off')
+plt.subplot(2,3,6)
+plt.imshow(pdhg.get_output().as_array()[tindex[2],:,:])
+plt.axis('off')
+im = plt.imshow(pdhg.get_output().as_array()[tindex[0],:,:])
+
+
+fig.subplots_adjust(bottom=0.1, top=0.9, left=0.1, right=0.8,
+ wspace=0.02, hspace=0.02)
+
+cb_ax = fig.add_axes([0.83, 0.1, 0.02, 0.8])
+cbar = fig.colorbar(im, cax=cb_ax)
+
+
+plt.show()
+
diff --git a/Wrappers/Python/wip/pdhg_TV_tomography2D_time.py b/Wrappers/Python/wip/pdhg_TV_tomography2D_time.py
index dea8e5c..5423b22 100644
--- a/Wrappers/Python/wip/pdhg_TV_tomography2D_time.py
+++ b/Wrappers/Python/wip/pdhg_TV_tomography2D_time.py
@@ -16,7 +16,7 @@ import matplotlib.pyplot as plt
from ccpi.optimisation.algorithms import PDHG, PDHG_old
from ccpi.optimisation.operators import BlockOperator, Identity, Gradient
-from ccpi.optimisation.functions import ZeroFun, L2NormSquared, \
+from ccpi.optimisation.functions import ZeroFunction, L2NormSquared, \
MixedL21Norm, BlockFunction, ScaledFunction
from ccpi.astra.ops import AstraProjectorSimple, AstraProjectorMC
@@ -100,7 +100,7 @@ operator = BlockOperator(op1, op2, shape=(2,1) )
alpha = 50
f = BlockFunction( alpha * MixedL21Norm(), \
0.5 * L2NormSquared(b = noisy_data) )
-g = ZeroFun()
+g = ZeroFunction()
# Compute operator Norm
normK = operator.norm()