├── README.md
├── generate_Laguerre_Gauss_SLM.py
├── generate_Laguerre_Gauss_split_SLM.py
└── LICENSE
/README.md:
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1 | # python-SLM
2 | Set of routines in Python used to control a Spatial Light Modulator. It is assumed that the SLM is connected to a secondary monitor.
3 |
4 | **Important!!!** The code requires the following modules installed:
5 | * opencv
6 | * numpy
7 | * wxPython
8 | * slmpy (file that can be downloaded from [Sébastien's POPOFF](http://wavefrontshaping.net/index.php/57-community/tutorials/spatial-lights-modulators-slms/124-how-to-control-a-slm-with-python)) page.
9 |
10 | ## Files
11 |
12 | File | Description
13 | ------------ | -------------
14 | generate_Laguerre_Gauss_SLM.py | File that generates a phase mask for a LG beam and displays it on a SLM
15 | generate_Laguerre_Gauss_split_SLM.py | Program that splits the SLM into two equal regions. In each region is generated an independent phase mask of a LG beam
16 |
17 | ## Files description
18 | ### generate_Laguerre_Gauss_SLM.py
19 | The file generates a phase mask for a LG beam with a charge specified by the user. The mask can be saved as a bmp file, displayed on the main monitor, or can be sent to the SLM.
20 |
21 | #### How to use it
22 | To use the function, just write `python generate_Laguerre_Gauss_SLM.py [options]`, where the options are the following:
23 |
24 | * -c CHARGE sets the **CHARGE** of the LG beam.
25 | * -w RADIUS use this option to put a circular mask centered in the screen center with radius **RADIUS**.
26 | * -g PERIOD add a grating to the LG phase. The period in pixels is specified with the variable **PERIOD**.
27 | * -s when added the image generated is sent to the SLM (by default the phase mask is not sent to the SLM).
28 | * -m when added, the SLM correction mask provided by the manufacturer is applied to the phase mask.
29 | * -b when added, the image of the phase mask is stored in the bmp file "LG_ch_CHARGE.bmp", where **CHARGE** is specified with the option -c.
30 |
31 | The correction mask file has to be stored in the same folder as the python file. To change the mask file name, just change the line after the comment **change 'correctionMaskFile' according to your correction mask file**.
32 |
33 | To exit, press 'q' after clicking on the 'phase mask' window.
34 |
35 | #### Usage examples
36 | * Use `python generate_Laguerre_Gauss_SLM.py -c 10`, to generate a phase mask (LG beam charge +10) that is shown only in the main screen.
37 | * To save the image in a bmp file, use `python generate_Laguerre_Gauss_SLM.py -c 10 -b`. The file will be saved as **LG_ch_10.bmp**.
38 | * To generate and send to the SLM a phase mask for a LG beam with charge -5, use `python generate_Laguerre_Gauss_SLM.py -c -5 -m -s`. Notice that the option **-m** specifies to use the correction mask provided by the manufacturer.
39 |
40 | ### generate_Laguerre_Gauss_split_SLM.py
41 | Program that splits the SLM into two equal regions and in each region generates a phase mask of an independent Laguerre Gauss beam with a CHARGE provided by the user.
42 |
43 | The whole image is sent to the second monitor output where the SLM is connected. The mask generated is also shown in the main monitor in a small window.
44 |
45 | #### How to use it
46 | To use the function, just write `python generate_Laguerre_Gauss_split_SLM.py [options]`, where the options are the following:
47 |
48 | * -c CHARGE sets the **CHARGE** of the LG beam. Two indices are required.
49 | * -w RADIUS use this option to put a circular mask centered in the screen center with radius **RADIUS**.
50 | * -g PERIOD add a grating to the LG phase. The period in pixels is specified with the variable **PERIOD**. Two indices are required.
51 | * -s when added the image generated is sent to the SLM (by default the phase mask is not sent to the SLM).
52 | * -m when added, the SLM correction mask provided by the manufacturer is applied to the phase mask.
53 | * -b when added, the image of the phase mask is stored in the bmp file "LG_ch_CHARGE.bmp", where **CHARGE** is specified with the option -c.
54 |
55 | The correction mask file has to be stored in the same folder as the python file. To change the mask file name, just change the line after the comment **change 'correctionMaskFile' according to your correction mask file**.
56 |
57 | To exit, press 'q' after clicking on the 'phase mask' window.
58 |
59 | #### Usage examples:
60 |
61 | * Use `python generate_Laguerre_Gauss_split_SLM.py -c 10 -5`, to split the screen into two regions | LG +10 | LG -5 |. In the left (right) region, a LG beam with charge +10 (-5) is displayed.
62 | * To send to the image generated in the previous example to the SLM, just add **-s** at the end. That is `python generate_Laguerre_Gauss_split_SLM.py -c 10 -5 -s`
63 | * To save a mask generated, use the command **-m**. The command `python generate_Laguerre_Gauss_split_SLM.py -c 10 -5 -b`. Saves the image in the bmp file **LG_ch_chargeLeft_chargeRight.bmp**; in this case **LG_ch_10_-5.bmp**.
64 |
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/generate_Laguerre_Gauss_SLM.py:
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1 | # -*- coding: utf-8 -*-
2 | """
3 | Created on Fri Aug 26 16:07:20 2016
4 |
5 | Filename: generate_Laguerre_Gauss_SLM.py
6 |
7 | Author:Luis José Salazar-Serrano
8 | totesalaz@gmail.com / luis-jose.salazar@icfo.es
9 | http://opensourcelab.salazarserrano.com
10 |
11 | Description:
12 |
13 | Program that generates a phase mask of a Laguerre Gauss beam with a CHARGE
14 | provided by the user. The mask is sent to the second monitor output where the SLM is
15 | connected. The mask generated is also shown in the main monitor in a small window.
16 |
17 | To use the program:
18 |
19 | >> python generate_Laguerre_Gauss_SLM.py [list of arguments] where:
20 |
21 | -c CHARGE sets the CHARGE of the LG beam.
22 | -w RADIUS use this option to put a circular mask centered in the screen center.
23 | -g PERIOD add a grating to the LG phase. The period in pixels is specified with the variable PERIOD.
24 |
25 | -s when added the image generated is sent to the SLM
26 | -m when added, the SLM correction mask provided by the manufacturer is applied to the phase mask.
27 | -b when added, the image of the phase mask is stored in the bmp file "LG_ch_CHARGE.bmp"
28 |
29 | The code requires the library slmpy.py, written by Sébastien Popoff that can be found on the link
30 | http://wavefrontshaping.net/index.php/57-community/tutorials/spatial-lights-modulators-slms/124-how-to-control-a-slm-with-python
31 |
32 | Usage examples:
33 |
34 | >>python LaguerreGauss.py -c 10 (image generated is not sent to the SLM)
35 | >>python LaguerreGauss.py -c 10 -b (add -b to save image as LG_ch_10.bmp)
36 | >>python LaguerreGauss.py -c -5 -m -s (LG beam charge -5, use correction mask and image sent to SLM)
37 |
38 | To exit, press 'q' after clicking on the 'phase mask' window.
39 |
40 | """
41 |
42 | import argparse
43 | import cv2
44 | import numpy as np
45 | import scipy.misc
46 | import slmpy
47 |
48 | # construct the argument parse and parse the arguments
49 | ap = argparse.ArgumentParser()
50 | ap.add_argument("-c", "--charge", help="LG beam charge (default = 1)", type=int, default = 1)
51 | ap.add_argument("-w", "--window", help="mask window radius (default = 0)", type=int, default = 0)
52 | ap.add_argument("-g", "--grating", help="grating period (default = 0)", type=int, default = 0)
53 |
54 | feature_parser = ap.add_mutually_exclusive_group(required=False)
55 | feature_parser.add_argument("-s","--slm", help="send image to SLM", action='store_true')
56 |
57 | feature_parser = ap.add_mutually_exclusive_group(required=False)
58 | feature_parser.add_argument("-m","--mask", help="apply correction mask", action='store_true')
59 |
60 | feature_parser = ap.add_mutually_exclusive_group(required=False)
61 | feature_parser.add_argument("-b","--bmp", help="save *.bmp file", action='store_true')
62 |
63 | args = vars(ap.parse_args())
64 |
65 | beamCharge = args["charge"]
66 | saveFlag = args["bmp"]
67 | slmFlag = args["slm"]
68 | correctionFlag = args["mask"]
69 | maskRadius = np.abs(args["window"])
70 | gratingPeriod = args["grating"]
71 |
72 | fileStr = 'LG_ch_' + str(beamCharge) + '.bmp'
73 |
74 | # change 'correctionMaskFile' according to your correction mask file
75 | correctionMaskFile = 'CAL_LSH0600780_633nm.bmp';
76 |
77 | # generate phase mask for LG beam
78 | def generate_LG_Mask(beamCharge):
79 |
80 | if beamCharge == 0:
81 | image = np.zeros([ImgResY, ImgResX])
82 | else:
83 | image = np.angle(np.exp((beamCharge*np.angle(X+Y*1j))*1j))
84 |
85 | image8bit = normalize_image(image)
86 |
87 | return image8bit
88 |
89 | def generate_displaced_LG_Mask(beamCharge, gratingPeriod):
90 |
91 | # if period = 0 ... show zero phase mask
92 | if gratingPeriod == 0:
93 | image = np.zeros([ImgResY, ImgResX])
94 | # if period > 0 ... shift beam to the RIGHT wrt period = 0
95 | elif gratingPeriod > 0:
96 | image = np.angle(np.exp((2*np.pi*X/gratingPeriod)*1j)*np.exp((beamCharge*np.angle(X+Y*1j))*1j))
97 | # if period < 0 ... shift beam to the LEFT wrt period = 0
98 | elif gratingPeriod < 0:
99 | image = np.angle(np.exp((2*np.pi*X/gratingPeriod+np.pi)*1j)*np.exp((beamCharge*np.angle(X+Y*1j))*1j))
100 |
101 | image8bit = normalize_image(image)
102 |
103 | return image8bit
104 |
105 | # normalize image to range [0, 1]
106 | def normalize_image(image):
107 | img = cv2.normalize(image, alpha=0, beta=1, norm_type=cv2.NORM_MINMAX, dtype=cv2.CV_32F)
108 | image8bit = np.round((2**8-1)*(img)).astype('uint8')
109 |
110 | return image8bit
111 |
112 | def apply_correction_mask(image):
113 |
114 | SLMcorrectionMask = np.zeros((ImgResY, ImgResX), dtype = "uint8")
115 |
116 | SLMbmpMask = cv2.imread(correctionMaskFile)
117 | SLMbmpMask = cv2.cvtColor(SLMbmpMask, cv2.COLOR_BGR2GRAY)
118 |
119 | rows,cols = SLMbmpMask.shape
120 |
121 | SLMcorrectionMask[0:rows, 0:cols] = SLMbmpMask
122 |
123 | return SLMcorrectionMask+image
124 |
125 | if slmFlag == True:
126 | # create the object that handles the SLM array
127 | slm = slmpy.SLMdisplay(isImageLock = True)
128 |
129 | # retrieve SLM resolution (defined in monitor options)
130 | ImgResX, ImgResY = slm.getSize()
131 | else:
132 |
133 | ImgResX = 792
134 | ImgResY = 600
135 |
136 | ImgCenterX = ImgResX/2
137 | ImgCenterY = ImgResY/2
138 |
139 | x = np.linspace(0,ImgResX,ImgResX)
140 | y = np.linspace(0,ImgResY,ImgResY)
141 |
142 | # initialize image matrix
143 | X, Y = np.meshgrid(x,y)
144 |
145 | X = X - ImgCenterX
146 | Y = Y - ImgCenterY
147 |
148 | # generate circular window mask
149 | maskCircle = np.zeros((ImgResY, ImgResX), dtype = "uint8")
150 | cv2.circle(maskCircle, (ImgCenterX, ImgCenterY), maskRadius, 255, -1)
151 | maskCircle = normalize_image(maskCircle)
152 |
153 | if slmFlag != True:
154 |
155 | if gratingPeriod != 0:
156 | image8bit = generate_displaced_LG_Mask(beamCharge, gratingPeriod)
157 | else:
158 | image8bit = generate_LG_Mask(beamCharge)
159 |
160 | if maskRadius > 0:
161 | image8bit = cv2.bitwise_and(image8bit, image8bit, mask = maskCircle)
162 |
163 | # apply SLM correction mask provided by manufacturer
164 | if correctionFlag == True:
165 | image8bit = apply_correction_mask(image8bit)
166 |
167 | cv2.imshow('phase hologram',image8bit)
168 | cv2.waitKey()
169 |
170 | if saveFlag == True:
171 | scipy.misc.imsave(fileStr, image8bit)
172 | print "file: " + fileStr + " saved! Press any key to continue."
173 |
174 | else:
175 |
176 | while True:
177 |
178 | if gratingPeriod != 0:
179 | image8bit = generate_displaced_LG_Mask(beamCharge, gratingPeriod)
180 | else:
181 | image8bit = generate_LG_Mask(beamCharge)
182 |
183 | if maskRadius > 0:
184 | image8bit = cv2.bitwise_and(image8bit, image8bit, mask = maskCircle)
185 |
186 | # apply SLM correction mask provided by manufacturer
187 | if correctionFlag == True:
188 | image8bit = apply_correction_mask(image8bit)
189 |
190 | image = cv2.resize(image8bit,(320, 240), interpolation = cv2.INTER_CUBIC)
191 | image = cv2.cvtColor(image, cv2.COLOR_GRAY2BGR)
192 | cv2.putText(image, "press q to exit...", (10, 20), cv2.FONT_HERSHEY_SIMPLEX, 0.7, (0,0,255), 2)
193 |
194 | # display image on window
195 | cv2.imshow('Phase mask',image)
196 |
197 | # send image to SLM
198 | slm.updateArray(image8bit)
199 |
200 | # press 'q' to exit
201 | key = cv2.waitKey(33)
202 | if key == ord('q'):
203 | break
204 |
205 | slm.close()
206 | cv2.destroyAllWindows()
207 |
208 |
209 |
210 |
211 |
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/generate_Laguerre_Gauss_split_SLM.py:
--------------------------------------------------------------------------------
1 | # -*- coding: utf-8 -*-
2 | """
3 | Created on Fri Aug 26 16:07:20 2016
4 |
5 | Filename: generate_Laguerre_Gauss_split_SLM.py
6 |
7 | Author:Luis José Salazar-Serrano
8 | totesalaz@gmail.com / luis-jose.salazar@icfo.es
9 | http://opensourcelab.salazarserrano.com
10 |
11 | Description:
12 |
13 | Program that splits the SLM into two equal regions and in each region generates
14 | a phase mask of a Laguerre Gauss beam with a CHARGE provided by the user.
15 |
16 | The whole image is sent to the second monitor output where the SLM is
17 | connected. The mask generated is also shown in the main monitor in a small window.
18 |
19 | To use the program:
20 |
21 | >> python generate_Laguerre_Gauss_SLM.py [list of arguments] where:
22 |
23 | -c CHARGE sets the CHARGE of the LG beam.
24 | -w RADIUS use this option to put a circular mask centered in the screen center.
25 | -g PERIOD add a grating to the LG phase. The period in pixels is specified with the variable PERIOD.
26 |
27 | -s when added the image generated is sent to the SLM
28 | -m when added, the SLM correction mask provided by the manufacturer is applied to the phase mask.
29 | -b when added, the image of the phase mask is stored in the bmp file "LG_ch_CHARGE.bmp"
30 |
31 | The code requires the library slmpy.py, written by Sébastien Popoff that can be found on the link
32 | http://wavefrontshaping.net/index.php/57-community/tutorials/spatial-lights-modulators-slms/124-how-to-control-a-slm-with-python
33 |
34 | Usage examples:
35 |
36 | >>python LaguerreGauss.py -c 10 -5 (SLM split in two masks | LG +10 | LG -5 |. The image generated is not sent to the SLM)
37 | >>python LaguerreGauss.py -c 10 -5 -b (add -b to save image as LG_ch_10_-5.bmp)
38 | >>python LaguerreGauss.py -c 10 -5 -m -s (image sent to SLM)
39 |
40 | To exit, press 'q' after clicking on the 'phase mask' window.
41 |
42 | """
43 |
44 | import argparse
45 | import cv2
46 | import numpy as np
47 | import scipy.misc
48 | import slmpy
49 | import imutils
50 |
51 | # construct the argument parse and parse the arguments
52 | ap = argparse.ArgumentParser()
53 | ap.add_argument('-c', '--charge', nargs='+', type=int, default= [10,10])
54 | ap.add_argument("-w", "--window", help="mask window radius (default = 0)", type=int, default = 0)
55 | ap.add_argument("-g", "--grating", nargs='+', type=int, default= [0,0])
56 |
57 | feature_parser = ap.add_mutually_exclusive_group(required=False)
58 | feature_parser.add_argument("-s","--slm", help="send image to SLM", action='store_true')
59 |
60 | feature_parser = ap.add_mutually_exclusive_group(required=False)
61 | feature_parser.add_argument("-m","--mask", help="apply correction mask", action='store_true')
62 |
63 | feature_parser = ap.add_mutually_exclusive_group(required=False)
64 | feature_parser.add_argument("-b","--bmp", help="save *.bmp file", action='store_true')
65 |
66 | args = vars(ap.parse_args())
67 |
68 | beamCharge = args["charge"]
69 | saveFlag = args["bmp"]
70 | slmFlag = args["slm"]
71 | correctionFlag = args["mask"]
72 | maskRadius = np.abs(args["window"])
73 | gratingPeriod1 = args["grating"][0]
74 | gratingPeriod2 = args["grating"][1]
75 |
76 | beamCharge1 = args["charge"][0]
77 | beamCharge2 = args["charge"][1]
78 |
79 | fileStr = 'LG_ch_' + str(beamCharge1) + '_' + str(beamCharge2) + '.bmp'
80 |
81 | # change 'correctionMaskFile' according to your correction mask file
82 | correctionMaskFile = 'CAL_LSH0600780_633nm.bmp';
83 |
84 | # generate phase mask for LG beam
85 | def generate_LG_Mask(beamCharge):
86 |
87 | if beamCharge == 0:
88 | image = np.zeros([ImgResY, ImgResX])
89 | else:
90 | image = np.angle(np.exp((beamCharge*np.angle(X+Y*1j))*1j))
91 |
92 | image8bit = normalize_image(image)
93 |
94 | return image8bit
95 |
96 | def generate_displaced_LG_Mask(beamCharge, gratingPeriod):
97 |
98 | # if period = 0 ... show zero phase mask
99 | if gratingPeriod == 0:
100 | image = np.zeros([ImgResY, ImgResX])
101 | # if period > 0 ... shift beam to the RIGHT wrt period = 0
102 | elif gratingPeriod > 0:
103 | image = np.angle(np.exp((2*np.pi*X/gratingPeriod)*1j)*np.exp((beamCharge*np.angle(X+Y*1j))*1j))
104 | # if period < 0 ... shift beam to the LEFT wrt period = 0
105 | elif gratingPeriod < 0:
106 | image = np.angle(np.exp((2*np.pi*X/gratingPeriod+np.pi)*1j)*np.exp((beamCharge*np.angle(X+Y*1j))*1j))
107 |
108 | image8bit = normalize_image(image)
109 |
110 | return image8bit
111 |
112 | # normalize image to range [0, 1]
113 | def normalize_image(image):
114 | img = cv2.normalize(image, alpha=0, beta=1, norm_type=cv2.NORM_MINMAX, dtype=cv2.CV_32F)
115 | image8bit = np.round((2**8-1)*(img)).astype('uint8')
116 |
117 | return image8bit
118 |
119 | def apply_correction_mask(image):
120 |
121 | SLMcorrectionMask = np.zeros((ImgResY, ImgResX), dtype = "uint8")
122 |
123 | # mask exclusive for Hamamatsu SLM S/N LSH0600780
124 | SLMbmpMask = cv2.imread(correctionMaskFile)
125 |
126 | SLMbmpMask = cv2.cvtColor(SLMbmpMask, cv2.COLOR_BGR2GRAY)
127 |
128 | rows,cols = SLMbmpMask.shape
129 |
130 | SLMcorrectionMask[0:rows, 0:cols] = SLMbmpMask
131 |
132 | return SLMcorrectionMask+image
133 |
134 | if slmFlag == True:
135 | # create the object that handles the SLM array
136 | slm = slmpy.SLMdisplay(isImageLock = True)
137 |
138 | # retrieve SLM resolution (defined in monitor options)
139 | ImgResX, ImgResY = slm.getSize()
140 | else:
141 |
142 | ImgResX = 792
143 | ImgResY = 600
144 |
145 | ImgCenterX = ImgResX/2
146 | ImgCenterY = ImgResY/2
147 |
148 | x = np.linspace(0,ImgResX,ImgResX)
149 | y = np.linspace(0,ImgResY,ImgResY)
150 |
151 | # initialize image matrix
152 | X, Y = np.meshgrid(x,y)
153 |
154 | X = X - ImgCenterX
155 | Y = Y - ImgCenterY
156 |
157 | # generate circular window mask
158 | maskCircle = np.zeros((ImgResY, ImgResX), dtype = "uint8")
159 | cv2.circle(maskCircle, (ImgCenterX, ImgCenterY), maskRadius, 255, -1)
160 | maskCircle = normalize_image(maskCircle)
161 |
162 | # generate and apply squared mask to image8bit
163 | windowSize = ImgResX/2
164 | maskWindow = np.zeros((ImgResY, ImgResX), dtype = "uint8")
165 | cv2.rectangle(maskWindow, (ImgCenterX-windowSize/2, ImgCenterY-windowSize/2), (ImgCenterX+windowSize/2, ImgCenterY+windowSize/2), 255, -1)
166 | maskWindow = normalize_image(maskWindow)
167 |
168 | if slmFlag != True:
169 |
170 | if gratingPeriod1 or gratingPeriod2 != 0:
171 |
172 | image8bit1 = generate_displaced_LG_Mask(beamCharge1, gratingPeriod1)
173 | image8bit2 = generate_displaced_LG_Mask(beamCharge2, gratingPeriod2)
174 |
175 | else:
176 |
177 | image8bit1 = generate_LG_Mask(beamCharge1)
178 | image8bit2 = generate_LG_Mask(beamCharge2)
179 |
180 | if maskRadius > 0:
181 | image8bit1 = cv2.bitwise_and(image8bit1, image8bit1 , mask = maskCircle)
182 | image8bit2 = cv2.bitwise_and(image8bit2, image8bit2 , mask = maskCircle)
183 | else:
184 | image8bit1 = cv2.bitwise_and(image8bit1, image8bit1 , mask = maskWindow)
185 | image8bit2 = cv2.bitwise_and(image8bit2, image8bit2 , mask = maskWindow)
186 |
187 | # translate the image x=100 pixels to the left and y=0 pixels up
188 | image8bit1 = imutils.translate(image8bit1, -ImgResX/4, 0)
189 | image8bit2 = imutils.translate(image8bit2, ImgResX/4, 0)
190 |
191 | image8bit = cv2.add(image8bit1,image8bit2)
192 |
193 | # apply SLM correction mask provided by manufacturer
194 | if correctionFlag == True:
195 | image8bit = apply_correction_mask(image8bit)
196 |
197 | cv2.imshow('phase hologram',image8bit)
198 | cv2.waitKey()
199 |
200 | if saveFlag == True:
201 | scipy.misc.imsave(fileStr, image8bit)
202 | print "file: " + fileStr + " saved! Press any key to continue."
203 |
204 | else:
205 |
206 | while True:
207 |
208 | if gratingPeriod1 or gratingPeriod2 != 0:
209 |
210 | image8bit1 = generate_displaced_LG_Mask(beamCharge1, gratingPeriod1)
211 | image8bit2 = generate_displaced_LG_Mask(beamCharge2, gratingPeriod2)
212 |
213 | else:
214 |
215 | image8bit1 = generate_LG_Mask(beamCharge1)
216 | image8bit2 = generate_LG_Mask(beamCharge2)
217 |
218 | if maskRadius > 0:
219 | image8bit1 = cv2.bitwise_and(image8bit1, image8bit1 , mask = maskCircle)
220 | image8bit2 = cv2.bitwise_and(image8bit2, image8bit2 , mask = maskCircle)
221 | else:
222 | image8bit1 = cv2.bitwise_and(image8bit1, image8bit1 , mask = maskWindow)
223 | image8bit2 = cv2.bitwise_and(image8bit2, image8bit2 , mask = maskWindow)
224 |
225 | # translate the image x=100 pixels to the left and y=0 pixels up
226 | image8bit1 = imutils.translate(image8bit1, -ImgResX/4, 0)
227 | image8bit2 = imutils.translate(image8bit2, ImgResX/4, 0)
228 |
229 | image8bit = cv2.add(image8bit1,image8bit2)
230 |
231 | # apply SLM correction mask provided by manufacturer
232 | if correctionFlag == True:
233 | image8bit = apply_correction_mask(image8bit)
234 |
235 | image = cv2.resize(image8bit,(320, 240), interpolation = cv2.INTER_CUBIC)
236 | image = cv2.cvtColor(image, cv2.COLOR_GRAY2BGR)
237 | cv2.putText(image, "press q to exit...", (10, 20), cv2.FONT_HERSHEY_SIMPLEX, 0.7, (0,0,255), 2)
238 |
239 | # display image on window
240 | cv2.imshow('SLM',image)
241 |
242 | # send image to SLM
243 | slm.updateArray(image8bit)
244 |
245 | # press 'q' to exit
246 | key = cv2.waitKey(33)
247 | if key == ord('q'):
248 | break
249 |
250 | slm.close()
251 | cv2.destroyAllWindows()
252 |
253 |
254 |
255 |
256 |
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1 | GNU GENERAL PUBLIC LICENSE
2 | Version 3, 29 June 2007
3 |
4 | Copyright (C) 2007 Free Software Foundation, Inc.
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585 | permissions. However, no additional obligations are imposed on any
586 | author or copyright holder as a result of your choosing to follow a
587 | later version.
588 |
589 | 15. Disclaimer of Warranty.
590 |
591 | THERE IS NO WARRANTY FOR THE PROGRAM, TO THE EXTENT PERMITTED BY
592 | APPLICABLE LAW. EXCEPT WHEN OTHERWISE STATED IN WRITING THE COPYRIGHT
593 | HOLDERS AND/OR OTHER PARTIES PROVIDE THE PROGRAM "AS IS" WITHOUT WARRANTY
594 | OF ANY KIND, EITHER EXPRESSED OR IMPLIED, INCLUDING, BUT NOT LIMITED TO,
595 | THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR
596 | PURPOSE. THE ENTIRE RISK AS TO THE QUALITY AND PERFORMANCE OF THE PROGRAM
597 | IS WITH YOU. SHOULD THE PROGRAM PROVE DEFECTIVE, YOU ASSUME THE COST OF
598 | ALL NECESSARY SERVICING, REPAIR OR CORRECTION.
599 |
600 | 16. Limitation of Liability.
601 |
602 | IN NO EVENT UNLESS REQUIRED BY APPLICABLE LAW OR AGREED TO IN WRITING
603 | WILL ANY COPYRIGHT HOLDER, OR ANY OTHER PARTY WHO MODIFIES AND/OR CONVEYS
604 | THE PROGRAM AS PERMITTED ABOVE, BE LIABLE TO YOU FOR DAMAGES, INCLUDING ANY
605 | GENERAL, SPECIAL, INCIDENTAL OR CONSEQUENTIAL DAMAGES ARISING OUT OF THE
606 | USE OR INABILITY TO USE THE PROGRAM (INCLUDING BUT NOT LIMITED TO LOSS OF
607 | DATA OR DATA BEING RENDERED INACCURATE OR LOSSES SUSTAINED BY YOU OR THIRD
608 | PARTIES OR A FAILURE OF THE PROGRAM TO OPERATE WITH ANY OTHER PROGRAMS),
609 | EVEN IF SUCH HOLDER OR OTHER PARTY HAS BEEN ADVISED OF THE POSSIBILITY OF
610 | SUCH DAMAGES.
611 |
612 | 17. Interpretation of Sections 15 and 16.
613 |
614 | If the disclaimer of warranty and limitation of liability provided
615 | above cannot be given local legal effect according to their terms,
616 | reviewing courts shall apply local law that most closely approximates
617 | an absolute waiver of all civil liability in connection with the
618 | Program, unless a warranty or assumption of liability accompanies a
619 | copy of the Program in return for a fee.
620 |
621 | END OF TERMS AND CONDITIONS
622 |
623 | How to Apply These Terms to Your New Programs
624 |
625 | If you develop a new program, and you want it to be of the greatest
626 | possible use to the public, the best way to achieve this is to make it
627 | free software which everyone can redistribute and change under these terms.
628 |
629 | To do so, attach the following notices to the program. It is safest
630 | to attach them to the start of each source file to most effectively
631 | state the exclusion of warranty; and each file should have at least
632 | the "copyright" line and a pointer to where the full notice is found.
633 |
634 | {one line to give the program's name and a brief idea of what it does.}
635 | Copyright (C) {year} {name of author}
636 |
637 | This program is free software: you can redistribute it and/or modify
638 | it under the terms of the GNU General Public License as published by
639 | the Free Software Foundation, either version 3 of the License, or
640 | (at your option) any later version.
641 |
642 | This program is distributed in the hope that it will be useful,
643 | but WITHOUT ANY WARRANTY; without even the implied warranty of
644 | MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
645 | GNU General Public License for more details.
646 |
647 | You should have received a copy of the GNU General Public License
648 | along with this program. If not, see .
649 |
650 | Also add information on how to contact you by electronic and paper mail.
651 |
652 | If the program does terminal interaction, make it output a short
653 | notice like this when it starts in an interactive mode:
654 |
655 | {project} Copyright (C) {year} {fullname}
656 | This program comes with ABSOLUTELY NO WARRANTY; for details type `show w'.
657 | This is free software, and you are welcome to redistribute it
658 | under certain conditions; type `show c' for details.
659 |
660 | The hypothetical commands `show w' and `show c' should show the appropriate
661 | parts of the General Public License. Of course, your program's commands
662 | might be different; for a GUI interface, you would use an "about box".
663 |
664 | You should also get your employer (if you work as a programmer) or school,
665 | if any, to sign a "copyright disclaimer" for the program, if necessary.
666 | For more information on this, and how to apply and follow the GNU GPL, see
667 | .
668 |
669 | The GNU General Public License does not permit incorporating your program
670 | into proprietary programs. If your program is a subroutine library, you
671 | may consider it more useful to permit linking proprietary applications with
672 | the library. If this is what you want to do, use the GNU Lesser General
673 | Public License instead of this License. But first, please read
674 | .
675 |
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