Bright and Dark reference images » History » Version 16
Anchi Cheng, 06/06/2012 07:09 PM
1 | 1 | Amber Herold | h1. Bright and Dark reference images |
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4 | Bright and Dark reference images need to be acquired for every camera setting that will |
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5 | be used. The camera settings include image dimension, bin size, and offset. Over time, |
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6 | references may need to be repeatedly acquired. |
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10 | h2. Correction Channels |
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14 | When two flat-field-corrected images are correlated, there is often an origin peak |
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15 | derived from the common normalization image even if both image acquisition contains only |
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16 | noise. In order to avoid this problem, two or more sets of bright/dark references, and hence |
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17 | normalization images can be obtained per CCD camera configuration. When a correlation |
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18 | 13 | Anchi Cheng | between two images are done, Leginon will check the channel of the correction the first |
19 | 1 | Amber Herold | acquired image has used and then force the new image to be corrected by a different |
20 | channel. |
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22 | 13 | Anchi Cheng | We recommend that you always acquire reference images on both channels. |
23 | 1 | Amber Herold | |
24 | h2. Acquire reference images |
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28 | 13 | Anchi Cheng | # scope> make sure that the digital camera will be acquiring images in an area with uniform |
29 | 1 | Amber Herold | beam intensity such as an empty area with no specimen nor support. You may skip a trip |
30 | to the scope room by sending one of the high mag preset to the scope from |
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31 | Leginon. |
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32 | 12 | Amber Herold | |
33 | # Leginon/Node Selector> Select "Correction" node. |
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34 | |
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35 | # Leginon/Correction/Toolbar> Open "Settings" window. |
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36 | |
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37 | # Leginon/Correction/Toolbar/Settings> Select one of the Common Camera |
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38 | 1 | Amber Herold | Configuration or select Custom mode and enter your own values based on the presets you |
39 | created. |
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40 | 12 | Amber Herold | |
41 | # Leginon/Correction/Settings/Camera Configuration> Enter the Exposure time. It |
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42 | 1 | Amber Herold | should be chosen so that the image is not saturated and ideally close to the condition |
43 | that will be used in the experiments. If unsure about the experimental condition, use an |
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44 | exposure time that gives high but not saturated counts. |
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45 | |
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46 | # Leginon/Correction/Settings>By default, the corrector node is set to average 3 |
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47 | images together to create one reference image and to despike the hot pixels with |
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48 | averaged neighbor hood values. These can be changed if desired. |
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49 | 12 | Amber Herold | |
50 | 1 | Amber Herold | # Leginon/Correction/Settings> Click OK to exit settings. |
51 | |
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52 | 13 | Anchi Cheng | # Leginon/Correction/Toolbar> Select "Channel 0" in the channel number |
53 | selector so that the next step will acquire only one image. |
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54 | |
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55 | 1 | Amber Herold | # Leginon/Correction/Toolbar> Select "Raw image " from the pull down list of |
56 | acquisition modes and then click on "Acquire" button next to the selector to view an |
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57 | image that is not corrected. |
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58 | 12 | Amber Herold | |
59 | 13 | Anchi Cheng | # Leginon/Correction/Toolbar> Select "Both Channels" in the channel number |
60 | selector so that the next steps will acquire images for both correction channels. |
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61 | |
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62 | 1 | Amber Herold | # Leginon/Correction/Toolbar> Select "Dark reference" in the acquisition mode |
63 | selector and then click "Acquire" to acquire the Dark reference image for this |
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64 | 12 | Amber Herold | particular camera configuration. |
65 | |
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66 | 1 | Amber Herold | # Leginon/Correction/Toolbar> Select "Bright reference" and repeat the acquisition |
67 | to obtain the Bright reference. |
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68 | 13 | Anchi Cheng | |
69 | # Leginon/Correction/Toolbar> Select "Channel 0" in the channel number |
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70 | selector so that the next step will acquire only one image. |
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71 | 12 | Amber Herold | |
72 | # Leginon/Correction/Toolbar> Select "Corrected image" and then "Acquire" to view |
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73 | 1 | Amber Herold | the corrected image. A corrected image should be free of artifacts and have smaller |
74 | standard deviation than the raw image, in general. |
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75 | 12 | Amber Herold | |
76 | 14 | Anchi Cheng | # Repeat steps 3-14 for all the images and bin sizes that will be used: |
77 | 12 | Amber Herold | |
78 | # If [[Bright and Dark reference images#Correction-Plan|a pixel, a column/row]] or a [[Bright and Dark reference images#Bad-Region-Correction|region]] gives bad values in the bright or dark image |
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79 | 1 | Amber Herold | after a few trials, it may be excluded in all corrected images. |
80 | 12 | Amber Herold | |
81 | 14 | Anchi Cheng | *Bright/Dark Reference Image Need for the Example MSI with 4kx4k camera:* |
82 | 11 | Amber Herold | |
83 | 3 | Anchi Cheng | |*Dimension after binning*|*Bin*|*number of correction channels*| |
84 | 16 | Anchi Cheng | |4096|1|1 or 2 if used for tomo preset|Notes| |
85 | |1024|4|2|(1)| |
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86 | |1024(centered)|1|1|(2)| |
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87 | |512|8|2|(3)| |
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88 | |512 (centered)|1|1|(3)) |
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89 | 1 | Amber Herold | |
90 | 16 | Anchi Cheng | (1)-This camera configuration is used in preset beam shift alignment even if you don't use it for a preset. |
91 | (2)-This camera configuration is used in Manual Application Manual Focusing even if you don't use it for a preset. |
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92 | (3)-These camera configurations are used in preset image shift alignment even if you don't use it for a preset. |
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93 | 1 | Amber Herold | |
94 | h2. Image Despike |
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98 | The Despike feature removes random bright or hot pixels from the acquired images. This |
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99 | hot pixel is assigned the average intensity of the surrounding area, a circle of the radius |
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100 | which is entered in Neighborhood Size. The Despike Threshold is the number of standard |
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101 | deviations away from the mean that qualifies a pixel for despike correction. The despike |
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102 | affects the flat-field corrected image saved on the disk and can not be recovered. |
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103 | Therefore, use a minimal neighborhood size to avoid artifact and set the threshold high to |
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104 | avoid over-despiking. |
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106 | Activation of this feature and its parameter settings are defined when in the pop-up dialog for "Edit Correction Plan". See below. |
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111 | 3 | Anchi Cheng | |
112 | 1 | Amber Herold | h2. Correction Plan |
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116 | Bad Pixel, Rows and Bad Cols are used to crop portions of the image that do not read |
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117 | well off of the CCD. The values entered into here are determined empirically for each |
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118 | instrument that Leginon operates on. If one column or row of the images is incorrect, |
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119 | measure the location of the row and column that need to be removed from this image. These |
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120 | values should then be entered as a sequence of values separated by commas by editing the |
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121 | Plan. Click Save after adjusting. |
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124 | Individual bad pixel can also be corrected by its surrounding pixels. Choose these |
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125 | pixels with the selection tool on the image and then click on "Grab From Image". |
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131 | 14 | Anchi Cheng | |
132 | 1 | Amber Herold | h2. Find A Single Bad Pixel |
133 | 3 | Anchi Cheng | |
134 | 1 | Amber Herold | |
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136 | When a single pixel is defected, it may not be easy to find it on a large image, even if |
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137 | it changes the stats dramatically. A tool is available to help finding these pixels: |
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140 | 12 | Amber Herold | # Leginon/Correction> Acquire either a corrected image that shows the bad |
141 | 1 | Amber Herold | stats. |
142 | 12 | Amber Herold | |
143 | # Leginon/Correction/Toolbar> Left-click on the !http://emg.nysbc.org/software/leginon/images/icons/stagelocations.png! |
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144 | 1 | Amber Herold | button to "Add extreme points to bad pixel list". There |
145 | 12 | Amber Herold | |
146 | # Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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147 | 1 | Amber Herold | "+". This adds the selected bad region to the bad pixel plan. |
148 | 12 | Amber Herold | |
149 | # Leginon/Corrections> Acquire a corrected image in the same configuration to |
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150 | 1 | Amber Herold | check if the apearance improves. |
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153 | h2. Bad Region Correction |
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155 | 14 | Anchi Cheng | Note: Bad region correction are corrected pixel-by-pixel. This can be *computational intensive* if a large region is included. If flat-field correction alone gives reasonable result, you should minimize usage of the this function. |
156 | 1 | Amber Herold | |
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158 | 14 | Anchi Cheng | When a large region is covered by a fallen chip, image correction through bright/dark reference may not be sufficient to produce a spike-free image since the bright and dark values in the region are almost identical. To add such a large region into bad pixel plan, do the following: |
159 | 1 | Amber Herold | |
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161 | 12 | Amber Herold | # Leginon/Correction> Acquire either a bright or corrected image that shows the |
162 | 1 | Amber Herold | bad region clearly. |
163 | 12 | Amber Herold | |
164 | # Leginon/Correction> Use "Regions" target tool next to the image to enclose the |
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165 | 1 | Amber Herold | bad region. The corners that the target tool identifies can be larger than the bad |
166 | region but should be close to its size so that not too much is corrected. |
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167 | 12 | Amber Herold | |
168 | # Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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169 | 1 | Amber Herold | "+". This adds the selected bad region to the bad pixel plan. |
170 | 12 | Amber Herold | |
171 | # Leginon/Corrections> Acquire a corrected image in the same configuration to |
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172 | 10 | Amber Herold | check if the appearance improves. |
173 | 2 | Amber Herold | |
174 | ______ |
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176 | [[Pixel Size Calibration|< Pixel Size Calibration]] | [[Image Shift matrix calibration|Image Shift matrix calibration >]] |
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177 | |||
178 | ______ |