Bright and Dark reference images » History » Version 6
Alex Kadokura, 05/28/2010 01:17 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 | between two images will be done, Leginon will check the channel of the correction the first |
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19 | acquired image has used and then force the new image to be corrected by a different |
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20 | channel. |
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23 | To use this function, simple set the number of channels to 2 or larger in |
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24 | Correction/Settings/Image Correction/Reference Creation> while creating the reference |
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25 | images. |
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31 | h2. Acquire reference images |
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35 | * scope> make sure that the CCD will be acquiring images in an area with uniform |
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36 | beam intensity such as an empty area with no specimen nor support. You may skip a trip |
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37 | to the scope room by sending one of the high mag preset to the scope from |
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38 | Leginon. |
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41 | * Leginon/Node Selector> Select "Correction" node. |
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42 | |||
43 | |||
44 | * Leginon/Correction/Toolbar> Open "Settings" window. |
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45 | |||
46 | |||
47 | * Leginon/Correction/Toolbar/Settings> Select one of the Common Camera |
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48 | Configuration or select Custom mode and enter your own values based on the presets you |
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49 | created. |
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52 | * Leginon/Correction/Settings/Camera Configuration> Enter the Exposure time. It |
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53 | should be chosen so that the image is not saturated and ideally close to the condition |
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54 | that will be used in the experiments. If unsure about the experimental condition, use an |
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55 | exposure time that gives high but not saturated counts. |
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58 | * Leginon/Correction/Settings>By default, the corrector node is set to average 3 |
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59 | images together to create one reference image and to despike the hot pixels with |
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60 | averaged neighbor hood values. These can be changed if desired. |
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63 | 3 | Anchi Cheng | * Leginon/Correction/Settings> It is recommended to use 2 correction channels for the camera configuration used |
64 | 1 | Amber Herold | for correlation peak search. |
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67 | * Leginon/Correction/Settings> Click OK to exit settings. |
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70 | * Leginon/Correction/Toolbar> Select "Raw image " from the pull down list of |
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71 | acquisition modes and then click on "Acquire" button next to the selector to view an |
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72 | image that is not corrected. |
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73 | |||
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75 | * Leginon/Correction/Toolbar> Select "Dark reference" in the acquisition mode |
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76 | selector and then click "Acquire" to acquire the Dark reference image for this |
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77 | particular camera configuration. |
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78 | |||
79 | |||
80 | * Leginon/Correction/Toolbar> Select "Bright reference" and repeat the acquisition |
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81 | to obtain the Bright reference. |
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84 | * Leginon/Correction/Toolbar> Select "Corrected image" and then "Acquire" to view |
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85 | the corrected image. A corrected image should be free of artifacts and have smaller |
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86 | standard deviation than the raw image, in general. |
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89 | * Repeat steps 3-11 for all the images and bin sizes that will be used: |
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92 | 6 | Alex Kadokura | * If [[Bright and Dark reference images#Image-Despike|a pixel, a column/row]] or a [[Bright and Dark reference images#Image-Despike|region]] gives bad values in the bright or dark image |
93 | 1 | Amber Herold | after a few trials, it may be excluded in all corrected images. |
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99 | 3 | Anchi Cheng | |*Dimension after binning*|*Bin*|*number of correction channels*| |
100 | |512|8|1*| |
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101 | 1 | Amber Herold | |512 (centered)|1|1| |
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107 | 3 | Anchi Cheng | |*Dimension after binning*|*Bin*|*number of correction channels*| |
108 | |4096|1|1 or 2 if used for tomo preset| |
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109 | 1 | Amber Herold | |1024|4|2| |
110 | |512|8|2*| |
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111 | |512 (centered)|1|1| |
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116 | * Only one channel is required for image shift alignment purpose. If the same camera |
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117 | configuration is used for presets that involves in correlation, two channels are strongly |
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118 | recommended. |
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124 | h2. Image Despike |
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128 | The Despike feature removes random bright or hot pixels from the acquired images. This |
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129 | hot pixel is assigned the average intensity of the surrounding area, a circle of the radius |
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130 | which is entered in Neighborhood Size. The Despike Threshold is the number of standard |
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131 | deviations away from the mean that qualifies a pixel for despike correction. The despike |
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132 | affects the flat-field corrected image saved on the disk and can not be recovered. |
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133 | Therefore, use a minimal neighborhood size to avoid artifact and set the threshold high to |
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134 | avoid over-dispiking. |
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136 | 3 | Anchi Cheng | Activation of this feature and its parameter settings are defined when in the pop-up dialog for "Edit Correction Plan". See below. |
137 | 1 | Amber Herold | |
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141 | 3 | Anchi Cheng | |
142 | 1 | Amber Herold | h2. Correction Plan |
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146 | Bad Pixel, Rows and Bad Cols are used to crop portions of the image that do not read |
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147 | well off of the CCD. The values entered into here are determined empirically for each |
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148 | instrument that Leginon operates on. If one column or row of the images is incorrect, |
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149 | measure the location of the row and column that need to be removed from this image. These |
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150 | values should then be entered as a sequence of values separated by commas by editing the |
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151 | Plan. Click Save after adjusting. |
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154 | Individual bad pixel can also be corrected by its surrounding pixels. Choose these |
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155 | pixels with the selection tool on the image and then click on "Grab From Image". |
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161 | h2. Find A Single Bad Pixel |
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165 | When a single pixel is defected, it may not be easy to find it on a large image, even if |
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166 | it changes the stats dramatically. A tool is available to help finding these pixels: |
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167 | |||
168 | |||
169 | * Leginon/Correction> Acquire either a corrected image that shows the bad |
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170 | stats. |
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173 | 3 | Anchi Cheng | * Leginon/Correction/Toolbar> Left-click on the !http://emg.nysbc.org/software/leginon/images/icons/stagelocations.png! |
174 | 1 | Amber Herold | button to "Add extreme points to bad pixel list". There |
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177 | * Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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178 | "+". This adds the selected bad region to the bad pixel plan. |
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179 | |||
180 | |||
181 | * Leginon/Corrections> Acquire a corrected image in the same configuration to |
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182 | check if the apearance improves. |
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190 | h2. Bad Region Correction |
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194 | When a large region is covered by a fallen chip, image correction through bright/dark |
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195 | reference may not be sufficient to produce a spike-free image since the bright and dark |
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196 | values in the region are almost identical. To add such a large region into bad pixel plan, |
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197 | do the following: |
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200 | * Leginon/Correction> Acquire either a bright or corrected image that shows the |
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201 | bad region clearly. |
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204 | * Leginon/Correction> Use "Regions" target tool next to the image to enclose the |
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205 | bad region. The corners that the target tool identifies can be larger than the bad |
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206 | region but should be close to its size so that not too much is corrected. |
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207 | |||
208 | |||
209 | * Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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210 | "+". This adds the selected bad region to the bad pixel plan. |
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211 | |||
212 | |||
213 | * Leginon/Corrections> Acquire a corrected image in the same configuration to |
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214 | check if the apearance improves. |
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215 | 2 | Amber Herold | |
216 | ______ |
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217 | |||
218 | [[Pixel Size Calibration|< Pixel Size Calibration]] | [[Image Shift matrix calibration|Image Shift matrix calibration >]] |
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219 | |||
220 | ______ |