Bright and Dark reference images » History » Version 12
Amber Herold, 06/24/2010 12:20 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 | 12 | Amber Herold | # scope> make sure that the CCD will be acquiring images in an area with uniform |
| 36 | 1 | Amber Herold | beam intensity such as an empty area with no specimen nor support. You may skip a trip |
| 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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| 39 | 12 | Amber Herold | |
| 40 | # Leginon/Node Selector> Select "Correction" node. |
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| 41 | |
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| 42 | # Leginon/Correction/Toolbar> Open "Settings" window. |
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| 43 | |
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| 44 | # Leginon/Correction/Toolbar/Settings> Select one of the Common Camera |
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| 45 | 1 | Amber Herold | Configuration or select Custom mode and enter your own values based on the presets you |
| 46 | created. |
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| 47 | 12 | Amber Herold | |
| 48 | # Leginon/Correction/Settings/Camera Configuration> Enter the Exposure time. It |
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| 49 | 1 | Amber Herold | should be chosen so that the image is not saturated and ideally close to the condition |
| 50 | that will be used in the experiments. If unsure about the experimental condition, use an |
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| 51 | exposure time that gives high but not saturated counts. |
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| 52 | 12 | Amber Herold | |
| 53 | # Leginon/Correction/Settings>By default, the corrector node is set to average 3 |
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| 54 | 1 | Amber Herold | images together to create one reference image and to despike the hot pixels with |
| 55 | averaged neighbor hood values. These can be changed if desired. |
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| 56 | 12 | Amber Herold | |
| 57 | # Leginon/Correction/Settings> It is recommended to use 2 [[Bright and Dark reference images#Correction-Channels|correction channels]] for the camera configuration used |
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| 58 | 1 | Amber Herold | for correlation peak search. |
| 59 | 12 | Amber Herold | |
| 60 | # Leginon/Correction/Settings> Click OK to exit settings. |
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| 61 | |
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| 62 | # Leginon/Correction/Toolbar> Select "Raw image " from the pull down list of |
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| 63 | 1 | Amber Herold | acquisition modes and then click on "Acquire" button next to the selector to view an |
| 64 | image that is not corrected. |
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| 65 | 12 | Amber Herold | |
| 66 | # Leginon/Correction/Toolbar> Select "Dark reference" in the acquisition mode |
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| 67 | 1 | Amber Herold | selector and then click "Acquire" to acquire the Dark reference image for this |
| 68 | particular camera configuration. |
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| 69 | 12 | Amber Herold | |
| 70 | # Leginon/Correction/Toolbar> Select "Bright reference" and repeat the acquisition |
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| 71 | 1 | Amber Herold | to obtain the Bright reference. |
| 72 | 12 | Amber Herold | |
| 73 | # Leginon/Correction/Toolbar> Select "Corrected image" and then "Acquire" to view |
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| 74 | 1 | Amber Herold | the corrected image. A corrected image should be free of artifacts and have smaller |
| 75 | standard deviation than the raw image, in general. |
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| 76 | 12 | Amber Herold | |
| 77 | # Repeat steps 3-11 for all the images and bin sizes that will be used: |
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| 78 | |
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| 79 | # 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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| 80 | 1 | Amber Herold | after a few trials, it may be excluded in all corrected images. |
| 81 | 12 | Amber Herold | |
| 82 | # Only one channel is required for image shift alignment purpose. If the same camera configuration is used for presets that involves in correlation, two channels are strongly recommended. |
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| 83 | 1 | Amber Herold | |
| 84 | 12 | Amber Herold | *Bright/Dark Reference Image Need for the Example MSI:* |
| 85 | 11 | Amber Herold | |
| 86 | 3 | Anchi Cheng | |*Dimension after binning*|*Bin*|*number of correction channels*| |
| 87 | 1 | Amber Herold | |4096|1|1 or 2 if used for tomo preset| |
| 88 | 9 | Anchi Cheng | |1024|4|2^*^| |
| 89 | |1024(centered)|1|1^**^| |
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| 90 | |512|8|2^***^| |
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| 91 | |512 (centered)|1|1^***^| |
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| 92 | 1 | Amber Herold | |
| 93 | 9 | Anchi Cheng | ^*^-This camera configuration is used in preset beam shift alignment even if you don't use it for a preset. |
| 94 | ^**^-This camera configuration is used in Manual Application Manual Focusing even if you don't use it for a preset. |
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| 95 | ^***^-These camera configurations are used in preset image shift alignment even if you don't use it for a preset. |
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| 96 | 1 | Amber Herold | |
| 97 | h2. Image Despike |
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| 101 | The Despike feature removes random bright or hot pixels from the acquired images. This |
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| 102 | hot pixel is assigned the average intensity of the surrounding area, a circle of the radius |
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| 103 | which is entered in Neighborhood Size. The Despike Threshold is the number of standard |
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| 104 | deviations away from the mean that qualifies a pixel for despike correction. The despike |
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| 105 | affects the flat-field corrected image saved on the disk and can not be recovered. |
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| 106 | Therefore, use a minimal neighborhood size to avoid artifact and set the threshold high to |
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| 107 | avoid over-despiking. |
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| 109 | 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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| 114 | 3 | Anchi Cheng | |
| 115 | 1 | Amber Herold | h2. Correction Plan |
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| 119 | Bad Pixel, Rows and Bad Cols are used to crop portions of the image that do not read |
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| 120 | well off of the CCD. The values entered into here are determined empirically for each |
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| 121 | instrument that Leginon operates on. If one column or row of the images is incorrect, |
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| 122 | measure the location of the row and column that need to be removed from this image. These |
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| 123 | values should then be entered as a sequence of values separated by commas by editing the |
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| 124 | Plan. Click Save after adjusting. |
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| 127 | Individual bad pixel can also be corrected by its surrounding pixels. Choose these |
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| 128 | pixels with the selection tool on the image and then click on "Grab From Image". |
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| 134 | h2. Find A Single Bad Pixel |
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| 135 | 3 | Anchi Cheng | |
| 136 | 1 | Amber Herold | |
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| 138 | When a single pixel is defected, it may not be easy to find it on a large image, even if |
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| 139 | it changes the stats dramatically. A tool is available to help finding these pixels: |
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| 142 | 12 | Amber Herold | # Leginon/Correction> Acquire either a corrected image that shows the bad |
| 143 | 1 | Amber Herold | stats. |
| 144 | 12 | Amber Herold | |
| 145 | # Leginon/Correction/Toolbar> Left-click on the !http://emg.nysbc.org/software/leginon/images/icons/stagelocations.png! |
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| 146 | 1 | Amber Herold | button to "Add extreme points to bad pixel list". There |
| 147 | 12 | Amber Herold | |
| 148 | # Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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| 149 | 1 | Amber Herold | "+". This adds the selected bad region to the bad pixel plan. |
| 150 | 12 | Amber Herold | |
| 151 | # Leginon/Corrections> Acquire a corrected image in the same configuration to |
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| 152 | 1 | Amber Herold | check if the apearance improves. |
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| 155 | h2. Bad Region Correction |
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| 159 | When a large region is covered by a fallen chip, image correction through bright/dark |
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| 160 | reference may not be sufficient to produce a spike-free image since the bright and dark |
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| 161 | values in the region are almost identical. To add such a large region into bad pixel plan, |
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| 162 | do the following: |
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| 165 | 12 | Amber Herold | # Leginon/Correction> Acquire either a bright or corrected image that shows the |
| 166 | 1 | Amber Herold | bad region clearly. |
| 167 | 12 | Amber Herold | |
| 168 | # Leginon/Correction> Use "Regions" target tool next to the image to enclose the |
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| 169 | 1 | Amber Herold | bad region. The corners that the target tool identifies can be larger than the bad |
| 170 | region but should be close to its size so that not too much is corrected. |
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| 171 | 12 | Amber Herold | |
| 172 | # Leginon/Correction/Tools> Left-click on the "Add Region" tool that looks like |
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| 173 | 1 | Amber Herold | "+". This adds the selected bad region to the bad pixel plan. |
| 174 | 12 | Amber Herold | |
| 175 | # Leginon/Corrections> Acquire a corrected image in the same configuration to |
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| 176 | 10 | Amber Herold | check if the appearance improves. |
| 177 | 2 | Amber Herold | |
| 178 | ______ |
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| 180 | [[Pixel Size Calibration|< Pixel Size Calibration]] | [[Image Shift matrix calibration|Image Shift matrix calibration >]] |
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| 182 | ______ |