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Pre-MSI Set-up » History » Version 2

Amber Herold, 04/27/2010 11:36 AM

1 1 Amber Herold
h1. Pre-MSI Set-up
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h2. Design Presets
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To start your own MSI experiment, you must decide what presets you want to use. Presets
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are used to define scope and camera parameters with which images are acquired.
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MSI presets can be customized to your need of data collection. By matching
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nodes/subnodes in MSI with presets and move types, the behavior of the node is
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defined.
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For easy reference, preset names in MSI has been standardized at NRAMM although there
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is no reason they have to be called in the way they are now. They are abbreviated to 2
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letter codes to reduce the length of the filenames that contains every preset used in its
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family history.
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|_.Preset name:|_.abbrev for:|_.in the context of:|
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|gr|grid|em grid|
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|sq|square|em grid square|
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|hl|hole|quantifoil hole|
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|fc|focus|focus image to be checked with fft|
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|fa|focus-auto|automatic focusing|
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|en|exposure-near|close-to-zero defocus exposure image in a focal pair|
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|ef|exposure-far|far-from-zero defocus exposure image in a focal pair|
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|_.Magnification:|_.Preset name:|_.Image Shift (x,y):|_.Dimension:|_.Binning:|_.Beam Coverage:|_.Exposure Time (ms):|_.Spot Size:|_.Defocus (m):|
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|120|gr|Aligned|512|8|max|20|4|0.0|
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|550|sq|Aligned|1024|4|1x CCD size|100|4|-2e-3|
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|5000|hl|Aligned|512|8|1x CCD|20|4|-1.5e-4|
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|50000|fc|0,0|512|1|<~ 1x CCD|300|4|-2e-6|
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|50000|fa|0,0|1024|4|>2x CCD|50|4|-2e-6|
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|50000|en|0,0|4096|1|2x CCD|170 (10e/A^2)|4|-1e-6|
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|50000|ef|0,0|4096|1|2x CCD|170 (10e/A^2)|4|-2e-6|
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The preset parameters in this example are chosen to give the following
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properties:
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* en and ef is for final exposure and therefore has highest resolution and
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dimension.
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* en stands for near focus exposure and therefore has lower defocus value than
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ef,the far-from-focus exposure.
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* fa is for high resolution autofocus and therefore need to be high mag. The
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dimension and binning is a result of compromizing speed, S/N ratio and sensitivity to
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details.
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* fc is for manual focus and ice melting and therfore more intense than fa. To get
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good FFT for checking Thon ring behavior, it is not binned. The small dimension is for
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increasing speed.
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* hl is for intermediate targeting. It needs to cover the error range of modeled
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stage position to allow final targeting by image shift only, hence the magnification.
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The binning is for speed.
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* sq is for grid square targeting. The image produced by the preset need to cover
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most if not all of the square but with enough resolution to evaluate the
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content.
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* gr is for producing grid atlas. It is selected based on the size number of tiles
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needed to cover the whole grid in an acceptable time and the amount of distortion
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common to very low mag imaging.
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In designing your own preset, follow the above properties using a mag that gives the
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required coverage with your scope, camera, and grid mesh. If you have a 2k or 1k camera,
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binning may not be as necessary as for a 4k camera whose data acquisition time is 10-30 sec
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without binning.
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h2. Calibrations
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If this is the first time calibrations have ever been completed for Leginon, complete
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all the calibrations listed in <link linkend="calapp_chapter">the chapter on
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calibrations</link>. Calibrations are extremely important to operate the TEM in a
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consistent manner. As long as the calibrations are stable, later users do not need to
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perform them. Most calibrations are HT and magnification dependent. Therefore, new
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calibration may be required if your presets use different HT and/or magnification from all
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previous users.
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[[Summary of MSI applications|< Summary of MSI applications]] | [[Initial MSI application preferences|Initial MSI application preferences >]]
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