Project

General

Profile

Pre-MSI Set-up » History » Version 1

Amber Herold, 04/22/2010 05:01 PM

1 1 Amber Herold
h1. Pre-MSI Set-up
2
3
4
5
h2. Design Presets
6
7
8
9
To start your own MSI experiment, you must decide what presets you want to use. Presets
10
are used to define scope and camera parameters with which images are acquired.
11
12
MSI presets can be customized to your need of data collection. By matching
13
nodes/subnodes in MSI with presets and move types, the behavior of the node is
14
defined.
15
16
For easy reference, preset names in MSI has been standardized at NRAMM although there
17
is no reason they have to be called in the way they are now. They are abbreviated to 2
18
letter codes to reduce the length of the filenames that contains every preset used in its
19
family history.
20
21
22
23
|_.Preset name:|_.abbrev for:|_.in the context of:|
24
|gr|grid|em grid|
25
|sq|square|em grid square|
26
|hl|hole|quantifoil hole|
27
|fc|focus|focus image to be checked with fft|
28
|fa|focus-auto|automatic focusing|
29
|en|exposure-near|close-to-zero defocus exposure image in a focal pair|
30
|ef|exposure-far|far-from-zero defocus exposure image in a focal pair|
31
32
33
34
35
36
|_.Magnification:|_.Preset name:|_.Image Shift (x,y):|_.Dimension:|_.Binning:|_.Beam Coverage:|_.Exposure Time (ms):|_.Spot Size:|_.Defocus (m):|
37
|120|gr|Aligned|512|8|max|20|4|0.0|
38
|550|sq|Aligned|1024|4|1x CCD size|100|4|-2e-3|
39
|5000|hl|Aligned|512|8|1x CCD|20|4|-1.5e-4|
40
|50000|fc|0,0|512|1|<~ 1x CCD|300|4|-2e-6|
41
|50000|fa|0,0|1024|4|>2x CCD|50|4|-2e-6|
42
|50000|en|0,0|4096|1|2x CCD|170 (10e/A^2)|4|-1e-6|
43
|50000|ef|0,0|4096|1|2x CCD|170 (10e/A^2)|4|-2e-6|
44
45
46
47
The preset parameters in this example are chosen to give the following
48
properties:
49
50
51
52
53
* en and ef is for final exposure and therefore has highest resolution and
54
dimension.
55
56
57
* en stands for near focus exposure and therefore has lower defocus value than
58
ef,the far-from-focus exposure.
59
60
61
* fa is for high resolution autofocus and therefore need to be high mag. The
62
dimension and binning is a result of compromizing speed, S/N ratio and sensitivity to
63
details.
64
65
66
* fc is for manual focus and ice melting and therfore more intense than fa. To get
67
good FFT for checking Thon ring behavior, it is not binned. The small dimension is for
68
increasing speed.
69
70
71
* hl is for intermediate targeting. It needs to cover the error range of modeled
72
stage position to allow final targeting by image shift only, hence the magnification.
73
The binning is for speed.
74
75
76
* sq is for grid square targeting. The image produced by the preset need to cover
77
most if not all of the square but with enough resolution to evaluate the
78
content.
79
80
81
* gr is for producing grid atlas. It is selected based on the size number of tiles
82
needed to cover the whole grid in an acceptable time and the amount of distortion
83
common to very low mag imaging.
84
85
86
87
88
89
90
In designing your own preset, follow the above properties using a mag that gives the
91
required coverage with your scope, camera, and grid mesh. If you have a 2k or 1k camera,
92
binning may not be as necessary as for a 4k camera whose data acquisition time is 10-30 sec
93
without binning.
94
95
96
97
98
99
h2. Calibrations
100
101
102
If this is the first time calibrations have ever been completed for Leginon, complete
103
all the calibrations listed in <link linkend="calapp_chapter">the chapter on
104
calibrations</link>. Calibrations are extremely important to operate the TEM in a
105
consistent manner. As long as the calibrations are stable, later users do not need to
106
perform them. Most calibrations are HT and magnification dependent. Therefore, new
107
calibration may be required if your presets use different HT and/or magnification from all
108
previous users.