Project

General

Profile

Importance of making calibrations » History » Version 4

Amber Herold, 06/23/2010 12:20 PM

1 1 Amber Herold
h1. Importance of making calibrations
2
3
4
5
Leginon will not function if calibrations have not been done. In essence, this (or a
6
similar combination of nodes) is the first application that should be used if calibrations do
7
not already exist. The term calibrations is an inclusive term that refers to different sets of
8
measurements such as image shift and stage position.
9
10
11
12
13
Unless you plan to perform calibration to all available magnification and camera
14 4 Amber Herold
configuration, the first step in performing calibration will be to [[Creating Presets for the first time|set up Presets]].
15 1 Amber Herold
16
17
The following lists all the calibrations that must be completed for Leginon MSI
18
application to function correctly. Some calibrations can not be performed without existing
19
calibration of the others. Therefore, it is necessary to follow the order listed below for the
20
very first calibration for an empty database:
21
22
23
24
25 3 Anchi Cheng
* [[Pixel Size Calibration|Pixel size calibration]] (for all the magnifications
26 1 Amber Herold
that will be used)
27
28
29 3 Anchi Cheng
* [[Bright and Dark reference images]] (for all the image dimension and binning that will be used)
30 1 Amber Herold
31
32 3 Anchi Cheng
*  (Optional) [[Beam Shift Matrix calibration]] (for all the magnifications that will be used)
33 1 Amber Herold
34
35 3 Anchi Cheng
* [[Image Shift Matrix calibration]] (for all the magnifications that will be used)
36 1 Amber Herold
37
38 3 Anchi Cheng
* [[Stage Position Matrix calibration]] (for the
39 1 Amber Herold
magnifications that will be used for gr preset in MSI... e.g. 120x)
40
41
42 3 Anchi Cheng
* [[>Modeled Stage Postion calibration]] (for magnifications
43 1 Amber Herold
in the range of ~550x to 1100x that will be used for sq preset in MSI...e.g.
44
550x)
45
46
47 3 Anchi Cheng
* [[Autofocus Calibration with Beam Tilt Node|Beam Tilt Defocus calibrations]] (for the magnifications
48 1 Amber Herold
focus will be corrected at, both for z and defocus correction. These are the hl and fa
49
presets in MSI, respectively... e.g. 5000x and 50kx)
50
51
52 3 Anchi Cheng
* [[Autofocus Calibration with Beam Tilt Node|Beam Tilt Stigmator calibrations]] (for the
53 1 Amber Herold
magnifications where the focus and astigmatism will be corrected at. These are the hl
54
and fa presets in MSI... e.g. 5000x, 50kx)
55
56
57 3 Anchi Cheng
* [[Autofocus Calibration with Beam Tilt Node|Store eucentric focus value]] (for the
58 1 Amber Herold
magnifications where the stage z will be used for defocus correction. The hl presets in
59
MSI is typical... e.g. 5000x)
60
61
62 3 Anchi Cheng
* [[Autofocus Calibration with Beam Tilt Node|Store rotation center beam tilt value]] (for the
63 1 Amber Herold
autofocus magnifications where the image shift is useded as move type in targeting if
64
the stage is to be tilted. For example, the "fa" preset in MSI... e.g. 50000x)
65
66
67 3 Anchi Cheng
* [[Dose (camera sensitivity) calibration]] (for one
68 1 Amber Herold
magnification, the rest are scaled by the program automatically).
69
70
71
72
73
74
!http://emg.nysbc.org/software/leginon/images/images/Cal_flow.png!
75
76
77
78 3 Anchi Cheng
In most cases, calibration only need to be done once. Through experience, we have found the Stage Position and Calibrations involving Beam Tilt need to be refined often. The other calibrations (in our experience) do not fluctuate as frequently as these two do. Modeled stage position calibration does gradually go off over several months and a full calibration of the modeled stage position matrix is required to rectify the problem.
79 1 Amber Herold
80
81
82
83 3 Anchi Cheng
Image Shift, Stage Position, and Modeled Stage Position matrix calibration are being completed so that targets can be accurated centered in the images at each different magnification. At the lowest magnifications, an image shift is too big without inducing significant beam shift so the stage has to be moved. As the magnification increases, a simple
84
calibration of stage movement (error typically of 1.5 um or more) is not adequate, so we have to model the stage movement (error typically of 1 um or less), but still move the stage. At
85
even higher magnifications (e.g. hl, en, ef, fc, and fa) image shifts (error of 0.3 um or less) can be used to go to targets.
86 1 Amber Herold
87
88
89
90
The following are magnifications and types of positioning calibrations that typically have
91
been completed at a very minimum:
92
93
94
95
|_.Magnification:|_.Calibrations:|
96
|120 (i..e., mag for "gr" preset)|modeled stage position(mag-only), image shift|
97
|550 (i.e., mag for "sq" preset)|modeled stage position(full), image shift|
98
|5000 (i.e., mag for "hl" preset)|image shift|
99
|50000 (i,e, mag for "fa","fc","en" and "ef" presets)|image shift|
100
101
102
103
104
105
106
The Presets Manager has a "Calibration Status" section that will show which calibrations
107
have been completed for the given mag the selected preset is set to. We usually calibrate for
108
a range of magnifications so that later we will not have to complete them.
109 2 Amber Herold
110
111
______
112
113
[[Grids for Calibration|Grids for Calibration >]]
114
115
______