dtprocess on-line help
Copyright (c) 1997 Molecular Structure Corporation
Setup calibration and scan info
The Setup menu is used to modify the calibration information and
scan template stored in the selected image or header file and to write an
initial header dtprocess.head for subsequent dtprocess steps. Controls
are available to change:
- Non-uniformity type
- Spatial distortion type
- Direct beam position
- Scan template
Use the Edit header items... command from the menubar for more
complex header edits.
Select a header file from the top list or an image file from the
bottom list.
Select the Non-uniformity type from the option menu.
Select the Spatial distortion type from the option menu.
Set the Direct beam position in pixels when the detector is
perpendicular to the source and its swing and translation values are all 0.
You may use dtdisplay to view images and determine the direct beam
position.
Set the Scan template.
Setup menu options
- Non-uniformity type
- Select the method of non-uniformity of response correction that you wish
to apply to images.
- None
- No correction will be applied.
- Simple mask
- No correction will be applied, but a separate image file will be used
to flag bad pixels, such as those in the shadow of the beam stop. Any pixels
with a value of 0 in this separate file will be flagged as bad to d*TREK.
Use dtdisplay with the Edit / Erase (edit nonunf) mode to create the
mask file and save it with File / Save as.... Then specify the
mask file in the Non-uniformity file field.
- Dark & Nonunf
- Each pixel will be corrected by subtracting a dark current value and
multiplying by a non-uniformity scale factor. The dark current value comes
from an image specified in the Dark file field. The non-uniformity scale
factor comes from an image specified in the Non-uniformity file field. Bad
pixels are flagged in the non-uniformity file.
- Spatial distortion type
- Select the method to convert from detector pixels to millimeters and
vice versa.
- Simple
- Pixel positions are simply multiplied by a scale factor to get millimeters.
Specify the pixel size in millimeters in each direction in the Pixel size (mm)
fields.
- Interp. tables
- Pixel positions are converted to millimeters by lookup and interpolation
tables created by the calibrate program. Specify the interpolation tables
basename in the Interp table basename field.
- Direct beam (px)
- Specify the pixel position that the direct beam would impinge on the
detector when the detector has no rotations and no translations applied.
This is, the swing angle of the detector is 0 and the translations of the
detector (X/Trans1 and Y/Trans2) are 0. If these values are incorrect or
not compensated by the detector X and Y translations, then indexing, refinement,
and prediction will be virtually impossible. The single most frequent
reason for failure to index and refine crystal properties is incorrect values
specified here.
- Master resolution
- Specify the resolution limits in Angstroms for other menus (except Strategy). The resolution limits in the Find, Index, Refine, Predict, Integrate, and Scale menus are set to these values if BOTH are non-zero AND you select 'Write dtprocess.head'. The default of values of 0.0, 0.0 usually will mean the entire resolution range on the image will be used.
- Spacegroup (maybe)
- Specify a 'suggested' spacegroup number to use in the Index menu. When
'Write dtprocess.head' is selected this number is copied to the Index menu.
It is not copied to the crystal properties in the header. The default is
normally 0 which lets the program select the spacegroup.
- Scan template
- Specify the scan template which is an image filename with question marks
(?). The ?s will be filled in by the sequence numbers of images contained
in the scan to generate the image filenames. Images that match the scan
template will appear in the Images list.