xprepfin
NAME
xprepfin - prepare fin files.
DEFINITION
Import/export fin files from/to other formats and to refor-
mat fin files. This is the main entry point for data into
XtalView. It is really set up for XENGEN mulist files (the
output of makemu -f).
USAGE
xprepfin in out
DESCRIPTION
Quit Exit prepfin.
Directory
The directory.
Input File
The input file can be either a fin or XENGEN mulist.
Input Format
Set this to the correct type.
Other Formats
Select a non-XtalView format from which to read in
data: Raxis (hkl fobs sigma Bijovet_difference), XDS
format with F's, XDS format with I's. For instructions
on adding another format see the file
$XTALVIEWHOME/data/OtherFormats.
Use Data
There six options as to how to switch the input to make
the output.
As is
No change to input.
Avg f1 and f2
If f1 and f2 exists, then they are averaged. If
one is missing, then the output is set to the
other one.
F1 then F2
If F1 exists, then use it first otherwise take F2.
F2 then F1
If F2 exists, then use it first otherwise take F1.
F1 Always use F1 if it exists.
F2 Always use F2 if it exists.
Switch F1 and F2
Select SWITCH to do this. This operation is done after
Use Data:.
Data are
This controls how some operations behave. If the data
are Bijvoet pairs, then when the indices are switched
it may be necessary to reverse the Bijvoet pair. Also,
when a centric reflection is output, Bijvoet pairs are
averaged, placed in the first field, and the second
field set to zero since centrics do not have an
anomalous scattering signal. Obviously, this should
not be done to isomorphous pair data.
Reduce Indices
The data indices are reduced to produce a unique value,
the reflections are sorted on h, k, l, and any dupli-
cates are merged. Unfortunately, the algorithm used
does not always put the data in the quadrant you
desire.
Output Format
Select the desired format from the 3 choices.
Output File
The name of the output file goes in here.
Apply
When you are ready, click here.
VERSION
Release 3.2 of XtalView
SEE ALSO
xtalview(1)