|
transf [a] | transform Miller indices of input reflections |
attenu [a] | attenuator factors |
stands [a] [b] | specification of standard reflection signals |
sthkls [a] [b] | alternative method of establishing standard reflections |
fetch | definition of the order of the quantities in data lines |
data | diffractometer data lines |
genscl [c] [d] | generation of intensity scale factors |
setscl [c] [d] | set intensity scale factors |
discon [c] | definition of discontinuities in scale factors |
[a] Must precede following option lines. [b] One or the other but not both may be used. [c] One of these lines must be present if the data is to be scaled. Otherwise, scale factors are calculated but not applied. [d] If a setscl line is input before a genscl line, the genscl line will be ignored. |
DIFDAT | Option | Code | Arg | Def | |
input data mode |
dat
|
data lines from input | |||
|
from archive file | ||||
|
CAD4 diffr. file
cad
|
||||
|
Nicolet (Vax)
[a]file
nic
|
||||
|
Nicolet (DG)
[a]file
nic
|
||||
|
Siemens ascii file
sie
|
||||
|
P3 special binary file
dct
|
||||
|
Tsukuba diffr. file
tsu
|
||||
|
special diffr. file
dif
|
||||
|
Rigaku Denki. file
rd5
|
||||
|
SHELX F4 fixed format file
.hkl
[b]
|
||||
|
SHELX F3 fixed format file
.hkl
[b]
|
||||
[b]
|
Rigaku Rapid .f2plus | ||||
[b]
|
alternate Rigaku Rapid .f2plus | ||||
[b]
|
Rigaku Rapid .f2 | ||||
[b]
|
Bruker Smart file
[c]
raw
|
||||
filename <256 characters |
|
|
change shx / rap input data filename | ||
Bruker raw file |
|
load direction cosines on to bdf | |||
Tsukuba
.tsu file data
[d]
|
|
|
monitor count smoothing across 1<n<21 refl'ns |
1
|
|
Nicolet scan mode |
|
Nicolet scan | |||
|
Nicolet scan | ||||
add bdf refln data |
noadd
|
do not add hkl from old bdf | |||
|
add new hkl to old bdf [e] | ||||
print reflection data |
noprint
|
print no reflections | |||
|
|
print n | all | ||
print raw data |
|
print n lines, defined above | |||
scale intensities |
|
do not apply scale | |||
fate of standards |
include
|
include on output bdf | |||
|
exclude from output bdf | ||||
backg. time each side |
|
|
time in seconds |
10
|
|
min. scan time [f] |
|
|
time in seconds |
10
|
|
observ. threshold [g] |
|
|
rcode=2 if I < n I |
2
|
|
set intensity if rcode 2 |
nobth
|
store as calculated | |||
|
|
store as m I [h] | |||
backg. imbalanced |
|
|
warn if(b1-b2) > q I |
10
|
|
damp stds variation |
|
|
scaledamping factor |
.5
|
|
instability option |
|
|
option, slope, intercept [i] | ||
instability calculation |
|
calc. before scaling | after | ||
instability calculation |
|
do not use raw counts | |||
I options |
|
|
use f*I as I | ||
|
|
incr. I with sI |
.02
|
||
output diffract. angles |
|
put angles on the bdf | no | ||
output Eulerian angles |
|
put angles on the bdf | no | ||
deadtime correction |
|
|
add n% to deadtime correction | ||
[a] Outputs input data as data lines to the punch file [b] data is stored as f2rl and not irel [c] The Bruker SMART .raw file contains primary and diffracted beam direction cosines, to represent the orientation of the crystal at reflection measurement time (generally anything other than the bisecting position). DIFDAT contains code to convert those direction cosines to an orientation specified in terms of the Crystal Based Azimuthal Psi Angle (lrefl: IDNUM n011), which should permit absorption correction using programs such as LSABS and LSLS (But NOT ABSORB). This requires the orientation matrix UB to be stored in STARTX. The azimuthal angle calculation has not been verified as correct! [d] adjustments for bugged software. Generally not required. [e] The
[f] If an encountered scan time is less than
[g] Reflections with intensities greater than
nσ above background as defined by the
[h] The
|
attenu [a] | 1- | attenuator factors (minimum of 1.0) | |
[a] The first attenuator factor does not refer to the open attenuator position. The attenuator factors are used as multiplicative factors. |
stands | 1 | character string that identifies standard or observed reflection [a] | |||
2 | integer assigned to reflection identified by string in field 1 | ||||
for a normal reflection |
|
||||
for a standard |
|
||||
3, 4 | same as 1 and 2 above | ||||
[a] The observed reflection/standard reflection identifiers may be either a character string or a single decimal digit. (e.g., #ST or 1). A maximum of 11 pairs (1 observed and up to 10 standards) may appear on the stands line. This line may be used as an alternative to the sthkls lines. Note that this line is used only in conjunction with data lines. |
sthkls [a] | 1-3 | hkl indices of first standard reflection | |
4-6 | hkl indices of second standard reflection , and so on | ||
[a] A maximum of 10 standards may be defined. More than one sthkls line may be used. The first blank h field terminates the scan. These lines may be used as an alternative to a stands line. Note that this line is used only in conjunction with data lines. |
fetch [a] | 1- | mnemonics defining the input fields on data lines | |||
field to be skipped [b] |
|
||||
signal reflections as standard or regular observation [c] |
|
||||
h index |
|
||||
k index |
|
||||
l index |
|
||||
scan time of scan [d] |
|
||||
scan counts |
|
||||
counts for background 1 [e] |
|
||||
counts for background 2 |
|
||||
attenuator number [f] |
|
||||
reflection sequence number [g] |
|
||||
|
|||||
|
|||||
|
|||||
|
|||||
|
|||||
|
|||||
2 |
|
||||
|
|||||
|
|||||
|
|||||
[a] The values for
[b] The
[c] If
[d] If
[e] If
[f] If
[g] If
|
data [a] | 1- | reflection input quantities | |
[a] These quantities are specified in the fetch line as described previously. In practice the use of a setid line or a field line followed by a setid line may be found useful. The intention is that the diffractometer output tape will be processed through local operating system utilities to form a coded file. This file will be edited using a text editor and then fed to the Xtal system in the input stream. (See examples in the Reference Manual.) |
genscl [a] | 1 | number of standard groups scale factors are smoothed |
5
|
[a] This line will be ignored if preceded by a setscl line. It causes the generation of scale factors based on observations of standard reflections. If setscl lines follow, they will replace specified group scale factors. |
setscl | 1 | scale factor to supersede value for specified standard group | |
2 | serial number [a]of the last standard reflection of the group of standards for which this scale supersedes | ||
[a] The serial number refers to the diffractometer serial number, if that has been supplied, otherwise it refers to the sequence number developed as the reflections are being treated on input. Smoothing will take place over the scale factors unless prevented by discon input lines. The serial number given must be that of the LAST standard reflection of the group of standards used to establish the scale. Otherwise, the setscl line will be ignored. |
discon [a] | 1- | serial number of the last standard reflection of the group of standards used to establish the scale factor | |
[a] A preliminary run of DIFDAT may have to be made to find discontinuities in the scale factors. |
transf [a] | 1-9 | transformation matrix , , , , , , , , | |
[a] The transformation is: h'k'l' = hkl* a -matrix |