Crystal structure solution
discussed above. The non-centrosymmetric space group Cmc2, looks more
promising as it has a 4-fold special position in the mirror plane perpendicular
to
X:
4(a) with coordinates
Oyz,
where all atoms can be located.
The structure was solved' using SHELXS-90 and partial least squares
refinement using SHELXL-97 programs.' The centrosymmetric space group
symmetry Cmcm was tested first, however, several attempts with varying
parameters produced no acceptable model. It may be difficult to recognize
the incorrect selection of space group symmetry based on a few failures to
find the model, especially when relatively low quality or truncated structure
factor data are employed
(e.g. those extracted from the powder pattern). If a
solution at certain conditions in the selected space group symmetry was not
found, this does not necessarily mean that it does not exist. Often, it may be
tricky to identify a true solution.
Taking into account that the number of formula units per cell
(Z
=
4)
gives a preference to the space group Cmc2,, it was chosen for the next
attempt. At first, the direct phase angles determination using SHELXS-90
was attempted with all default parameters. The program automatically
assigns heavy atoms to the peaks from the E-map, and in this case, the first
three peaks were treated as Mn. Analysis of interatomic distances indicated,
however, that the second strongest peak cannot be a metal and therefore, this
solution was
aband~ned.~
The following step, which is usually recommended when working with
powder data and when the default parameters do not result in an acceptable
solution, is to decrease the minimum normalized structure amplitude (Efi,,)
employed in the generation of phases.
In
general, this reduction decreases
the probability of phase relationships (see Eqs. 2.144, 2.147, and 2.148) but
it increases the number of reflections included in the process.
In
our case,
decreasing E,, from the default 1.2 to Ed,
=
1.1, increases the number of
reflections from 11 to 14. The best solution, shown in
Table
6.35,
contains
the first two peaks that are suitable as metals and the next three can be
suitable as oxygen atoms.4 Peaks beginning from
44
and below are
unacceptable because they are too close to the already assigned peaks.
Ready to use reflection file
Ch6ExOS.hkl
and crystal data file
Ch6ExOS.ins
are found on
the
CD.
Both can be used as input files for SHELXS-90.
G. M. Sheldrick, Phase annealing in SHELXS-90: direct methods for larger structures,
Acta Cryst.
A46,
467 (1990); G. M. Sheldrick, SHELXL-97. University of Gottingen,
Germany, (1997). See the footnote on page
515
on how to obtain the programs.
Generally, a situation like that does not necessarily mean that the model of the crystal
structure cannot be completed using this solution. It may take longer and it may be harder
to make decisions about which peaks should be included, and what atom types should be
assigned to them.
The suitability of peaks as atoms has been judged based on the relative heights of the
peaks on the E-map and from the shortest interatomic distances. The distance Mn2
-
42