
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