Copper clusters with diameters of approximately 2.0 to 4.0 nm (355 to 2840
atoms) served as models to obtain more detailed information of the complica
ted oxidation process of copper surfaces. In addition to the cluster size,
the amount of oxygen embedded in the clusters and their structure were chos
en as key parameters. SEELFS (surface extended electron energy loss fine st
ructure) above the M-2,M-3 edge of copper and HRTEM (high resolution transm
ission electron microscopy) were used for the in situ investigations. The c
ombination of the two techniques allowed a clear and sound interpretation o
f the spectroscopic results. SEELFS measurements on copper clusters prepare
d by inert gas aggregation and on clusters primarily oxidised by adding pur
e oxygen of different partial pressures to the aggregation gas during the m
etal evaporation, i.e., during the nucleating process, were performed. Ther
eby a positive shift of the first nearest neighbour distance (FNND) was obs
erved when compared to pure copper clusters. This dilatation is caused by o
xygen embedded in the clusters. The shape of the FNND peaks indicate heavy
distortions within the primarily oxidised clusters. Furthermore, oxygen red
uces the fractional amount of multiply twinned particles (MTPs) and the cri
tical diameter D-crit for the structural change to fcc in a significant way
compared to pure copper clusters.