The laboratory wavelength calibration of the SWS has been successfully
transferred to the in orbit situation. The achieved accuracies for th
e grating sections are lambda/delta lambda similar to 10000. Any remai
ning errors in the wavelength scale are dominated by uncertainties of
the relative position of the target in the 14'' - 20'' wide slits. The
grating spectral profile is very well represented by a Gaussian shape
. The width of the grating spectral profile can be accurately predicte
d by a theoretical model. The wavelength calibration of the FP's is ac
curate to within 1/3 Of a resolution element, corresponding to lambda/
delta lambda similar to 10(5). The wavelength stability of the grating
s and FP is excellent, no measurable changes were found during the fir
st 6 months of the ISO mission.