  The identifications of Fe VII emission lines in the wavelength range 193-197
{\AA} are discussed in the light of new measurements of laboratory spectra and
atomic data calculations. This region is of importance to studies of solar
spectra from the EUV Imaging Spectrometer (EIS) on board the Hinode spacecraft,
which has its peak sensitivity at these wavelengths. Ten lines are measured,
arising from seven fine structure levels in the $3p^53d^3$ configuration. Two
lines have not previously been reported and lead to new experimental energies
for the $(a^2D)^3F_{2,3}$ levels. Updated experimental energies are obtained
for the remaining levels. The new atomic model is used to compute theoretical
values for the two density diagnostic ratios $\lambda$196.21/$\lambda$195.39
and $\lambda$196.21/$\lambda$196.06, and densities are derived from EIS spectra
of coronal loop footpoints.
