We present a detailed mode identification performed on the 1994 Whole Earth
Telescope (WET) run on GD 358. The results are compared with that obtained
for the same star from the 1990 WET data. The two temporal spectra show ve
ry few qualitative differences, although amplitude changes are seen in most
modes, including the disappearance of the mode identified as k = 14 in the
1990 data. The excellent coverage and signal-to-noise ratio obtained durin
g the 1994 run lead to the secure identification of combination frequencies
up to fourth order, i.e. peaks that are sums or differences of up to four
parent frequencies, including a virtually complete set of second-order freq
uencies, as expected from harmonic distortion. We show how the third-order
frequencies are expected to affect the triplet structure of the normal mode
s by back-interacting with them. Finally, a search for l = 2 modes was unsu
ccessful, not verifying the suspicion that such modes had been uncovered in
the 1990 data set.