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GD 358 has been observed twice with the WET, four years apart. The basic temporal spectral pattern did not change during this period. Large changes in relative amplitude were observed for the high power oscillations, and noticeable changes occurred on a time scale of a few days. Our physical models must be improved to explain short time scale variations.doi:10.1515/astro-1995-0306 fatcat:iuewfj5fj5hq3cn7hede4tdmei