Light curves for ϵ Eri over the entire time period of the FUSE observations. The left-hand panel show the O vi light curve (1032 + 1038 Å lines) and the right-hand one an expanded view of the first 25 ks, which has the greatest level of stellar activity. Labels for phases 00 to 29, for intervals that had non-zero exposure of good signal-to-noise, are given and correspond to the Specnum names in the last column of Table 2; i.e., phase 02 did not have sufficient signal and is not in Table 2. The bin size is 200 s for both light curves. Spectral bins are indicated by the dashed vertical lines.