We present and interpret observations of the preflare phase of the eru
ptive flare of 15 November, 1991 in NOAA AR 6919. New flux emerged in
this region, indicated by arch filaments in Ha and increasing vertical
flux in vector magnetograms. With increasing frequency before the eru
ption, transient dark H alpha fibrils were observed that crossed Ha br
ight plage and the magnetic inversion line to extend from the region o
f flux emergence to the filament, whose eruption was associated with t
he flare. These crossing fibrils were dynamic, and were often associat
ed with sites of propagating torsional motion. These sites propagated
from the region of flux emergence into the filament Aux system. We int
erpret these morphological and dynamic features in terms of relaxation
after magnetic reconnection episodes which create longer held lines w
ithin the filament Aux system, as envisioned in the tether cutting mod
el, and transfer twist to it, as well.