  The latest outburst of the recurrent nova RS Oph occurred in 2006 February.
Photometric data presented here show evidence of the resumption of optical
flickering, indicating re-establishment of accretion by day 241 of the
outburst. Magnitude variations of up to 0.32 mag in V-band and 0.14 mag in B on
timescales of 600-7000 s are detected. Over the two week observational period
we also detect a 0.5 mag decline in the mean brightness, from V~11.4 to V~11.9,
and record B~12.9 mag. Limits on the mass accretion rate of ~10^{-10} to
10^{-9} Msun/yr are calculated, which span the range of accretion rates modeled
for direct wind accretion and Roche lobe overflow mechanisms. The current
accretion rates make it difficult for thermonuclear runaway models to explain
the observed recurrence interval, and this implies average accretion rates are
typically higher than seen immediately post-outburst.
