  We report the results of observations designed to investigate the
spectroscopic signatures of dust clouds on the L2 brown dwarf Kelu-1. Time
resolved medium resolution spectra show no significant evidence of variability
in the dust sensitive TiO, CrH and FeH bandheads on the timescale of 1--24
hours. We do however report periodic variability in the psuedo-equivelent width
of H-alpha consistent with the 1.8 hour rotation period previously reported for
this object Clarke, Tinney & Tolley (2002). Near-contemporaneous I-band
photometry shows evidence for non-periodic variability at the level of 2%.
