Large-scale storms are rarely observed in Saturn's atmosphere, but the
ir appearance traces the wind velocity field, providing information on
the vertical structure of the clouds and on the dynamics of the atmos
phere. Two large-scale atmospheric disturbances formed by clouds highl
y reflective in the visible part of the spectrum were observed on Satu
rn during 1994. An equatorial disturbance with a longitudinal size of
similar to 27,000 kilometers drifted in longitude with a velocity of 2
73.6 meters per second. A second disturbance, a rapidly evolving conve
ctive storm with an initial size similar to 7000 kilometers, was obser
ved at 56 degrees south, moving with a zonal velocity of 15.5 meters p
er second.