A physically based, shear-relative, and Galilean invariant method for predi
cting supercell motion using a hodograph is presented. It is founded on num
erous observational and modeling studies since the 1940s, which suggest a c
onsistent pattern to supercell motion exists. Two components are assumed to
be largely responsible for supercell motion: (i) advection of the storm by
a representative mean wind, and (ii) propagation away from the mean wind e
ither toward the right or toward the left of the vertical wind shear-due to
internal supercell dynamics,Using 290 supercell hodographs, this new metho
d is shown to be statistically superior to existing methods in predicting s
upercell motion for both right- and left-moving storms. Other external fact
ors such as interaction with atmospheric boundaries and orography can have
a pronounced effect on supercell motion, but these are difficult to quantif
y prior to storm development using only a hodograph.