Define . The linearization about givesThe Galilean transformation , has and . It removes the leading advection, leavingFor a normal mode proportional to , the second and fourth derivatives contribute and . The dispersion relation is thereforeFor and , the unstable wavenumbers satisfy . In the laboratory coordinates, the temporal exponent is , so this linear stability calculation predicts growth together with downslope transport at dimensionless speed .
Articles by others on the same topic
There are currently no matching articles.