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It is defined as:
- where D is a characteristic (usually vertical) length scale of a phenomenon; ν, the kinematic eddy viscosity; Ω, the angular velocity of planetary rotation; and φ, the latitude. The term 2 Ω sin φ is the Coriolis acceleration.
When the Ekman number is small, disturbances are able to propagate before decaying owing to frictional effects.