& Tornado Alley
a Rankine Vortex on a Sphere
One approach to modeling tropical cyclones is as rankine vortices. A Rankine vortex is one in which the inner part turns as a disk and in the outer part the velocity is inversely proportional to the distance from the center; i.e.,
where va is the tangential velocity at r=a. In a cyclone a would be the radius of the eyewall.
In computing the angular momentum in a Rankine vortex each band of width Δr in the outer portion has the same angular momentum so a Rankine vortex that extends to infinity would have an infinite angular momentum. Or, stated another way, the angular momentum of a Rankine vortex is directly proportional to the outer limit of the vortex even though the velocity at the outer limit may be negligibly small. But tropical cyclones are on the sphere of the Earth and therefore necessarily of finite extent.
Let θ be the angle from the center of the vortex to a point a distance r from the center and let R be the radius of the sphere. The distance r is then Rθ and hence the formula for the velocities in a Rankine vortex on a sphere is:
The angular momentum of an infinitesimal element with respect to the spin axis of the vortex is the areal density ρ times the velocity times the distance s of the element from the spin axis. The distance s of a point at angle θ from the spin axis is Rsin(θ). The area of a band of with dθ centered at an angle θ is (2πs)Rdθ=(2πRsin(θ)dθ.
The angular momentum L is then the integral of the angular momenta in bands of width Rdθ; i.e.,
In meteorology quantities are usually stated per unit mass. The mass of the vortex is ρ(4πR2) so the angular momentem of the vortex per unit mass is
The integral must be evaluated for the inner and outer parts of the vortex separately. For the inner part of the vortex the angle θ ranges from 0 to a/R so the integral is
The indefinite integral of
so the angular momentum of the inner portion of the vortex evaluates to
The evaluation of the angular momentum for the outer part of the vortex involves the integral of sin2(θ)/θ. The indefinite integral of this quantity is
Thus the angular momentum per unit mass for the outer portion of the vortex evaluates to
where again θa is the angular distance of the eyewall of the vortex from the center of the sphere; i.e., a/R.
In SI units the typical values for a hurricane are:
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