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Update copyright for Kepert wind field
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wind/windmodels.f90

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subroutine fkerpert(R, lam, f, rMax, Vm, thetaFm, vFm, d2Vm, dVm, dP, beta, rho, Ux, Uy, n)
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!$ use omp_lib
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! Kepert, J., 2001: The Dynamics of Boundary Layer Jets within the
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! Analytical linear model of the tropical cyclone boundary layer
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! as in Kepert, J., 2001: The Dynamics of Boundary Layer Jets within the
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! Tropical Cyclone Core. Part I: Linear Theory. J. Atmos. Sci., 58,
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! 2469-2484
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! Written Jeff Kepert, Bureau of Meteorology, 1998-2000.
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! Copyright the Bureau of Meteorology.
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! Please do not distribute without my knowledge.
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! The model is, so far as I know, robust, except if the storm is
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! close to inertially neutral (e.g. b too big). Note that it was written
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! to understand the dynamics, not to make accurate predictions -
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! the constants (C, K, etc) have not been tuned to observations.
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! Note also that because of a linearisation in the derivation, the
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! model does not produce the correct limit in the limit r -> infinity.
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! Modified by Craig Arthur, Geoscience Australia
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! This calculates the Kepert wind field with a Holland pressure profile.
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wind/windmodels.py

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@@ -1054,9 +1054,23 @@ def field(self, R, lam, vFm, thetaFm, thetaMax=0.):
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class KepertWindField(WindFieldModel):
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"""
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Kepert, J., 2001: The Dynamics of Boundary Layer Jets within the
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Analytical linear model of the tropical cyclone boundary layer
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as in Kepert, J., 2001: The Dynamics of Boundary Layer Jets within the
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Tropical Cyclone Core. Part I: Linear Theory. J. Atmos. Sci., 58,
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2469-2484
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Written Jeff Kepert, Bureau of Meteorology, 1998-2000.
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Copyright the Bureau of Meteorology.
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Please do not distribute without my knowledge.
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The model is, so far as I know, robust, except if the storm is
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close to inertially neutral (e.g. b too big). Note that it was written
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to understand the dynamics, not to make accurate predictions -
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the constants (C, K, etc) have not been tuned to observations.
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Note also that because of a linearisation in the derivation, the
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model does not produce the correct limit in the limit r -> infinity.
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Modified by Craig Arthur, Geoscience Australia
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"""
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