Potential vorticity structure of simulated hurricanes
Potential vorticity structure of simulated hurricanes
复制标题
DOI:
10.1175/jas3601.1
复制
发表时间:
2006-01-01
影响因子:
3.1
通讯作者:
Schubert, WH
中科院分区:
文献类型:
--
作者:
Hausman, SA;Ooyama, KV;Schubert, WH
To better understand the processes involved in tropical cyclone development, the authors simulate an axisymmetric tropical-cyclone-like vortex using a two-dimensional model based on nonhydrostatic dynamics, equilibrium thermodynamics, and bulk microphysics. The potential vorticity principle for this nonhydrostatic, moist, precipitating atmosphere is derived. The appropriate generalization of the dry potential vorticity is found to be P=rho(-1){(-partial derivative upsilon/partial derivative z) (partial derivative theta(rho)/partial derivative r) + [f+partial derivative(r upsilon)/r partial derivative r] (partial derivative theta(rho)/partial derivative z)}, where rho is the total density, upsilon is the azimuthal component of velocity, and theta(p) is the virtual potential temperature. It is shown that P carries all the essential dynamical information about the balanced wind and mass fields. In the fully developed, quasi-steady-state cyclone, the P field and the theta(p) field become locked together, with each field having an outward sloping region of peak values on the inside edge of the eyewall cloud. In this remarkable structure, the P field consists of a narrow, leaning tower in which the value of P can reach several hundred potential vorticity (PV) units.Sensitivity experiments reveal that the simulated cyclones are sensitive to the effects of ice, primarily through the reduced fall velocity of precipitation above the freezing level rather than through the latent heat of fusion, and to the effects of vertical entropy transport by precipitation.