AbstractThis letter obtains a typhoon-like vortex solution by solving the Bragg-Hawthorne equation. The solution describes spiral paths of fluid material element on the Bernoulli surface, whereas some new exact solutions are obtained which are bounded in the whole region. The first one is a continued umbrella vortex solution, which is a typhoon-like vortex. The second one is a multi-planar solution, which is periodic in z-coordinate. Within each layer, there is an umbrella vortex solution similar to the first one. The above explicit solutions can be applied to the study of radial structure of typhoon. Both the solutions and the approaches used in the present work can also be applied to other complex flows
An important issue in the formation of concentric eyewalls in a tropical cyclone is the development ...
We investigate the interaction between a typhoon and the background winds, the easterlies and the we...
As the first step of the investigation of the wind distribution in the planetary boundary layer near...
AbstractThis letter obtains a typhoon-like vortex solution by solving the Bragg-Hawthorne equation. ...
On the basis of Newton's second motion law, the perturbation-condensed water is added to the mo...
AbstractIn this paper, Digital-Kakejiku typhoon model is constructed based on fluid mechanics. The s...
The thesis is focused on the asymmetric dynamics of tropical cyclones. The first step of this resear...
The structure of typhoon spiral cloud band and its transportation characteristics are difficult theo...
The article of record as published may be found at http://dx.doi.org/10.1002/2016JD025317In observat...
The dynamics and evolution of spiral rainbands in numerical simulations of tropical cyclones are exa...
The steady axis-symmetrical atmosphere dynamical equations are used for describing spiral structure ...
An important issue in the formation of concentric eyewalls in a tropical cy-clone is the development...
This is the second part of a study that examines spiral rainbands in a numerical simulation of Hurri...
A vortex sheet is a surface across which the velocity field of incompressible and inviscid flows has...
The 3D Navier-Stokes equation for incompressible fluid is resolved by using the Lie group analysis m...
An important issue in the formation of concentric eyewalls in a tropical cyclone is the development ...
We investigate the interaction between a typhoon and the background winds, the easterlies and the we...
As the first step of the investigation of the wind distribution in the planetary boundary layer near...
AbstractThis letter obtains a typhoon-like vortex solution by solving the Bragg-Hawthorne equation. ...
On the basis of Newton's second motion law, the perturbation-condensed water is added to the mo...
AbstractIn this paper, Digital-Kakejiku typhoon model is constructed based on fluid mechanics. The s...
The thesis is focused on the asymmetric dynamics of tropical cyclones. The first step of this resear...
The structure of typhoon spiral cloud band and its transportation characteristics are difficult theo...
The article of record as published may be found at http://dx.doi.org/10.1002/2016JD025317In observat...
The dynamics and evolution of spiral rainbands in numerical simulations of tropical cyclones are exa...
The steady axis-symmetrical atmosphere dynamical equations are used for describing spiral structure ...
An important issue in the formation of concentric eyewalls in a tropical cy-clone is the development...
This is the second part of a study that examines spiral rainbands in a numerical simulation of Hurri...
A vortex sheet is a surface across which the velocity field of incompressible and inviscid flows has...
The 3D Navier-Stokes equation for incompressible fluid is resolved by using the Lie group analysis m...
An important issue in the formation of concentric eyewalls in a tropical cyclone is the development ...
We investigate the interaction between a typhoon and the background winds, the easterlies and the we...
As the first step of the investigation of the wind distribution in the planetary boundary layer near...