Sanjay Kumar Pandey, Kriti Yadav
Abstract In this paper, we present an analytical model for atmospheric vortices that includes three velocity components---axial, azimuthal, and radial, and a pressure distribution. The model modifies a stream function with a central low-pressure core and applies a correction to the azimuthal velocity to capture the Reynolds number-dependent shear-layer behavior near the ground. The proposed model effectively confines
rotational motion to a compact region around the core, with the
azimuthal velocity decaying super-exponentially with radial distance,
in contrast to classical vortex models such as those by Burgers,
Vatistas, and Rankine, where the azimuthal velocity decays only
algebraically and remains non-negligible at large radii. A range of
vortex intensities can be represented using parametric control via a
shape factor and Reynolds number. Comparative analysis shows that the
present model produces sharper, more localized velocity peaks and
pronounced vertical pressure variations, consistent with field
observations. This model provides a more physically realistic
description of atmospheric vortices.