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Updated: Feb 13, 2026

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Stability of barotropic vortex strip on a rotating sphere
Sung-Ik Sohn1, Takashi Sakajo2, Sun-Chul Kim3
1Department of Mathematics, Gangneung-Wonju National University, Gangneung 25457, Korea.
Summary
This study models jet streams using a barotropic vortex strip on a rotating sphere. Increased strip width or rotation speed enhances stability, while complex instabilities arise with differing polar vorticity signs.
Area of Science:
- Fluid dynamics
- Geophysical fluid dynamics
- Atmospheric science
Background:
- Jet streams are crucial atmospheric phenomena influencing global weather patterns.
- Barotropic vortex strips serve as simplified models for understanding jet stream dynamics.
Purpose of the Study:
- To analyze the linear and nonlinear stability of a barotropic vortex strip on a rotating sphere.
- To model atmospheric jet streams and investigate their stability characteristics.
- To explore the geophysical relevance to planetary jet streams.
Main Methods:
- Linear stability analysis of a piecewise-continuous vorticity distribution.
- Numerical computation of nonlinear vortex strip evolution.
- Comparison of linear and nonlinear results.
Main Results:
- Vortex strip stability increases with width and rotation speed.
- The inner flow region is most unstable when polar vorticities are positive and equal.
- Complex instabilities and remote instability regions emerge with opposing polar vorticities.
- Nonlinear simulations show good agreement with linear analysis for small widths, leading to rolling-up vortex cores.
Conclusions:
- The barotropic vortex strip model provides insights into jet stream stability.
- Planetary rotation and vorticity distribution significantly impact jet stream behavior.
- The model's findings have relevance for understanding jet streams on Jupiter, Saturn, and Earth.
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