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7.1: Introduction

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    Figure \(\PageIndex{1}\): A toroidal vortex, created in an eruption of Mt. Etna and made visible by volcanic steam. The bright spot is the sun (photo by Dr. J. Alean; details on page iii).

    Even in the most chaotic, turbulent flow, long-lived coherent vortices can be identified (e.g., Figure \(\PageIndex{1}\)). In this section we will establish three theorems that tell us why vortices have such a remarkable tendency to stay together. To begin with, we will study the basic aspects of vorticity in the simplest possible form, by neglecting complications due to viscosity and inhomogeneity, i.e., we will assume that \(\mu=v=0\) and \(\rho=\rho_0\). Later, we will add the effects of viscosity and allow \(\rho\) to vary.

    This page titled 7.1: Introduction is shared under a CC BY-NC 4.0 license and was authored, remixed, and/or curated by Bill Smyth via source content that was edited to the style and standards of the LibreTexts platform; a detailed edit history is available upon request.