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This document discusses the transformation of a torus in active galactic nuclei (AGN) into a dipole toroidal vortex due to twisting by radiation or wind. It explores the implications of this transformation on accretion disks, potential instability responsible for quasar radiation flares, and proposes a \'matreshka\' scheme to explain AGN variability and evolution. The model parameters are estimated numerically and shown to correlate well with observations.
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Dipole toroidal vortexes refer to a specific configuration of fluid motion characterized by two counter-rotating toroidal (ring-shaped) vortices. This phenomenon is studied in fluid dynamics and has applications in various fields such as meteorology, oceanography, and engineering.
Typically, researchers, scientists, and engineers who study or utilize dipole toroidal vortexes in their work may be required to file documentation or reports about their findings or applications in specific regulatory contexts.
Filling out documentation related to dipole toroidal vortexes involves collecting relevant data on the characteristics of the vortices, their effects, and any experimental or analytical results. Standard forms or templates should be followed as per the regulatory requirements in the specific field.
The purpose of studying dipole toroidal vortexes is to understand their behavior and interactions in fluid systems. This knowledge can be applied in various fields, such as improving fluid flow in engineering applications or predicting weather patterns.
Information that must be reported typically includes the size, strength, and stability of the vortices, experimental conditions, observations, and conclusions drawn from the studies.
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