"Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observati" by K. Tziotziou, E. Scullion et al.
 

Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling

Document Type

Article

Publication Date

2-1-2023

Abstract

Vortex flows, related to solar convective turbulent dynamics at granular scales and their interplay with magnetic fields within intergranular lanes, occur abundantly on the solar surface and in the atmosphere above. Their presence is revealed in high-resolution and high-cadence solar observations from the ground and from space and with state-of-the-art magnetoconvection simulations. Vortical flows exhibit complex characteristics and dynamics, excite a wide range of different waves, and couple different layers of the solar atmosphere, which facilitates the channeling and transfer of mass, momentum and energy from the solar surface up to the low corona. Here we provide a comprehensive review of documented research and new developments in theory, observations, and modelling of vortices over the past couple of decades after their observational discovery, including recent observations in H α, innovative detection techniques, diverse hydrostatic modelling of waves and forefront magnetohydrodynamic simulations incorporating effects of a non-ideal plasma. It is the first systematic overview of solar vortex flows at granular scales, a field with a plethora of names for phenomena that exhibit similarities and differences and often interconnect and rely on the same physics. With the advent of the 4-m Daniel K. Inouye Solar Telescope and the forthcoming European Solar Telescope, the ongoing Solar Orbiter mission, and the development of cutting-edge simulations, this review timely addresses the state-of-the-art on vortex flows and outlines both theoretical and observational future research directions.

Identifier

85145974028 (Scopus)

Publication Title

Space Science Reviews

External Full Text Location

https://doi.org/10.1007/s11214-022-00946-8

e-ISSN

15729672

ISSN

00386308

Issue

1

Volume

219

Grant

262622

Fund Ref

Australian Government

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