Do Coronal Loops Oscillate in Isolation?
Bradley W. Hindman, Rekha Jain

TL;DR
This paper challenges the common view that coronal loops oscillate independently, showing instead that they are part of a larger, coupled 3D magnetic arcade, which affects how their oscillations should be interpreted.
Contribution
It introduces a multidimensional perspective on coronal loop oscillations, demonstrating that loops are coupled with the surrounding arcade, impacting seismic diagnostics of the solar corona.
Findings
Most loops are too close to other structures to oscillate in isolation.
The true wave cavity is larger and multidimensional than a single loop.
Eigenmodes of the arcade and loop are coupled, complicating mode identification.
Abstract
Images of the solar corona by extreme-ultraviolet (EUV) telescopes reveal elegant arches of glowing plasma that trace the corona's magnetic field. Typically, these loops are preferentially illuminated segments of an arcade of vaulted field lines and such loops are often observed to sway in response to nearby solar flares. A flurry of observational and theoretical effort has been devoted to the exploitation of these oscillations with the grand hope that seismic techniques might be used as probes of the strength and structure of the corona's magnetic field. The commonly accepted viewpoint is that each visible loop oscillates as an independent entity and acts as a one-dimensional (1D) wave cavity for magnetohydrodynamic (MHD) kink waves. We argue that for many events, this generally accepted model for the wave cavity is fundamentally flawed. In particular, the 3D magnetic arcade in which…
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