Line-tied boundary conditions can cause resonant absorption models to generate unphysically large boundary layers
A. P. K. Prokopyszyn, A. N. Wright, A. W. Hood

TL;DR
This study investigates how line-tied boundary conditions in resonant absorption models can lead to overestimated boundary layer amplitudes, emphasizing the importance of wave propagation conditions in solar plasma modeling.
Contribution
The paper demonstrates that line-tied boundary conditions can produce unphysically large boundary layers and highlights the significance of wave propagation in the chromosphere for accurate modeling.
Findings
Line-tied conditions can overestimate boundary layer amplitudes.
Fast wave propagation in the chromosphere affects boundary layer size.
Line-tied models are valid if fast waves are propagative, not evanescent.
Abstract
This paper uses linear magnetohydrodynamics to model resonant absorption in coronal plasma with a Cartesian coordinate system. We impose line-tied boundary conditions and tilt the background magnetic field to be oblique to the transition region. Halberstadt & Goedbloed (1993, 1995); Goedbloed& Halberstadt (1994); Arregui et al. (2003) show that line-tied boundary conditions cause their resonant absorption models to produce steep boundary layers/evanescent fast waves. We aim to study the importance of the boundary layers and assess their significance in a solar context. We calculate the solutions in a model where we impose line-tied boundary conditions and compare this with a model where we include the chromosphere instead. Results are calculated analytically and then verified numerically. We show that line-tied boundary conditions can cause the model to overestimate the boundary layers'…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Magnetic confinement fusion research
