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Cited article:

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Measurements of the Solar Coronal Magnetic Field Based on Coronal Seismology with Propagating Alfvénic Waves: Forward Modeling

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3D Magnetohydrodynamic Wave Propagation and Energy Transport in a Simulated Solar Vortex

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Variations in Dominant Wave Period in the Solar Atmosphere

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Using Bright Point Shapes to Constrain Wave Heating of the Solar Corona: Predictions for DKIST

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Kelvin-Helmholtz instability and heating in oscillating loops perturbed by power-law transverse wave drivers

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Alfvénic Motions Arising from Asymmetric Acoustic Wave Drivers in Solar Magnetic Structures

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Influence of the Lower Atmosphere on Wave Heating and Evaporation in Solar Coronal Loops

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How numerical treatments of the transition region modify energy flux into the solar corona

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Modeling of Transverse Oscillations Driven by p-modes in Short Coronal Loops

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Estimating the energy flux of transverse waves associated with Kelvin-Helmholtz instability in solar coronal loops

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