On Kelvin–Helmholtz and parametric instabilities driven by coronal waves

Author:

Hillier Andrew1ORCID,Barker Adrian2,Arregui Iñigo34,Latter Henrik5

Affiliation:

1. Department of Mathematics, CEMPS, University of Exeter, Exeter EX4 4QF, UK

2. Department of Applied Mathematics, School of Mathematics, University of Leeds, Leeds LS2 9JT, UK

3. Instituto de Astrofísica de Canarias, Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain

4. Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain

5. Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wiblerforce Road, Cambridge CB3 0WA, UK

Funder

Science and Technology Facilities Council

Ministerio de Economía y Competitividad

Bayesian Analysis of the Solar Corona

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Nonlinear Wave Damping by Kelvin–Helmholtz Instability-induced Turbulence;The Astrophysical Journal;2024-04-25

2. Parametric resonance of Alfvén waves driven by ionization-recombination waves in the weakly ionized solar atmosphere;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2024-04-25

3. The Fine-scale Structure of Polar Coronal Holes;The Astrophysical Journal;2023-08-25

4. Damping of coronal oscillations in self-consistent 3D radiative magnetohydrodynamics simulations of the solar atmosphere;Astronomy & Astrophysics;2023-08

5. Alfvénic waves in the inhomogeneous solar atmosphere;Reviews of Modern Plasma Physics;2023-03-21

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