243 citations · 1.5k across the 32 of their papers we have counts for
31 papers
Nonlinear wave damping by Kelvin-Helmholtz instability induced turbulence
Andrew Hillier, Iñigo Arregui, Takeshi Matsumoto
Magnetohydrodynamic kink waves naturally form as a consequence of perturbations to a structured medium, for example transverse oscillations of coronal loops. Linear theory has prov…
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
Andrew Hillier, Ben Snow, Inigo Arregui
In many astrophysical systems, mixing between cool and hot temperature gas/plasma through Kelvin-Helmholtz-instability-driven turbulence leads to the formation of an intermediate t…
Bayesian evidence for a nonlinear damping model for coronal loop oscillations
I. Arregui
Recent observational and theoretical studies indicate that the damping of solar coronal loop oscillations depends on the oscillation amplitude. We consider two mechanisms, linear r…
Coronal heating by MHD waves
Tom Van Doorsselaere, Abhishek K. Srivastava, Patrick Antolin +9
The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction…
Quantifying the evidence for resonant damping of coronal waves with foot-point wave power asymmetry
M. Montes-Solís, I. Arregui
We use Coronal Multi-channel Polarimeter (CoMP) observations of propagating waves in the solar corona and Bayesian analysis to assess the evidence of models with resonant damping a…
Coronal cooling as a result of mixing by the nonlinear Kelvin--Helmholtz instability
Andrew Hillier, Inigo Arregui
Recent observations show cool, oscillating prominence threads fading when observed in cool spectral lines and appearing in warm spectral lines. A proposed mechanism to explain this…