46 citations · 199 across the 13 of their papers we have counts for
13 papers
A comparison of pendulum models for large-amplitude longitudinal prominence oscillations
Iñigo Arregui
Large-amplitude prominence oscillations offer diagnostic information relevant to understanding the magnetic and plasma structure of solar prominences. Accurate prominence seismolog…
Signatures of Damping Nonlinear Oscillations by KHI-induced Turbulence in Synthetic Observations
Sihui Zhong, Andrew Hillier, Iñigo Arregui
Large-amplitude decaying kink oscillations of coronal loops are strongly influenced by nonlinear processes, such as Kelvin-Helmholtz instability (KHI) and turbulence, though compre…
Inferring physical parameters of solar filaments from simultaneous longitudinal and transverse oscillations
Upasna Baweja, Vaibhav Pant, Iñigo Arregui +1
Context. Different modes of oscillations are frequently observed in solar prominences/filaments, and prominence seismology helps estimate important physical parameters like the mag…
MHD waves with mixed properties / Alfvén waves with pressure variations: a review
Marcel Goossens, Iñigo Arregui, Roberto Soler +2
Non-uniformity plays an important role for MHD waves. For a uniform plasma of infinite extent the MHD waves can be subdivided in two classes with distinct properties. The first cla…
Identification of Nonlinear Damping of Transverse Loop Oscillations by KHI-induced Turbulence
Sihui Zhong, Andrew Hillier, Iñigo Arregui
Kink oscillations in coronal loops have been extensively studied for their potential contributions to coronal heating and their role in plasma diagnostics through coronal seismolog…
Coronal heating
Iñigo Arregui, Tom Van Doorsselaere
Coronal heating refers to the physical processes that shape and structure the corona of the Sun and are responsible for its multi-million Kelvin temperatures. These processes are r…