activity
20002021
most citedOn the nature of kink MHD waves in magnetic flux tubes

205 citations · 1.7k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.SR2021

Acoustic wave properties in footpoints of coronal loops in 3D MHD simulations

Julia M. Riedl, Tom Van Doorsselaere, Fabio Reale +3

Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of…

astro-ph.SR2021★ 36 cited

Non-linear damping of standing kink waves computed with Elsasser variables

Tom Van Doorsselaere, Marcel Goossens, Norbert Magyar +2

In a previous paper, we computed the energy density and the non-linear energy cascade rate for transverse kink waves using Elsasser variables. In this paper, we focus on the standi…

astro-ph.SR2021★ 39 cited

Chromospheric Heating by MHD Waves and Instabilities

A. K. Srivastava, J. L. Ballester, P. S. Cally +7

The importance of the chromosphere in the mass and energy transport within the solar atmosphere is now widely recognised. This review discusses the physics of magnetohydrodynamic (…

astro-ph.SR2020★ 12 cited

Damping of slow surface kink modes in solar photospheric waveguides modeled by one-dimensional inhomogeneities

Shao-Xia Chen, Bo Li, Tom Van Doorsselaere +3

Given the recent interest in magnetohydrodynamic (MHD) waves in pores and sunspot umbrae, we examine the damping of slow surface kink modes (SSKMs) by modeling solar photospheric w…

astro-ph.SR2020★ 16 cited

Resonant absorption: transformation of compressive motions into vortical motions

M. Goossens, I. Arregui, R. Soler +1

This paper investigates the changes in spatial properties when magnetohydrodynamic (MHD) waves undergo resonant damping in the Alfvén continuum. The analysis is carried out for a 1…

astro-ph.SR2020★ 25 cited

Wave pressure and energy cascade rate of kink waves computed with Elsasser variables

Tom Van Doorsselaere, Bo Li, Marcel Goossens +2

Numerical simulations have revealed a new type of turbulence of unidirectional waves in a plasma that is perpendicularly structured (Magyar et al. 2017), named uniturbulence. For t…