Wave heating in gravitationally stratified coronal loops in the presence of resistivity and viscosity

Context. In recent years, coronal loops have been the focus of studies related to the damping of different magnetohydrodynamic (MHD) surface waves and their connection with coronal seismology and wave heating. For a better understanding of wave heating, we need to take into account the effects of di...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2019-03, Vol.623, p.A53
Hauptverfasser:	Karampelas, K., Van Doorsselaere, T., Guo, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	magnetohydrodynamics (MHD) Sun: corona Sun: oscillations
Online-Zugang:	Volltext
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