Investigating coronal wave energy estimates using synthetic non-thermal line widths

Aims. Estimates of coronal wave energy remain uncertain as a large fraction of the energy is likely hidden in the non-thermal line widths of emission lines. In order to estimate these wave energies, many previous studies have considered the root mean squared wave amplitudes to be a factor of $ \sqrt...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-12, Vol.656, p.A56
Hauptverfasser:	Fyfe, L. E., Howson, T. A., De Moortel, I., Pant, V., Van Doorsselaere, T.
Format:	Artikel
Sprache:	eng
Schlagworte:	Amplitudes Emission analysis Estimates Fluid flow Magnetic fields Magnetohydrodynamics Numerical models Robustness (mathematics) Simulation Three dimensional models Transverse waves Upper bounds Wave power
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