Transverse energy injection scales at the base of the solar corona

Alfvén wave turbulence models lie at the heart of many investigations into the winds and extreme-ultraviolet and X-ray emission from cool, solar-like stars. The models provide insights into mass loss, magnetic spin down and exoplanet habitability. Yet they currently rely on ad hoc estimates of criti...

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Veröffentlicht in:	Nature astronomy 2023-11, Vol.7 (11), p.1301-1308
Hauptverfasser:	Sharma, Rahul, Morton, Richard J.
Format:	Artikel
Sprache:	eng
Schlagworte:	639/33 639/33/34 Astronomy Astrophysics and Cosmology Atmospheric turbulence Lattice theory Physics Physics and Astronomy Turbulence models
Online-Zugang:	Volltext
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