Temporal and Spatial Scales for Coronal Heating by Alfvén Wave Dissipation in Transverse Loop Oscillations

Terradas, Jaume; Arregui, I.
Bibliographical reference

Research Notes of the American Astronomical Society, Volume 2, Issue 4, article id. 196, 0 pp. (2018).

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2018
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Solar and Stellar Magnetism

Magnetic fields are at the base of star formation and stellar structure and evolution. When stars are born, magnetic fields brake the rotation during the collapse of the mollecular cloud. In the end of the life of a star, magnetic fields can play a key role in the form of the strong winds that lead to the last stages of stellar evolution. During

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