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

Bibcode
2018RNAAS...2d.196T
DOI
10.3847/2515-5172/aaeb26
Terradas, Jaume; Arregui, I.
Bibliographical reference

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

Advertised on:
10
2018
Number of authors
2
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Not Available
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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
Tobías
Felipe García
In progress
Type
Refereed
Solar Physics (FS)

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