On Coronal Loop Heating by Torsional Alfvén Waves

Details On Coronal Loop Heating by Torsional Alfvén Waves On Coronal Loop Heating by Torsional Alfvén Waves

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..199..307n&link_type=abstract

Solar Physics, v. 199, Issue 2, p. 307-315 (2001).

Physics

5

Scientific paper

Heating of coronal loops by linear resonant Alfvén waves, excited by the footpoints motions in the photosphere, has been studied. The analysis of single-layer heating is extended to multilayer heating, in semiempirical treatment. Heating and nonthermal velocities in different layers of loops in X-ray bright points, active regions, and large-scale structures are estimated. The average value of velocity is found to be in agreement with the observations.

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