Alfven Wave Transmission and Heating of Solar Coronal Loops

Details Alfven Wave Transmission and Heating of Solar Coronal Loops Alfven Wave Transmission and Heating of Solar Coronal Loops

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...499..945l&link_type=abstract

Astrophysical Journal v.499, p.945

Astronomy and Astrophysics

Astronomy

10

Magnetohydrodynamics: Mhd, Sun: Corona, Sun: Magnetic Fields, Waves

Scientific paper

We discuss the problem of wave transmission from the solar photosphere
into coronal loops. We conclude that wave energy can be efficiently
transmitted into loops with a sufficiently twisted magnetic field. The
value of the required twist is below but close to the threshold for kink
instability.

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