On the Propagation and Dissipation of Alfvén Waves in Coronal Holes

Details On the Propagation and Dissipation of Alfvén Waves in Coronal Holes On the Propagation and Dissipation of Alfvén Waves in Coronal Holes

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006soph..237..143d&link_type=abstract

Solar Physics, Volume 237, Issue 1, pp.143-152

Physics

10

Scientific paper

We underline the importance of Alfvén wave dissipation in the
magnetic funnels through the viscous and resistive plasma. Our results
show that Alfvén waves are one of the primary energy sources in
the innermost part of coronal holes where the solar wind outflow starts.

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