Long period slow MHD waves in the solar wind source region

Details Long period slow MHD waves in the solar wind source region Long period slow MHD waves in the solar wind source region

2006-12-19

arxiv.org/abs/astro-ph/0612524v2

NewAstron.13:581-586,2008

Astronomy and Astrophysics

Astrophysics

18 pages, 5 figures

Scientific paper

10.1016/j.newast.2008.03.004

We consider compressive viscosity and thermal conductivity to study the
propagation and dissipation of long period slow longitudinal MHD waves in polar
coronal holes. We discuss their likely role in the line profile narrowing, and
in the energy budget for coronal holes and the solar wind. We compare the
contribution of longitudinal MHD waves with high frequency Alfven waves.

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