Long period slow MHD waves in the solar wind source region

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dc.creatorDwivedi, B. N.
dc.creatorSrivastava, A. K.
dc.date2006-12-19
dc.date2007-12-17
dc.date.accessioned2026-07-07T11:42:41Z
dc.date.available2026-07-07T11:42:41Z
dc.descriptionWe 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.
dc.description18 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0612524
dc.identifierhttp://arxiv.org/abs/astro-ph/0612524
dc.identifierNewAstron.13:581-586,2008
dc.identifierdoi:10.1016/j.newast.2008.03.004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200974
dc.subjectAstrophysics
dc.titleLong period slow MHD waves in the solar wind source region
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