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On the propagation and dissipation of Alfvén waves in coronal holes

dc.contributor.authorDwivedi B.N.; Srivastava A.K.
dc.date.accessioned2025-05-24T09:56:52Z
dc.description.abstractWe 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. © Springer 2006.
dc.identifier.doihttps://doi.org/10.1007/s11207-006-0141-2
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/21457
dc.relation.ispartofseriesSolar Physics
dc.titleOn the propagation and dissipation of Alfvén waves in coronal holes

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