Long period slow MHD waves in the solar wind source region

dc.contributor.author	Dwivedi, B.N.
dc.contributor.author	Srivastava, A.K.
dc.date.accessioned	2021-09-23T06:26:57Z
dc.date.available	2021-09-23T06:26:57Z
dc.date.issued	2008-11
dc.identifier.issn	13841076
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/1714
dc.description.abstract	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 Alfvén waves.	en_US
dc.description.sponsorship	New Astronomy	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	Issue 8;Volume 13
dc.subject	Coronal holes;	en_US
dc.subject	MHD waves;	en_US
dc.subject	Solar wind;	en_US
dc.title	Long period slow MHD waves in the solar wind source region	en_US
dc.type	Article	en_US