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Long period slow MHD waves in the solar wind source region
| dc.contributor.author | Dwivedi B.N.; Srivastava A.K. | |
| dc.date.accessioned | 2025-05-24T09:56:25Z | |
| 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. © 2008 Elsevier B.V. All rights reserved. | |
| dc.identifier.doi | https://doi.org/10.1016/j.newast.2008.03.004 | |
| dc.identifier.uri | http://172.23.0.11:4000/handle/123456789/20965 | |
| dc.relation.ispartofseries | New Astronomy | |
| dc.title | Long period slow MHD waves in the solar wind source region |