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| dc.contributor.author | Núñez Jiménez, Manuel | |
| dc.date.accessioned | 2017-03-22T15:12:17Z | |
| dc.date.available | 2017-03-22T15:12:17Z | |
| dc.date.issued | 2016 | |
| dc.identifier.citation | .International Journal of Non-Linear Mechanics 86, 96-103 | es |
| dc.identifier.uri | http://uvadoc.uva.es/handle/10324/22706 | |
| dc.description.abstract | Magnetosonic waves traveling in a MHD equilibrium may evolve into shocks. We develop a criterion for the creation of fast shocks in the equatorial plane of axisymmetric equilibria and analyze the influence of the most important parameters. The results are applied to Grad-Shafranov equilibria and accretion disks. | es |
| dc.format.mimetype | application/pdf | es |
| dc.language.iso | eng | es |
| dc.publisher | Elsevier | es |
| dc.rights.accessRights | info:eu-repo/semantics/openAccess | es |
| dc.title | Generation of axisymmetric magnetosonic shock waves: applications to static equilibria and accretion disks | es |
| dc.type | info:eu-repo/semantics/article | es |
| dc.peerreviewed | SI | es |
