Generation of axisymmetric magnetosonic shock waves: applications to static equilibria and accretion disks

Título

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