<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-05-05T11:13:57Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/22703" metadataPrefix="dim">https://uvadoc.uva.es/oai/request</request><GetRecord><record><header><identifier>oai:uvadoc.uva.es:10324/22703</identifier><datestamp>2021-06-23T09:45:49Z</datestamp><setSpec>com_10324_1129</setSpec><setSpec>com_10324_931</setSpec><setSpec>com_10324_894</setSpec><setSpec>col_10324_1193</setSpec></header><metadata><dim:dim xmlns:dim="http://www.dspace.org/xmlns/dspace/dim" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.dspace.org/xmlns/dspace/dim http://www.dspace.org/schema/dim.xsd">
<dim:field mdschema="dc" element="contributor" qualifier="author" authority="35f5f517760adfdd" confidence="500" orcid_id="">Núñez Jiménez, Manuel</dim:field>
<dim:field mdschema="dc" element="date" qualifier="accessioned">2017-03-22T12:27:36Z</dim:field>
<dim:field mdschema="dc" element="date" qualifier="available">2017-03-22T12:27:36Z</dim:field>
<dim:field mdschema="dc" element="date" qualifier="issued">2016</dim:field>
<dim:field mdschema="dc" element="identifier" qualifier="citation" lang="es">Physics Letters A 380, 3817-3822</dim:field>
<dim:field mdschema="dc" element="identifier" qualifier="uri">http://uvadoc.uva.es/handle/10324/22703</dim:field>
<dim:field mdschema="dc" element="description" qualifier="abstract" lang="es">The evolution of fast magnetosonic waves of high frequency propa-&#xd;
gating into an axisymmetric equilibrium plasma is studied. By using&#xd;
the methods of weakly nonlinear geometrical optics, it is shown that the&#xd;
perturbation travels in the equatorial plane while satisfying a transport&#xd;
equation which enables us to predict the time and location of formation of&#xd;
shock waves. For plasmas of large magnetic Prandtl number, this would&#xd;
result into the creation of sheet currents which may give rise to magnetic&#xd;
reconnection and destruction of the original equilibrium.</dim:field>
<dim:field mdschema="dc" element="format" qualifier="mimetype" lang="es">application/pdf</dim:field>
<dim:field mdschema="dc" element="language" qualifier="iso" lang="es">eng</dim:field>
<dim:field mdschema="dc" element="publisher" lang="es">Elsevier</dim:field>
<dim:field mdschema="dc" element="rights" qualifier="accessRights" lang="es">info:eu-repo/semantics/restrictedAccess</dim:field>
<dim:field mdschema="dc" element="title" lang="es">Generation of sheet currents by high frequency fast magnetosonic waves</dim:field>
<dim:field mdschema="dc" element="type" lang="es">info:eu-repo/semantics/article</dim:field>
<dim:field mdschema="dc" element="peerreviewed" lang="es">SI</dim:field>
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