<?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>2026-05-05T21:09:27Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/39943" metadataPrefix="qdc">https://uvadoc.uva.es/oai/request</request><GetRecord><record><header><identifier>oai:uvadoc.uva.es:10324/39943</identifier><datestamp>2021-06-23T09:46:24Z</datestamp><setSpec>com_10324_1129</setSpec><setSpec>com_10324_931</setSpec><setSpec>com_10324_894</setSpec><setSpec>col_10324_1193</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
<dc:title>On the asymptotic balance between electric and magnetic energies for hydromagnetic relativistic flows</dc:title>
<dc:creator>Núñez Jiménez, Manuel</dc:creator>
<dcterms:abstract>In the equations of classical magnetohydrodynamics, the displacement current is considered&#xd;
vanishingly small due to low plasma velocities. For velocities comparable to the speed of light, the&#xd;
full relativistic electromagnetic equations must be used. In the absence of gravitational forcings&#xd;
and with an isotropic Ohm’s law, it is proved that for poloidal magnetic field and velocity and&#xd;
toroidal electric field, the electric and magnetic energies tend to be equivalent in average for large&#xd;
times. This represents a partial extension of Cowling’s theorem for axisymmetric fields.</dcterms:abstract>
<dcterms:dateAccepted>2019-12-18T12:45:13Z</dcterms:dateAccepted>
<dcterms:available>2019-12-18T12:45:13Z</dcterms:available>
<dcterms:created>2019-12-18T12:45:13Z</dcterms:created>
<dcterms:issued>2013</dcterms:issued>
<dc:type>info:eu-repo/semantics/article</dc:type>
<dc:identifier>PHYSICS OF PLASMAS 20, 062902 (2013)</dc:identifier>
<dc:identifier>1070-664X</dc:identifier>
<dc:identifier>http://uvadoc.uva.es/handle/10324/39943</dc:identifier>
<dc:identifier>10.1063/1.4812197</dc:identifier>
<dc:identifier>062902-1</dc:identifier>
<dc:identifier>6</dc:identifier>
<dc:identifier>062902-7</dc:identifier>
<dc:identifier>Physics of Plasmas</dc:identifier>
<dc:identifier>20</dc:identifier>
<dc:identifier>1089-7674</dc:identifier>
<dc:language>eng</dc:language>
<dc:relation>https://aip.scitation.org/doi/pdf/10.1063/1.4812197?class=pdf</dc:relation>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:rights>http://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights>
<dc:rights>Attribution-NonCommercial-NoDerivatives 4.0 Internacional</dc:rights>
<dc:publisher>American Institute of Physics</dc:publisher>
</qdc:qualifieddc></metadata></record></GetRecord></OAI-PMH>