<?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>2026-04-27T13:47:00Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/39943" metadataPrefix="mods">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><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
<mods:name>
<mods:namePart>Núñez Jiménez, Manuel</mods:namePart>
</mods:name>
<mods:extension>
<mods:dateAvailable encoding="iso8601">2019-12-18T12:45:13Z</mods:dateAvailable>
</mods:extension>
<mods:extension>
<mods:dateAccessioned encoding="iso8601">2019-12-18T12:45:13Z</mods:dateAccessioned>
</mods:extension>
<mods:originInfo>
<mods:dateIssued encoding="iso8601">2013</mods:dateIssued>
</mods:originInfo>
<mods:identifier type="citation">PHYSICS OF PLASMAS 20, 062902 (2013)</mods:identifier>
<mods:identifier type="issn">1070-664X</mods:identifier>
<mods:identifier type="uri">http://uvadoc.uva.es/handle/10324/39943</mods:identifier>
<mods:identifier type="doi">10.1063/1.4812197</mods:identifier>
<mods:identifier type="publicationfirstpage">062902-1</mods:identifier>
<mods:identifier type="publicationissue">6</mods:identifier>
<mods:identifier type="publicationlastpage">062902-7</mods:identifier>
<mods:identifier type="publicationtitle">Physics of Plasmas</mods:identifier>
<mods:identifier type="publicationvolume">20</mods:identifier>
<mods:identifier type="essn">1089-7674</mods:identifier>
<mods: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.</mods:abstract>
<mods:language>
<mods:languageTerm>eng</mods:languageTerm>
</mods:language>
<mods:accessCondition type="useAndReproduction">info:eu-repo/semantics/openAccess</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">http://creativecommons.org/licenses/by-nc-nd/4.0/</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">Attribution-NonCommercial-NoDerivatives 4.0 Internacional</mods:accessCondition>
<mods:titleInfo>
<mods:title>On the asymptotic balance between electric and magnetic energies for hydromagnetic relativistic flows</mods:title>
</mods:titleInfo>
<mods:genre>info:eu-repo/semantics/article</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>