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		<citationkey>GomesDomiMend:2016:VeAdTh</citationkey>
		<title>On the verification of an adaptive three-dimensional magnetohydrodynamic model</title>
		<year>2016</year>
		<secondarytype>PRE CI</secondarytype>
		<author>Gomes, Anna Karina Fontes,</author>
		<author>Domingues, Margarete Oliveira,</author>
		<author>Mendes, Odim,</author>
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		<group>LAC-CTE-INPE-MCTI-GOV-BR</group>
		<group>DGE-CEA-INPE-MCTI-GOV-BR</group>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<electronicmailaddress>anna.gomes@inpe.br</electronicmailaddress>
		<electronicmailaddress>margarete.domingues@inpe.br</electronicmailaddress>
		<electronicmailaddress>odim.mendes@inpe.br</electronicmailaddress>
		<conferencename>International Conference on Nonlinear Science and Complexity, 6</conferencename>
		<conferencelocation>São José dos Campos, SP</conferencelocation>
		<date>16</date>
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		<contenttype>External Contribution</contenttype>
		<keywords>Fluidodynamics, Plasma and Turbulence, Modeling, Numerical Simulation and Optimization , Geophysical Nonlinear Dynamics , Magnetohydrodynamics, Adaptive Multiresolution Analysis.</keywords>
		<abstract>The magnetohydrodynamics (MHD) is an important tool to study the dynamics of the plasma in Space Physics. In this context, we introduce a 3D-MHD solver with divergence-cleaning in the adaptive multiresolution (MR) CARMEN code. This code uses finite volume method that ensures the conservation of physical quantities and the MR approach, that allows the automatic identification of local structures in the numerical solution. The last provides an adaptive mesh refined only where the solution needs more resolution. The goal is to verify the 3D-MHD CARMEN code in comparing its results with the ones from the well known FLASH code.</abstract>
		<area>COMP</area>
		<language>en</language>
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