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		<citationkey>FariaStepSawa:2009:BrDeAr</citationkey>
		<title>Brazilian decimetric array configuration in a nutshell</title>
		<format>On-line</format>
		<project>Brazilian Decimetric Array</project>
		<year>2009</year>
		<date>July 28 – August 1, 2008</date>
		<numberoffiles>1</numberoffiles>
		<size>117 KiB</size>
		<author>Faria, Cláudio,</author>
		<author>Stephany, Stephan,</author>
		<author>Sawant, Hanumant S.,</author>
		<resumeid></resumeid>
		<resumeid>8JMKD3MGP5W/3C9JJ9D</resumeid>
		<group></group>
		<group>LAC-CTE-INPE-MCT-BR</group>
		<group>DAS-CEA-INPE-MCT-BR</group>
		<affiliation>Pontifícia Universidade Católica de Minas Gerais - PUCMinas</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<electronicmailaddress>cfaria@pucpcaldas.br</electronicmailaddress>
		<electronicmailaddress>stephan@lac.inpe.br</electronicmailaddress>
		<electronicmailaddress>sawant@das.inpe.br</electronicmailaddress>
		<editor>Scientific,</editor>
		<editor>Sawant, Hanumant Shankar,</editor>
		<editor>Rao, A. Pramesh,</editor>
		<editor>Gopalswamy, Natchimuthukonar,</editor>
		<editor>Hurford, Gordon J.,</editor>
		<editor>Ananthakrishnan, Subramaniam,</editor>
		<editor>Executive,</editor>
		<editor>Fernandes, Francisco Carlos Rocha,</editor>
		<editor>Moraes, Luís Cesar Pereira de,</editor>
		<e-mailaddress>lcmoraes@das.inpe.br</e-mailaddress>
		<conferencename>Brazilian Decimetric Array Workshop.</conferencename>
		<conferencelocation>INPE</conferencelocation>
		<pages>41-46</pages>
		<booktitle>Proceedings</booktitle>
		<publisher>INPE</publisher>
		<publisheraddress>São José dos Campos</publisheraddress>
		<secondarytype>PRE CI</secondarytype>
		<tertiarytype>Paper</tertiarytype>
		<transferableflag>1</transferableflag>
		<keywords>ANTENNAS, CONFIGURATION, BDA.</keywords>
		<abstract>Here we present the proposed configuration for the second phase of the BDA, Brazilian Decimetric Array. The corresponding u-v coverage and synthesized beam are also presented as well as results obtained employing simulated solar images from the Nobeyama data.</abstract>
		<area>COMP</area>
		<language>en</language>
		<targetfile>41-46 brazilian.pdf</targetfile>
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