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	<metadata ReferenceType="Thesis">
		<site>mtc-m16d.sid.inpe.br 806</site>
		<holdercode>{isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}</holdercode>
		<identifier>8JMKD3MGP7W/36G6PES</identifier>
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		<lastupdate>2022:05.30.17.25.06 sid.inpe.br/mtc-m19@80/2009/08.21.17.02 sergio</lastupdate>
		<metadatarepository>sid.inpe.br/mtc-m19@80/2009/11.30.12.58.18</metadatarepository>
		<metadatalastupdate>2022:05.30.17.25.09 sid.inpe.br/mtc-m19@80/2009/08.21.17.02 sergio {D 2010}</metadatalastupdate>
		<secondarykey>INPE-16649-TDI/1612</secondarykey>
		<citationkey>Silva:2010:DeDiSo</citationkey>
		<title>Detecção de distúrbios solar-interplanetários combinando observações de satélite e de raios cósmicos de superfície para aplicação em clima espacial</title>
		<alternatetitle>Solar-interplanetary disturbances detection combining satellite and ground cosmic rays observations for space weather aplication</alternatetitle>
		<course>GES-SPG-INPE-MCT-BR</course>
		<year>2010</year>
		<date>2009-12-18</date>
		<thesistype>Tese (Doutorado em Geofísica Espacial)</thesistype>
		<secondarytype>TDI</secondarytype>
		<numberofpages>140</numberofpages>
		<numberoffiles>1</numberoffiles>
		<size>21058 KiB</size>
		<author>Silva, Marlos Rockenbach da,</author>
		<group>GES-SPG-INPE-MCT-BR</group>
		<committee>Muralikrisna, Polinaya (presidente), ,</committee>
		<committee>Dal Lago, Alisson (orientador), ,</committee>
		<committee>Echer, Ezequiel ,</committee>
		<committee>Alves, Maria Virgínia ,</committee>
		<committee>Schuch, Nelson Jorge ,</committee>
		<committee>Raulin, Jean-Pierre ,</committee>
		<committee>Serbeto, Antonio de Padua Brito,</committee>
		<e-mailaddress>marlosrs@gmail.com</e-mailaddress>
		<university>Instituto Nacional de Pesquisas Espaciais (INPE)</university>
		<city>São José dos Campos</city>
		<transferableflag>1</transferableflag>
		<keywords>tempestades geomagnéticas, raios cósmicos, estruturas solares, previsão de tempestades geomagnéticas, clima espacial, cosmic rays, geomagnetic storms, solar structures, geomagnetic storms prediction, space weather.</keywords>
		<abstract>Nesta tese é mostrada que a nova metodologia proposta para a análise dos dados da Rede de Muons, em operação desde 2001, passando a chamar-se Rede Global de Detectores de Muons (Global Muon Detector Network) - GMDN após 2006, pode ser uma importante ferramenta para a previsão de estruturas solares que causam tempestades geomagnéticas. Para isto foram utilizados dados registrados pelos instrumentos a bordo do satélite Advanced Composition Explorer - ACE, e dados de raios cósmicos de superfície dos telescópios que formam a GMDN no período de 2001 a 2007. Os telescópios cintiladores de muons encontram-se instalados no Observatório Espacial do Sul - OES/CRS/CIE/INPE-MCT em São Martinho da Serra, Brasil, Nagoya University em Nagoya, Japão, Australian Antartic Division - University of Tansmania em Hobart, Australia e Kuwait University no Kuwait. Os eventos foram classificados de acordo com a intensidade das tempestades medida pelo índice Dst, da seguinte forma: Tempestades Moderadas - MS (- 50 > Dst > -100), Tempestades Intensas - IS (-100 > Dst > -250) e Tempestades Superintensas - SS (Dst < -250). A nova metodologia foi comparada a metodologia de Munakata et al. (2000), sendo observado o dobro de precursores para os três tipos de tempestades com a metodologia proposta nesta tese. As tempestades superintensas são as de maior "previsibilidade", seguidas pelas tempestades intensas e a de menor observação de precursores são as tempestades moderadas. Também foi comprovada a melhoria da metodologia proposta nesta tese, tanto no número de precursores observados, quanto na qualidade de observação dos efeitos, em relação à metodologia de Munakata et al, (2000), e pela primeira vez, há indícios de precursores de tempestades causadas por regiões de interação corotantes (Corotating Interaction Region - CIR). ABSTRACT: In this thesis we show that the new methodology to analize data from the Muon Network in operation since 2001, being called Global Muon Detector Network - GMDN after 2006, can be considered an important tool for the forecasting of solar structures causing geomagnetic storms. Interplanetary and cosmic ray ground based data registered by the instruments onboard the Advanced Composition Explorer (ACE) satellite, and ground based cosmic rays detectors that compose the Muon Network were analyzed from 2001 to 2007. Four different muon cintillator telescopes were used for this study: one installed in the Southern Space Observatory - SSO/CRS/CIE/INPE-MCT, in São Martinho da Serra, Brazil; the other one in Nagoya University, in Nagoya, Japan; another one in the Australian Antartic Division - University of Tansmania in Hobart, Australia; and the last one in the Kuwait University in Kuwait City, Kuwait. The events analyzed were classified into three cathegories according to the storm intensity measured by the Dst index: Moderate Storms (MS) (-50 > Dst > -100 nT), Intense Storms (IS) (-100 > Dst > -250 nT), and Superstorms (SS) (Dst < -250 nT). The new methodology were compared with Munakata et al. (2000) methodology, where were observed that two times of precursors for that three kinds of storms were observed by the methodology proposed in this thesis. Super storms are the ones with the largest "previsibility", followed by the intense storms, and the smaller precursors observation are moderate storms. We could verify that the Proposed Methodology improved, as much in the number of observed precursors, as in the quality of the effects observed, compared to the Munakata et al, (2000)'s methodology, and for the first time, there is indication of precursors of geomagnetic storms caused by Corotating Interaction Region - CIR.</abstract>
		<area>CEA</area>
		<language>pt</language>
		<targetfile>publicacao.pdf</targetfile>
		<usergroup>administrator  </usergroup>
		<usergroup>camila  </usergroup>
		<usergroup>marlosrs@gmail.com  </usergroup>
		<usergroup>ricardo  </usergroup>
		<usergroup>viveca@sid.inpe.br  </usergroup>
		<usergroup>yolanda.souza@mcti.gov.br</usergroup>
		<visibility>shown</visibility>
		<copyright>urlib.net/www/2012/11.12.15.10</copyright>
		<copyholder>SID/SCD</copyholder>
		<readpermission>allow from all</readpermission>
		<documentstage>not transferred</documentstage>
		<mirrorrepository>sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53</mirrorrepository>
		<nexthigherunit>8JMKD3MGPCW/3F2PBEE</nexthigherunit>
		<dissemination>NTRSNASA; BNDEPOSITOLEGAL.</dissemination>
		<hostcollection>sid.inpe.br/mtc-m19@80/2009/08.21.17.02</hostcollection>
		<username>sergio</username>
		<agreement>{TERMO DE DEPOSITO ASSINADO MARLOS ROCKENBACK DA SILVA.pdf} .htaccess .htaccess2</agreement>
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		<supervisor>Dal Lago, Alisson ,,</supervisor>
		<url>http://mtc-m16d.sid.inpe.br/rep-/sid.inpe.br/mtc-m19@80/2009/11.30.12.58</url>
	</metadata>
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