%0 Journal Article
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%@resumeid 8JMKD3MGP5W/3C9JH3D
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%@resumeid 8JMKD3MGP5W/3C9JGH3
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%X We present a review on the interplanetary causes of intense geomagnetic storms (Dsta parts per thousand currency signa'100 nT), that occurred during solar cycle 23 (1997-2005). It was reported that the most common interplanetary structures leading to the development of intense storms were: magnetic clouds, sheath fields, sheath fields followed by a magnetic cloud and corotating interaction regions at the leading fronts of high speed streams. However, the relative importance of each of those driving structures has been shown to vary with the solar cycle phase. Superintense storms (Dsta parts per thousand currency signa'250 nT) have been also studied in more detail for solar cycle 23, confirming initial studies done about their main interplanetary causes. The storms are associated with magnetic clouds and sheath fields following interplanetary shocks, although they frequently involve consecutive and complex ICME structures. Concerning extreme storms (Dsta parts per thousand currency signa'400 nT), due to the poor statistics of their occurrence during the space era, only some indications about their main interplanetary causes are known. For the most extreme events, we review the Carrington event and also discuss the distribution of historical and space era extreme events in the context of the sunspot and Gleissberg solar activity cycles, highlighting a discussion about the eventual occurrence of more Carrington-type storms.
%8 Jan
%N 1
%T Interplanetary Origin of Intense, Superintense and Extreme Geomagnetic Storms
%@electronicmailaddress alicia@dge.inpe.br
%@electronicmailaddress eecher@dge.inpe.br
%@electronicmailaddress
%@electronicmailaddress
%@electronicmailaddress dallago@dge.inpe.br
%@secondarytype PRE PI
%K Intense geomagnetic storms, Atividade Geomagnetica.
%@usergroup administrator
%@usergroup banon
%@usergroup lattes
%@usergroup marciana
%@usergroup tereza@sid.inpe.br
%@group DGE-CEA-INPE-MCT-BR
%@group DGE-CEA-INPE-MCT-BR
%@group
%@group DGE-CEA-INPE-MCT-BR
%@group DGE-CEA-INPE-MCT-BR
%@e-mailaddress alicia@dge.inpe.br
%3 GonzalezA-SpaceSciRev-v158-n1-p69-89fulltext[1].pdf
%@secondarykey INPE--PRE/
%@secondarymark B1_ASTRONOMIA_/_FÍSICA A2_GEOCIÊNCIAS
%F lattes: 7209946672198332 1 GonzalezEchTsuGonLag:2011:InOrIn
%U http://www.springerlink.com/content/l515762587945q1k/
%@issn 0038-6308
%2 dpi.inpe.br/plutao/2011/06.11.14.29.46
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation CALTECH, Jet Prop Lab, Pasadena, CA
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@project FAPESP 2008/06650-9 e 2007/52533-1; CNPq PQ-300321/2005-8, PQ-300211/2008-2, PQ-342734/2008-2
%B Space Science Reviews
%@versiontype publisher
%P 69-89
%4 dpi.inpe.br/plutao/2011/06.11.14.29
%@documentstage not transferred
%D 2011
%V 158
%@doi 10.1007/s11214-010-9715-2
%O Setores de Atividade: Atividades profissionais, científicas e técnicas.
%A Gonzalez, Alicia Luisa Clúa de,
%A Echer, Ezequiel,
%A Tsurutani, Bruce T.,
%A Gonzalez, Alicia L.,
%A Dal Lago, Alisson,
%@dissemination WEBSCI; PORTALCAPES; MGA; COMPENDEX.
%@area CEA