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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3KQ6RCP
Repositóriosid.inpe.br/mtc-m21b/2015/12.17.17.50
Repositório de Metadadossid.inpe.br/mtc-m21b/2015/12.17.17.50.27
Última Atualização dos Metadados2018:06.04.02.55.59 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoAlvesEchTsuCosLak:2015:HiLaHe
TítuloHigh latitude heliospheric magnetic decrease properties observed by Ulysses
Ano2015
Data de Acesso28 abr. 2024
Tipo SecundárioPRE CI
2. Contextualização
Autor1 Alves, Maria Virgínia
2 Echer, Ezequeil
3 Tsurutani, B. T.
4 Costa Júnior, E. da
5 Lakhina, G. S.
Identificador de Curriculo1 8JMKD3MGP5W/3C9JHRS
Grupo1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Jet Propulsion Laboratory
4 Instituto Federal de Minas Gerais
5 Indian Institute for Geomagnetism
Endereço de e-Mail do Autor1 mvirginia.alves@inpe.br
2 eecher@dge.inpe.br
Nome do EventoIUGG General Assembly, 26
Localização do EventoPrague, Czech Republic
Data22 June - 02 July
Histórico (UTC)2015-12-17 17:50:28 :: simone -> administrator ::
2018-06-04 02:55:59 :: administrator -> simone :: 2015
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoMagnetic Decreases (MDs) are regions with abrupt decreases in the interplanetary magnetic field (IMF) magnitude. Ulysses spacecraft magnetic field and plasma data provide a unique opportunity to study MDs at high heliographic latitudes (HHL). We use a computer code on Ulysses high-resolution magnetic field data to obtain the MD occurrence rates and features under a variety of solar cycle and solar wind conditions. Ulysses first orbit had polar passes in 1994 (South Pole, S1) and 1995 (North Pole, N1), near the declining and solar minimum phases. The second orbit, with polar passes in 2000 (S2) and 2001 (N2), occurred during a solar maximum phase. The third orbit, with polar passes in 2007 (S3) and 2008 (N3), occurred near solar minimum, with an opposite solar magnetic field polarity of first pass. Among the six polar passes we found S1 and N1 are representatives for MDs occurring at HHLs during a typical solar minimum, when the solar plasma is mainly composed of high speed streams coming from coronal holes. For S1 we found a MD occurrence rate of ~12 MDs/day, an angular variation of IMF (Da) of ~27° and a duration time for MDs (Dt) of ~17s. For N1 we found a MD occurrence rate of ~15 MDs/day, Da~26° and Dt~20s. These results are quite different from the ones found for MDs at low heliographic latitudes: ~4 MDs/day, Dt~42s, and Da~6°. MDs that present Da<10° are usually attributed to mirror instability. The origin of MDs observed at HHLs is still an open question, and depends on a careful analysis of high resolution plasma parameters where MDs occur. The S2 pass shows several days where the MD occurrence rate is zero. Preliminary results indicate the absence of MDs are associated with low solar wind velocities, <500km/s, low density Np <1cm-3, and low beta, <1.0.
ÁreaCEA
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4. Condições de acesso e uso
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Visibilidadeshown
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Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhosid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
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