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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
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Identifier8JMKD3MGP3W34P/3KQ6RCP
Repositorysid.inpe.br/mtc-m21b/2015/12.17.17.50
Metadata Repositorysid.inpe.br/mtc-m21b/2015/12.17.17.50.27
Metadata Last Update2018:06.04.02.55.59 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyAlvesEchTsuCosLak:2015:HiLaHe
TitleHigh latitude heliospheric magnetic decrease properties observed by Ulysses
Year2015
Access Date2024, May 17
Secondary TypePRE CI
2. Context
Author1 Alves, Maria Virgínia
2 Echer, Ezequeil
3 Tsurutani, B. T.
4 Costa Júnior, E. da
5 Lakhina, G. S.
Resume Identifier1 8JMKD3MGP5W/3C9JHRS
Group1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 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
Author e-Mail Address1 mvirginia.alves@inpe.br
2 eecher@dge.inpe.br
Conference NameIUGG General Assembly, 26
Conference LocationPrague, Czech Republic
Date22 June - 02 July
History (UTC)2015-12-17 17:50:28 :: simone -> administrator ::
2018-06-04 02:55:59 :: administrator -> simone :: 2015
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractMagnetic 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.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > High latitude heliospheric...
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Update Permissionnot transferred
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Mirror Repositorysid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Next Higher Units8JMKD3MGPCW/3EU29DP
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6. Notes
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