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1. Identity statement
Reference TypeBook Section
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PNKPJE
Repositorysid.inpe.br/mtc-m21b/2017/10.02.16.32   (restricted access)
Last Update2017:10.02.16.32.49 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2017/10.02.16.32.49
Metadata Last Update2021:02.06.22.00.00 (UTC) administrator
Secondary KeyINPE--/
DOI10.1017/S1743921317003738
Citation KeyMagalhãesGoEcEcLoMoRa:2016:GrObSI
TitleGround-based observations of the [SII] 6731 ˚A emission lines of the Io plasma torus
Year2016
Access Date2024, May 05
Secondary TypePRE LI
Number of Files1
Size153 KiB
2. Context
Author1 Magalhães, Fabíola Pinho
2 Gonzalez Alarcon, Walter Demétrio
3 Echer, Ezequiel
4 Echer, Mariza Pereira Souza
5 Lopes, Rosaly
6 Morgenthaler, Jeffrey P.
7 Rathbum, Julie
Group1 DGE-CEA-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
3 DGE-CEA-INPE-MCTI-GOV-BR
4 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 fabiola.magalhaes@inpe.br
2 walter.gonzalez@inpe.br
3 ezequiel.echer@inpe.br
4 mariza.echer@inpe.br
5
6 jpmorgen@psi.edu
EditorNandy, D.
Valio, A.
Petit, P.
Book TitleLiving around active stars: Proceedings IAU Symposium
PublisherIAU
Volume328
Pages227-229
History (UTC)2017-10-02 16:40:31 :: simone -> administrator :: 2016
2021-02-06 22:00:00 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsIo
Io Plasma Torus
Instrumentation
Volcanism
Jupiter magnetosphere
AbstractThe Io Plasma Torus (IPT) is a doughnut-shaped structure of charged particles, composed mainly of sulfur and oxygen ions. The main source of the IPT is the moon Io, the most volcanically active object in the Solar System. Io is the innermost of the Galilean moons of Jupiter, the main source of the magnetospheric plasma and responsible for injecting nearly 1 ton/s of ions into Jupiters magnetosphere. In this work ground-based observations of the [SII] 6731 ˚A emission lines are observed, obtained at the MacMath-Pierce Solar Telescope. The results shown here were obtained in late 1997 and occurred shortly after a period of important eruptions observed by the Galileo mission (1996-2003). Several outbursts were observed and periods of intense volcanic activity are important to correlate with periods of brightness enhancements observed at the IPT. The time of response between an eruption and enhancement at IPT is still not well understood.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Ground-based observations of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
Languageen
Target Filemagalhaes_ground.pdf
User Groupsimone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationBNDEPOSITOLEGAL
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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