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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/38Q5L7P
Repositorysid.inpe.br/mtc-m19/2010/12.16.15.26
Last Update2011:03.01.20.09.31 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2010/12.16.15.26.13
Metadata Last Update2018:06.05.04.34.57 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1051/0004-6361/200913305
ISSN0004-6361
1432-0746
Citation KeyEcher:2010:SoWiEf
TitleSolar wind effects on Jupiter non-Io DAM emissions during Ulysses distant encounter (2003-2004)
Year2010
MonthSet.
Access Date2024, May 17
Secondary TypePRE PI
Number of Files1
Size604 KiB
2. Context
AuthorEcher, Ezequiel
Resume Identifier8JMKD3MGP5W/3C9JH3D
GroupDGE-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
e-Mail Addresslise@dpi.inpe.br
JournalAstronomy & Astrophysics
Volume519
NumberA84
Pages8
History (UTC)2011-01-05 12:30:13 :: marciana -> administrator :: 2010
2011-02-26 22:28:34 :: administrator -> marciana :: 2010
2011-03-01 20:06:09 :: marciana -> lise@dpi.inpe.br :: 2010
2011-09-13 12:40:31 :: lise@dpi.inpe.br -> marciana :: 2010
2012-01-26 10:55:24 :: marciana -> administrator :: 2010
2018-06-05 04:34:57 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsplanets and satellites: general
solar wind
DECAMETRIC RADIO-EMISSION
BROAD-BAND
MAGNETOSPHERE
ORIGIN
SHOCKS
STORMS
AbstractAims. We analyze solar wind data from the Ulysses spacecraft during the distant Jupiter encounter from 2003 November to 2004 March as well as Nancay decametric (DAM) radio observations non-controlled by Io. Methods. The Ulysses solar wind data are balistically propagated towards Jupiter and are correlated with Nancay non-Io DAM emissions. Results. It is found that the average solar wind dynamic pressure around the time of DAM emissions is 1.7 times higher than its average value during the Ulysses encounter. The occurrence of fast forward (FS) and reverse (RS) interplanetary shocks and heliospheric current sheet crossings (HCS) is correlated with the occurrence of non-Io DAM emissions. We note an enhanced probability of occurrence of non-Io DAM emissions after the expected arrival of FS, RS and HCS at Jupiter. However, about half emissions (54%) did not seem to be associated with these interplanetary structures. We also note that the average duration and power of non-Io DAM emissions are enhanced during periods associated with those interplanetary structures. Conclusions. From the results obtained in this work it seems that non-Io DAM emissions occur during intervals of enhanced solar wind dynamic pressure. Yet, there is no direct correlation between the non-Io DAM emissions duration or power versus the solar wind pressure values and the interplanetary shock Mach number.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Solar wind effects...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 16/12/2010 13:26 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/38Q5L7P
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/38Q5L7P
Languageen
Target File12.16.15.26__0004-6361.pdf
User Groupadministrator
lise@dpi.inpe.br
marciana
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 2
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 2
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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7. Description control
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