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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/397BN5B
Repositorysid.inpe.br/mtc-m19/2011/02.17.12.51
Last Update2011:02.17.13.05.41 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/02.17.12.51.47
Metadata Last Update2018:06.05.04.35.31 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN0102-261X
Citation KeyEcher:2010:WaAnUL
TitleWavelet analysis of ULF waves in the Mercury's magnetosphere
Year2010
Access Date2024, May 17
Secondary TypePRE PN
Number of Files1
Size946 KiB
2. Context
AuthorEcher, Ezequiel
Resume Identifier8JMKD3MGP5W/3C9JH3D
GroupDGE-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
JournalRevista Brasileira de Geofísica
Volume28
Number2
Pages175-182
History (UTC)2011-09-13 18:17:37 :: marciana -> administrator :: 2010
2011-09-13 18:18:47 :: administrator -> marciana :: 2010
2011-09-13 18:19:25 :: marciana -> administrator :: 2010
2018-06-05 04:35:31 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsMercury’s magnetosphere
ULF waves
wavelet analysis. magnetosfera de Merc´urio
ondas ULF
an´alise por ondeletas
AbstractUltra-low-frequency (ULF) waves have been observed in the Mercury's magnetosphere. In this work, Mariner-10 and MESSENGER high resolution magnetic field data are studied with wavelet analysis. Two ULF wave intervals have been selected: 29 March 1974 (Mariner-10) and 14 January 2008 (MESSENGER). Non-stationary oscillations, with strong amplitude and narrow bandwidth have been found. The Mariner-10 ULF wave interval showed periods of ~1.5-3.0 s, and the MESSENGER ULF wave interval had periods of ~0.5-1.0 s. These periods of ULF waves are slightly longer than the proton gyroperiods (~0.8 and ~0.5 s, respectively). Therefore, these waves are most likely kinetic, not magnetohydrodynamic waves. RESUMO. Ondas de frequencia ultrabaixa (ULF) foram observadas na magnetosfera de Merc´urio. Neste trabalho, dados de campo magn´etico de alta resoluc¸ao das sondas Mariner-10 e MESSENGER sao estudados com an´alise por ondeletas. Dois intervalos de ondas ULF foram selecionados: 29 de marc¸o de 1974 (Mariner-10) e 14 de janeiro de 2008 (MESSENGER). Oscilac¸oes nao estacion´arias, de banda estreita e forte amplitude foram encontradas. As ondas ULF do intervalo da Mariner-10 tinham per´ıodos entre1,5-3,0 s, e as ondas ULF do intervalo da MESSENGER tinham per´ıodos de0,5-1,0 s. Esses per´ıodos das ondas ULF sao ligeiramente maiores que os giro-per´ıodos do pr´oton (0,8 s e0,5 s, respectivamente). Portanto, essas ondas nao sao ondas do tipo magnetohidrodinamico, mas sao provavelmente ondas do tipo cin´etico.
AreaCOMP
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Wavelet analysis of...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/397BN5B
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/397BN5B
Languageen
Target Filev28n2a03.pdf
User Groupadministrator
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
DisseminationPORTALCAPES; SCIELO.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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