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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36HLAMB
Repositorysid.inpe.br/mtc-m19@80/2009/12.09.18.33   (restricted access)
Last Update2009:12.09.18.33.36 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.09.18.33.37
Metadata Last Update2018:06.05.04.36.00 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2009.05.024
ISSN0273-1177
Citation KeyEcher:2009:FoMaWa
TitleForeshock and magnetosheath waves at Uranus and Neptune studied with wavelet analysis
Year2009
MonthNov.
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size521 KiB
2. Context
AuthorEcher, Ezequiel
Resume Identifier8JMKD3MGP5W/3C9JH3D
GroupDGE-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
JournalAdvances in Space Research
Volume44
Number9
Pages1030-1037
Secondary MarkB3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B2_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2009-12-09 18:33:43 :: simone -> administrator ::
2010-05-11 01:02:47 :: administrator -> simone ::
2011-05-22 13:54:26 :: simone -> administrator ::
2012-11-20 18:34:08 :: administrator -> banon :: 2009
2013-02-19 13:54:17 :: banon -> administrator :: 2009
2018-06-05 04:36:00 :: administrator -> marciana :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsForeshock waves
Magnetosheath waves
Uranus magnetosphere
Neptune magnetosphere
Solar wind
Wavelet analysis
AbstractForeshock and magnetosheath waves in Uranus and Neptune magnetospheres are studied in this work with wavelet analysis. In order to conduct this study, Voyager-2 magnetometer 3-s averaged data are used. The Morlet wavelet transform is applied to the magnetic field vector data. Waves present in the magnetosheath and foreshock regions are highly non-stationary, showing large amplitude variations. It was found that the dominant periods of these waves are longer than the H+ cyclotron period. Overall, high frequency waves are seen near the bow shock crossing and low frequency oscillations near the magnetopause crossing. It can be concluded that non-stationary foreshock and magnetosheath planetary waves can be well characterized with wavelet analysis.
AreaCEA
Arrangementurlib.net > DIDGE > Foreshock and magnetosheath...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Fileforeshock.pdf
User Groupadministrator
banon
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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7. Description control
e-Mail (login)marciana
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