1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP7W/36HLAMB |
Repository | sid.inpe.br/mtc-m19@80/2009/12.09.18.33 (restricted access) |
Last Update | 2009:12.09.18.33.36 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m19@80/2009/12.09.18.33.37 |
Metadata Last Update | 2018:06.05.04.36.00 (UTC) administrator |
Secondary Key | INPE--PRE/ |
DOI | 10.1016/j.asr.2009.05.024 |
ISSN | 0273-1177 |
Citation Key | Echer:2009:FoMaWa |
Title | Foreshock and magnetosheath waves at Uranus and Neptune studied with wavelet analysis |
Year | 2009 |
Month | Nov. |
Access Date | 2024, May 02 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 521 KiB |
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2. Context | |
Author | Echer, Ezequiel |
Resume Identifier | 8JMKD3MGP5W/3C9JH3D |
Group | DGE-CEA-INPE-MCT-BR |
Affiliation | Instituto Nacional de Pesquisas Espaciais (INPE) |
Journal | Advances in Space Research |
Volume | 44 |
Number | 9 |
Pages | 1030-1037 |
Secondary Mark | B3_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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Keywords | Foreshock waves Magnetosheath waves Uranus magnetosphere Neptune magnetosphere Solar wind Wavelet analysis |
Abstract | Foreshock 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. |
Area | CEA |
Arrangement | urlib.net > DIDGE > Foreshock and magnetosheath... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | foreshock.pdf |
User Group | administrator banon simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Mirror Repository | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
Next Higher Units | 8JMKD3MGPCW/3EU29DP |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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