1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3PE7N6B |
Repository | sid.inpe.br/mtc-m21b/2017/08.11.17.39 (restricted access) |
Last Update | 2017:08.11.17.39.31 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21b/2017/08.11.17.39.31 |
Metadata Last Update | 2022:03.18.22.12.14 (UTC) administrator |
DOI | 10.1007/s11207-017-1113-4 |
ISSN | 0038-0938 1573-093X |
Citation Key | AlvesSJSMBAKMMDBRDMVBSGBWA:2017:RoSoWi |
Title | The role of solar wind structures in the generation of ULF waves in the inner magnetosphere |
Year | 2017 |
Month | July |
Access Date | 2024, May 17 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 5386 KiB |
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2. Context | |
Author | 1 Alves, Livia Ribeiro 2 Souza, V. M. 3 Jauer, Paulo Ricardo 4 Silva, Ligia Alves da 5 Medeiros, Cláudia 6 Braga, Carlos Roberto 7 Alves, Maria Virginia 8 Koga, Daiki 9 Marchezi, José Paulo 10 Mendonça, Rafael Rodrigues Souza de 11 Dallaqua, Renato Sergio 12 Barbosa, Marcos Vinicius Grala 13 Rockenbach, Marlos 14 Dal Lago, Alisson 15 Mendes Júnior, Odim 16 Vieira, Luis Eduardo Antunes 17 Banik, Marcelo 18 Sibeck, D. G. 19 G., Kanekal. S. 20 Baker, D. N. 21 Wygant, J. R. 22 A., Kletzing. C. |
Resume Identifier | 1 2 3 4 5 6 7 8JMKD3MGP5W/3C9JHRS 8 9 10 11 8JMKD3MGP5W/3C9JJ5K 12 13 14 8JMKD3MGP5W/3C9JGH3 15 8JMKD3MGP5W/3C9JJ28 |
Group | 1 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 5 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR 6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 7 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 8 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 9 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR 10 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 11 LABAP-COCTE-INPE-MCTIC-GOV-BR 12 GESAST-CEA-SESPG-INPE-MCTIC-GOV-BR 13 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 14 15 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 16 DIDGE-CGCEA-INPE-MCTIC-GOV-BR 17 DIDGE-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | 1 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) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 Instituto Nacional de Pesquisas Espaciais (INPE) 10 Instituto Nacional de Pesquisas Espaciais (INPE) 11 Instituto Nacional de Pesquisas Espaciais (INPE) 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Instituto Nacional de Pesquisas Espaciais (INPE) 14 Instituto Nacional de Pesquisas Espaciais (INPE) 15 Instituto Nacional de Pesquisas Espaciais (INPE) 16 Instituto Nacional de Pesquisas Espaciais (INPE) 17 Instituto Nacional de Pesquisas Espaciais (INPE) 18 NASA/Goddard Space Flight Center 19 NASA/Goddard Space Flight Center 20 University of Colorado Boulde 21 University of Minnesota 22 University of Iowa |
Author e-Mail Address | 1 livia.alves@inpe.br 2 3 paulo.jauer@inpe.br 4 ligia.silva@inpe.br 5 claudia.medeiros@inpe.br 6 carlos.braga@inpe.br 7 mvirginia.alves@inpe.br 8 daiki.koga@inpe.br 9 jose.marchezi@inpe.br 10 rafael.mendonca@inpe.br 11 renato.dallaqua@inpe.br 12 marcos.barbosa@inpe.br 13 marlos.silva@inpe.br 14 alisson.dallago@inpe.br 15 odim.mendes@inpe.br 16 luis.vieira@inpe.br 17 marcelo.banik@inpe.br |
Journal | Solar Physics |
Volume | 292 |
Number | 7 |
Secondary Mark | A2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO |
History (UTC) | 2017-08-11 17:39:31 :: simone -> administrator :: 2017-08-11 17:39:32 :: administrator -> simone :: 2017 2017-08-11 17:42:36 :: simone -> administrator :: 2017 2017-08-12 13:42:59 :: administrator -> simone :: 2017 2017-12-14 15:08:31 :: simone -> administrator :: 2017 2022-03-18 22:12:14 :: administrator -> simone :: 2017 |
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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 |
Version Type | publisher |
Keywords | Solar wind transients Solar wind geoeffectiveness ULF waves Earth's outer radiation belts MHD simulation |
Abstract | The plasma of the solar wind incident upon the Earth's magnetosphere can produce several types of geoeffective events. Among them, an important phenomenon consists of the interrelation of the magnetospheric-ionospheric current systems and the charged-particle population of the Earth's Van Allen radiation belts. Ultra-low-frequency (ULF) waves resonantly interacting with such particles have been claimed to play a major role in the energetic particle flux changes, particularly at the outer radiation belt, which is mainly composed of electrons at relativistic energies. In this article, we use global magnetohydrodynamic simulations along with in situ and ground-based observations to evaluate the ability of two different solar wind transient (SWT) events to generate ULF (few to tens of mHz) waves in the equatorial region of the inner magnetosphere. Magnetic field and plasma data from the Advanced Composition Explorer (ACE) satellite were used to characterize these two SWT events as being a sector boundary crossing (SBC) on 24 September 2013, and an interplanetary coronal mass ejection (ICME) in conjunction with a shock on 2 October 2013. Associated with these events, the twin Van Allen Probes measured a depletion of the outer belt relativistic electron flux concurrent with magnetic and electric field power spectra consistent with ULF waves. Two ground-based observatories apart in 90 degrees. longitude also showed evidence of ULF-wave activity for the two SWT events. Magnetohydrodynamic (MHD) simulation results show that the ULF-like oscillations in the modeled electric and magnetic fields observed during both events are a result from the SWT coupling to the magnetosphere. The analysis of the MHD simulation results together with the observations leads to the conclusion that the two SWT structures analyzed in this article can be geoeffective on different levels, with each one leading to distinct ring current intensities, but both SWTs are related to the same disturbance in the outer radiation belt, i.e. a dropout in the relativistic electron fluxes. Therefore, minor disturbances in the solar wind parameters, such as those related to an SBC, may initiate physical processes that are able to be geoeffective for the outer radiation belt. |
Area | CEA |
Arrangement 1 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAP > The role of... |
Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The role of... |
Arrangement 3 | urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > The role of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
Target File | alves_role.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ET2RFS 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3F2PBEE |
Citing Item List | sid.inpe.br/bibdigital/2013/10.01.22.11 6 sid.inpe.br/mtc-m21/2012/07.13.14.57.24 4 sid.inpe.br/mtc-m21/2012/07.13.14.55.54 4 |
Dissemination | WEBSCI; PORTALCAPES; SCOPUS. |
Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
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