1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34T/45D52JB |
Repository | sid.inpe.br/mtc-m21d/2021/09.07.15.24 |
Last Update | 2021:09.07.15.24.34 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21d/2021/09.07.15.24.34 |
Metadata Last Update | 2022:04.03.19.24.01 (UTC) administrator |
DOI | 10.1029/2021JA029363 |
ISSN | 2169-9402 |
Citation Key | SilvaSASMMVACSDJWLLAS:2021:StAn |
Title | High-Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to the Alfvénic Fluctuations Within High-Speed Solar Wind Stream: A Statistical Analysis |
Year | 2021 |
Month | Aug. |
Access Date | 2024, May 16 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 9474 KiB |
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2. Context | |
Author | 1 Silva, Ligia Alves da 2 Shi, J. 3 Alves, Livia Ribeiro 4 Sibeck, D. 5 Marchezi, José Paulo 6 Medeiros, Cláudia 7 Vieira, Luís Eduardo Antunes 8 Agapitov, O. 9 Cardoso, F. R. 10 Souza, Vitor Moura Cardoso e Silva 11 Dal Lago, Alisson 12 Jauer, Paulo Roberto 13 Wang, C. 14 Li, H. 15 Liu, Z. 16 Alves, Maria Virgínia 17 Silva, Marlos Rockenbach da |
Resume Identifier | 1 2 3 4 5 6 7 8 9 10 11 8JMKD3MGP5W/3C9JGH3 12 13 14 15 16 8JMKD3MGP5W/3C9JHRS |
ORCID | 1 0000-0002-8822-5030 2 0000-0002-8008-0527 3 0000-0002-5680-7271 4 0000-0003-3240-7510 5 0000-0002-2904-6411 6 0000-0002-6914-5799 7 0000-0002-9376-475X 8 0000-0001-6427-1596 9 0000-0001-7239-0894 10 0000-0001-7294-7963 11 0000-0002-4361-6492 12 0000-0002-8064-5030 13 0000-0001-6991-9398 14 0000-0002-4839-4614 15 0000-0001-8034-5575 16 0000-0002-7477-1233 17 0000-0002-9737-9429 |
Group | 1 DIHPA-CGCE-INPE-MCTI-GOV-BR 2 3 DIHPA-CGCE-INPE-MCTI-GOV-BR 4 5 DIHPA-CGCE-INPE-MCTI-GOV-BR 6 DIHPA-CGCE-INPE-MCTI-GOV-BR 7 DIHPA-CGCE-INPE-MCTI-GOV-BR 8 9 10 DIHPA-CGCE-INPE-MCTI-GOV-BR 11 DIHPA-CGCE-INPE-MCTI-GOV-BR 12 DIHPA-CGCE-INPE-MCTI-GOV-BR 13 14 15 16 DIHPA-CGCE-INPE-MCTI-GOV-BR 17 DIHPA-CGCE-INPE-MCTI-GOV-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Chinese Academy of Sciences 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 NASA Goddard Space Flight Center 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Instituto Nacional de Pesquisas Espaciais (INPE) 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 University of California 9 Universidade de São Paulo (USP) 10 Instituto Nacional de Pesquisas Espaciais (INPE) 11 Instituto Nacional de Pesquisas Espaciais (INPE) 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Chinese Academy of Sciences 14 Chinese Academy of Sciences 15 Chinese Academy of Sciences 16 Instituto Nacional de Pesquisas Espaciais (INPE) 17 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 ligia.alves01@gmail.com |
Journal | Journal of Geophysical Research: Space Physics |
Volume | 126 |
Number | 8 |
Pages | e2021JA029363 |
History (UTC) | 2021-09-07 15:24:34 :: simone -> administrator :: 2021-09-07 15:24:35 :: administrator -> simone :: 2021 2021-09-07 15:30:32 :: simone -> administrator :: 2021 2022-04-03 19:24:01 :: administrator -> simone :: 2021 |
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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 | electron flux enhancement high speed solar wind stream high-energy electron flux outer radiation belt ultra low frequency waves whistler-mode chorus waves |
Abstract | The coupling response between solar wind structures and the magnetosphere is highly complex, leading to different effects in the outer radiation belt electron fluxes. Most Coronal Mass Ejections cause strong geomagnetic storms with short recovery phases, often 12 days. By contrast, High-Speed Solar Wind Streams lead to moderate and weak storms often with much longer recovery phases, from several to ∼10 days. The magnetosphere receives energy for a long time under the influence of the HSSs, considerably changing its dynamics. This in turn has an effect on the charged particles trapped in the outer radiation belt. Although the high-energy electron flux enhancements have received considerable attention, the high-energy electron flux enhancement pattern (L > 4) has not. This paper identifies 37 events with this enhancement pattern in the high-energy electron flux during the Van Allen Probes era. We find the enhancements coincident with HSS occurrence. The interplanetary magnetic field (IMF) exhibits north/south Bz fluctuations of Alfvénic nature with moderate amplitudes. The high-energy electron flux enhancements also correspond to long periods of auroral activity indicating a relationship to magnetotail dynamics. However, the AE index only reaches moderate values. Ultra-Low Frequency waves were present in all of the events and whistler-mode chorus waves were present in 89.1% of the events, providing a convenient scenario for wave-particle interactions. The radial gradient of the ULF wave power related to the L, under the influence of the HSSs, is necessary to trigger the physical processes responsible for this type of high-energy electron flux enhancement pattern. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > High-Energy Electron Flux... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
data URL | http://urlib.net/ibi/8JMKD3MGP3W34T/45D52JB |
zipped data URL | http://urlib.net/zip/8JMKD3MGP3W34T/45D52JB |
Language | en |
Target File | silva_high.pdf |
User Group | simone |
Visibility | shown |
Archiving Policy | denypublisher6 allowfinaldraft |
Read Permission | allow from all |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/46KTFK8 |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.55.54 5 sid.inpe.br/mtc-m21/2012/07.13.14.39.46 2 |
Dissemination | WEBSCI; AGU; MGA; COMPENDEX. |
Host Collection | urlib.net/www/2021/06.04.03.40 |
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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 parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
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