| 1. Identity statement | ||||
| Reference Type | Conference Paper (Conference Proceedings) | |||
| Site | mtc-m21c.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34R/44CP24P | |||
| Repository | sid.inpe.br/mtc-m21c/2021/03.23.12.17 | |||
| Metadata Repository | sid.inpe.br/mtc-m21c/2021/03.23.12.17.42 | |||
| Metadata Last Update | 2022:04.03.19.25.05 (UTC) administrator | |||
| Secondary Key | INPE--PRE/ | |||
| Citation Key | SilvaSRABSVWSJMDZL:2021:EnPaDy | |||
| Title | Energetic particle dynamic on the radiation belts and the generation of the sporadic E- layer (Esa) on the SHMA  | |||
| Year | 2021 | |||
| Access Date | 2024, May 18 | |||
| Secondary Type | PRE CN | |||
| 2. Context | ||||
| Author | 1 Silva, L. A. 2 Shi, J. 3 Resende, Laysa Cristina Araújo 4 Alves, Livia Ribeiro 5 Batista, Inez Staciarini 6 Sibeck, D. 7 Vieira, Luis Eduardo Antunes 8 Wang, C. 9 Souza, Vitor Moura Cardoso e Silva 10 Jauer, P. R. 11 Marchezi, José Paulo 12 Denardini, Clezio Marcos 13 Zhang, S. Y. 14 Liu, Z. | |||
| Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JHDA | |||
| Group | 1 2 3 DICEP-CGCE-INPE-MCTI-GOV-BR 4 DIHPA-CGCE-INPE-MCTI-GOV-BR 5 DIHPA-CGCE-INPE-MCTI-GOV-BR 6 7 DIHPA-CGCE-INPE-MCTI-GOV-BR 8 9 DIHPA-CGCE-INPE-MCTI-GOV-BR 10 11 12 DIHPA-CGCE-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 State Key Laboratory of Space Weather 2 State Key Laboratory of Space Weather 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 Instituto Nacional de Pesquisas Espaciais (INPE) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 NASA Goddard Space Flight Center 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 State Key Laboratory of Space Weather 9 Instituto Nacional de Pesquisas Espaciais (INPE) 10 State Key Laboratory of Space Weather 11 jose.marchezi@inpe.br 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 Chinese Academy of Sciences 14 State Key Laboratory of Space Weather | |||
| Author e-Mail Address | 1 2 3 laysa.resende@gmail.com 4 livia.alves@inpe.br 5 inez.batista@inpe.br 6 7 luis.vieira71@googlemail.com 8 9 vitormoura21@gmail.com 10 11 12 clezio.denardin@inpe.br | |||
| Conference Name | Simpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA) | |||
| Conference Location | Online | |||
| Date | 22-26 mar. | |||
| History (UTC) | 2021-03-23 12:17:42 :: simone -> administrator :: 2021-06-22 19:11:15 :: administrator -> simone :: 2021 2021-06-22 20:59:50 :: simone -> administrator :: 2021 2022-04-03 19:25:05 :: administrator -> simone :: 2021 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Abstract | The energetic particle population in the radiation belts can be affected through the coupling between the solar wind structures and the Earths magnetosphere. When such particles precipitate into the upper atmosphere they may also affect both the ionosphere and the neutral atmosphere, especially at high-latitudes and the Southern Hemisphere Magnetic Anomaly (SHMA). Presently, the impact of the energetic particle precipitation into the highlatitude ionosphere is well understood. On the other hand, the direct impact into the SHMA ionosphere is still lacking in more information. Therefore, a case study (May 28, 2017) is selected during the strong geomagnetic-storm (Dst: -125 nT) associated with an Interplanetary Coronal Mass Ejection. The Van Allen Probes recorded a significant reduction on the radiation belts electron fluxes concomitant with a shock detected by ACE-satellite in the Interplanetary Medium. Particles in a wide range of energy levels were lost to the atmosphere. POES satellite data and FengYun series spacecraft 3C confirm a strong increase of the energetic particle flux in the SHMA region during this storm. Data from a digisonde installed near the center of the SHMA (29.68◦S, 53.81◦W) show the type sporadic E-layer (Esa), unusual in low-latitudes, during several hours. The increase of charged particles in this region can be related to the generation of the Esa layers, which occurrence is associated with particle precipitation. We conclude that the radiation belt dynamics, as well as the particle precipitation on the SHMA region during this storm, are the main components responsible for the generation of the Esa layers over the Brazilian region. | |||
| Area | CEA | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Energetic particle dynamic... | |||
| doc Directory Content | there are no files | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/46KTFK8 | |||
| Host Collection | urlib.net/www/2017/11.22.19.04 | |||
| 6. Notes | ||||
| Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||