1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3LKHJK2 |
Repository | sid.inpe.br/mtc-m21b/2016/05.03.12.18 |
Last Update | 2016:07.13.12.47.16 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21b/2016/05.03.12.18.01 |
Metadata Last Update | 2021:07.28.22.15.55 (UTC) administrator |
DOI | 10.1002/2015JA022146 |
ISSN | 2169-9402 |
Citation Key | SantosAbdSouSobBat:2016:DiZoVe |
Title | Disturbance zonal and vertical plasma drifts in the Peruvian sector during solar minimum phases |
Year | 2016 |
Month | Mar. |
Access Date | 2024, May 11 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 15941 KiB |
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2. Context | |
Author | 1 Santos, Angela Machado dos 2 Abdu, Mangalathayil Ali 3 Souza, Jonas Rodrigues de 4 Sobral, José Humberto Andrade 5 Batista, Inez Staciarini |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JHNK 3 8JMKD3MGP5W/3C9JHFE 4 8JMKD3MGP5W/3C9JHHA 5 8JMKD3MGP5W/3C9JHDA |
Group | 1 DAE-CEA-INPE-MCTI-GOV-BR 2 DAE-CEA-INPE-MCTI-GOV-BR 3 DAE-CEA-INPE-MCTI-GOV-BR 4 DAE-CEA-INPE-MCTI-GOV-BR 5 DAE-CEA-INPE-MCTI-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) |
Author e-Mail Address | 1 angela.santos@inpe.br 2 maabdu@dae.inpe.br 3 jonas.souza@inpe.br 4 jsobral@dae.inpe.br 5 inez.batista@inpe.br |
Journal | Journal of Geophysical Research: Space Physics |
Volume | 121 |
Number | 3 |
Pages | 2503-2521 |
History (UTC) | 2016-05-03 12:18:01 :: simone -> administrator :: 2016-06-04 05:08:29 :: administrator -> simone :: 2016 2016-06-20 15:52:06 :: simone -> administrator :: 2016 2016-07-04 12:30:00 :: administrator -> simone :: 2016 2016-07-13 12:47:16 :: simone -> administrator :: 2016 2021-07-28 22:15:55 :: administrator -> simone :: 2016 |
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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 | electric field ionospheric drifts magnetic storms |
Abstract | In the present work, we investigate the behavior of the equatorial F region zonal plasma drifts over the Peruvian region under magnetically disturbed conditions during two solar minimum epochs, one of them being the recent prolonged solar activity minimum. The study utilizes the vertical and zonal components of the plasma drifts measured by the Jicamarca (11.95°S; 76.87°W) incoherent scatter radar during two events that occurred on 10 April 1997 and 24 June 2008 and model calculation of the zonal drift in a realistic ionosphere simulated by the Sheffield University Plasmasphere-Ionosphere Model-INPE. Two main points are focused: (1) the connection between electric fields and plasma drifts under prompt penetration electric field during a disturbed periods and (2) anomalous behavior of daytime zonal drift in the absence of any magnetic storm. A perfect anticorrelation between vertical and zonal drifts was observed during the night and in the initial and growth phases of the magnetic storm. For the first time, based on a realistic low-latitude ionosphere, we will show, on a detailed quantitative basis, that this anticorrelation is driven mainly by a vertical Hall electric field induced by the primary zonal electric field in the presence of an enhanced nighttime E region ionization. It is shown that an increase in the field line-integrated Hall-to-Pedersen conductivity ratio ∑H∑P, which can arise from precipitation of energetic particles in the region of the South American Magnetic Anomaly, is capable of explaining the observed anticorrelation between the vertical and zonal plasma drifts. Evidence for the particle ionization is provided from the occurrence of anomalous sporadic E layers over the low-latitude station, Cachoeira Paulista (22.67°S; 44.9°W)-Brazil. It will also be shown that the zonal plasma drift reversal to eastward in the afternoon two hours earlier than its reference quiet time pattern is possibly caused by weakening of the zonal wind system during the prolonged solar minimum period. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Disturbance zonal and... |
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/8JMKD3MGP3W34P/3LKHJK2 |
zipped data URL | http://urlib.net/zip/8JMKD3MGP3W34P/3LKHJK2 |
Language | en |
Target File | santos_disturbance.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Archiving Policy | denypublisher6 allowfinaldraft |
Read Permission | allow from all |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | urlib.net/www/2011/03.29.20.55 |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Citing Item List | sid.inpe.br/bibdigital/2013/09.29.20.43 3 sid.inpe.br/mtc-m21/2012/07.13.14.51.12 2 sid.inpe.br/mtc-m21/2012/07.13.14.54.26 1 |
Dissemination | WEBSCI; PORTALCAPES; COMPENDEX; 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 nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
update | |
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