1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZGivnJVY/LBDT7 |
Repository | sid.inpe.br/mtc-m16@80/2006/06.30.18.18 (restricted access) |
Last Update | 2006:06.30.18.18.19 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m16@80/2006/06.30.18.18.21 |
Metadata Last Update | 2018:06.05.01.16.51 (UTC) administrator |
Secondary Key | INPE-13810--PRE/8996 |
ISSN | 0273-1177 |
Citation Key | BrumAbdBatCarTer:2006:NuSiNi |
Title | Numerical simulation of nighttime electron precipitation in the lower ionosphere over a sub-auroral region |
Year | 2006 |
Access Date | 2024, May 02 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 462 KiB |
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2. Context | |
Author | 1 Brum, Crhistiano Garnett Marques 2 Abdu, Mangalathayil Ali 3 Batista, Inez Starciarini 4 Carrasco, Alexander Jos¨¦ 5 Terra, Petrina Morais |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JHNK |
Group | 1 DAE-INPE-MCT-BR 2 DAE-INPE-MCT-BR 3 DAE-INPE-MCT-BR 4 DAE-INPE-MCT-BR 5 DAE-INPE-MCT-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais, Divisã 2 o de Aeronomia (INPE.DAE) 3 Instituto Nacional de Pesquisas Espaciais, Divisã 4 o de Aeronomia (INPE.DAE) 5 Instituto Nacional de Pesquisas Espaciais, Divisã |
Journal | Advances in Space Research |
Volume | 37 |
Number | 5 |
Pages | 1051-1057 |
History (UTC) | 2006-08-03 12:12:10 :: simone -> administrator :: 2018-06-05 01:16:51 :: administrator -> marciana :: 2006 |
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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 | Computational simulation of electron precipitation events Sub-auroral lower ionosphere Cosmic noise absorption |
Abstract | This work presents computational simulations of electron precipitation events in the lower ionosphere to explain 30 MHz riometer absorption events registered at the Brazilian Antarctic Station ¨C BAS (62.56¡ãS; 58.39¡ãW). The simulations are based on the calculation of ion production rates from different sources (interplanetary and geocoronal ultraviolet radiations, energetic electrons and cosmic rays) and the use of a detailed ion chemical scheme to obtain the electron density which is then used to calculate the absorption at 30 MHz. The electron density calculations were performed using the continuity equations for 25 positive ions and 10 negative ions, involving 175 chemical reactions, that are solved under chemical equilibrium condition. The simulation results show that a flux of ¡Ö2.5 ¡Á 106 electrons cm−2 s−1 can increase the ionospheric cosmic noise absorption by 1 dB. The results also show that the amplitude of the maximum absorption is sensitive to variations in the precipitated electron flux in the energy range of 98¨C320 keV that affect most the height region of 65¨C85 km, and that a larger contribution of the ionospheric absorption due to electron precipitation arising from above the height of absorption peak (rather than from below it), that is, the lower energy range of the precipitated electron spectra has a more dominant contribution to the attenuation of the galactic cosmic noise signal. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Numerical simulation of... |
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 | Numerical simulation of nighttime electron precipitation.pdf |
User Group | administrator simone |
Visibility | shown |
Copy Holder | SID/SCD |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | transferred to simone |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark 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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