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1. Identity statement
Reference TypeConference Abstract (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/38TTRRP
Repositorysid.inpe.br/mtc-m19/2011/01.09.03.44   (restricted access)
Last Update2011:01.09.03.44.18 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/01.09.03.44.18
Metadata Last Update2018:06.05.04.35.11 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyAlvesMurSchMorMac:2010:StIoPl
TitleStudy of the Ionospheric Plasma in the South Atlantic Magnetic Anomaly SAMA Region with Riometers and VLF Receiver at the Brazilian Southern Space Observatory
Year2010
Access Date2024, Apr. 28
Secondary TypePRE CI
Number of Files1
Size60 KiB
2. Context
Author1 Alves, Dimas Igor
2 Muralikrishna, Polinaya
3 Schuch, Nelson Jorge
4 Moro, Juliano
5 Machado, Coelho
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ4G
3 8JMKD3MGP5W/3C9JHUD
Group1 CRS-CCR-INPE-MCT-BR
2 DAE-CEA-INPE-MCT-BR
3 CRS-CCR-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference NameAmerican Advanced Studies Institute School on the Dynamics and Chemistry of the Middle Atmosphere (PASI).
Conference LocationSan Juan, Argentina
Date4-9 October
Book TitleAbstracts
History (UTC)2011-01-09 03:44:31 :: seeger05 -> administrator :: 2010
2018-06-05 04:35:11 :: administrator -> seeger05 :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe South Atlantic Magnetic Anomaly (SAMA) is the region which has the lowest intensity of Earths magnetic field. In this region energetic particles can precipitate, contributing for the ionization of the Earths Ionosphere. In order to study the dynamics of SAMA, the SAVNET (South America Very Low Frequency Network) and SARINET (South America Riometer Network) networks were installed in the Southern Space Observatory (SSO/CRS/CCR/INPE MCT, 29.4ºS, 53.8ºW, 480 m a.s.l), São Martinho da Serra, RS, Brazil. The SAVNET network is composed by three antennas being two loop and one vertical, used for VLF wave propagation (Very Low Frequency, 3 30 kHz). The SAVNET network studies the properties of the successive reflections between the transmitter station and the receiver station through the wave guide formed by the Earths surface and the base of the Ionosphere. Thus it is possible to study the D diurnal layer and the nocturnal E layer of the Ionosphere through analyzes of the phase and amplitude of the VLF waves. The SARINET project aims to study the Ionospheres ionization due the particle precipitation in the SAMA region. The study is carried out by the analyzes of the ionospheric cosmic radio noise absorption in the 38 and 38.2 MHz range, using one channel riometer and an imaging riometer. The absorption is calculated by comparing the intensity of cosmic noise incident in the Earths surface between geomagnetic quiet periods and periods in which there is a high Ionospheres ionization. The present work has as objective to present the SAVNET and SARINET networks used at the Southern Space Observatory, and some results for one geomagnetic disturbed period using an imaging riometer and a VLF receiver.
AreaCEA
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4. Conditions of access and use
Languagefr
Target FilePASI_2010_Abstract_Dimas Irion Alves.pdf
User Groupadministrator
seeger05
Visibilityshown
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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