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1. Identity statement
Reference TypeSlides (Audiovisual Material)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP8W/34BG6CR
Repositorysid.inpe.br/mtc-m18@80/2008/12.04.19.27.23   (restricted access)
Last Update2008:12.04.19.27.22 (UTC) seeger05
Metadata Repositorysid.inpe.br/mtc-m18@80/2008/12.04.19.27.26
Metadata Last Update2018:06.04.04.05.51 (UTC) administrator
Citation KeyAntunesSchuSiquTriv:2008:RaInMo
TitleRadio interference monitoring at the Brazilian Southern Space Observatory
FormatOn-line
Year2008
Access Date2024, Apr. 27
Number of Files1
Size9500 KiB
2. Context
Author1 Antunes, Cassio Espíndola
2 Schuch, Nelson Jorge
3 Siqueira, Josemar de
4 Trived, Nalin Babulal
Group1 RSU-CIE-INPE-MCT-BR
2 RSU-CIE-INPE-MCT-BR
3 RSU-CIE-INPE-MCT-BR
4 DGE-CEA-INPE-MCT-BR
Affiliation1 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)
Conference NameInternational Astronautical Congress, (59th).
Conference LocationGlasgow, Scotland
Date29 september - 03 October
PublisherInstituto Nacional de Pesquisas Espaciais
Publisher CitySão José dos Campos
History (UTC)2008-12-04 19:27:26 :: seeger05 -> administrator ::
2018-06-04 04:05:51 :: administrator -> seeger05 ::
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractThe Southern Space Observatory - SSO/CRS/CIE/INPE - MCT, (29S, 53W) at São Martinho da Serra, RS, in South of Brazil, carried out several radio sciences experiments. One of the main points for the success of such researches is the observed low level of electromagnetic noise, either natural or anthropogenic radio frequency sources. This was one of the main factors for choosing the site location for the SSO. For monitoring the interference level at the Observatorys site it is realized, since 1992, the periodic data acquisition on the 10-240MHz range of radio frequency. The procedures to determine the radio noise level were realized using one spectrum analyzer and an omnidirectional antenna. The methodology of data acquisitions was to amplify the signal from the antenna, then evaluate this signal in one spectrum analyzer, through a GPIB. The data is instantly transmitted from SSO to the Radio Frequency and Telecommunication Laboratory at the Southern Regional Space Research Center - CRS/CIE/INPE - MCT, in Santa Maria, RS, for further analysis and stored, allowing monitoring the Electromagnetic Spectrum power for long periods. The site quality is remarkable, as the power of the Electromagnetic Spectrum is much lower than that measured at the Radio Frequency and Telecommunication Laboratory, in Santa Maria,RS, where the signals do not exceed -60 dB. On the Site at the SSO, due to the low power observed, weak radio signals can only be received by using good quality amplifiers. Another important feature is that in the frequency range between 115 to 180 MHz, no significant signal power is observed in this Electromagnetic Spectrum range The several observations of the Electromagnetic Spectrum at the SSO, obtained since 1992, are compared with the currents observations. The analyze among different frequency bands, during these periods of data acquisition, show that the SSO remain free of any strong electromagnetic interference, being ideal for the installation of radio astronomic instrumentation.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Radio interference monitoring...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Radio interference monitoring...
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4. Conditions of access and use
Languageen
Target FileIAC 2008 presentation IAC-08-B1.I.6 Cassio V_1.2 Comparative studies...pps
User Groupseeger05
Visibilityshown
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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