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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44CTACP
Repositorysid.inpe.br/mtc-m21c/2021/03.24.11.50
Metadata Repositorysid.inpe.br/mtc-m21c/2021/03.24.11.50.55
Metadata Last Update2022:04.03.19.25.07 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyCecattoMMSRGCF:2021:SoPhPo
TitleSolar phenomena, the possibility to predict their occurrence, and what to expect for next years
Year2021
Access Date2024, May 19
Secondary TypePRE CN
2. Context
Author1 Cecatto, José Roberto
2 Martins, M. V.
3 Mota, Jesuania Maria da Silva Campos
4 Silva, A. E. A. da
5 Ribeiro, M. X.
6 Gradvohl, A. L. S.
7 Coelho, G. P.
8 Fernandes, M. M.
Resume Identifier1 8JMKD3MGP5W/3C9JHJB
Group1 DIAST-CGCE-INPE-MCTI-GOV-BR
2
3 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade Estadual de Campinas (UNICAMP)
5 Universidade Federal de São Carlos (UFSCar)
6 Universidade Estadual de Campinas (UNICAMP)
7 Universidade Estadual de Campinas (UNICAMP)
8 Universidade Federal de São Carlos (UFSCar)
Author e-Mail Address1 jr.cecatto@inpe.br
2
3 jesuaniamaria@outlook.com
Conference NameSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Conference LocationOnline
Date22-26 mar.
History (UTC)2021-03-24 11:50:55 :: simone -> administrator ::
2022-04-03 19:25:07 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractSpace Weather deals mainly with solar phenomena, their generation, interaction with the Earth environment, the way affect technological services / systems as well as methods to mitigate the disturbances, damages and risks to human. Depending on the solar phenomenon and respective characteristics, there is a proper previous time to take decision and realize mitigating actions or not. For example, the solar wind velocity typically varies in the range 250-900 km/s. In this case, assuming a constant velocity since the departure from the Sun up to its arrival at the Earth, there exists a lapse of 2 to 7 days. So, it is possible to predict the wind arrival at the Earth with a due anticipation. This allows mitigating actions be taken. By the other side, a solar flare takes just about 8 minutes to arrive to the Earth. And the registering occurs when the detectors orbiting the Earth measure its electromagnetic radiation. Therefore, in this extreme case the recording is simultaneous with the arrival. Here, we present and discuss about the occurrence, and detection of solar phenomena. Also, we discuss about the recent research and current status on solar flare forecasting.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Solar phenomena, the...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Solar phenomena, the...
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4. Conditions of access and use
Languageen
User Groupsimone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
Empty Fieldsarchivingpolicy 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 readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Description control
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