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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/JwEKp
Repositorysid.inpe.br/iris@1916/2005/12.21.12.35.35   (restricted access)
Last Update2005:12.22.15.35.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2005/12.21.12.35.41
Metadata Last Update2021:07.18.04.01.21 (UTC) administrator
Secondary KeyINPE-12715-PRE/8005
ISSN1364-6826
Citation KeyCecattoSoFeMaAnSa:2005:RaEmOb
TitleRadio emission observed in decimetric waves associated with the onset of CMEs
Year2005
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size434 KiB
2. Context
Author1 Cecatto, José Roberto
2 Soares, Alfredo de Carvalho
3 Fernandes, Francisco Carlos Rocha
4 Madsen, F. R. H.
5 Andrade, Maria Conceição de
6 Sawant, Hanumant Shankar
Resume Identifier1 8JMKD3MGP5W/3C9JHJB
2
3
4
5 8JMKD3MGP5W/3C9JHR2
6 8JMKD3MGP5W/3C9JHBU
Group1 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE, DAS)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume67
Number17-18
Pages1673-1678
History (UTC)2005-12-22 15:35:19 :: jefferson -> administrator ::
2021-07-18 04:01:21 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsRadio emission
CME
Decimetric waves
Solar bursts
AbstractSince the first observations by Skylab and SMM satellites coronal mass ejections (CME) have been more and more investigated. However, until now their origin and trigger mechanism remain an open question no matter if they are associated to flares or not. Recent observations over a broad spectrum suggest that flare energy is released in regions from where the decimetric emission is coming. Then, investigations of decimetric radio emission observed in association with CME phenomena may give clues to solve the previously mentioned questions. Using the Brazilian solar spectroscope (BSS), observations of solar bursts dynamic spectra with high time (100, 50, 20 ms) and frequency (50100 channels) resolutions have been carried out daily (1119 UT) within the range of 10002500 MHz. A sample of 274 CMEs were recorded by the large angle spectroscopic coronagraph (LASCO) instrument, on board the solar and heliospheric observatory (SOHO) satellite, within 1119 UT, during the period of 19992002. From those, 42 CMEs are associated to BSS data and selected for analysis. It is interesting to note that in about half of the cases only one type of burst radio emission was recorded while in the remaining cases either two or more types were observed. There is a dominance of either continuum and/or pulsations. Here, we describe the association of burst radio emission with the starting time of CME phenomena.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Radio emission observed...
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4. Conditions of access and use
Languageen
Target FileRadio emission observed.pdf
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jefferson
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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