Close

1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/36HELGE
Repositorysid.inpe.br/mtc-m19@80/2009/12.08.11.44
Last Update2009:12.08.11.44.14 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2009/12.08.11.44.15
Metadata Last Update2018:06.05.04.35.56 (UTC) administrator
Secondary KeyINPE-16653-PRE/11141
DOI10.1017/S1743921309029482
Citation KeyCecatto:2009:ObRaSp
TitleObservations of radio spectra at 1–2.5 GHz associated with CME start time
ProjectFísica do meio interplanetário
Year2009
Access Date2024, May 19
Secondary TypePRE CI
Number of Files1
Size876 KiB
2. Context
AuthorCecatto, José Roberto
Resume Identifier8JMKD3MGP5W/3C9JHJB
GroupDAS-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Conference NameIAU Symposium, 257.
Date2008
Book TitleProceedings
History (UTC)2010-02-10 17:58:28 :: simone -> administrator ::
2018-06-05 04:35:56 :: administrator -> marciana :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsCME
radio
bursts
AbstractWe know Coronal Mass Ejections (CME) and flares are the most energetic phenomena happening on the Sun. Until now the information about origin and trigger mechanism of CMEs remains scarce. Also, there is unconclusive information about the association between them and flares although progress has been made in recent years. Multi-spectral observations suggested that the flare energy release occurs in regions from where the decimetric radio emission originates. In this case, investigations of the solar emission in this wavelength range can give us valuable information about these questions. During last solar maximum the Brazilian Solar Spectroscope (BSS) observed the solar radio spectrum (12.5 GHz) with high time (10020 ms) and frequency (50100 channels) resolutions on a daily (1119 UT) basis. A survey during the period 19992002, shows that a significant fraction (20% −57 events) of CMEs recorded by LASCO has an association with the spectra of radio bursts recorded by BSS. Analysis of the radio spectrum associated to CME shows there is a dominance of continuum and/or pulsation and that the association becomes stronger when we consider the CME acceleration since its origin on the Sun. A statistics of this association between CME dynamics and the characteristics of decimetric radio bursts recorded by BSS is presented. Emphasis is given to observations of the association with CME start time.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Observations of radio...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/36HELGE
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/36HELGE
Languageen
Target Filececatto.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.52.30 1
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber conferencelocation copyright creatorhistory descriptionlevel dissemination documentstage e-mailaddress edition editor electronicmailaddress format isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
e-Mail (login)marciana
update 


Close