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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/EFtuz
Repositorysid.inpe.br/marciana/2005/01.05.08.47
Last Update2005:01.05.02.00.00 (UTC) marcelo.pazos@inpe.br
Metadata Repositorysid.inpe.br/marciana/2005/01.05.08.47.30
Metadata Last Update2018:07.31.14.43.55 (UTC) marcelo.pazos@inpe.br
Secondary KeyINPE-11850-PRE/7197
ISSN0273-1177
Labelself-archiving-INPE-MCTIC-GOV-BR
Citation KeyCecattoSaFeKrNeMo:2003:HiReTi
TitleHigh resolution time profile of decimetric type-III bursts
Year2003
Access Date2024, May 16
Secondary TypePRE PI
Number of Files1
Size649 KiB
2. Context
Author1 Cecatto, José Roberto
2 Sawant, Hanumant Shankar
3 Fernandes, F. C. R.
4 Krishan, Vinod
5 Neri, Jose Angelo da Costa Ferreira
6 Moraes Filho, J. C.
Resume Identifier1 8JMKD3MGP5W/3C9JHJB
2 8JMKD3MGP5W/3C9JHBU
3
4
5 8JMKD3MGP5W/3C9JHFQ
Group1 DAS-INPE-MCT-BR
Affiliation1 Indian Institute of Astrophysics, Bangalore, India
e-Mail Addressjrc@das.inpe.br
JournalAdvances in Space Research
Volume32
Number12
Pages2533-2537
History (UTC)2005-01-05 10:48:52 :: jefferson -> administrator ::
2006-09-28 22:26:04 :: administrator -> banon ::
2007-02-23 19:19:32 :: banon -> administrator ::
2012-07-17 12:44:54 :: administrator -> jefferson ::
2012-10-03 16:06:11 :: jefferson -> administrator :: 2003
2018-06-05 01:21:20 :: administrator -> marciana :: 2003
2018-07-31 14:43:05 :: marciana -> marcelo.pazos@inpe.br :: 2003
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typefinaldraft
AbstractType-III bursts are signatures of the electron beams accelerated during the solar flares, their observation and investi- gation provide information of the acceleration processes, the characteristics of the exciting agent and the acceleration site. The Brazilian Solar Spectroscope (BSS), in operation at INPE, Brazil, have recorded type-III radio bursts in decimetric range (2050-2250 MHz) with high time resolution of 20 ms. Decimetric reverse drift bursts are possi- bly generated in a dense loop by electron beams travelling towards the photosphere. Hence their time profiles should carry signatures of the density inhomogenities in the loop. Here the temporal and spectral characteristics of decimetric type-111 bursts are presented. 0 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > High resolution time...
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/6qtX3pFwXQZsFDuKxG/EFtuz
zipped data URLhttp://urlib.net/zip/6qtX3pFwXQZsFDuKxG/EFtuz
Languageen
Target Filehigh reso_2004.pdf
User Groupadministrator
jefferson
marcelo.pazos@inpe.br
Reader Groupadministrator
jefferson
marcelo.pazos@inpe.br
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.52.30 2
sid.inpe.br/mtc-m21/2012/07.13.14.51.22 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi electronicmailaddress format isbn keywords lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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