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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/NigMs
Repositorysid.inpe.br/mtc-m17@80/2006/11.28.16.16   (restricted access)
Last Update2006:11.28.16.18.20 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2006/11.28.16.16.19
Metadata Last Update2018:06.05.03.44.05 (UTC) administrator
Secondary KeyINPE-14366-PRE/9453
ISSN0273-1177
Citation KeySawantFKMKCMA:2006:HaReDe
TitleHarmonically related decimetric fine structures
Year2006
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size1329 KiB
2. Context
Author1 Sawant, Hanumant Shankar
2 Fernandes, Francisco Carlos Rocha
3 Karlicky, M.
4 Mészárosova, H.
5 Krishan, V.
6 Cecatto, José Roberto
7 Madsen, Felipe Ramos Hald
8 Andrade, Maria Conceição de
Resume Identifier1 8JMKD3MGP5W/3C9JHBU
Group1 DAS-INPE-MCT-BR
2 DAS-INPE-MCT-BR
3
4
5
6 DAS-INPE-MCT-BR
7 DAS-INPE-MCT-BR
8 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Ondrejov Observatory
4 Ondrejov Observatory
5 Indian Institute of Astrophysics
6 Instituto Nacional de Pesquisas Espaciais (INPE)
7 Instituto Nacional de Pesquisas Espaciais (INPE)
8 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalAdvances in Space Research
Volume38
Number3
Pages406-410
History (UTC)2006-11-28 16:18:21 :: simone -> administrator ::
2012-11-24 01:39:08 :: administrator -> banon :: 2006
2013-02-19 13:56:01 :: banon -> simone :: 2006
2013-02-20 15:19:51 :: simone -> administrator :: 2006
2018-06-05 03:44:05 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar flares
Radio radiation
Harmonically related decimetric fine structures
Plasma emission
Acceleration region
AbstractWe report rare events, above 1000 MHz, in which emission at the fundamental and at second harmonic frequencies show nearly identical fine structures. These high resolution observations are obtained from the Brazilian Solar Radio Spectrograph operating in the frequency range (2150 ± 100) MHz, and the Ondrejov observatory Solar Radio Spectrograph operating in the frequency range of (8002000) MHz. These bursts have flux values of about 300 s.f.u. and total duration between 100 and 500 ms. The frequency and flux ratios of the harmonically related narrow band bursts varied from 1.76 to 2.29 and 1.28 to 3.57, respectively. The lower observed flux of the fundamental component in comparison to the second harmonic could be due to its higher collisional absorption assuming that the generation mechanism of these bursts is due to the beam plasma interaction. The heights of the acceleration regions estimated from the starting frequencies of the decimetric fine structures are 104 km.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Harmonically related decimetric...
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4. Conditions of access and use
Languageen
Target FileHarmonically related decimetric.pdf
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simone
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; MGA; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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7. Description control
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