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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP8W/35GGST5
Repositorysid.inpe.br/mtc-m18@80/2009/06.19.18.32   (restricted access)
Last Update2009:06.19.18.32.14 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m18@80/2009/06.19.18.32.16
Metadata Last Update2020:04.28.17.48.41 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2009.01.032
ISSN0273-1177
Citation KeyMeszarosovaSCRKFAJ:2009:CoFaWa
TitleCoronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare
Year2009
MonthMay
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size598 KiB
2. Context
Author1 Meszarosova, H.
2 Sawant, Hanumant Shankar
3 Cecatto, José Roberto
4 Rybak, J.
5 Karlicky, M.
6 Fernandes, F. C. R.
7 Andrade, M. C.
8 Jiricka, K.
Resume Identifier1
2 8JMKD3MGP5W/3C9JHBU
Group1
2 DAS-CEA-INPE-MCT-BR
3 DAS-CEA-INPE-MCT-BR
Affiliation1
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 hana@asu.cas.cz
2 sawant@das.inpe.br
3 cecattojr@gmail.br
JournalAdvances in Space Research
Volume43
Number10
Pages1479-1483
Secondary MarkA_ASTRONOMIA_/_FÍSICA A_ECOLOGIA_E_MEIO_AMBIENTE A_ENGENHARIAS_III A_ENGENHARIAS_IV A_INTERDISCIPLINAR B_CIÊNCIAS_BIOLÓGICAS_I B_GEOCIÊNCIAS C_ENSINO_DE_CIÊNCIAS_E_MATEMATICA
History (UTC)2009-06-19 18:32:37 :: simone -> administrator ::
2010-05-11 01:08:22 :: administrator -> simone ::
2011-05-20 05:35:22 :: simone -> administrator :: 2009
2012-12-14 14:45:37 :: administrator -> banon :: 2009
2013-02-19 13:54:53 :: banon -> administrator :: 2009
2020-04-28 17:48:41 :: administrator -> simone :: 2009
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe 22 min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ondrejov radiospectrograph in frequency range 1200-4500 MHz has been analyzed. We have round that the characteristic periods of about 60 s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200-4500 MHz. The behavior of individual wave trains at lower frequencies is different from that at higher frequencies. These individual wave trains have some common as well as different properties. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters in their wavelet power and global spectra are studied and discussed.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Coronal fast wave...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filecoronal fast.pdf
User Groupadministrator
banon
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m18@80/2008/03.17.15.17.24
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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