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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3D538F5
Repositorydpi.inpe.br/plutao/2012/11.28.14.20   (restricted access)
Last Update2013:01.23.16.11.05 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2012/11.28.14.20.04
Metadata Last Update2018:06.05.00.01.56 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN0038-0938
1573-093X
Labellattes: 1272123236892781 5 GimenezdecastroCrSiMaCoKa:2012:BuDoRa
Citation KeyGimenezdeCastroCrSiMaCoKa:2012:BuDoRa
TitleA burst with double radio spectrum observed up to 212 GHz
ProjectFAPESP (Proc. 2009/18386-7); UBACyT 20020100100733; PIP 2009- 100766 (CONICET); PICT 2007-1790 (ANPCyT); FAPESP (Proc. 2008/09339-2); European Commission (project HESPE FP7-2010-SPACE-1-263086)
Year2012
Access Date2024, May 14
Secondary TypePRE PI
Number of Files1
Size635 KiB
2. Context
Author1 Gimenez de Castro, Carlos Guillermo
2 Cristiani, G. D.
3 Simões, Paulo J A
4 Mandrini, Cristina
5 Correia, Emilia
6 Kaufmann, P.
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JH2C
Group1
2
3
4
5 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1
2
3
4
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4
5 ecorreia@craam.mackenzie.br
e-Mail Addressecorreia@craam.mackenzie.br
JournalSolar Physics
Volumexx
Pagesx-x
Secondary MarkB1_ASTRONOMIA_/_FÍSICA B1_BIOTECNOLOGIA B2_CIÊNCIA_DA_COMPUTAÇÃO B1_ENGENHARIAS_IV A1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
History (UTC)2012-11-28 23:06:22 :: lattes -> administrator :: 2012
2013-01-20 15:54:25 :: administrator -> marciana :: 2012
2013-01-23 16:11:05 :: marciana -> administrator :: 2012
2018-06-05 00:01:56 :: administrator -> marciana :: 2012
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordssolar bursts
submillimeter emission
radio spectra
AbstractWe study a solar flare that occurred on September 10, 2002, in active region NOAA 10105 starting around 14:52 UT and lasting approximately 5 minutes in the radio range. The event was classified as M2.9 in X-rays and 1N in H. Solar Submillimeter Telescope observations, in addition to microwave data give us a good spectral coverage between 1.415 and 212 GHz. We combine these data with ultraviolet images, hard and soft X-rays observations and full-disk magnetograms. Images obtained from Ramaty High Energy Solar Spectroscopic Imaging data are used to identify the locations of X-ray sources at different energies and to determine the X-ray spectrum, while ultra violet images allow us to characterize the coronal flaring region. The magnetic field evolution of the active region is analyzed using Michelson Doppler Imager magnetograms. The burst is detected at all available radio-frequencies. X-ray images (between 12 keV and 300 keV) reveal two compact sources and 212 GHz data, used to estimate the radio source position, show a single compact source displaced by 25′′ from one of the hard X-ray footpoints. We model the radio spectra using two homogeneous sources, and combine this analysis with that of hard X-rays to understand the dynamics of the particles. Relativistic particles, observed at radio wavelengths above 50 GHz, have an electron index evolving with the typical softhardsoft behaviour.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A burst with...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1208.5904v1.pdf
User Groupadministrator
lattes
marciana
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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7. Description control
e-Mail (login)marciana
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