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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GT7gD
Repositorysid.inpe.br/iris@1905/2005/07.27.00.03.52   (restricted access)
Last Update2018:04.19.15.27.46 (UTC) marciana
Metadata Repositorysid.inpe.br/iris@1905/2005/07.27.00.04.01
Metadata Last Update2018:06.06.04.22.39 (UTC) administrator
Secondary KeyINPE-3241
DOI10.1038/313380a0
ISSN0028-0836
Label4999
Citation KeyKaufmannCorCosVazDen:1985:SoBuMm
TitleSolar bursts with mm-wave emission at high frequency only
ProjectRADIO
Year1985
Access Date2024, May 08
Secondary TypePRE PI
Number of Files1
Size357 KiB
2. Context
Author1 Kaufmann, Pierre
2 Correia, Emilia
3 Costa, Joaquim Eduardo Rezende
4 Vaz, Ana Maria Zodi
5 Dennis, B. R.
Group1
2 DAS-INPE-BR
3 DAS-INPE-BR
4 DAS-INPE-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, Maryland 20771, USA.
Author e-Mail Address1
2 ecorreia@craam.mackenzie.br
3 jercosta@das.inpe.br
4 ana.zodi@inpe.br
JournalNature
Volume313
Number6001
Pages380-382
History (UTC)2013-03-14 16:21:25 :: administrator -> jefferson :: 1985
2013-04-17 13:08:21 :: jefferson -> administrator :: 1985
2016-06-04 23:02:25 :: administrator -> marciana :: 1985
2018-04-19 15:27:47 :: marciana -> administrator :: 1985
2018-06-06 04:22:39 :: administrator -> marciana :: 1985
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsRADIOASTRONOMIA
AbstractSolar burst emission data at shorter millimetre wavelengths have been based on a few events measured with low sensitivity and relatively poor time resolution. We present here the first high sensitivity and high time-resolution observations taken simultaneously at 90 GHz (lambda =3.3 mm) and at 30 GHz (lambda = 10 mm). These have identified a unique impulsive burst on 21 May 1984 with fast pulsed emission that was considerably more intense at 90 GHz than at lower frequencies. Hard X-ray time structures at energies above 25 keV were almost identical to the 90 GHz structures to better than 1 s. The structure of the onset of the major 90-GHz burst coincided with the hard X-ray structure to within 128 ms. All 90-GHz major time structures consisted of trains of multiple sub-second pulses with rise times as short as 0.03 s and amplitudes that were large compared with the mean flux. When detectable, the 30-GHz sub-second pulses had smaller relative amplitude and were in phase with the corresponding 90-GHz pulses.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Solar bursts with...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
User Groupadministrator
jefferson
Visibilityshown
Archiving Policydenypublisher denyfinaldraft6
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
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7. Description control
e-Mail (login)marciana
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