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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/M3js3
Repositorysid.inpe.br/mtc-m16@80/2006/08.03.14.12   (restricted access)
Last Update2006:08.03.14.12.51 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/08.03.14.12.52
Metadata Last Update2018:06.05.01.16.56 (UTC) administrator
Secondary KeyINPE-13952--PRE/9128
ISSN0038-0938
1573-093X
Citation KeyTrottetCorAulYanKau:2006:34UT
TitleElectron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT
Year2006
MonthJune
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size474 KiB
2. Context
Author1 Trottet, G.
2 Correia, Emilia
3 Aulanier, G.
4 Yan, Y.
5 Kaufmann, P.
Resume Identifier1
2 8JMKD3MGP5W/3C9JH2C
Group1
2 DAS-INPE-MCT-BR
Affiliation1 Observatoire de Paris, Section de Meudon
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
3 Observatoire de Paris, Section de Meudon
4 National Astronomical Observatories, Chinese Academy of Sciences
5 CRAAM, Universidade Presbiteriana Mackenzie
JournalSolar Physics
Volume236
Number1
Pages75-95
History (UTC)2006-08-03 14:12:52 :: simone -> administrator ::
2018-06-05 01:16:56 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsHARD X-RAY
RECONNECTING CURRENT SHEETS
DOUBLE-LOOP CONFIGURATION
GAMMA-RAY
MAGNETIC-FIELD
GYROSYNCHROTRON RADIATION
TIME STRUCTURES
MICROWAVE
RADIO
MILLIMETER
AbstractThis paper deals with a detailed analysis of spectral and imaging observations of the November 5, 1998 (H alpha 1B, GOES M1.5) flare obtained over a large spectral range, i.e., from hard X-rays to radiometric wavelengths. These observations allowed us to probe electron acceleration and transport over a large range of altitudes that is to say within small-scale (a few 10(3) km) and large-scale (a few 10(5) km) magnetic structures. The observations combined with potential and linear force-free magnetic field extrapolations allow us to show that: (i) Flare energy release and electron acceleration are basically driven by loop-loop interactions at two independent, low lying, null points of the active region magnetic field; (ii) < 300 keV hard X-ray-producing electrons are accelerated by a different process (probably DC field acceleration) than relativistic electrons that radiate the microwave emission; and (iii) although there is evidence that hard X-ray and decimetric/metric radio-emitting electrons are produced by the same accelerator, the present observations and analysis did not allow us to find a clear and direct magnetic connection between the hard X-ray emitting region and the radio-emitting sources in the middle corona.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Electron acceleration and...
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4. Conditions of access and use
Languageen
Target FileElectron acceleration and transport.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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