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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, Oct. 31
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
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
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
e-Mail (login)marciana
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