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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/M2HvV
Repositorysid.inpe.br/mtc-m16@80/2006/08.02.14.51   (restricted access)
Last Update2006:08.02.14.51.47 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/08.02.14.51.49
Metadata Last Update2018:06.05.01.16.55 (UTC) administrator
Secondary KeyINPE-13941--PRE/9121
ISSN0273-1177
Citation KeyTsurutaniMaGuGoJuGaPa:2006:ExHa20
TitleThe extreme Halloween 2003 solar flares (and Bastille Day, 2000 Flare), ICMEs, and resultant extreme ionospheric effects: A review
Year2006
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size319 KiB
2. Context
Author1 Tsurutani, Bruce T.
2 Mannucci, A. J.
3 Guarnieri, Fernando Luís
4 Gonzalez, Walter Demétrio
5 Judge, D. L.
6 Gangopadhyay, P.
7 Pap, J.
Group1
2
3 DGE-INPE-MCT-BR
4 DGE-INPE-MCT-BR
Affiliation1 University of Southern California
2 California Institute of Technology
3 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
4 Instituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
5 University of Southern California
6 University of Southern California
7 Goddard Space Flight Center
JournalAdvances in Space Research
Volume37
Number8
Pages1583-1588
History (UTC)2006-08-02 14:51:49 :: simone -> administrator ::
2018-06-05 01:16:55 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar flares
Ionospheric effects
Halloween events
AbstractExtreme solar flares can cause extreme ionospheric effects. The Oct 28, 2003 flare caused a 25 TECU (a total electron content unit is 1016 electron/m2 column density), or a 30%, increase in the local noon equatorial ionospheric column density. This enhancement occurred within 5 min. This TEC increase was 5 times the TEC increases detected for the Oct 29, 2003, Nov 4, 2003, and the July 14, 2000 (Bastille Day) flares. In the 260340 EUV wavelength range, the Oct 28 flare peak count rate was more than twice as large as for the other three flares. Another strong ionospheric effect is the delayed influence (due to solar wind propagation) of interplanetary coronal mass ejection (ICME) electric fields on the ionosphere. For the Oct 28 and 29 flares, the associated ICMEs propagated from the sun to the Earth at particularly high speeds. The prompt penetration of the interplanetary electric field caused the dayside equatorial ionospheric to be strongly convected upward. This led to enhanced TEC to values >300% nominal values in 2 h. Proposed mechanisms for this TEC enhancement will be discussed.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The extreme Halloween...
doc Directory Contentaccess
source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target FileThe extreme halloween 2003 solar flares.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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