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1. Identity statement
Reference TypeJournal Article
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Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP5W34M/3HE6FGJ
Repositorysid.inpe.br/mtc-m21b/2014/11.18.23.59.49
Last Update2015:02.11.11.21.10 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2014/11.18.23.59.50
Metadata Last Update2018:06.04.03.04.32 (UTC) administrator
DOI10.1002/2013JA019748
ISSN2169-9402
Labelscopus 2014-11 KozyraLCZEEFFFGHHLMMPRRSSSTTV:2014:GeCo
Citation KeyKozyraLCZEEFFFGHHLMMPRRSSSTTV:2014:GeCo
TitleSolar filament impact on 21 January 2005: Geospace consequences
Year2014
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size15444 KiB
2. Context
Author 1 Kozyra, J. U.
 2 Liemohn, M. W.
 3 Cattell, C.
 4 De Zeeuw, D.
 5 Escoubet, C. P.
 6 Evans, D. S.
 7 Fang, X.
 8 Fok, M. -C.
 9 Frey, H. U.
10 Gonzalez, Walter Demétrio
11 Hairston, M.
12 Heelis, R.
13 Lu, G.
14 Manchester, W. B.
15 Mende, S.
16 Paxton, L. J.
17 Rastaetter, L.
18 Ridley, A.
19 Sandanger, M.
20 Soraas, F.
21 Sotirelis, T.
22 Thomsen, M. W.
23 Tsurutani, B. T.
24 Verkhoglyadova, O.
Resume Identifier 1
 2
 3
 4
 5
 6
 7
 8
 9
10 8JMKD3MGP5W/3C9JJC4
Group 1
 2
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 8
 9
10 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation 1 University of Michigan
 2 University of Michigan
 3 School of Physics and Astronomy, University of Minnesota
 4 University of Michigan
 5 ESA
 6 University of Colorado Boulder
 7 NASA Goddard Space Flight Center
 8 University of California
 9 University of Texas at Dallas
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 High Altitude Observatory
12 High Altitude Observatory
13 Johns Hopkins University
14 University of Michigan
15 University of California
16 Community Coordinated Modeling Center (GSFC)
17 Birkeland Centre for Space Science, Department of Physics and Technology, University of Bergen, Bergen, Norway
18 University of Michigan
19 Los Alamos National Laboratory
20 Los Alamos National Laboratory
21 Community Coordinated Modeling Center (GSFC)
22 Jet Propulsion Laboratory
23 Jet Propulsion Laboratory
24 Jet Propulsion Laboratory
Author e-Mail Address 1 jukozyra@umich.edu
 2
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 4
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10 gonzales@dge.inpe.br
e-Mail Addressmarcelo.pazos@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume119
Number7
Pages5401-5448
History (UTC)2018-06-04 03:04:32 :: administrator -> marcelo.pazos@inpe.br :: 2014
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractOn 21 January 2005, a moderate magnetic storm produced a number of anomalous features, some seen more typically during superstorms. The aim of this study is to establish the differences in the space environment from what we expect (and normally observe) for a storm of this intensity, which make it behave in some ways like a superstorm. The storm was driven by one of the fastest interplanetary coronal mass ejections in solar cycle 23, containing a piece of the dense erupting solar filament material. The momentum of the massive solar filament caused it to push its way through the flux rope as the interplanetary coronal mass ejection decelerated moving toward 1 AU creating the appearance of an eroded flux rope (see companion paper by Manchester et al. (2014)) and, in this case, limiting the intensity of the resulting geomagnetic storm. On impact, the solar filament further disrupted the partial ring current shielding in existence at the time, creating a brief superfountain in the equatorial ionosphere - an unusual occurrence for a moderate storm. Within 1 h after impact, a cold dense plasma sheet (CDPS) formed out of the filament material. As the interplanetary magnetic field (IMF) rotated from obliquely to more purely northward, the magnetotail transformed from an open to a closed configuration and the CDPS evolved from warmer to cooler temperatures. Plasma sheet densities reached tens per cubic centimeter along the flanks - high enough to inflate the magnetotail in the simulation under northward IMF conditions despite the cool temperatures. Observational evidence for this stretching was provided by a corresponding expansion and intensification of both the auroral oval and ring current precipitation zones linked to magnetotail stretching by field line curvature scattering. Strong Joule heating in the cusps, a by-product of the CDPS formation process, contributed to an equatorward neutral wind surge that reached low latitudes within 1-2 h and intensified the equatorial ionization anomaly. Understanding the geospace consequences of extremes in density and pressure is important because some of the largest and most damaging space weather events ever observed contained similar intervals of dense solar material.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Solar filament impact...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
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zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP5W34M/3HE6FGJ
Languageen
Target FileKozyra_solar.pdf
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5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; AGU; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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