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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3QRD3L8
Repositorysid.inpe.br/mtc-m21c/2018/04.03.16.22
Last Update2018:04.03.16.22.16 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/04.03.16.22.16
Metadata Last Update2020:12.07.21.11.20 (UTC) administrator
DOI10.1002/2017JA024779
ISSN2169-9402
Citation KeyTsurutaniLaEcHaNaMaMe:2018:Co“MEx
TitleComment on “Modeling Extreme “Carrington-Type” Space Weather Events Using Three-Dimensional Global MHD Simulations” by C. M. Ngwira, A. Pulkkinen, M. M. Kuznetsova, and A. Glocer”
Year2018
MonthFeb.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size446 KiB
2. Context
Author1 Tsurutani, Bruce T.
2 Lakhina, Gurbax S.
3 Echer, Ezequiel
4 Hajra, Rajkumar
5 Nayak, Chinmaya
6 Mannucci, Anthony J.
7 Meng, Xing
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH3D
ORCID1 0000-0001-7299-9835
2 0000-0002-8956-486X
3 0000-0002-8351-6779
4 0000-0003-0447-1531
5 0000-0002-3067-2313
6 0000-0003-2391-8490
7 0000-0001-6154-9150
Group1
2
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 California Institute of Technology
2 Indian Institute of Geomagnetism
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 LPC2E, CNRS
5 George Mason University
6 California Institute of Technology
7 California Institute of Technology
Author e-Mail Address1
2
3 ezequiel.echer@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume123
Number2
Pages1388-1392
History (UTC)2018-04-03 16:22:16 :: simone -> administrator ::
2018-04-03 16:22:17 :: administrator -> simone :: 2018
2018-04-03 16:26:03 :: simone -> administrator :: 2018
2020-12-07 21:11:20 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractAn alternative scenario to the Ngwira et al. (2014, https://doi.org/10.1002/2013JA019661) high sheath densities is proposed for modeling the Carrington magnetic storm. Typical slow solar wind densities (~5 cm3 ) and lower interplanetary magnetic cloud magnetic field intensities (~90 nT) can be used to explain the observed initial and main phase storm features. A second point is that the fast storm recovery may be explained by ring current losses due to electromagnetic ion cyclotron wave scattering.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Comment on “Modeling...
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source Directory Contentthere are no files
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3QRD3L8
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3QRD3L8
Languageen
Target Filetsurutani_comment.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
sid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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