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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3K3ARD5
Repositorysid.inpe.br/mtc-m21b/2015/08.11.11.38
Metadata Repositorysid.inpe.br/mtc-m21b/2015/08.11.11.38.17
Metadata Last Update2018:06.04.02.55.36 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBalanSSRSOBEON:2015:SeSpWe
TitleSevere space weather including historical events
Year2015
Access Date2024, May 16
Secondary TypePRE CI
2. Context
Author 1 Balan, Nanan
 2 Skoug, R.
 3 Sudarsanam, Tulasi Ram
 4 Rajesh, P. K.
 5 Shiokawa, Kazuo
 6 Otsuka, Yuichi
 7 Batista, Inez Staciarini
 8 Ebihara, Yusuke
 9 Omura, Yoshiharu
10 Nakamura, Takuji
Resume Identifier 1
 2
 3
 4
 5
 6
 7 8JMKD3MGP5W/3C9JHDA
Group 1
 2
 3
 4
 5
 6
 7 DAE-CEA-INPE-MCTI-GOV-BR
Affiliation 1 Nagoya University
 2 Los Alamos National Laboratory
 3 Indian Institute of Geomagnetism
 4 National Cheng Kung University
 5 Nagoya University
 6 Solar-Terrestrial Environment Laboratory
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Kyoto University
 9 Kyoto University
10 National Institute of Polar Research
Author e-Mail Address 1
 2
 3
 4
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 7 inez.batista@inpe.br
Conference NameAnnual Meetings Asia Oceania Geosciences Society (AOGS)
Conference LocationSingapore
Date2-7 Aug.
History (UTC)2015-08-11 11:38:17 :: simone -> administrator ::
2018-06-04 02:55:36 :: administrator -> simone :: 2015
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThanks to the work of a number of scientists starting with Carrington [1859] it is known that severe space weather can causeextensive social and economic disruptions in the modern high-tech society. It is therefore important to understand what determines the severity of space weather, and whether it can be predicted. We present the results obtained from the analysis of coronal mass ejections (CME), solar energetic particle (SEP) events, interplanetary magnetic field (IMF), CME-magnetosphere coupling and geomagnetic storms associated with the major space weather events since 1998 by combining data from the ACE and GOES satellites with geomagnetic parameters, and the Carrington event of 1859, the Quebec event of 1989, and an event in 1958. The results seem to indicate that (1) it is the impulsive energy mainly due to the impulsive velocity and orientation of IMF Bz at the leading edge of the CMEs (or CME front) that determine the severity of space weather. (2) CMEs having high impulsive velocity (sudden non-fluctuating increase by over 275 km s-1 over the background) caused severe space weather (SvSW) effects in ACE (failure of the SWI mode of SWEPAM in ACE). (3) The impact of such CMEs which also show the IMF Bz southward from the leading edge caused SvSW at the Earth including extreme geomagnetic storms of mean DstMP < -250 nT during main phases; and the known electric power outages happened during some of these SvSW events. (4) The higher the impulsive velocity, the more severe the space weather, like faster weather fronts and tsunami fronts causing more severe damages through impulsive action. (5) The CMEs having IMF Bz northward at the leading edge do not seem to cause SvSW on Earth though, later when the IMF Bz turns southward, they can lead to super geomagnetic storms of intensity (DstMin) less than even -400 nT.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Severe space weather...
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4. Conditions of access and use
User Groupself-uploading-INPE-MCTI-GOV-BR
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Reader Groupadministrator
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Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item List
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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