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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QAhqk
Repositorysid.inpe.br/mtc-m17@80/2007/06.28.15.22   (restricted access)
Last Update2007:06.28.15.22.27 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/06.28.15.22.29
Metadata Last Update2021:07.18.04.01.33 (UTC) administrator
Secondary KeyINPE-14764-PRE/9735
ISSN1364-6826
Citation KeyKaneEche:2007:PhShTi
TitlePhase shift (time) between storm-time maximum negative excursions of geomagnetic disturbance index Dst and interplanetary Bz
Year2007
MonthJuly
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size303 KiB
2. Context
Author1 Kane, Rajaram Purushotam
2 Echer, Ezequiel
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
Group1 DGE-INPE-MCT-BR
2 DGE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 kane@dge.inpe.br
2 eecher@dge.inpe.br
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume69
Number9
Pages1009-1020
History (UTC)2007-12-19 14:23:22 :: simone -> administrator ::
2012-10-23 23:55:39 :: administrator -> simone :: 2007
2013-02-20 15:20:00 :: simone -> administrator :: 2007
2021-07-18 04:01:33 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGeomagnetism
Dst
Interplanetary parameters
Bz
AbstractThe evolutions of severe geomagnetic storms (Dst<−200 nT) during solar cycle 23 were examined. For each storm, certain timing landmarks (starting of increases of interplanetary total field B, its Bz component, Dst changes, etc.) were noted and from these, various antecedence intervals were calculated. It was noticed that the various delays varied in a very wide range from storm to storm. Thus, some storms had a warning of only 4 h at the ACE location, while others had a warning of up to 30 h. These variations do not depend upon the SunEarth transit time. Also, faster interplanetary structures do not necessarily give quicker or stronger Dst evolutions, though larger negative Bz seems to give stronger negative Dst, but not necessarily earlier.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Phase shift (time)...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filephase shift.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; AGU; MGA; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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