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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3S29A9P
Repositorysid.inpe.br/mtc-m21c/2018/10.10.12.08
Last Update2018:10.10.12.08.30 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/10.10.12.08.30
Metadata Last Update2019:04.06.04.53.15 (UTC) administrator
DOI10.1029/2018JA025683
ISSN2169-9402
Citation KeyRawatEcheGonz:2018:HoDiAr
TitleHow Different Are the Solar Wind-Interplanetary Conditions and the Consequent Geomagnetic Activity During the Ascending and Early Descending Phases of the Solar Cycles 23 and 24?
Year2018
MonthAug.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2618 KiB
2. Context
Author1 Rawat, Rashmi
2 Echer, Ezequiel
3 Gonzalez Alarcon, Walter Demétrio
Resume Identifier1
2 8JMKD3MGP5W/3C9JH3D
3 8JMKD3MGP5W/3C9JJC4
ORCID1 0000-0002-5917-8693
2 0000-0002-8351-6779
3 0000-0002-4859-9310
Group1
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 National Centre for Antarctic and Ocean Research
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 ezequiel.echer@inpe.br
3 walter.gonzalez@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume123
Number8
Pages6621-6638
History (UTC)2018-10-10 12:08:30 :: simone -> administrator ::
2018-10-10 12:08:30 :: administrator -> simone :: 2018
2018-10-10 12:08:47 :: simone -> administrator :: 2018
2019-04-06 04:53:15 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe current work investigates the possible solar wind-interplanetary (SW-IP) drivers of geomagnetic storms during the longest period (ascending to early descending phases) of the ongoing solar cycle (24). We present a comparative analysis between the two consecutive solar cycles (SCs) 23 and 24. Both the cycles exhibited dual peak feature as observed in the smoothed sunspot numbers SSNsmoothed. For both the cycles, second peak in the SSNsmoothed is higher than the first one as exhibited in the revised SSNsmoothed version. During the entire interval between the ascending to early descending phases (December 2008 to December 2016) of SC-24, the southward directed Bz and the dawn-dusk electric field (Ey) were consistently weaker as compared to that during similar interval of SC-23 (May 1996 to July 2004). The geomagnetic field response represented by Dst index concurrently exhibited similar variation patterns during both the periods. A striking reduction in the intense storm occurrence rate by ∼75% was observed during the considered period of the current solar cycle in comparison to the previous cycle. However, moderate storm occurrence was reduced only by 32% in SC-24 as compared to SC-23, which could be attributed to the dominance of corotating interaction regions during SC-24. No significant difference is found between the intense storm rates around the vernal and autumnal equinoxes in cycle 24, whereas distinct autumnal equinoctial dominance is evident for cycle 23. Further, within each cycle, there is no significant difference in the moderate storm rates around vernal and autumnal equinoxes.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > How Different Are...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3S29A9P
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3S29A9P
Languageen
Target Filerawat_how.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/mtc-m21/2012/07.13.14.45.47 3
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 2
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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