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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3A7MBDH
Repositorysid.inpe.br/mtc-m19/2011/08.04.19.10   (restricted access)
Last Update2011:12.20.16.57.08 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/08.04.19.10.43
Metadata Last Update2018:06.05.04.24.43 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1007/s11207-011-9712-y
ISSN0038-0938
1573-093X
Citation KeyKane:2011:HyCoRa
TitleHysteresis of Cosmic Rays with Respect to Sunspot Numbers During the Recent Sunspot Minimum
ProjectFINEP-537/CT.
Year2011
MonthApr
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size247 KiB
2. Context
AuthorKane, R. P.
GroupDGE-CEA-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addresskane@dge.inpe.br
e-Mail Addresssecretaria.cpa@dir.inpe.br
JournalSolar Physics
Volume269
Number2
Pages451-454
History (UTC)2011-08-04 19:12:24 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2011-08-04 19:12:48 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2011-11-01 11:45:46 :: secretaria.cpa@dir.inpe.br -> tereza@sid.inpe.br :: 2011
2011-12-20 16:57:21 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 04:24:43 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsCosmic rays
Hysteresis
Cycle 24
AbstractCosmic ray neutron monitors show intensity changes (counts) anti-correlated with sunspot number R(z), but with a lag of a few months. The lag is similar to 3 months for even cycles and similar to 9-15 months for odd cycles. Thus, for the recently started even Cycle 24, a lag of similar to 3 months was expected. However, for Cycle 24, whereas R(z) had a minimum value (zero) in August 2009, cosmic ray intensity decreased only after March 2010, with a lag of seven months with respect to R(z). Thus, Cycle 24 did not conform to the known pattern of even cycles (lag of similar to 3 months). It may be noted that the minimum at the juncture of Cycle 23-24 was abnormally long, tens of months instead of few months as in earlier cycles. Also, in this solar minimum, the cosmic ray intensity was much higher than in previous cycles.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Hysteresis of Cosmic...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
User Groupadministrator
secretaria.cpa@dir.inpe.br
tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
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7. Description control
e-Mail (login)tereza@sid.inpe.br
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