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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/Ltx5P
Repositorysid.inpe.br/mtc-m16@80/2006/06.16.18.06   (restricted access)
Last Update2006:06.16.18.06.33 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/06.16.18.06.34
Metadata Last Update2018:06.05.01.16.50 (UTC) administrator
Secondary KeyINPE-13790--PRE/8976
ISSN0038-0938
1573-093X
Citation KeyKane:2006:CoRaAn
TitleCosmic ray anisotropies around the Forbush decrease of April 11, 2001
Year2006
MonthApr
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size332 KiB
2. Context
AuthorKane, Rajaram Purushottam
Resume Identifier8JMKD3MGP5W/3C9JJ4U
GroupDGE-INPE-MCT-BR
AffiliationInstituto Nacional de Pesquisas Espaciais, Divisão de Geofísica Espacial (INPE.DGE)
JournalSolar Physics
Volume234
Number2
Pages353-362
History (UTC)2006-06-16 18:06:34 :: simone -> administrator ::
2018-06-05 01:16:50 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSOLAR CORONA
HELIOSPHERE
PARAMETERS
GRADIENT
DENSITY
FLOWS
AbstractDuring the Forbush decrease of April 11, 2001, the Ooty (11.4 degrees N, 76.7 degrees E, 2200 m altitude, South India) high energy muon detectors showed considerable anisotropies. Some anisotropies and asymmetries indicated that the Earth did not pass the middle of the interplanetary structure (blob), and passed its northern part. Some anisotropies which occurred when the Earth was outside the blob (notably before the Forbush decrease) could be the precursory increases due to reflection from the shock fronts, but some others could not be understood as these appeared in a direction away from the blob.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Cosmic ray anisotropies...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
Target FileCosmic ray anisotropies around the forbush.pdf
User Groupadministrator
simone
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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