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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/EpeS6
Repositorysid.inpe.br/marciana/2004/12.08.08.30
Last Update2005:02.01.02.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/12.08.08.30.26
Metadata Last Update2018:06.05.01.21.11 (UTC) administrator
Secondary KeyINPE-12159-PRE/7500
ISSN0094-8276
Citation KeyKuwabaraFTKMDHSTGSMYKAKBEP:2004:GeInCM
TitleGeometry of an interplanetary CME on October 29, 2003 deduced from cosmic rays
Year2004
MonthOct.
Access Date2024, May 18
Secondary TypePRE PI
Number of Files1
Size305 KiB
2. Context
Author 1 Kuwabara, T.
 2 Fujii, Z.
 3 Tokumaru, M.
 4 Kojima, M.
 5 Marubashi, K.
 6 Duldig, M. L.
 7 Humble, J. E.
 8 Silva, M. R.
 9 Trivedi, Nalin Babulal
10 Gonzalez, Walter Demetrio
11 Schuch, Nelson Jorge
12 Munakata, K.
13 Yasue, S.
14 Kato, C.
15 Akahane, S.
16 Koyama, M.
17 Bieber, J. W.
18 Evenson, P.
19 Pyle, R.
Resume Identifier 1
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 9 8JMKD3MGP5W/3C9JHTS
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11 8JMKD3MGP5W/3C9JHUD
Group 1 RSU-INPE-MCT-BR
 2 RSU-INPE-MCT-BR
 3 RSU-INPE-MCT-BR
Affiliation 1 Kuwabara T (reprint author), Shinshu Univ, Dept Phys, Matsumoto, Nagano 3908621 Japan
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12 Shinshu Univ, Dept Phys, Matsumoto, Nagano 3908621 Japan
13 Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
14 Australian Antarctic Div, Kingston, Tas 7050 Australia
15 Nagoya Univ, Solar Terr Environm Lab, Aichi, 4648601 Japan
16 Natl Inst Space Res, So Reg Space Res Ctr, OES CRSPE INPE, Santa Maria, RS BR-97110970 Brazil
17 Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001 Australia
18 Natl Inst Informat & Commun Technol, Tokyo, 1848795 Japan
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JournalGeophysical Research Letters
Volume31
Number19
Pages1-5
History (UTC)2006-06-21 16:50:09 :: sergio -> administrator ::
2006-09-28 22:28:12 :: administrator -> sergio ::
2008-01-07 12:53:38 :: sergio -> administrator ::
2018-06-05 01:21:11 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGEOMAGNETIC STORMS
AbstractA coronal mass ejection (CME) associated with an X17 solar flare reached Earth on October 29, 2003, causing an similar to11% decrease in the intensity of high-energy Galactic cosmic rays recorded by muon detectors. The CME also produced a strong enhancement of the cosmic ray directional anisotropy. Based upon a simple inclined cylinder model, we use the anisotropy data to derive for the first time the three-dimensional geometry of the cosmic ray depleted region formed behind the shock in this event. We also compare the geometry derived from cosmic rays with that derived from in situ interplanetary magnetic field (IMF) observations using a Magnetic Flux Rope model.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Geometry of an...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/6qtX3pFwXQZsFDuKxG/EpeS6
zipped data URLhttp://urlib.net/zip/6qtX3pFwXQZsFDuKxG/EpeS6
Languageen
Target File2004kuwabara.pdf
User Groupadministrator
sergio
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissiontransferred to sergio
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.56.48 1
DisseminationWEBSCI; PORTALCAPES; SCIELO; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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