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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/mtc-m17@80/2007/11.20.22.26   (restricted access)
Last Update2008:10.16.18.55.17 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/11.20.22.26.07
Metadata Last Update2018:06.05.03.35.15 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyKuwabaraBEMYKFDHSTGLS:2007:DeICGe
TitleDetermination of ICME Geometry and Orientation from Ground Based Observations of Galactic Cosmic Rays
Year2007
Access Date2024, May 02
Secondary TypePRE CI
Number of Files1
Size155 KiB
2. Context
Author 1 Kuwabara, Takao
 2 Bieber, John
 3 Evenson, Paul
 4 Munakata, Kazuoki
 5 Yasue, Shin-ichi
 6 Kato, Chihiro
 7 Fujii, Zenjiro
 8 Duldig, Marcus
 9 Humble, John
10 Silva, Marlos rockenbach da
11 Trivedi, Nalin Babulal
12 Gonzalez, Walter
13 Lago, Alisson Dal
14 Schuch, Nelson Jorge
Resume Identifier 1
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11 8JMKD3MGP5W/3C9JHTS
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13 8JMKD3MGP5W/3C9JGH3
14 8JMKD3MGP5W/3C9JHUD
Group 1
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10 RSU-INPE-MCT-BR
11 RSU-INPE-MCT-BR
12 DAE-INPE-MCT-BR
13 DGE-INPE-MCT-BR
14 RSU-INPE-MCT-BR
Affiliation 1 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware
 2 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware
 3 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware
 4 Department of Physics, Shinshu University
 5 School of General Education, Shinshu University
 6 Department of Physics, Shinshu University
 7 STE Laboratory, Nagoya University
 8 Australian Antarctic Division
 9 School of Mathematics and Physics, University of Tasmania
10 National Institute for Space Research
11 National Institute for Space Research
12 National Institute for Space Research
13 National Institute for Space Research
14 Southern Regional Space Research Center - CRS/INPE
Conference Name30 Th International Cosmic Ray Conference
Conference LocationYucatan, Mexico
DateJuly 3 - 11
Tertiary TypePoster Session
History (UTC)2008-05-19 14:05:40 :: seeger05 -> administrator ::
2008-06-29 14:49:05 :: administrator -> seeger05 ::
2009-06-24 23:48:45 :: seeger05 -> administrator ::
2018-06-05 03:35:15 :: administrator -> seeger05 :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractWe have developed a method for determining ICME (Interplanetary coronal mass ejection) geometry from galactic cosmic ray data recorded by the ground-based muon detector network. The cosmic ray density depression inside the ICME, which is the cause of a Forbush decrease, is represented as an expanding cylinder based on a theoretical model of the cosmic ray particle diffusion. ICME geometry and orientation are deduced from observed time variations of density and density gradient, and are compared with that deduced from a magnetic flux rope model. From March 2001 to May 2005, 11 ICME events that produced Forbush decreases >2% were observed, and clear variations of the density gradient due to ICME passage were observed in 8 of 11 events. In 3 of these 8 events, clear signatures of magnetic flux rope structure (large, smooth rotation of magnetic field) were also seen, and the ICME geometry and orientation deduced from the two methods were very similar. This suggests that the cosmic ray-based method may provide a more robust method for deducing ICME geometry than the flux rope method for events where a large Forbush decrease is observed.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Determination of ICME...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Determination of ICME...
Arrangement 3urlib.net > CRCRS > Determination of ICME...
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4. Conditions of access and use
Languageen
Target FileICRC2007_Kuwabara Determination of ICME Geometry and Orientation from Ground .. pdf.pdf
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Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3EUFCFP
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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