| 1. Identity statement | |
| Reference Type | Conference Paper (Conference Proceedings) |
| Site | mtc-m16b.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Repository | sid.inpe.br/mtc-m17@80/2007/11.20.22.50 (restricted access) |
| Last Update | 2008:10.16.19.02.49 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m17@80/2007/11.20.22.50.19 |
| Metadata Last Update | 2018:06.05.03.35.15 (UTC) administrator |
| Secondary Key | INPE--PRE/ |
| Citation Key | OkazakiMEDHSSSFFNCYK:2007:LaDiGa |
| Title | Latitudinal Distribution of Galactic cosmic Ray Density and its Effect on the CIR-Driven Modulations of Density and Density Gradient measured by the Muon Detector Network  |
| Year | 2007 |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE CI |
| Number of Files | 1 |
| Size | 155 KiB |
| 2. Context | |
| Author | 1 Okazaki, Yoshitaka 2 Munakata, Kazuoki 3 Evenson, Paul 4 Duldig, Marcus L. 5 Humble, John E. 6 Schuch, Nelson Jorge 7 Silva, Marlos R. da 8 lago, Alisson Dal 9 Sabbah, Ismail 10 Fukunishi, Hiroshi 11 Fukushita, Akira 12 Narumi, Takuya 13 Chiba, Tatsuo 14 Yasue, Shin-ichi 15 Kato, Chihiro |
| Resume Identifier | 1 2 3 4 5 6 8JMKD3MGP5W/3C9JHUD 7 8 8JMKD3MGP5W/3C9JGH3 |
| Group | 1 2 3 4 5 6 RSU-INPE-MCT-BR 7 DGE-INPE-MCT-BR 8 DGE-INPE-MCT-BR |
| Affiliation | 1 Department of Geophysics, Tohoku University 2 Faculty of Science, Shinshu University, Japan 3 Bartol Research Institute and Department of Physics and Astronomy, University of Delaware 4 Australian Government Antarctic Division, Australia 5 School of Mathematics and Physics, University of Tasmania, Australia 6 Southern Regional Space Research Center, Brazil 7 National Institute for Space Research, Brazil 8 National Institute for Space Research, Brazil 9 Faculty of Science, Kuwait University, Kuwait 10 Department of Geophysics, Tohoku University, Japan 11 Faculty of Science, Shinshu University, Japan 12 Faculty of Science, Shinshu University, Japan 13 School of General Education, Shinshu University, Japan 14 School of General Education, Shinshu University, Japan 15 School of General Education, Shinshu University, Japan |
| Conference Name | 30 Th International Cosmic Ray Conference |
| Conference Location | Yucatan, Mexico |
| Date | July 3 – 11 |
| Tertiary Type | Poster Session |
| History (UTC) | 2007-11-20 22:50:19 :: seeger05 -> administrator :: 2008-06-29 14:49:07 :: administrator -> seeger05 :: 2008-10-16 19:02:49 :: 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 Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Abstract | Richardson et al. [1996] statistically investigated CIR-driven modulations of Galactic Cosmic Ray (GCR) density with the data obtained by satellites. By examining depressions caused by CIRs with and without the Sector Boundary (SBs), they concluded that SBs do not organize the GCR density. On the other hand, a 22-year cycle in the amplitude of depressions was also confirmed. They suggested that this is caused by changes in large-scale heliospheric magnetic field. In order to reveal an effect of the large-scale magnetic field on GCR density distributions, we have investigated a relationship between interplanetary magnetic field and GCR density gradient measured by the Muon detector network. It has been found that GCR density tends to have its maximum (minimum) at SBs when A is positive (negative). We have also investigated individual CIR-driven modulation, distinguishing whether or not CIR includes a SB. Moreover, a suming a slab-shaped modulated region we have deduced the structure reproducing the observed variations of GCR density and density gradient. For 2001-2006 (A is negative), the structure which has its maximum of GCR density along a SB tends to be deduced in case of CIR with a SB. We will report these results.. |
| Area | CEA |
| Arrangement 1 | urlib.net > DIDGE > Latitudinal Distribution of... |
| Arrangement 2 | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Latitudinal Distribution of... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | ICRC_2007 Okazaki Latitudinal distribution of galactic cosmic ray density and its effect on the CIR-driven modulations of density and density gradient...pdf |
| User Group | administrator seeger05 administrator |
| Visibility | shown |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3EU29DP 8JMKD3MGPCW/3EUFCFP |
| Host Collection | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
| 6. Notes | |
| Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume |
| 7. Description control | |
| e-Mail (login) | seeger05 |
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