| 1. Identity statement | ||||
| Reference Type | Conference Paper (Conference Proceedings) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34T/4AC834H | |||
| Repository | sid.inpe.br/mtc-m21d/2023/12.11.13.19 | |||
| Metadata Repository | sid.inpe.br/mtc-m21d/2023/12.11.13.19.45 | |||
| Metadata Last Update | 2024:01.02.17.16.56 (UTC) administrator | |||
| Secondary Key | INPE--PRE/ | |||
| Citation Key | KozaiHKMMISDMESBBADSHKKMSMKE:2023:PrNeAn | |||
| Title | North-South Anisotropy of Galactic Cosmic Rays: Proposal for a New Analysis Method  | |||
| Year | 2023 | |||
| Access Date | 2024, May 17 | |||
| Secondary Type | PRE CI | |||
| 2. Context | ||||
| Author | 1 Kozai, Masayoshi 2 Hayashi, Yuki 3 Kato, Chihiro 4 Munukata, Kazuoki 5 Masuda, Yoshiki 6 Iwai, Kazumasa 7 Silva, Marlos Rockenbach da 8 Dal Lago, Alisson 9 Mendonça, Rafael Rodrigues Souza de 10 Echer, Ezequiel 11 Schuch, Nelson Jorge 12 Bageston, José Valentin 13 Braga, C. R. 14 Al Jassar, Hala K. 15 Duldig, Marcus 16 Sharma, Madan M. 17 Humble, John E. 18 Kadokura, Akira 19 Kataoka, Ryuho 20 Miyake, Shoko 21 Sabbah, Ismail S. 22 Mangeard, Pierre-Simon 23 Kuwabara, Takao 24 Evenson, Paul Arthur | |||
| Resume Identifier | 1 2 3 4 5 6 7 8 8JMKD3MGP5W/3C9JGH3 9 10 8JMKD3MGP5W/3C9JH3D 11 8JMKD3MGP5W/3C9JHUD | |||
| Group | 1 2 3 4 5 6 7 DIHPA-CGCE-INPE-MCTI-GOV-BR 8 DIHPA-CGCE-INPE-MCTI-GOV-BR 9 DIHPA-CGCE-INPE-MCTI-GOV-BR 10 DIHPA-CGCE-INPE-MCTI-GOV-BR 11 COESU-CGGO-INPE-MCTI-GOV-BR 12 COESU-CGGO-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 Research Organization of Information and Systems 2 Shinshu University 3 Shinshu University 4 Shinshu University 5 Shinshu University 6 Nagoya University 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 Instituto Nacional de Pesquisas Espaciais (INPE) 9 Instituto Nacional de Pesquisas Espaciais (INPE) 10 Instituto Nacional de Pesquisas Espaciais (INPE) 11 Instituto Nacional de Pesquisas Espaciais (INPE) 12 Instituto Nacional de Pesquisas Espaciais (INPE) 13 George Mason University Fairfax 14 Kuwait University 15 University of Tasmania 16 Kuwait University 17 University of Tasmania 18 Research Organization of Information and Systems 19 The Graduate University for Advanced Studies 20 National Institute of Technology (KOSEN) 21 Public Authority of Applied Education and Training 22 University of Delaware 23 University of Delaware 24 University of Delaware | |||
| Author e-Mail Address | 1 2 3 4 5 6 7 marlos.silva@inpe.br 8 alisson.dallago@inpe.br 9 10 ezequiel.echer@inpe.br 11 nelson.schuch@inpe.br 12 jose.bageston@inpe.br | |||
| Conference Name | AGU FAll Meeting | |||
| Conference Location | San Francisco, CA | |||
| Date | 11-15 Dec. 2023 | |||
| Publisher | AGU | |||
| Book Title | Proceedings | |||
| History (UTC) | 2023-12-11 19:41:45 :: simone -> administrator :: 2023 2024-01-02 17:16:56 :: administrator -> simone :: 2023 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Version Type | publisher | |||
| Abstract | The north-south (NS) anisotropy, or NS asymmetry of galactic cosmic-ray (GCR) intensity, indicates a GCR flow perpendicular to the ecliptic plane which contains both the interplanetary magnetic field (IMF) and radial density gradient of GCRs induced by the solar modulation on average. This uniqueness of the pointing direction of NS anisotropy results in a phenomenon unseen in other anisotropy components, a reversal of its polarity according to the IMF sector polarity. The magnitude of the NS anisotropy reversal allows us to estimate the density gradient of GCRs, making it a unique indicator of the solar modulation of GCRs. Ground-based muon detectors are proven to provide more significant measurements of the NS anisotropy than neutron monitors, thanks to the small degradation of muon momentum directions in the atmospheric propagation and its relatively higher response rigidity to primary cosmic rays where the NS anisotropy is enhanced. However, the NS anisotropy measurements have suffered from the atmospheric temperature effect on muons. Recently a new correction method for the temperature effect using atmospheric re-analysis data was proposed. We are attempting a precise calculation of the NS anisotropy utilizing this correction method. Solar cycle variations of the NS anisotropy, or GCR density gradient, and its rigidity spectrum will be presented with unprecedented accuracy. | |||
| Area | CEA | |||
| Arrangement 1 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > North-South Anisotropy of... | |||
| Arrangement 2 | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > North-South Anisotropy of... | |||
| doc Directory Content | there are no files | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| Language | en | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/46KTFK8 8JMKD3MGPCW/46KUBT5 | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notes | ||||
| Empty Fields | archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url volume | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||