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1. Identity statement
Reference TypeSlides (Audiovisual Material)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP8W/34B6FGP
Repositorysid.inpe.br/mtc-m18@80/2008/12.02.14.38   (restricted access)
Last Update2008:12.02.14.38.56 (UTC) seeger05
Metadata Repositorysid.inpe.br/mtc-m18@80/2008/12.02.14.38.58
Metadata Last Update2018:06.04.04.05.47 (UTC) administrator
Citation KeySabbahMKYKBESLSDK:2008:FiGeSt
TitleFirst geomagnetic storm ever observed from the Middle East using cosmic
FormatOn-line
Year2008
Access Date2024, Apr. 27
Number of Files1
Size293 KiB
2. Context
Author 1 Sabbah, Ismail
 2 Munakata, Kazuoki
 3 Akira Fushishita
 4 Kato, Chihiro
 5 Yasue, Shinichi
 6 Kuwabara, Takao
 7 Bieber, John W.
 8 Evenson, Paul
 9 Silva, Marlos Rochenback da
10 Lago, Alisson Dal
11 Schuch, Nelson Jorge
12 Z. Fujii
13 Duldig, Marcus L.
14 J. E. Humble
15 Kota, Jozsef
Group 1
 2
 3
 4
 5
 6
 7
 8
 9 DAE-CEA-INPE-MCT-BR
10 DAE-CEA-INPE-MCT-BR
11 RSU-CIE-INPE-MCT-BR
Affiliation 1
 2
 3
 4
 5
 6
 7
 8
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
11 Instituto Nacional de Pesquisas Espaciais (INPE)
Conference NameEuropean Cosmic Ray Symposium.
Conference LocationKosice, Slovakia
Date9-12 th September
PublisherInstituto Nacional de Pesquisas Espaciais
Publisher CitySão José dos Campos
History (UTC)2008-12-02 14:38:58 :: seeger05 -> administrator ::
2018-06-04 04:05:47 :: administrator -> seeger05 ::
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractThe Global Muon Detector Network (GMDN) was almost completed by installing a multi-directional cosmic-ray muon hodoscope in Kuwait in March 2006. The GMDN is currently consisting of four multi-directional muon telescopes located at Nagoya (Japan), Hobart (Australia), Sao Martinho (Brazil) and Kuwait University (Kuwait). This Network is continuously monitoring the galactic cosmic rays intensity in a total of 60 directional channels covering almost the entire sky. Maximum Entropy analysis has been used to compute the power spectral density for each detector during the period March 2006 - December 2007. The spectrum is expressed by a single power law dependence of the form f-n, where n is rigidity dependent. The first two harmonics of the solar daily variation are well defined at each station. The atmospheric temperature effect has been removed for the data and the cosmic rays anisotropy in three dimensions was calculated. .
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > First geomagnetic storm...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > First geomagnetic storm...
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source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target Fileposter  Ismail Sabbah First geomagnetic storm ever observed from...pdf
User Groupseeger05
Visibilityshown
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
8JMKD3MGPCW/3EUFCFP
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress electronicmailaddress isbn issn keywords label lineage mark mirrorrepository nextedition notes numberofslides orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark secondarytype session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
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