1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP8W/34B62C8 |
Repository | sid.inpe.br/mtc-m18@80/2008/12.02.11.58 (restricted access) |
Last Update | 2008:12.02.14.17.54 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m18@80/2008/12.02.11.58.46 |
Metadata Last Update | 2018:06.04.04.05.47 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | SabbahMFYKBESLSK:2008:FiGeSt |
Title | First geomagnetic storm ever observed from the Middle East using cosmic rays |
Year | 2008 |
Access Date | 2024, May 13 |
Secondary Type | PRE CI |
Number of Files | 1 |
Size | 6 KiB |
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2. Context | |
Author | 1 Sabbah, Ismail 2 Munakata, Kazuoki 3 Fushishita, Akira 4 Chihiro Kato 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 Marcus L. Duldig 14 J. E. Humble 15 Kota, Jozsef |
Resume Identifier | 1 2 3 4 5 6 7 8 9 10 8JMKD3MGP5W/3C9JGH3 11 8JMKD3MGP5W/3C9JHUD |
Group | 1 2 3 4 5 6 7 8 9 DAE-CEA-INPE-MCT-BR 10 DAE-CEA-INPE-MCT-BR |
Conference Name | European Cosmic Ray Symposium. |
Conference Location | Kosice, Slovakia |
Date | 9-12 th September |
Tertiary Type | Oral Session |
History (UTC) | 2008-12-02 14:32:56 :: seeger05 -> administrator :: 2018-06-04 04:05:47 :: administrator -> seeger05 :: 2008 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Abstract | The 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > First geomagnetic storm... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | Fist geomagnetic storm ever observed from the middle east using cosmic rays show_abstract.php.htm |
User Group | administrator seeger05 administrator |
Visibility | shown |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETL868 |
Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
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6. Notes | |
Empty Fields | affiliation archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format 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 |
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7. Description control | |
e-Mail (login) | seeger05 |
update | |
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