Close

1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/MTC-m13@80/2005/10.13.15.55
Last Update2006:06.14.04.42.44 (UTC) administrator
Metadata Repositorysid.inpe.br/MTC-m13@80/2005/10.13.15.55.54
Metadata Last Update2018:06.04.04.12.28 (UTC) administrator
Secondary KeyINPE-13196-PRE/8452
Citation KeyFrigoSaSiLaTrSc:2005:AnGeSt
TitleAnalysis of the Geomagnetic Storm Variations and the count-rate of Cosmic Ray Muons recorded at the Brazilian Southern Space Observatory
Year2005
Access Date2024, May 18
Number of Files1
Size133 KiB
2. Context
Author1 Frigo, Everton
2 Savian, Jairo F.
3 Silva, Marlos R. da
4 Lago, Alisson Dal
5 Trivedi, Nalin Babulal
6 Schuch, Nelson Jorge
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JGH3
5 8JMKD3MGP5W/3C9JHTS
6 8JMKD3MGP5W/3C9JHUD
Group1 INPE-MCT-BR
Conference NameInternational Congress of the Brazilian Geophysical Society, 9.
Conference LocationSalvador,
Date11-14 Sept.
History (UTC)2005-10-13 16:06:33 :: seeger05 -> marciana ::
2005-11-24 12:47:20 :: marciana -> banon ::
2008-04-30 21:59:25 :: banon -> marciana ::
2008-05-02 14:59:03 :: marciana -> administrator ::
2018-06-04 04:12:28 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
AbstractAn analysis of geomagnetic storm variations and the count rate of cosmic ray muons recorded at the Brazilian Southern Space Observatory -OES/CRSPE/INPE-MCT, in São Martinho da Serra, RS during the month of November 2004, is presented in this paper. The geomagnetic measurements are done by a three component low noise fluxgate magnetometer and the count rate of cosmic ray muons, are recorded by a multidirectional muon detector, both instruments installed at the Observatory. The fluxgate magnetometer measures variations in the three orthogonal component of Earth magnetic field, H (Nort-South), D (East-West) and Z (Vertical), with data sampling rate of 0.5 Hz. The muon detector records hourly count rates. The arrival of a solar disturbance can be identify observing the decrease in the muon count rate. The goal of this work is to describe the physical morphology and phenom
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/MTC-m13@80/2005/10.13.15.55
zipped data URLhttp://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/10.13.15.55
Target Fileanalysis geomagnetic.pdf
User Groupadministrator
Visibilityshown
5. Allied materials
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.57.02 1
sid.inpe.br/mtc-m21/2012/07.13.14.39.46 1
sid.inpe.br/mtc-m21/2012/07.13.14.56.48 1
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
Empty Fieldsaffiliation archivingpolicy archivist area booktitle callnumber contenttype copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label language lineage mark mirrorrepository nextedition nexthigherunit notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark secondarytype serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url versiontype volume
7. Description control
e-Mail (login)marciana
update 


Close