1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Repository | sid.inpe.br/MTC-m13@80/2005/10.13.15.55 |
Last Update | 2006:06.14.04.42.44 (UTC) administrator |
Metadata Repository | sid.inpe.br/MTC-m13@80/2005/10.13.15.55.54 |
Metadata Last Update | 2018:06.04.04.12.28 (UTC) administrator |
Secondary Key | INPE-13196-PRE/8452 |
Citation Key | FrigoSaSiLaTrSc:2005:AnGeSt |
Title | Analysis of the Geomagnetic Storm Variations and the count-rate of Cosmic Ray Muons recorded at the Brazilian Southern Space Observatory |
Year | 2005 |
Access Date | 2024, May 18 |
Number of Files | 1 |
Size | 133 KiB |
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2. Context | |
Author | 1 Frigo, Everton 2 Savian, Jairo F. 3 Silva, Marlos R. da 4 Lago, Alisson Dal 5 Trivedi, Nalin Babulal 6 Schuch, Nelson Jorge |
Resume Identifier | 1 2 3 4 8JMKD3MGP5W/3C9JGH3 5 8JMKD3MGP5W/3C9JHTS 6 8JMKD3MGP5W/3C9JHUD |
Group | 1 INPE-MCT-BR |
Conference Name | International Congress of the Brazilian Geophysical Society, 9. |
Conference Location | Salvador, |
Date | 11-14 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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Abstract | An 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 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 | |
data URL | http://urlib.net/ibi/sid.inpe.br/MTC-m13@80/2005/10.13.15.55 |
zipped data URL | http://urlib.net/zip/sid.inpe.br/MTC-m13@80/2005/10.13.15.55 |
Target File | analysis geomagnetic.pdf |
User Group | administrator |
Visibility | shown |
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5. Allied materials | |
Citing Item List | sid.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 Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
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6. Notes | |
Empty Fields | affiliation 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 |
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7. Description control | |
e-Mail (login) | marciana |
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